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ESTCube-1 In-Orbit Experience and Lessons Learned (Harry Rowe Mimno Award 2016)

Authors:
  • UT Tartu Observatory

Abstract and Figures

ESTCube-1 is a one-unit CubeSat that has been in orbit since May 2013. It was launched to a Sun-synchronous 670 km altitude polar low Earth orbit, and its primary mission objective was to centrifugally deploy a tether as a part of the first in-orbit demonstration of electric solar wind sail (E-sail) technology. The electrical power system, the communication system and the command and data handling system remain fully functional after almost two years in orbit. The camera, developed to image the end-mass of the tether, has taken more than 270 images for camera characterization, for validating the attitude determination system, and for public outreach purposes. The attitude determination accuracy is better than 2°, and the attitude control system is able to spin up the satellite to more than two rotations per second around an axis that suits the E-sail experiment. In this article, we present our in-orbit experience of operating and preparing the satellite for the experiment, as well as lessons learned from development and in-orbit phases.
Content may be subject to copyright.
magazine
Aerospace and Electronic
IEEE
SYSTEMS
August 2015
ISSN 0885-8985
Volume 30 Number 8
12 IEEE A
&
E SYSTEMS MAGAZINE AUGUST 2015
ESTCube-1 In-Orbit Experience and Lessons Learned
Andris Slavinskis
Mihkel Pajusalu
Henri Kuuste
Erik Ilbis
Tõnis Eenmäe
Indrek Sünter
Kaspars Laizans
Hendrik Ehrpais
Paul Liias
Erik Kulu
Jaan Viru
Jaanus Kalde
Urmas Kvell
Johan Kütt
Karlis Zalite
Karoli Kahn
Silver Lätt
Jouni Envall
Petri Toivanen
Jouni Polkko
Pekka Janhunen
Roland Rosta
Taneli Kalvas
Riho Vendt
Viljo Allik
Mart Noorma
Tartu Observatory
Toravere, Estonia
INTRODUCTION
ESTCube-1 is a student satellite project lead by the University
of Tartu, Estonia, and supported by the European Space Agen-
cy (ESA) via Plan for European Cooperating States (PECS).
Development of ESTCube-1 has been a collaborative effort
with many international partners. The satellite is shown on
Figure 1 [1].
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periment [1]–[3]. Implemented according to the one-unit Cube-
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10×10×10 cm and mass of slightly over 1 kg. ESTCube-1 con-
sists of the following subsystems: electrical power system (EPS)
[5]; communication system (COM); command and data handling
system (CDHS) [6]; attitude determination and control system
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payload [11]. All subsystems and payloads were custom built
mostly using commercial off-the-shelf (COTS) components. The
satellite was intended to prepare for and to perform the E-sail
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In-orbit validation.
1. Characterize novel subsystems (EPS, ADCS, and camera).
2. Spin-up the satellite to one rotation per second.
3. Test tether deployment.
4. If deployment successful, charge the tether synchronously
with the satellite spin and measure changes in the spin rate
caused by Coulomb drag interaction between the tether and
the ionospheric plasma.
5. Characterize on-board electron guns.
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cellent platform for educational and in-orbit demonstration (IOD)
projects that are at the same time challenging from the engineer-
ing point of view [12]. The CubeSat standard and the associated
philosophy allow for rapid development [13] and provide the
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eral CubeSat programs have demonstrated how lessons learned
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performed studies of large plasma formations in the ionosphere
Authors’ current address: Tartu Observatory, Space Technol-
ogy, Observatooriumi 1, Tõravere, Tartu county, 00560 Estonia.
E-mail: (andris.slavinskis@estcube.eu). Current addresses for
all authors appear on page 22.
Manuscript received March 5, 2015 and ready for publication
June 15, 2015.
DOI No. 10.1109/MAES.2015.150034.
Review handled by M. Jah.
0885/8985/15/$26.00© 2015 IEEE
Figure 1.
ESTCube-1 satellite before delivering it to the launch provider.
AUGUST 2015 IEEE A
&
E SYSTEMS MAGAZINE 13
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mission to end two months into the mission after it was launched
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mission outcomes and focus on compiling a list of lessons learned
has allowed for the AAUSAT program from Aalborg University
to be successful and continue for more than ten years [19]–[21].
([DPSOHVRIRWKHUVXFFHVVIXO&XEH6DWVHULHVLQFOXGHWKHVDWHOOLWHV
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lin Institute of Technology [24], [25]; the CP CubeSats from Cali-
fornia Polytechnic University [26]; the two DICE satellites from
Utah State University [27]; the Cute series from Tokyo Institute
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Nevertheless, the project has achieved most of its objectives. The
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mission, a need for in-orbit recalibration of attitude determination
sensors, ferromagnetic materials aligning the satellite frame with
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However, from developing all subsystems in-house and operating
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the follow-up missions.
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from the point of view of system engineering, electrical engineer-
ing, mechanical engineering, software engineering, testing and
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IN-ORBIT EXPERIENCE
ESTCube-1 was launched on May 7, 2013 on-board the Vega
rocket by Arianespace. After successful early operations, several
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minimal software functionality to eliminate the risk of activating
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maturely enabling the high voltage supply, unlocking the tether
reel or the tether end-mass.
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functionality: power saving methods, including satellite-wide
timed sleep modes and battery level thresholds for automatically
turning off other subsystems; variety of data logging functions;
a callable timed beacon function for public outreach purposes;
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Similarly to the EPS, the CDHS has been improved by adding
functionality: power saving mode, variety of data logging func-
tions, high time-resolution functions for sensor measurements,
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measurements, as well as attitude determination and control al-
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all calculations take place on the CDHS microcontroller (MCU).
A secondary objective of the ESTCube-1 mission was to take
images of Estonia. Firstly, to validate the camera for this purpose,
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was taken on May 15, 2013. During its lifetime, ESTCube-1 has
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es. These images have been used to characterize the camera and
to validate on-board attitude determination. Due to challenges
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and only at the one-year anniversary was the team able to present
an image of Estonia, Latvia, and a part of Finland (Figure 2). The
most important software updates for the camera were histogram
analysis that allowed automatic detection of the Earth and clouds,
and optimization of power consumption.
Attitude determination sensors were prelaunch calibrated in
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surements. For calibration, statistical methods were used, and at-
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14 IEEE A
&
E SYSTEMS MAGAZINE AUGUST 2015
ESTCube-1 In-Orbit Experience and Lessons Learned
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the system. The accuracy of the system is better than 1.5° [9].
Due to ferromagnetic steel structural components and battery
casings, as well as ferromagnetic nickel anode and cathode of elec-
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with the engineering model and Helmholtz coils in an anechoic
chamber revealed that the residual magnetic moment is larger than
the on-board coils can produce and the direction is roughly diago-
nal from one edge to another. Under stable unactuated conditions
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magnetic moment vector (see Figure 3), which in turn follows the
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tion is not stable and over time the satellite returns to its natural
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was able to reach the spin rate of 360 deg/s.
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by camera nor angular velocity measurements. The most prob-
able reason is that the tether reel is not rotating because either the
rotator is jammed or reel lock deployment has failed (see Section
VIII for more details). To enhance the centrifugal pull force of the
end-mass in an attempt to release the possible mechanical jam,
the spin rate was increased to as high as possible which resulted
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emission-based electron guns, intended to charge up the satellite
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were still tested by powering up the high-voltage source and ap-
plying a potential difference of around 510 V between the electron
gun anode and cathode. Currents going to electron guns measured
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increases the cathode current, indicating that electron guns func-
tion. A voltage of 510 V produced a cathode current of 300 ȝA.
The reliability of the technology still seems to be of concern. One
of the electron guns appears to have disconnected from the power
supply and the functioning one short circuited during tests (after
the successful measurement of the cathode current).
After two years and two weeks of being operational, due to
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ergy-negative mode and consumed the available energy stored in
the batteries to keep operating. Once the batteries were drained,
the satellite did not have enough energy available to be opera-
tional.
