Mikhailo Lomonosov (satellite)

Mikhailo Lomonosov
Mission type Astronomy
Operator MSU
COSPAR ID 2016-026A
SATCAT № 41464
Mission duration Planned: 3 years[1]
Spacecraft properties
Manufacturer VNIIEM
Launch mass 620 kg (1,370 lb)[1]
Payload mass 170 kg (370 lb)[1]
Power ~300 W[1]
Start of mission
Launch date 28 April 2016, 02:01 UTC (planned)
Rocket Soyuz-2.1a/Volga
Launch site Vostochny Site 1S
Contractor Roscosmos
Orbital parameters
Reference system Geocentric
Regime Sun-synchronous
Semi-major axis 6,856 kilometers (4,260 mi)[2]
Perigee 478.2 km (297.1 mi)[2]
Apogee 492.9 km (306.3 mi)[2]
Inclination 97.3 degrees[2]
Period 94.2 minutes[2]
Instruments

Mikhailo Lomonosov (or MVL-300) is an astronomical satellite of MSU named after Mikhail Lomonosov.[3]

Mission

The objective of the mission is the observation of gamma-ray bursts, high-energy cosmic rays and transient phenomena in the Earth's upper atmosphere.[3]

One of the instruments on board is the TUS (Tracking Ultraviolet Set Up) system, which is designed to measure fluorescence light radiated by EAS (Extensive Air Showers) of Ultra High Energy Cosmic Rays (UHECR) in the earth atmosphere as well as for transients’ studies within UV-range.[4]

For studying gamma-ray bursts Lomonosov has UFFO and BDRG instruments.

References

  1. 1 2 3 4 "Космический аппарат «Ломоносов»" (in Russian). Retrieved 21 March 2016.
  2. 1 2 3 4 5 "MVL 300 Satellite details 2016-026A NORAD 41464". N2YO. 4 May 2016. Retrieved 4 May 2016.
  3. 1 2 "Soyuz prepared for first flight from Siberian cosmodrome". Spaceflight Now. Retrieved 21 March 2016.
  4. "MVL-300 (Mikhailo Lomonosov)". Gunter's Space Page. Retrieved 21 March 2016.
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