This article's factual accuracy may be compromised due to out-of-date information.(April 2016) |
The Canadian Advanced Nanospace eXperiment (CanX) program is a Canadian CubeSat nanosatellite program operated by the University of Toronto Institute for Aerospace Studies, Space Flight Laboratory (UTIAS/SFL). The program's objectives are to involve graduate students in the process of spaceflight development, and to provide low-cost access to space for scientific research and the testing of nanoscale devices. The CanX projects include CanX-1, CanX-2, the BRIght Target Explorer (BRITE), and CanX-4&5. [1]
The Canadian Advanced Nanospace eXperiment (CanX) program is the first Canadian nanosatellite program, and the only one of its kind at present. It is operated by teachers and graduate students at the University of Toronto Institute for Aerospace Studies, Space Flight Laboratory (UTIAS/SFL). The program was established in 2001 by Dr. Robert E. Zee, manager of UTIAS/SFL, and is based on the CubeSat program started by Stanford University and California Polytechnic State University. Its projects include CanX-1, CanX-2, CanX-3 (BRITE), and CanX-4&5.
The program's objectives are to involve graduate students in the process of spacecraft development, and to provide relatively low cost access to space for scientific research and the testing of nanoscale devices in orbital space. In March 2009 CanX-2 completed its first year in orbit. [2]
The Canadian Advanced Nanospace eXperiment 1 (CanX-1, COSPAR 2003-031H) is Canada's first nanosatellite and a one unit CubeSat. ; it has a mass of under 1 kg, fits in a 10 cm cube, and operates on less than 2 watts.
CanX-1 was completed in 22 months and was launched, along with the Microvariability and Oscillations of STars telescope, on June 30, 2003 at 14:15 UTC by Eurockot Launch Services from Plesetsk, Russia. It lost contact with Earth after launch.
The operation modes of CanX-1 are:
In each mode, the OBC is always collecting telemetry data from the temperature, voltage, and current sensors present on every solar panel and interior circuit board.2
In Safe-Hold mode, the OBC maintains minimum power and the radio is in receive mode. If there is sufficient power available, the radio will transmit a beacon pulse just under once per minute. All payloads, magnetorquers and the magnetometer are switched off. CanX-1 switches into safe-hold mode in any emergency situation, and it stays in this mode until instructed to resume normal operations after any required fixes are implemented. It can also be placed in safe-hold mode by the ground operator whenever it is not performing any missions or experiment for a long period of time.
CanX-1 only switches into the detumbling/torquing mode when it is instructed to do so. It is for reducing the tumbling rate of the nanosatellite so that any images taken are not blurred as a result of CanX-1's motion. This mode can also be used to increase the tumbling rate of CanX-1 so that images can be taken in multiple directions without long delays. It uses maximum power when all three magnetorquers and the magnetometer are on simultaneously, and all payloads are switched off because sufficient power may not be available.
Payload Active is the normal operation mode of CanX-1. The picosatellite switches to this mode whenever it is instructed to do so. While in payload active mode all payloads are switched on, and CanX-1 transmits a beacon pulse every minute until it is instructed to send all collected telemetry and images to the ground operators.
The CanX-1 mission was intended to demonstrate a highly capable spacecraft, and it incorporates a number of payloads and experimental subsystems.1 These include:
The imager payload aboard CanX-1 consists of two Agilent CMOS imagers. The color imager in conjunction with a wide-angle lens was intended primarily for taking photographs of Earth, and the monochrome imager in conjunction with a narrow-angle lens was for testing the feasibility of taking star, moon, and horizon pictures which could then be used for attitude determination and control.
CanX-1 had a COTS magnetometer along with three custom-built magnetorquer coil systems as part of the active magnetic attitude control system (ACS). The magnetic ACS is for detumbling the satellite to assure that any images taken by CanX-1 are not blurred due to the rotation of the picosatellite. Also, CanX-1 was scheduled to perform active coarse pointing.
A commercial-off-the-shelf (COTS) GPS receiver was also aboard CanX-1. Connected to two antennas for omni-directional coverage, the picosatellite was meant to test the functionality of the GPS receiver in space in order to determine whether the receiver could be used to help determine the orbital position of CanX-1.
CanX-1 was launched with a custom designed On-Board Computer (OBC) based on the low-power ARM7 core, which operates on up to 40 MHz. The functionality of this OBC was to be monitored throughout the entire lifetime of CanX-1.
The mission of the CanX-2 nanosatellite, weighing 3.5 kilograms, is to evaluate new technologies that will be used on the CanX-4/CanX-5 dual satellite mission in 2009 to demonstrate controlled formation flying in space. It is hoped that this formation flying technology will allow larger missions for high resolution Earth observation and interferometric imaging that can also be used for space astronomy. The technologies to be tested on the CanX-2 nanosatellite included:
In addition to evaluating these technologies, the satellite will also perform experiments for other university researchers across Canada. These experiments include a GPS radio occultation experiment to characterize the upper atmosphere, an atmospheric spectrometer to measure greenhouse gases (Argus) developed by York University, and a network communications experiment. It will also carry out several space materials experiments.