SYSTEM ENGINEERING
MODEL PHILOSOPHY
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deliver the satellite on time. On August 2012 the schedule was ac-
celerated by moving the delivery date from May 2013 to January
2013. The decision was a trade-off between engineering risks and
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the risk of components becoming damaged before the launch. In
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reel to turn and break the tether into small pieces, which covered
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solved (solution in Section VIII), in the future, we plan to use a
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(parts of the payload, reaction wheels, thrusters) might not be in-
cluded in all models.
Figure 2.
A composite image showing Estonia, Latvia and a part of Finland taken
on April 23, 2014.
Figure 3.
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The magnetic moment is determined in a laboratory using the engineer-
ing model which did not have electron guns and could be magnetized
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aligned with sides of the satellite.
AUGUST 2015 IEEE A
&
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Slavinskis et al.
STANDARDIZATION
During ESTCube-1 development, each subsystem team was able
to make design decisions independently. Such approach did not
cause any major problems, but we think that all subsystems should
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development tools where applicable, to allow reusability, to save
development time, and to facilitate mobility of team members be-
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XVHG²RQH IRU FRPSXWDWLRQLQWHQVLYH VXEV\VWHPV DQG DQRWKHU IRU
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STANDARDS AND DOCUMENTATION
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Space Standardization (ECSS) can be used as a best practice, sub-
missive following of the ECSS standards introduces too much
overhead for CubeSat projects which usually use agile develop-
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lite. However, the team must use standards and conventions that
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dards (e.g., [33]) have to be followed by CubeSat teams operating
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suggest using web-based documentation tools and/or versioning
and revision control systems. In that case all members can easily
access the newest version (as well as the history of versions) and
maintaining versions is much easier.
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a functionality to log a static set of housekeeping data, but for
in-orbit debugging, dynamic logging of various parameters was
UHTXLUHGDQGLPSOHPHQWHGLQRQHRIWKHVRIWZDUHXSGDWHV
Interface documents must contain detailed descriptions of
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surement units (radians and degrees) between functions imple-
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by updating software. The units must be agreed beforehand but,
as a safety measure for such a risk, a team can introduce correc-
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In addition to the recommendations listed above, we would
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radation, attitude determination and control, as well as payload.
INTEGRATION
The ESTCube-1 team, similar to other CubeSat teams, faced
PDQ\FKDOOHQJHV ZKHQ¿WWLQJ YDULRXVZLUHVDQGFDEOHKDUQHVVHV
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include them in computer-aided design (CAD) mechanical mod-
els. Integration of subsystems and components should be prac-
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gest maintaining as fully functional as possible a prototype of the
satellite that contains the latest subsystems to test prototypes of
new subsystems. In this case, many problems could be detected
right when the new revision of the component is inserted into the
satellite assembly. Another option is assembling as complete a
model of the satellite as possible on a periodical basis and per-
forming conformity tests.
In which order the side panels attach to the satellite frame
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side panel before all connections under that side panel have been
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panels as independent of each other as possible to reduce the ef-
fect of these problems.
To remember to integrate all components, they should be laid
out on a table. A simple but effective way to ensure a success-
ful integration is to make a checklist of all components and pro-
cesses. Development of the checklist should start early and all
subsystems should be involved.
Prior to the integration in the cleanroom all the components
KDYHWREHFOHDQHGWKRURXJKO\WR PHHWWKHVWDQGDUGVUHTXLUHGE\
the launch provider and the middlemen, and to ensure that the
components like solar panels and lenses will not become con-
taminated. Contamination can accumulate on lenses, causing arti-
facts on images, and on solar panels, reducing the amount of solar
photons that can reach solar cells (therefore, effectively reducing
WKHHI¿FLHQF\8VLQJ SURWHFWLYH ¿OPV ZKLOH LQWHJUDWLQJDQGUH-
moving them before the launch can help to avoid contamination.
In the case of ESTCube-1, the satellite was successfully in-
tegrated and some of the suggestions listed above were followed
but by fully following them the integration process can be opti-
PL]HGIXUWKHUDQGPDGHPRUHWLPHHI¿FLHQW
ELECTRICAL ENGINEERING
COMMERCIAL OFF-THE-SHELF COMPONENTS
The electronics on-board ESTCube-1 were assembled solely from
COTS components, a market which is developing rapidly, and
WKHUHIRUHKLJKSHUIRUPDQFHFRPSRQHQWVFDQEHREWDLQHGTXLFNO\
and at low cost. To ensure reliability, automotive or industrial-
grade components were used, where possible, and several redun-
dancy measures were applied to assure that a component failure
would not jeopardize the mission and also several tests were per-
formed (see Section VII).
7KHLQÀLJKWH[SHULHQFHVKRZVWKDWWKLVDSSURDFKZDV DVXF-
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sor and a failed memory) did not cause any larger problems due
to redundant counterparts of components. Applying redundant
16 IEEE A
&
E SYSTEMS MAGAZINE AUGUST 2015
ESTCube-1 In-Orbit Experience and Lessons Learned
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ciency due to power electronics components working in parallel
and sharing the load.
DATA CONNECTIONS WITHIN THE SATELLITE
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bus standards, both between the components of a single subsys-
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ferent subsystems, we used the universal asynchronous receiver/
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according to our in-house developed internal communication
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(e.g., analog-to-digital converters (ADCs), magnetometers, input/
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grated circuit (I2C) and serial peripheral interface (SPI) buses [1].
The main challenges arose from cases when the same com-
munications bus was shared between several components, espe-
cially when the systems connected could be powered on and off
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operational due to the current supplied through a communications
bus, even if the component itself is not powered through its power
pins. Also, a single unpowered device on a bus can drain enough
current to make the whole bus inoperable when communicating
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of a switch for disconnecting unpowered devices from buses or
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latter might not always achieve the results needed.
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two electrical connections, one for transferring data and the other
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the state machine behind I2C communications can malfunction,
leading to the loss of communication capability with the compo-
nent. Therefore, it should be possible to separately power off I2C
devices to reset their internal state. This is not a problem with the
SPI bus. It also has happened that communicating with a single
device using the I2C bus causes other devices on the shared bus
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oscillator chip for beacon systematically malfunctioned when an
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arise from the fact that on an I2C bus, a single data line is oper-
ated both by the bus master and the bus slave, making level con-
version complicated.
All in all, we would suggest refraining from using I2C in sat-
ellites, especially for critical communications. If an I2C bus is
shared between several components, it is advisable to implement
some form of a chip select functionality and have an option to
separately power off or reset components. As another note, SPI
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MEMORY
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for nonvolatile storage of system-critical data because the un-
derlying technology is highly radiation tolerant. However, one
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ample, secure digital (SD) cards. This allows using third-party
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than developing them in-house. However, in the case of memory
devices with integrated controllers, abrupt power loss becomes
an issue.
Parallel memory devices should be used where applicable.
Although the current consumption of parallel memory is higher
when compared with serial memory devices, parallel interface
provides greater performance and makes them easier to address.
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mission success.
ELECTRICAL POWER
Producing and distributing electrical power proved to be a chal-
lenging task both while designing the system and during opera-
tions in orbit. For more details about the design, see [5].
In the design phase, one of the largest challenges was imple-
menting redundancy measures, especially due to the large number
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regulators were duplicated within the EPS in a hot redundant con-
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to monitor redundant systems. Fortunately, no power component
failures were detected during the operations period. The power
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critically analyzing the need for redundancy, during shorter mis-
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lite and before the launch; this time period can be easily over-
looked in the design process. During this time the satellite has to
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tery energy consumption when the satellite is inside the satellite
deployer, since the satellite might remain in that state for months
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the satellite in orbit (overdraining the batteries during this period
might also cause irreversible damage).
