|Mission type||Solar observatory|
|Mission duration||2 years (nominal)|
|Launch mass||CSC: 339 kilograms (747 lb)|
OSC: 211 kilograms (465 lb)
|Dry mass||CSC: 327 kilograms (721 lb)|
OSC: 190 kilograms (420 lb)
|Dimensions||CSC: 1.1 by 1.8 by 1.7 metres (3.6 ft × 5.9 ft × 5.6 ft)|
OSC: 0.9 by 1.4 metres (3.0 ft × 4.6 ft)
|Start of mission|
|Launch site||Kourou ELV|
|Regime||Highly-elliptical Earth Orbit|
|Semi-major axis||36,943 kilometres (22,955 mi)|
|Perigee||600 kilometres (370 mi)|
|Apogee||60,530 kilometres (37,610 mi)|
|Argument of perigee||188 degrees|
|Diameter||50 millimetres (2.0 in)|
|Focal length||1.15 metres (3.8 ft)|
PROBA-3 is the third satellite mission in the European Space Agency's series of PROBA low-cost satellites that are being used to validate new spacecraft technologies while also carrying scientific instruments.
PROBA-3 will be composed of two independent, three-axis stabilized spacecraft flying at 150 meters to one another with the ability to accurately control the attitude and separation of the two craft. Their alignment with the Sun will be maintained for 6 hours, creating ″artificial solar eclipse″ for the back satellite. The spacecraft pair will fly a highly elliptical orbit divided between periods of accurate formation flying around apogee, when payload operations will be possible, and periods of free flight. The length of the formation control period will be a trade-off involving the increasing amount of fuel needed to maintain the orbits in formation when away from apogee.
The primary mission of PROBA-3 is solar coronagraphy by using the telescope on the larger of the two satellites to view the Sun's corona while the other spacecraft is maneuvered to accurately occult the disc of the Sun.
- "Mission / PROBA-3". ESA. 13 November 2014. Retrieved 30 November 2015.
- "Science Payload / PROBA-3". ESA. 13 November 2014. Retrieved 30 November 2015.
- "ESA Bulletin 160 (November 2014)" (PDF). ESA. November 2014. p. 61. ISSN 0376-4265. Retrieved 30 November 2015.
- "About PROBA-3". ESA. 13 November 2014. Retrieved 30 November 2015.
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