Conference Paper

COSMOS — An innovative nodal architecture for controlling large numbers of small satellites and other diverse assets

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Abstract

The Hawaii Space Flight Laboratory (HSFL) at the University of Hawaii at Manoa developed the Comprehensive Open-architecture Solution for Mission Operations Systems (COSMOS) under a three-year NASA grant. This innovative suite of software and hardware was initially designed for supporting the operations of multiple small satellites, but during its development, it evolved into a comprehensive system of systems that is capable of providing nearly all operations functions to support an integrated system of objects to be monitored and controlled, called nodes. These nodes are not limited to spacecraft, but can be almost any type of vehicle or electronic entity that has communication connectivity with the distributed COSMOS system. Even the vehicles themselves can operate COSMOS as their onboard controlling software. HSFL built a 55-kg satellite called Hiakasat that is due to launch on the ORS-4 mission in 2015. This satellite uses COSMOS for its onboard flight software, which integrates seamlessly with the COSMOS system that is being used to operate the mission on the ground. COSMOS is currently being used to monitor research ship gathering data, and even controlling rovers on simulated lunar missions. This innovative nodal architecture will allow a fully integrated system that can combine satellites with UAVs, submersible, ships, and other robotic craft.

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The Hawaii Space Flight Laboratory (HSFL) at the University of Hawaii at Manoa under a NASA grant is developing a comprehensive open-architecture space mission operations system (COSMOS) designed particularly to provide operations support for multiple small spacecraft. HSFL was recently on a Canadian-led team to perform a conceptual study for the Canadian Space Agency on the feasibility of doing a micro-rover (30 kg) mission to the Moon for no more than $100 million (Canadian). This mission was called the Canadian American British Lunar Explorer (CABLE) mission. As part of the CABLE mission plan, the Inter-Stage Adapter that is used to provide support for the lander during launch and also propellant for following propulsive burns, after separation becomes a cis-lunar spacecraft called ISAS to provide measurements of the environment in cis-lunar space. This paper examines the adaption of the COSMOS system to provide operations support for the CABLE mission. It was determined during the study that not only is COSMOS suitable for supporting operations for the lander spacecraft and ISAS, it could also provide operations support for the lunar rover. For monitor and control of the two spacecraft and rover we are using the Mission Operations Support Tool (MOST) of COSMOS, This tool, which is based on the LUNOPS tool developed for the Clementine lunar mission in 1994, also provides monitoring of the mission trajectories, including the descent and landing on the Moon. Working prototypes of MOST to demonstrate these capabilities were completed for the CSA study. To further demonstrate the suitability of COSMOS and MOST to support lunar operations, MOST was used in a student project at the University of Hawaii at Manoa to provide operations for a simulated Mars lander and rover mission. It is planned to use a version of the CABLE MOST software to assist the second field deployment of the CSA Mars Methane Mission (MMM) in a terrestrial analogue environment. This will employ the Kapvik micro-rover to conduct field-investigations simulating a remote Mars mission in serpentinite geology relevant to Mars to verify the methodologies and instrumentation for the in-situ search for methane sources and relevant microbial bio signatures related to methanogens.
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The Hawaii Space Flight Laboratory (HSFL) at the University of Hawaii at Manoa is developing the capabilities to design, build, and operate constellations of small satellites than can be tailored to efficiently execute a variety of remote sensing missions. With the Operationally Responsive Space (ORS) Office, HSFL is developing the Super Strypi launch vehicle that on its initial mission in 2013 will launch the HSFL 55-kg HawaiiSat-1 into a near polar orbit, providing the first deployment of these technologies. This satellite will be carrying a miniature hyperspectral thermal imager developed by the Hawaii Institute of Geophysics and Planetology (HIGP). HSFL has also developed a method to efficiently deploy a constellation of small satellites using a minimal number of launch vehicles. Under a three-year NASA grant, HSFL is developing a Comprehensive Open-architecture Space Mission Operations System (COSMOS) to support these types of missions. COSMOS is being designed as a System of Systems (SoS) software integrator, tying together existing elements from different technological domains. This system should be easily adaptable to new architectures and easily scalable. It will be provided as Open Source to qualified users, so will be adoptable by even universities with very restricted budgets. In this paper we present the use of COSMOS as a System of Systems integrator for satellite constellations of up to 100 satellites and numerous ground stations and/or contact nodes, including a fully automated “lights out” satellite contact capability.
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