As mentioned in Section II, one serious problem we encoun-
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panel degradation will take place during every satellite mission
and this often determines the mission lifetime. Therefore, we sug-
gest a highly granular power distribution system in which com-
ponents and subsystems can be powered off independently, con-
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automatic battery voltage thresholds, which caused automatic
subsystem turn-off when the power level became critical. This
AUGUST 2015 IEEE A
&
E SYSTEMS MAGAZINE 17
Slavinskis et al.
system can be developed to automatically achieve power posi-
tivity, even in case of communication problems. To further save
power, we also used timer-based sleep modes, in which only the
EPS was powered. Still, great care must be taken so that the sys-
WHPH[LWVWKHVHPRGHVUHOLDEO\HYHQLQWKHFDVHRIPHPRU\RYHU-
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used control areas before and after critical memory sections, in
addition to checksums of these sections. It is also a good idea to
implement an automatic system to hard-reset the whole satellite
if the satellite has not been successfully communicated with for
VRPHWLPH:HXVHGDKRXUWLPHUIRUWKLV
An important conclusion from automatic power saving fea-
tures is that all critical data should be kept in nonvolatile mem-
ories. In the case of ESTCube-1, we lost some camera images,
IRUH[DPSOHGXHWRWKHLUQRQYRODWLOHVWRUDJHV\VWHP6KRUWWLPH
power failures might also happen for other reasons, including ra-
diation effects and software errors.
All in all, the power system implementation managed to pro-
vide enough power for the satellite to reduce the problem of solar
panel degradation from a mission stopper to a minor inconvenience.
OTHER
The ESTCube-1 CDHS has two cold redundant MCUs that are
VHOHFWHG E\ WKH (36 7R UHGXFH LQWHUVXEV\VWHP FRPSOH[LW\WKH
on-board computer can have its own low-power radiation-tolerant
processor for critical administrative tasks as well as for switching
the main MCUs.
,QWUDVXEV\VWHPEXVHVVKRXOGQRWEHH[SRVHGWRRWKHUVXEV\V-
tems to avoid possible compatibility issues that would affect the
performance of components within a subsystem.
MECHANICAL ENGINEERING
MAIN STRUCTURE
A mono-block aluminum structure was used on ESTCube-1 be-
cause it is lightweight and it makes it easier to achieve the re-
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tegration, we will not use a mono-block structure in the future.
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for the main structure compared with the one suggested by the
CubeSat standard (aluminum alloy 6061 or 7075) [4] because
it was easier to order in Europe. Changes in the main structure
material did not cause any problems, but the last minute change
from titanium to steel bolts introduced ferromagnetic material on
board. Suppliers and products should be secured early to avoid
late changes.
In a perfect case, the launcher should be known during the de-
YHORSPHQWSKDVHRIWKHVWUXFWXUHEHFDXVHWKHUHTXLUHGWROHUDQFHV
change from launcher to launcher.
8QLTXHPDWHULDOVVKRXOGEHDYRLGHGWRKDYHDFKDQFHWRUHSUR-
duce mechanical structures after the launch.
Apart from the ferromagnetic bolts, all ESTCube-1 issues re-
garding the main structure are minor.
SOLAR PANELS
Solar panel cover glass should be used to avoid rapid degradation
of solar cells. In the case of ESTCube-1, we did not use cover
JODVVVLQFHLWVLQKRXVHDSSOLFDWLRQLVFRPSOH[DQGLWUHGXFHVWKH
EHJLQQLQJRIOLIH HI¿FLHQF\ RI VRODU SDQHOV :H DOVR XQGHUHVWL-
PDWHGWKHH[WHQWRIGHJUDGDWLRQGXULQJWKHWLPHUHTXLUHGWRFRP-
plete the mission. Lack of solar panel cover glass was likely the
main cause of the rapid solar panel degradation on ESTCube-1,
and in hindsight we strongly suggest using cover glass, even for
shorter missions, and especially on polar orbits (higher amount of
trapped particles encountered).
SUN SENSORS
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WLYLW\RIWKHVHQVRUPDVN²LQWHUQDOVXUIDFHVVKRXOGEHDEVRUELQJ
black to avoid stray light on position sensitive devices. In a per-
fect case, the mechanical design of the sensor mask would not
allow the incident light to illuminate internal surfaces. In the case
of ESTCube-1, the aluminum mask was anodized black and the
GHVLJQFDQEHLPSURYHGWRDYRLGXQZDQWHGUHÀHFWLRQVLQVLGHWKH
mask.
CAMERA
The basic aluminum structure of the ESTCube-1 camera lens
HQFORVXUHSURYLGHVD VXI¿FLHQWDPRXQWRIUDGLDWLRQSURWHFWLRQLQ
DORZ(DUWK RUELW 5DGLDWLRQ DIIHFWV WKHFDPHUD5$0ZKLFK LV
located right behind a 1 mm thick side panel [10]. The effect can
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sensor can produce. For ESTCube-1, these effects are not critical
but, if they would be, memory devices could be protected with
shielding.
The imaging sensor is also prone to radiation effects. Perma-
QHQWO\GDPDJHGKRWSL[HOVFDQEHDYRLGHGZLWKWKHKHOSRIDVKXW-
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VSHFWUDOUDGLDWLRQ¿OPVDQGUREXVW¿OWHUVFDQEHXVHG
MOMENT OF INERTIA
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FULWLFDOWRGHWHUPLQHWKHDWWLWXGHSUHFLVHO\ZKHQSHUIRUPLQJ¿QH
attitude maneuvers and especially when high spin rate maneuvers
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control and an attitude estimator with a prediction step is used
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tant because in the prediction step the attitude is propagated using
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QDOYDOXHVRIWKHLQHUWLDPDWUL[ZHUHHVWLPDWHGDQDO\]LQJLQRUELW
PHDVXUHPHQWVRIWKHVSLQSODQH6XFKDSSURDFKSURYLGHGUHTXLUHG
results for attitude determination for low spin rates. However, an
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to grow when the angular velocity increased.
18 IEEE A
&
E SYSTEMS MAGAZINE AUGUST 2015
ESTCube-1 In-Orbit Experience and Lessons Learned
CONNECTORS
On ESTCube-1, the system bus is based on the PC/104+ standard
connector that has 4×SLQVDQGLWVVWLIIQHVVPDNHVLWGLI¿FXOWWR
assemble or disassemble the satellite. The placement and stiffness
of the connectors must be planned thoroughly and coordinated
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to minimize mechanical tensions during integration or disintegra-
tion. As the standard connector heights were not properly taken
into account in the structure design, the pins of some connectors
had to be trimmed. However, challenges with connectors did not
cause any major problems.
SOFTWARE ENGINEERING
OPERATING SYSTEM
In order to minimize the computational overhead and memory foot-
print of the on-board software, a lightweight real-time operating sys-
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important reason to use an operating system was the need for task
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vices that cannot be accessed directly and due to a limited amount of
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the parts that have changed), which would have been useful. If pos-
sible, we suggest using an operating system that provides most of the
QHHGHGIXQFWLRQDOLW\IRUH[DPSOHDIRUPRIHPEHGGHG/LQX[
SOFTWARE UPDATES
A large proportion of ESTCube-1 software was written after the
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orbit software updates and the mission is delayed, increasing a risk
RIVDWHOOLWHIDLOXUHEHIRUHSHUIRUPLQJDOOWKHSODQQHGH[SHULPHQWV
However, we think that functionality of in-orbit software updates
of all active subsystems is critical for a CubeSat mission, especial-
O\IRUWHDPVZLWKRXWSULRUH[SHULHQFH7KDWIXQFWLRQDOLW\FDQPRVW
importantly, save the mission and it also allows using the satellite
IRURWKHUSXUSRVHVWKDQLQLWLDOO\SODQQHG:KHQLPSOHPHQWLQJVXS-
port for software updates, the bootloader must be designed to keep
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IHULQWKHFDVHRI(67&XEHSDJHE\SDJHXSORDGVDQGYHUL¿FD-
tion by pagemaps and checksum have served well.
