India’s Aditya-L1 spacecraft has reached its final destination point (Lagrange point L1) in space to study the sun at about 4 p.m. IST (or 10:30 UTC) on January 6, 2024, according to the Indian Space Agency, ISRO.
It is the first space-based, observatory-class spacecraft of India to study Aditya (in Sanskrit, Aditya means the sun).
Here, the final destination point, Lagrange point L1, is an imaginary position in space that is located 1.5 million km away from Earth and directed towards the Sun. It is approximately four times the earth-moon distance.
Aditya-L1 spacecraft will stay there for 5 years (mission duration) and orbit the Lagrange point L1 periodically (orbital period of 177.86 days). Please remember that Aditya-L1 spacecraft will neither land on the sun nor approach the sun any closer than L1.
During the course of its five years, the spacecraft will observe the photosphere, chromosphere, and outermost layers of the sun (the corona) with its seven scientific instruments (payloads).
The spacecraft takes a little more than 4 months to reach its final destination point in space, as it was launched on September 2, 2023, at 11:50 a.m. IST (or 6:20 UTC) from Satish Dhawan Space Centre (SDSC) SHAR, Sriharikota, a spaceport of India.
Why L1?
Scientifically, Lagrange Point 1 (L1) of the Sun-Earth system is a region in space where the gravitational forces of the Sun and Earth create an equilibrium. It is also called the parking spot in space. Please remember there are five Lagrange Points (L1, L2, L3, L4 and L5) of the Sun-Earth system.
As Lagrange Point 1 (L1) is an equilibrium position, that’s why Aditya-L1 can carry out its scientific work with minimum fuel consumption and with minimum maintenance from the ground control room.
Scientific payloads (instruments) of Aditya-L1:
Aditya-L1 carries seven scientific payloads to study the sun from space. All payloads are indigenously developed in close collaboration with ISRO.
Scientific payloads | Full name | Function | Developed by |
---|---|---|---|
VELC | Visible Emission Line Coronagraph | To study solar corona and dynamics of coronal mass ejections | Indian Institute of Astrophysics, Bengaluru |
SUIT | Solar Ultra-violet Imaging Telescope | To image the solar photosphere and chromosphere in near ultraviolet (UV) | Inter University Centre for Astronomy and Astrophysics, Pune |
SoLEXS | Solar Low Energy X-ray Spectrometer | To study the X-ray flares from the Sun over a wide X-ray energy range | U R Rao Satellite Centre, Bengaluru |
HEL1OS | High Energy L1 Orbiting X-ray Spectrometer | To study the X-ray flares from the Sun over a wide X-ray energy range | U R Rao Satellite Centre, Bengaluru |
ASPEX | Aditya Solar wind Particle EXperiment | To study the solar wind and energetic ions | Physical Research Laboratory, Ahmedabad |
PAPA | Plasma Analyser Package for Aditya | To study the solar wind and energetic ions | Space Physics Laboratory, Vikram Sarabhai Space Centre, Thiruvananthapuram |
MAG | Magnetometer | To measure interplanetary magnetic fields at the L1 point | Laboratory for Electro Optics Systems, Bengaluru |
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