CanX-2 was launched on 28 April 2008 from the Satish Dhawan Space Centre (SHAR) as part of the NLS-4 group of satellites, aboard the Polar Satellite Launch Vehicle (PSLV) C-9. [4]
According to the manufacturer of the reaction wheel used on CanX-2, "The wheel has been turned on and spun [and] is performing properly on orbit." [5]
CanX-3, also known as the BRIght Target Explorer (BRITE), is a nanosatellite planned to make photometric observations of some of the brightest stars in the sky in order to examine them for variability. These observations should be about ten times more precise than any ground-based observations.
The satellites are 20 cm cube which uses a number of technologies qualified on CanX-2.
A preliminary design for BRITE has been completed with the support of ETech, and the components to be integrated into the nanosatellite are currently being evaluated at UTIAS/SFL.[ needs update ]
CanX-4 & 5 are a two satellite pair that will be utilized to demonstrate formation flying using nanosatellite scale technology. [6] These two satellites will be launched together, commissioned together, and then separated in orbit. Formations that will be examined include: a circulation of one space craft by the other (termed a projected circular orbit), an orbit where one satellite trails the other (termed an along track orbit), and a maneuver to move from the projected circular to along track formation.
The CanX-4 & 5 launch took place on 30 June 2014 on the Indian Polar Satellite Launch Vehicle (PSLV). [7] The dual spacecraft mission were the first nanosattelites to demonstrate autonomous formation flights with centimetre-level positional control. [8]
CanX-6 was a follow-up nanosattelite demonstration for the University of Toronto and Institute for Aerospace Studies. CanX-6 was started in October 2007, and was developed to demonstrate key aspects of the COM DEV spaceborne Automatic Identification System. [9]
CanX-7 (COSPAR 2016-059F, SATCAT 41788) was launched 26 September 2016 and decayed from orbit 21 April 2022. [10]
A CubeSat is a class of small satellite with a form factor of 10 cm (3.9 in) cubes. CubeSats have a mass of no more than 2 kg (4.4 lb) per unit, and often use commercial off-the-shelf (COTS) components for their electronics and structure. CubeSats are deployed into orbit from the International Space Station, or launched as secondary payloads on a launch vehicle. As of December 2023, more than 2,300 CubeSats have been launched.
A small satellite, miniaturized satellite, or smallsat is a satellite of low mass and size, usually under 1,200 kg (2,600 lb). While all such satellites can be referred to as "small", different classifications are used to categorize them based on mass. Satellites can be built small to reduce the large economic cost of launch vehicles and the costs associated with construction. Miniature satellites, especially in large numbers, may be more useful than fewer, larger ones for some purposes – for example, gathering of scientific data and radio relay. Technical challenges in the construction of small satellites may include the lack of sufficient power storage or of room for a propulsion system.
The Space Test Program (STP) is the primary provider of spaceflight for the United States Department of Defense (DoD) space science and technology community. STP is managed by a group within the Advanced Systems and Development Directorate, a directorate of the Space and Missile Systems Center of the United States Space Force. STP provides spaceflight via the International Space Station (ISS), piggybacks, secondary payloads and dedicated launch services.
The Multi-Application Survivable Tether (MAST) experiment was an in-space investigation designed to use CubeSat spacecraft connected by tethers to better understand the survivability of tethers in space. It was launched as a secondary payload on a Dnepr rocket on 17 April 2007 into a 98°, 647 x 782 km orbit. The MAST payload incorporated three picosatellites, named "Ralph," "Ted," and "Gadget," which were intended to separate and deploy a 1 km (0.62 mi) tether. The experiment hardware was designed under a NASA Small Business Technology Transfer (STTR) collaboration between Tethers Unlimited, Inc. (TUI) and Stanford University, with TUI developing the tether, tether deployer, tether inspection subsystem, satellite avionics, and software, and Stanford students developing the satellite structures and assisting with the avionics design.
The Nanosatellite Launch System (NLS) is a series of satellite launch missions launched 2003–2010, coordinated by the Space Flight Laboratory (SFL) of the University of Toronto Institute for Aerospace Studies (UTIAS).
SNAP-1 is a British nanosatellite in low Earth orbit. The satellite was built at the Surrey Space Centre by Surrey Satellite Technology Ltd (SSTL) and members of the University of Surrey. It was launched on 28 June 2000 on board a Kosmos-3M rocket from the Plesetsk Cosmodrome in northern Russia. It shared the launch with a Russian Nadezhda search and relay spacecraft and the Chinese Tsinghua-1 microsatellite.
DRAGONSat was a 2000s pair of nanosatellites that were to demonstrate autonomous rendezvous and docking (ARD) in low Earth orbit (LEO) for NASA. It was intended to gather flight data with a global positioning system (GPS) receiver strictly designed for space applications to gather flight data in the space environment. ARD is the capability of two independent spacecraft to rendezvous in orbit and dock without crew intervention. The mission failed when the DRAGONSats failed to separate from their carrier spacecraft.