OTHER
The camera was designed following a principle of using as few
components as possible, which has worked well to provide a small,
simple, modular, and independent camera. However, it should be
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The CDHS is able to log a single command response to a
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UDPHWHUV WR ¿OHV VLPXOWDQHRXVO\ FDQ HDVH WKH SUHSDUDWLRQ DQG
compression of the telemetry.
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reset the MCU) can be used to optimize power consumption of
a system.
A central communication bus is preferred so that subsystems
would be able to communicate with each other without forward-
ing packets through each other.
Developing on-board algorithms in C can save time spent on
SRUWLQJ)RUH[DPSOH$'&6IXQFWLRQVZULWWHQLQ&FDQEHWHVWHG
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directly used in on-board software.
Downlink data rate could be improved further if the COM were
able to buffer several packets in its memory and transmit them in a
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ing a forward error correction coding on the downlink channel.
An obvious but important lesson learned is to document the
code and keep user manuals up to date.
Lessons learned presented in this subsection did not cause any
major problems but can make development and operations more
HI¿FLHQW
TESTING AND MEASUREMENTS
CALIBRATION AND CHARACTERIZATION
All on-board sensors have to be calibrated and characterized to
gain measurement reliability. It should include as many test cases
as possible. Planning of tests has to start early in the project be-
FDXVHVRSKLVWLFDWHGWHVWEHQFKHVPLJKWEHUHTXLUHG)RUH[DPSOH
DWWLWXGHVHQVRUVVKRXOGEHURWDWHGDURXQGDOOD[HVVLPXOWDQHRXVO\
to develop reliable calibration curves.
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LQJWHPSHUDWXUH VHQVRUV LQFORVHSUR[LPLW\WR RWKHU VHQVRUVDQG
performing temperature-calibration for all on-board sensors can
improve the accuracy of other sensor measurements remarkably.
Combining laboratory calibration with in-orbit calibration
might give the best result because not all cases can be tested in a
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)RUH[DPSOHHQGWRHQG$'&6WHVWLQJPLJKWDOZD\VKDYHVRPH
limitations.
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mal vacuum and vibration tests on a subsystem level before the
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perfect case, sensors must be calibrated under conditions that are
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Sun sensor could measure an incidence angle of light while being
placed in a thermal vacuum chamber.
To decrease analog sensor uncertainty, a temperature-com-
pensated reference voltage should be measured on board.
In the case of ESTCube-1, some sensors were well calibrated
before the launch but on multiple occasions in-orbit measure-
ments had to be used to recalibrate them. For attitude determina-
tion sensors, we were lacking test benches that would provide
the needed variety of tests. More temperature and voltage sensors
will be used on board upcoming satellites.
Another important aspect is the timing of measurements. In
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AUGUST 2015 IEEE A
&
E SYSTEMS MAGAZINE 19
Slavinskis et al.
HDVLO\KDSSHQ WKDWFXUUHQWDQG YROWDJHYDOXHVWDNHQ LQVHTXHQFH
actually correspond to different power states, making calculations
based on multiple sensor readings problematic. A solution would
be an independent telemetry system with synchronized input buf-
fers to be certain that all measurements correspond to the same
moment of time. Filtering can also be used to reduce this problem.
INFANT MORTALITY
Infant mortality is an early component failure caused by not test-
LQJVXI¿FLHQWO\ZHDULQJDVHQVRUEHIRUHWKHODXQFK:HKDYHH[-
perienced failure of one of four hot redundant gyroscopic sensors
soon after the launch and one of the two cold redundant MCUs of
WKH&'+6VXIIHUHGGDPDJHWRWKHLQWHUQDOÀDVKMXVWWKUHHPRQWKV
DIWHUWKHODXQFK7ZRRXWRIWKUHH63,EXVÀDVKPHPRU\GHYLFHV
on the ESTCube-1 engineering model stopped working a few
weeks after the integration. Flight and spare components should
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PLWLJDWHWKHULVNDVZHOO:HFRQVLGHUWKLVLVVXHHVSHFLDOO\LPSRU-
tant with COTS components.
MAGNETISM
Having ferromagnetic materials on-board the satellite has caused
WKHELJJHVWFKDOOHQJHLQSUHSDULQJWKHVDWHOOLWHIRUWKHH[SHULPHQW
It took more than half a year to partly characterize the magnetic
properties of the satellite using the engineering model, to fully
characterize the motion of the satellite in orbit, and to iteratively
improve and test attitude controllers. Nevertheless, the spin-up
PDQHXYHUFRXOGQRW EH SHUIRUPHG DV SODQQHGIRUWKH(VDLOH[-
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GHSOR\ZLWKRXWVLJQL¿FDQWGHÀHFWLRQDJDLQVWWKHVDWHOOLWHVLGHVHH
)LJXUH:HVWURQJO\VXJJHVWFKDUDFWHUL]LQJPDJQHWLFSURSHU-
WLHV RI ÀLJKW FRPSRQHQWV DQG WKH PRGHO SULRU WR WKH ODXQFK LQ
WKHFDVH DQDWWLWXGH FRQWURODFWLYHRUSDVVLYHLV UHTXLUHGLQ WKH
magnetosphere of the Earth. Note that this issue affects not only
VDWHOOLWHVWKDWXVHPDJQHWRUTXHUV
OTHER
A practice of early prototyping should be combined with regu-
lar subsystem-level functional tests followed by early integration
tests (starting with electrical/software and later adding mechani-
cal tests) to develop a well-functioning and reliable system.
'HGLFDWHG ERDUGV IRU HDUO\ WHVWV FDQ EH FRQVLGHUHG IRU H[-
ample, to test and perform preliminary characterization of a va-
riety of sensors from which the best ones can be chosen for the
mission.
To make debugging and diagnostics easier, test-ports can be
OHIWRQDÀLJKWPRGHODQGDXQLYHUVDOVHULDOEXV86%FRQQHFWRU
can be used at least until an engineering model is prepared.
The power budget must account for the degradation of solar
cells and batteries.
In the case of ESTCube-1, we incrementally learned lessons,
listed in this subsection, and applied them to our activities on the
go.
ELECTRIC SOLAR WIND SAIL (E-SAIL) PAYLOAD
The ESTCube-1 tether payload consists of a piezoelectric motor
driven reel, 25 ȝm and 50 ȝm wires forming a 15 m long tether,
an end-mass of the tether, a high voltage source to charge the
tether, and a slip ring to connect the high voltage supply to the
WHWKHU5HHOLQJRIWKHWHWKHULVPRQLWRUHGE\WDNLQJLPDJHVRIWKH
HQGPDVV%RWKWKHHQGPDVVDQGWKHUHHODUH¿[HGZLWKGHGLFDWHG
locks that use burn wires [11].
:HFDUULHGRXWWKH WHWKHUGHSOR\PHQW WHVWLQ RUELWDQGLWZDV
not successful. Since the payload design suffers from a lack of
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failed is not known. Some of the future design improvements for
the E-sail payload are sensors to detect whether locks have de-
SOR\HGLIWKHUHHO LVWXUQLQJ DQGLI WKHHQGPDVV LVPRYLQJ%\
having the camera inside the tether enclosure, it will be possible
to monitor the end-mass even before deployment. In the case of
(67&XEHWKHHQGPDVVZRXOGDSSHDULQWKH¿HOGRIYLHZRQO\
after tether deployment of a few centimeters. To improve end-
mass monitoring even further, a light-emitting diode (LED) is
VXJJHVWHGWREHDGGHGQHDUWKHHQGPDVVHQFORVXUHIRUSUR[LPLW\
imaging. Such LED would allow imaging of the most critical pe-
riod of tether deployment without depending on sunlight and/or
DWWLWXGH7KH(67&XEHFDPHUDLVOLPLWHGWRVWRULQJDPD[LPXP
of four images. More memory would allow monitoring deploy-
ment in detail. Nonvolatile memory should be used to avoid los-
LQJH[SHULPHQWGDWDLQWKHFDVHRIDUHVHW
As described in Section II, the reel started to turn during the
TXDOL¿FDWLRQ YLEUDWLRQ WHVW DQG WKH WHWKHU JRW EURNHQ$V D ODWH
design change, a reel lock was introduced. To avoid late design
FKDQJHVVXEV\VWHPVKDYHWREHTXDOL¿HGVHSDUDWHO\EHIRUHLQWH-
gration. In the case of the payload, vibration tests were envisaged
EXWGXHWRDODFNRIUHTXLUHGWHVWVSHFL¿FDWLRQVWKH\FRXOGQRWEH
accomplished.
To couple the tether rotation to the spacecraft spin, the tether
mechanical attachment point should reside as far from the space-
craft center of mass as possible. The tether then resembles a rotat-
ing pendulum (rod attached to a spinning plate) maintaining its
nominal orientation with respect to the spacecraft body. However,
given the dimensions of the tether reel and one-unit CubeSat, this
LVKDUGWRDFFRPSOLVK7KXVWKH(67&XEHWHWKHU ZDVH[SHFWHG
WRRVFLOODWHLQDFRQHRIDERXWGH¿QHGURXJKO\E\WKHGLPHQ-
VLRQV RI WKH HQGPDVV RSHQLQJ +RZHYHU LI WKH WHWKHU GHÀHFWV
more than about 20°, it would touch the conductive side panel.
This would lead to wearing of the tether and even a short circuit.
To avoid these risks, an additional grommet should be placed to
the side panel opening. The grommet must be of antistatic mate-
rial to avoid the triple junction with the plasma, high voltage, and
nonconducting material. For ESTCube-1, tether movement also
decreases the chance to image the end-mass as the end-mass is in
WKH¿HOGRIYLHZRQO\ZKHQWKHWHWKHULVQHDULWVQRPLQDORULHQWD-
tion, normal of the satellite side panel.
Another part of the E-sail payload is the high voltage (HV)
supply system and the electron guns. On the HV supply side, the
PRVWFRQFHSWXDOO\GLI¿FXOWSUREOHPZDVPDQDJLQJZKLFKSDUWVRI
the payload and the satellite are referenced to the HV source and
20 IEEE A
&
E SYSTEMS MAGAZINE AUGUST 2015
ESTCube-1 In-Orbit Experience and Lessons Learned
WRWKHUHTXLUHGHOHFWURQLFV7HVWVSHUIRUPHGLQRUELWVKRZWKDWWKH
HV supply board is operational. Developing the telemetry col-
lection system of the HV board was a challenge due to the fact
WKDWWKHHOHFWULFDOJURXQGOHYHORIWKHV\VWHPÀRDWHGZLWKUHVSHFW
to the satellite ground, since ADCs were referenced to the satel-
lite ground. In the future, we suggest putting telemetry collection
HOHFWURQLFVFRPSOHWHO\LQWKHÀRDWLQJJURXQGVLGHDQGRQO\XVLQJ
digital communication lines to interface them. This should also
make the calibration of the system easier.
In the case of the electron guns, reliability remains the major
concern. In our tests, one gun did not work at all (open circuit)
and the other short circuited during tests (although it was con-
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the reliability would have been to test the whole HV and electron
gun system together in the laboratory before the launch. In the
time frame of ESTCube-1, this was not possible; also it would
KDYHUHTXLUHGDUDWKHUFRPSOH[YDFXXPFKDPEHUVHWXS$QRWKHU
possible cause for problems was the fact that the electron guns
were not covered during deployment and their surface might have
gotten contaminated before their use (even a small particle could
short circuit the system). This could be mitigated by using protec-
tive covers that would be removed in orbit or by increasing the
distance between the cathode and the anode.
MANAGEMENT
TEAM LEADING
Having a visionary leading the team is key to successfully car-
rying out a technically challenging and long project, especially
a project where team members must be regularly motivated by
RWKHUWKDQ¿QDQFLDOPHDQV7HDPPHPEHUVPXVWNQRZDQGDFFHSW
that an ultimate measure of success might come after years of
development, after launching, and after successfully operating a
satellite. However, it is up to leaders and the management team to
GH¿QHIUHTXHQWPLOHVWRQHV
ADVISORY
Another key to success is having professional advisers to su-
pervise and to review student work. In the case of ESTCube-1,
SURIHVVLRQDODGYLFH ZDVUHFHLYHG LQWKH¿HOGV RIHOHFWULFDO HQJL-
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and measurement sciences. Advisers from the amateur radio com-
munity helped to avoid many problems with practical commu-
nication and ground station set-up. Similarly, a system engineer
should be a professional with a wide knowledge of involved en-
JLQHHULQJ¿HOGV
MANAGEMENT
Management of the ESTCube-1 project has been successful in
FDUU\LQJRXWVRPHRILWVIXQFWLRQV)RUH[DPSOHWKHWHDPKDVDF-
cess to various tools and services like the team collaboration soft-
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versioning and revision control system SVN, Google services
(Mail, Documents, Hangouts, Calendar), the chat and video con-
ference system HipChat, a remote desktop computer with access
WR VSHFLDOL]HG VRIWZDUH 0$7/$% 6LPXOLQN 6ROLG:RUNV WKH
3&%VRIWZDUH($*/(HWF+RZHYHUZHKDYHLGHQWL¿HGWKDWWKH
management team cannot consist of people whose main duties are
other than management of the ESTCube-1 project. At least one
person should respond to issues on a daily basis, especially during
critical moments such as integration, testing, prelaunch servicing,
and launch. Special attention should be paid to procurement han-
dling. For management to be responsive, it should be supported
¿QDQFLDOO\
The team should acknowledge the possibility of failures and
EHSUHSDUHGIRUWKHP0DQDJHPHQWFDQSOD\DVLJQL¿FDQWUROHLQ
leading the team to this understanding. Management must take
into account that students can contribute only a limited amount of
time to the project and that they can leave at any time.
In case the project schedule is accelerated, it should be agreed
XSRQZLWKH[WHUQDOSDUWQHUVDQGVXEFRQWUDFWRUV7KHPDQDJHPHQW
team has to follow the development progress on a weekly basis
in order to successfully schedule milestones and ultimately the
launch.
:HWKLQNWKDWFKRRVLQJDFKDOOHQJLQJVFLHQWL¿FPLVVLRQLVEHW-
ter than a simple one (e.g., optical camera being the main pay-
load) in an educational project. In that case, the project outcomes
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motivation. In the ESTCube team, some members have decided
to continue their professional careers with the E-sail.
TEAM
A student team should be motivated and open. Students and the
team will gain the most if members are able to work on various
subsystems and different types of tasks, including leading, man-
agement, article writing, and outreach. Such approach will also
help to avoid alienation between subsystem teams and teams in
different geographical locations.
From the early stages, subsystem teams should discuss re-
TXLUHPHQWVDVZHOODVGHVLJQFKRLFHVDQGPRVWLPSRUWDQWO\LQWHU-
IDFHVIRUH[DPSOHWRQRWFDXVHGLVFUHSDQF\EHWZHHQWUDQVPLWWLQJ
and receiving interfaces.
The team should have a clear understanding of the importance
of the work and the priorities of its subtasks. Everybody in the
WHDPVKRXOGXQGHUVWDQGDQGVKRXOGEHDEOHWRH[SODLQWKHPLVVLRQ
DQGLWVUHTXLUHPHQWV)LJXUH
2SHQLQJDOOTXHVWLRQVIRUDGLVFXVVLRQFDQOHDGWREHWWHUGHFL-
sions, can contribute to team building and can serve as an infor-
mative media for updating on current progress and future plans.
)RU H[DPSOH DOO PHPEHUV VKRXOG EH LQYROYHG LQ FKRRVLQJ WKH
launch provider and in satellite operations.
3HUVRQDO FRQÀLFWV VKRXOG EH VROYHG ZLWKRXW KHVLWDWLRQ DQG
with the help of peers and leaders.