ITUpSAT1, short for Istanbul Technical University picoSatellite-1, is a single CubeSat built by the Faculty of Aeronautics and Astronautics at the Istanbul Technical University. It was launched on 23 September 2009 atop a PSLV-C14 satellite launch vehicle from Satish Dhawan Space Centre, Sriharikota, Andhra Pradesh in India, and became the first Turkish university satellite to orbit the Earth. It was expected to have a minimum of six-month life term, but it is still functioning for over two years. It is a picosatellite with side lengths of 10 centimetres (3.9 in) and a mass of 0.990 kilograms (2.18 lb).
SSETI Express was the first spacecraft to be designed and built by European students and was launched by the European Space Agency. SSETI Express is a small spacecraft, similar in size and shape to a washing machine. On board the student-built spacecraft were three CubeSat picosatellites, extremely small satellites weighing around one kg each. These were deployed one hour and forty minutes after launch. Twenty-one university groups, working from locations spread across Europe and with very different cultural backgrounds, worked together via the internet to jointly create the satellite. The expected lifetime of the mission was planned to be 2 months. SSETI Express encountered an unusually fast mission development: less than 18 months from kick-off in January 2004 to flight-readiness.
Chasqui I is a one-kilogram nanosatellite developed by students at Peru's National University of Engineering (UNI) based on CubeSat technology. Developed with assistance from the Russian Southwest State University (SWSU), Kursk, it was part of an educational project to acquire the experience and ability in developing satellites.
Radio Aurora Explorer (RAX) is the first National Science Foundation sponsored CubeSat mission. The RAX mission is a joint effort between SRI International in Menlo Park, California and the University of Michigan in Ann Arbor, Michigan. The chief scientist at SRI International, Dr. Hasan Bahcivan, led his team at SRI to develop the payload while the chief engineer, Dr. James Cutler, led a team of students to develop the satellite bus in the Michigan Exploration Laboratory. There are currently two satellites in the RAX mission.
Jugnu, is an Indian technology demonstration and remote sensing CubeSat satellite which was operated by the Indian Institute of Technology Kanpur. Built under the guidance of Dr. N. S. Vyas, it is a nanosatellite which will be used to provide data for agriculture and disaster monitoring. It is a 3-kilogram (6.6 lb) spacecraft, which measures 34 centimetres (13 in) in length by 10 centimetres (3.9 in) in height and width. Its development programme cost around 25 million rupee. It has a design life of one year.
SARAL is a cooperative altimetry technology mission of Indian Space Research Organisation (ISRO) and Centre National d'Études Spatiales (CNES). SARAL performs altimetric measurements designed to study ocean circulation and sea surface elevation.
RAX-2 is a CubeSat satellite built as a collaboration between SRI International and students at the University of Michigan College of Engineering. It is the second spacecraft in the RAX mission. The RAX-1 mission ended after approximately two months of operation due to a gradual degradation of the solar panels that ultimately resulted in a loss of power. RAX team members applied the lessons learned from RAX-1 to the design of a second flight unit, RAX-2, which performs the same mission concept of RAX-1 with improved bus performance and additional operational modes. Science measurements are enhanced through interactive experiments with high power ionospheric heaters where FAI will be generated on demand.
SRMSAT is a Nanosatellite built by faculty and students at Sri Ramaswamy Memorial University in India. The satellite is an Indian Technology demonstration and Earth observation satellite which is operated by the SRM Institute of Science and Technology. This nanosatellite was used to monitor Greenhouse gases in atmosphere.
TUGSAT-1, also known as BRITE-Austria and CanX-3B, is the first Austrian satellite. It is an optical astronomy spacecraft operated by the Graz University of Technology as part of the international BRIght-star Target Explorer programme.
UniBRITE-1 is, along with TUGSAT-1, one of the first two Austrian satellites to be launched. Along with TUGSAT, it operates as part of the BRIght Target Explorer constellation of satellites. The two spacecraft were launched aboard the same rocket, an Indian PSLV-CA, in February 2013. UniBRITE is an optical astronomy spacecraft operated by the University of Vienna as part of the BRIght Target Explorer programme.
PhoneSat is an ongoing NASA project of building nanosatellites using unmodified consumer-grade off-the-shelf smartphones and Arduino platform and launching them into Low Earth Orbit. This project is part of NASA's Small Spacecraft Technology Program and was started in 2009 at NASA Ames Research Center.
BRITE-Constellation is an ongoing space mission carrying out two-band photometry in wide fields with a constellation of six (presently, three operational) BRIght Target Explorer (BRITE) nanosatellites. The mission was built by a consortium of three countries, Canada, Austria, and Poland, each operating two BRITE satellites. The six satellites were launched into low-Earth orbits between February 2013 and August 2014. Each satellite is a cube-shaped spacecraft with sides of 20 centimetres (7.9 in) hosting an optical telescope of 3 centimetres (1.2 in) aperture feeding an uncooled CCD with a field of view of approximately 20° × 24°. The satellites were intended for photometry of the brightest stars in single passband located in the blue (three satellites) or red (the other three satellites) part of the optical range.
OPTOS was a Spanish nanosatellite designed and developed by INTA with support from the European Cooperation for Space Standardization (ECSS) as a low-cost technology demonstrator. It was launched in 2013 and had a service life of three years.