CONCLUSIONS
In this article, we presented an overview of the ESTCube-1 in-
RUELWH[SHULHQFH DQGGLVFXVVWKH OHVVRQVOHDUQHG$IWHUXSGDWLQJ
AUGUST 2015 IEEE A
&
E SYSTEMS MAGAZINE 21
Slavinskis et al.
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for four problems.
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However, the amount of the produced power was enough to pro-
ceed with the mission. In the future, the problem can be solved by
using solar panel cover glass.
Second, a need to recalibrate attitude determination sensors
in orbit. After recalibrating the sensors, debugging software, and
¿QHWXQLQJ WKH .DOPDQ ¿OWHUWKH DWWLWXGH GHWHUPLQDWLRQ V\VWHP
ZDV SUHSDUHG IRU DWWLWXGH FRQWURO PDQHXYHUV DQG WKH (VDLO H[-
periment. In the future, all sensors have to be calibrated before
the launch better than was done on ESTCube-1, as well as full
integration of the system has to be tested on the ground. However,
in-orbit calibration methods can serve as a backup or can be used
WR¿QHWXQHFRUUHFWLRQSDUDPHWHUV
Third, ferromagnetic materials used on-board aligning the
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possible to prepare the satellite for tether deployment. In the fu-
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ization of on-board materials.
Fourth, the inability to deploy the tether made it impossible
WRPHDVXUHWKH(VDLOIRUFH:KLOHIRU(67&XEHLWZDVQRWSRV-
VLEOHWRH[DFWO\GHWHUPLQHZKDWFDXVHGWKHSUREOHPZHZHUHDEOH
to identify design improvements, some of which have already
been implemented on the Aalto-1 satellite [34]. The tether de-
ployment system has to be thoroughly tested and it has to have
means to detect which part is not working (e.g., locks, the reel, or
the tether is broken).
In addition to learning from the four major problems, we have
GLVFXVVHGRWKHUOHVVRQVOHDUQHGLQWKH¿HOGVRIV\VWHPHQJLQHHU-
ing, electrical engineering, mechanical engineering, software
engineering, testing and measurements, as well as management.
Since the satellite delivery schedule was accelerated, the mis-
sion encountered delays. After launching the satellite, only pre-
liminary validation was feasible. New software updates allowed
to fully validate the on-board systems, provide full functionality,
and optimize power consumption.
Lessons learned, discussed in this article, have already been,
DQGFRQWLQXHWR EH DSSOLHG WR VXEVHTXHQW PLVVLRQVLQWKH(67-
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lite size, the target audience for this article is the nanosatellite
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consider standards like the ECSS highly useful. However, they
are not fully compatible with agile development methods that
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:HWKLQNWKDWIRU,2'PLVVLRQVWKDWQDQRVDWHOOLWHVDUHRIWHQXVHG
IRUWKHVWDQGDUGVFDQ EHPDGHORRVHUWRNHHSWKHFRVWHI¿FLHQF\
and short development time.
For teams that are developing satellite series for IODs and
IRUHGXFDWLRQDOSURSRVHVZHHQFRXUDJHXVLQJWKHSKLORVRSK\³À\
HDUO\À\RIWHQ´6XFKSKLORVRSK\HQDEOHVUDSLGWHFKQRORJ\GH-
YHORSPHQWIROORZHGE\LQRUELWWHVWV:KLOHLW LQFUHDVHVWKHULVN
the team can learn from mistakes and unsuccessful missions to
TXLFNO\GHYHORSVHTXHQWLDOVDWHOOLWHV6RPHRIWKHOHVVRQVFDQEH
learned only by launching and operating satellites. Fly early &
À\RIWHQHPSOR\VWKHFRVWHI¿FLHQF\RIQDQRVDWHOOLWHVDQG&276
components. Moreover, launching a satellite soon after freezing
the design allows utilization of the latest developments in the
COTS market.
ACKNOWLEDGMENTS
The authors would like to thank everybody who has contributed
to the development of ESTCube-1. The European Space Agency
and the Ministry of Economic Affairs and Communication of
Estonia have supported ESTCube-1 via the ESA PECS project
“Technology demonstration for space debris mitigation and elec-
WULFSURSXOVLRQ RQ (67&XEH VWXGHQWVDWHOOLWH´:HZRXOG OLNH
to thank all institutions that contributed to ESTCube-1 develop-
ment. The research by Andris Slavinskis was supported by the
European Social Fund’s Doctoral Studies and the International-
L]DWLRQ3URJUDP'R5D7KHUHVHDUFKRQVRIWZDUHHQJLQHHULQJZDV
VXSSRUWHGE\WKH(XURSHDQ5HJLRQDO'HYHORSPHQW)XQGDQGWKH
Investment and Development Agency of Latvia via the Latvian
(OHFWURQLFDQG2SWLFDO(TXLSPHQW&RPSHWHQFH&HQWUHLQ3URGXF-
tion Sector (agreement no. L-KC-11-0006) project number 2.9
³5HFHLYLQJYDOLGDWLRQDQGERRWORDGLQJV\VWHPRIVPDOOVDWHOOLWH
software as an enabler for safe and reliable satellite development
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[21] 1LHOVHQ-'DQG/DUVHQ-$([SHULHQFHVDQGOHVVRQVOHDUQHGGXU-
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LQJWKH SODVPDEUDNH H[SHULPHQWRQERDUG WKH$DOWRVDWHOOLWHPro-
ceedings of the Estonian Academy of Sciences, Vol. 63(2S) (2014),
±
A. Slavinskis, H. Kuuste, T. Eenmäe, I. Sünter, K. Laizans, E.
Kulu, U. Kvell, J. Kütt, K. Zalite, S. Lätt, R. Vendt, V. Allik and
M. Noorma are with Tartu Observatory, Department of Space
Technology, Observatooriumi 1, 61602, Tõravere, Estonia, e-
mail: andris.slavinskis@estcube.eu). A. Slavinskis, M. Pajusalu,
H. Kuuste, E. Ilbis, T. Eenmäe, K. Zalite, H. Ehrpais, J. Viru, J.
Kalde, U. Kvell, K. Kahn, S. Lätt, P. Janhunen and M. Noorma
are with the University of Tartu, Institute of Physics, Ravila
14C, 50411, Tartu, Estonia. A. Slavinskis, J. Envall, P. Toivanen,
J. Polkko and P. Janhunen are with the Finnish Meteorologi-
cal Institute, Erik Palménin aukio 1, P.O. Box 503, FI-00101,
Helsinki, Finland. A. Slavinskis, I. Sünter, U. Kvell, J. Kütt, and
R. Vendt are also with SIA Robotiem, Paula Lejin¸ a iela 5-70,
LV-1029, Rı¯ga, Latvia. P. Liias is with Tallinn University of Tech-
nology, Ehitajate tee 5, 19086, Tallinn, Estonia. K. Zalite is with
Engineering Research Institute Ventspils International Radio
Astronomy Centre of Ventspils University College, Inženieru
101a, LV-3601, Ventspils, Latvia. R. Rosta is with the German
Aerospace Center (DLR), Robert Hooke 7, 28359, Bremen, Ger-
many. T. Kalvas is with the University of Jyväskylä, Department
of Physics, P.O. Box 35 (YFL), FI-40014, Jyväskylä, Finland.
... To be demonstrated onboard the ESTCube-2 [7], the ionospheric plasma brake has the potential to be the safest propellantless LEO deorbiting solution. The ESTCube-1 and Aalto-1 satellites have attempted to demonstrate the ionospheric plasma brake in LEO, but the first-generation ionospheric plasma brake required several improvements [8,9] which have been implemented onboard the ESTCube-2 and Foresail-1 [10]. ...
... The ESTCube-2 mission is an integral part of the Estonian Student Satellite Program-ESTCube-2 builds upon the ESTCube-1 lessons learned [8]. The ESTCube-2 will test technologies necessary to bring CubeSats and nanospacecraft into deep interplanetary space [18][19][20]. ...
... The team operated the satellite to (a) take images of the Earth, including Estonia, which was the secondary mission objective, (b) spin the satellite to 2.5 revolutions per second [24], which was required for tether deployment [25,26], (c) take images for attitude determination characterization [27], and d) make tens of firmware updates [28]. However, the ESTCube-1 tether deployment was not successful [8]. A similar tether payload was carried on board Aalto-1, which also did not deploy [9,29]. ...
Article
Full-text available
Nanosatellites have established their importance in low-Earth orbit (LEO), and it is common for student teams to build them for educational and technology demonstration purposes. The next challenge is the technology maturity for deep-space missions. The LEO serves as a relevant environment for maturing the spacecraft design. Here we present the ESTCube-2 mission, which will be launched onboard VEGA-C VV23. The satellite was developed as a technology demonstrator for the future deep-space mission by the Estonian Student Satellite Program. The ultimate vision of the program is to use the electric solar wind sail (E-sail) technology in an interplanetary environment to traverse the solar system using lightweight propulsion means. Additional experiments were added to demonstrate all necessary technologies to use the E-sail payload onboard ESTCube-3, the next nanospacecraft targeting the lunar orbit. The E-sail demonstration requires a high-angular velocity spin-up to deploy a tether, resulting in a need for a custom satellite bus. In addition, the satellite includes deep-space prototypes: deployable structures; compact avionics stack electronics (including side panels); star tracker; reaction wheels; and cold–gas propulsion. During the development, two additional payloads were added to the design of ESTCube-2, one for Earth observation of the Normalized Difference Vegetation Index and the other for corrosion testing in the space of thin-film materials. The ESTCube-2 satellite has been finished and tested in time for delivery to the launcher. Eventually, the project proved highly complex, making the team lower its ambitions and optimize the development of electronics, software, and mechanical structure. The ESTCube-2 team dealt with budgetary constraints, student management problems during a pandemic, and issues in the documentation approach. Beyond management techniques, the project required leadership that kept the team aware of the big picture and willing to finish a complex satellite platform. The paper discusses the ESTCube-2 design and its development, highlights the team’s main technical, management, and leadership issues, and presents suggestions for nanosatellite and nanospacecraft developers.
... In addition, some space missions have been approved to demonstrate the feasibility of this advanced concept in a geocentric mission scenario. In particular, the Estonian 1U CubeSat ESTCube-1 [38][39][40][41], designed by the University of Tartu with the support of ESA and launched on 7 May 2013 aboard a Vega rocket, was the first ever satellite to attempt on-orbit deployment of an E-sail-charged tether. In fact ESTCube-1, with a mass of about 1 kg, was designed to deploy by centrifugal force a 10 m Heytether [37], positively charged to 500 volts with its bias maintained by two electron emitters [42]. ...
... Unfortunately, the tether deployment failed, possibly due to a stuck reel, and the mission ended on 17 February 2015. Subsequent ground tests showed that the piezoelectric motor was damaged by launch phase vibrations [43], which meant that the failure was not due to an intrinsic flaw in the charged tether-related technology, and that the problem could have been solved with suitable spacecraft design improvements [39]. ...
Article
Full-text available
The plasma brake is a propellantless device conceived for de-orbiting purposes. It consists of an electrically charged thin tether that generates a Coulomb drag by interacting with the ionosphere. In essence, a plasma brake may be used to decelerate an out-of-service satellite and to ensure its atmospheric re-entry within the time limits established by the Inter-Agency Space Debris Coordination Committee. Moreover, since it only needs a small amount of electric power to work properly, the plasma brake is one of the most cost-effective systems for space debris mitigation. This paper exploits a recent plasma brake acceleration model to construct an iterative algorithm for the rapid evaluation of the decay time of a plasma-braked CubeSat, which initially traced a circular low Earth orbit. The altitude loss at the end of each iterative step was calculated using the linearized Hill–Clohessy–Wiltshire equations. It showed that the proposed algorithm, which was validated by comparing the approximate solution with the results from numerically integrating the nonlinear equations of motion, reduced computational time by up to four orders of magnitude with negligible errors in CubeSat position.
... Both missions carried E-sail payloads with piezoelectric motors and tethers, which were ultrasonically bonded [14]. While neither ESTCube-1 [15] nor Aalto-1 [16] managed to deploy an E-sail successfully, both teams learned to develop and prepare for operations of plasma brake and E-sail experiments [17][18][19][20]. ...
Article
Full-text available
The electric solar wind sail, or E-sail, is a novel deep space propulsion concept which has not been demonstrated in space yet. While the solar wind is the authentic operational environment of the electric sail, its fundamentals can be demonstrated in the ionosphere where the E-sail can be used as a plasma brake for deorbiting. Two missions to be launched in 2023, Foresail-1p and ESTCube-2, will attempt to demonstrate Coulomb drag propulsion (an umbrella term for the E-sail and plasma brake) in low Earth orbit. This paper presents the next step of bringing the E-sail to deep space—we provide the initial modelling and trajectory analysis of demonstrating the E-sail in solar wind. The preliminary analysis assumes a six-unit cubesat being inserted in the lunar orbit where it deploys several hundred meters of the E-sail tether and charges the tether at 10–20 kV. The spacecraft will experience acceleration due to the solar wind particles being deflected by the electrostatic sheath around the charged tether. The paper includes two new concepts: the software architecture of a new mission design tool, the Electric Sail Mission Expeditor (ESME), and the initial E-sail experiment design for the lunar orbit. Our solar-wind simulation places the Electric Sail Test Cube (ESTCube) lunar cubesat with the E-sail tether in average solar wind conditions and we estimate a force of 1.51e−4 N produced by the Coulomb drag on a 2 km tether charged to 20 kV. Our trajectory analysis takes the 15 kg cubesat from the lunar back to the Earth orbit in under three years assuming a 2 km long tether and 20 kV. The results of this paper are used to set scientific requirements for the conceptional ESTCube lunar nanospacecraft mission design to be published subsequently in the Special Issue “Advances in CubeSat Sails and Tethers”.
... Yet, there are a couple of noteworthy differences between them that merit mention. First, prototypes of electric sails have been demonstrated in the past decade: the nanosatellites ESTCube-1 [204] and Aalto-1. 13 In contrast, no such prototypes of magnetic sails appear to exist, reducing its TRL accordingly. ...
Article
Full-text available
Nomadic worlds, i.e., objects not gravitationally bound to any star(s), are of great interest to planetary science and astrobiology. They have garnered attention recently due to constraints derived from microlensing surveys and the recent discovery of interstellar planetesimals. In this paper, we roughly estimate the prevalence of nomadic worlds with radii of 100 km ≲ ≲ 10 4 km. The cumulative number density > (>) appears to follow a heuristic power law given by > ∝ −3. Therefore, smaller objects are probably much more numerous than larger rocky nomadic planets, and statistically more likely to have members relatively close to the inner Solar system. Our results suggest that tens to hundreds of planet-sized nomadic worlds might populate the spherical volume centered on Earth and circumscribed by Proxima Centauri, and may thus comprise closer interstellar targets than any planets bound to stars. For the first time, we systematically analyze the feasibility of exploring these unbounded objects via deep space missions. We investigate what near-future propulsion systems could allow us to reach nomadic worlds of radius > in a 50-year flight timescale. Objects with ∼ 100 km are within the purview of multiple propulsion methods such as electric sails, laser electric propulsion, and solar sails. In contrast, nomadic worlds with ≳ 1000 km are accessible by laser sails (and perhaps nuclear fusion), thereby underscoring their vast potential for deep space exploration.
... A sketch of the basic structure of an Esail is shown in Fig. 1 A first validation test of the E-sail working principle was attempted with the Estonian satellite EstCube-1 (Lätt et al., 2014), whose aim was to test the plasma brake concept (Janhunen, 2010), a derivation of the E-sail working principle useful for spacecraft deorbiting from LEO (Bassetto et al., 2018;Niccolai et al., 2017b;Orsini et al., 2018). Unfortunately, the tether unreel mechanism failed, probably due to vibrational loads during the launch phase (Slavinskis et al., 2015). The first experimental in-situ data on the E-sail principle should therefore be provided by the Finnish satellite Aalto-1 (Kestilä et al., 2013), which was launched in June 2018 and is equipped with a 100 m-long plasma brake tether to perform an end-of-life deorbiting 1. Displaced non-Keplerian orbits for Sun and. . . ...
Chapter
A displaced non-Keplerian orbit is a trajectory whose orbital plane does not contain the center of mass of the primary body, so that its orbital maintenance requires the application of a suitable continuous thrust. Although the latter could be provided, in principle, by a low-thrust electric propulsion system, innovative propellantless propulsive technologies are well suited to such a mission scenario, due to their ability to generate thrust without requiring any propellant, thus significantly extending mission lifetime. This chapter focuses on the possibility of maintaining a displaced non-Keplerian orbit by means of both solar sails and electric solar wind sails (or E-sails). In fact, these advanced propulsion systems are both capable of generating a propulsive acceleration without consuming any propellant, by exploiting the solar radiation pressure (in case of solar sails) or the solar wind dynamic pressure (E-sails). This analysis uses recent models to provide a mathematical description of the propulsive acceleration generated by both propulsion systems, and different scenarios involving non-Keplerian orbits are analyzed. Particular focus is given to Type II displaced orbits, non-Keplerian orbits lying on the ecliptic plane, and heliostationary positions. Performance and attitude requirements are provided for each scenario. A linear stability analysis is also performed, in order to identify the combination of orbital parameters that characterize stable non-Keplerian orbits. The results suggest the feasibility of the mission scenarios discussed, but for most of them performance requirements are very demanding. A possible exception is non-Keplerian orbits lying on the ecliptic, which represent a very promising near-term scenario.
... The first test mission of the PB technology was planned to be the Estonian satellite EstCube-1 [23], but a failure occurred in the conducting tether unreel mechanism [24]. More recently, a similar problem in the unreeling motor caused the failure of a PB test [25] in the Finnish 3U-CubeSat Aalto-1 [26,27]. ...
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The presence of a number of space debris in low Earth orbits poses a serious threat for current spacecraft operations and future space missions. To mitigate this critical problem, international guidelines suggest that an artificial satellite should decay (or be transferred to a graveyard orbit) within a time interval of 25 years after the end of its operative life. To that end, in recent years deorbiting technologies are acquiring an increasing importance both in terms of academic research and industrial efforts. In this context, the plasma brake concept may represent a promising and fascinating innovation. The plasma brake is a propellantless device, whose working principle consists of generating an electrostatic Coulomb drag between the planet’s ionosphere ions and a charged tether deployed from a satellite in a low Earth orbit. This paper discusses an analytical method to approximate the deorbiting trajectory of a small satellite equipped with a plasma brake device. In particular, the proposed approach allows the deorbiting time to be estimated through an analytical equation as a function of the design characteristics of the plasma brake and of the satellite initial orbital elements.
... As access to space is becoming more affordable, the number of standardized CubeSats [4] being launched into orbit is increasing [5] (as of 2020). Most of these satellites are University of Tartu, Tartu Observatory, Observatooriumi 1, Tõravere, Estonia, 61602 either built by universities (e.g., AAUSAT3 [6], ALLSTAR-1 [7], ESTCube-1 [8]) or new emerging companies, such as Planet, that operate a fleet of remote sensing satellites for hightemporal imagery of Earth [9]. Moreover, numerous CubeSats have been launched with Earth Observation capabilities [10]. ...
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This paper describes the optical design and analysis of Theia: a miniature, scientific-grade, multispectral Earth observation imager for nanosatellites that can be used for quantitative remote sensing. The instrument is designed to take images with a 5 radiometric accuracy throughout its three-year lifetime. The sustained accuracy is achieved with a post-launch calibration module. The instrument can capture frames at a 33 m ground sampling distance at an orbit height of 650 km. The design can take diffractionlimited images with a modulation transfer function of at least 0.13 at the sensor’s Nyquist frequency, which is comparable with Sentinel-2’s MultiSpectral Instrument. The instrument works in two user-defined bands, fits inside one CubeSat unit and weighs 600 g. The successful analysis of the system is presented, including optical performance, radiometric, stray-light, and tolerance analyses.
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This paper presents a novel low-power imaging system for nanosatellite proximity operations. A robust independent camera module with on-board image processing, based on the ARM Cortex-M3 microcontroller and fast static random access memory, has been developed and characterized for the requirements of the ESTCube-1 mission. The imaging system, optimized for use in a single unit Cube Sat, utilizes commercial off-the-shelf components and standard interfaces for a cost-effective reusable design. The resulting 43.3 mm x 22 mm x 44.2 mm (W x H x D) aluminium camera module weighs 30 g and consumes on the average of 118 mW of power, with peaks of 280 mW during image capture. Space qualification and stress tests have been performed. A detailed case study for the ESTCube-1 10 m tether deployment monitoring and Earth imaging mission is presented. For this purpose a 4.4 mm telecentric lens, 10 bit 640 x 480 pixel CMOS image sensor, 700 nm infrared cut-off filter and a 25% neutral density filter are used. The resolution of the assembled system is 12.7 mm and 1 km per pixel at distances of 10 m and 700 km, respectively. Custom on-board image evaluation and high dynamic range imaging algorithms for ESTCube-1 have been implemented and tested. Optical calibration of the assembled system has been performed.
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The nanographite (NG) films consisting of tiny graphite crystallites (nanowalls) are produced by carbon condensation from methane–hydrogen gas mixture activated by a direct current discharge. High aspect ratio and structural features of the NG crystallites provides efficient field electron emission (FE). Applicability and performance of the NG films in an electron gun (E-gun) of a solar wind thruster system with an electric sail (E-sail) is tested. The long-term tests are demonstrated suitability of E-gun assembly with the NG cathodes for the real space missions. The results of the tests are analyzed and physical mechanisms of the cathode aging and practical methods for improvement performance of the E-gun are proposed.
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The second Radio Aurora Explorer satellite, RAX-2, is a triple CubeSat studying the formation of plasma irregularities in Earth's ionosphere. The spacecraft was developed jointly by SRI International and the University of Michigan, and it is the first satellite funded by the National Science Foundation. RAX-2 launched October 28, 2011 and is currently operating on orbit. RAX uses a bistatic radar configuration to study the ionospheric irregularities: a ground-based incoherent scatter radar station illuminates the irregularities, and the RAX-based radar receiver measures radar scatter from the irregularities. RAX has successfully measured radar scatter from the ionospheric irregularities, providing unprecedented auroral region measurements. In this paper, we review the mission goals and satellite development, and discuss initial flight results from the mission. This includes a summary of results from the first detection of radar scatter, power system performance, spacecraft attitude dynamics, global UHF noise measurements, and data download strategies and results of partnering with the amateur radio community.
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This paper presents an overview and the current status of hosting the electrostatic plasma brake (EPB) experiment on-board the Finnish Aalto-1 satellite. The goal of the experiment is to demonstrate the use of an electrostatically charged tether for satellite attitude and orbital maneuvers. The plasma brake device is based on electrostatic solar sail concept, invented in Finnish Meteorological Institute (FMI). The electrostatic solar sail is designed to utilize the solar wind charged particles to propel the spacecraft by using long conductive tethers, surrounded by electrostatic field. Similar phenomenon can be used in low Earth orbit plasma environment, where the relative motion between the electrostatically charged tether and the ionospheric plasma can produce a significant amount of drag. This drag can be utilized for deorbiting the satellite. The Aalto-1, a multi-payload CubeSat, will carry, among others, the plasma brake payload. Plasma brake payload consists of a 100 m long conductive tether, a reel mechanism for tether storage, a high voltage source, and electron guns to maintain the tether charge. The experiment will be performed in positive and negative tether charge modes and includes a long term passive deorbiting mode. The experiment hardware, the satellite mission and different phases of the experiment are presented.