Aditya Mission by ISRO

Aditya-L1, India's first Solar mission to be launched on September 2 πŸš€


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PSLV-C57/Aditya-L1 Mission:


The launch of Aditya-L1 by PSLV-C57 is accomplished successfully.


The vehicle has placed the satellite precisely into its intended orbit.


India’s first solar observatory has begun its journey to the destination of Sun-Earth L1 point.






























The launch of Aditya-L1 by ISRO - Indian Space Research Organisation is the first space-based Indian observatory to study the Sun☀️


πŸ—“️September 2, 2023 : The Spacecraft is ready to be launched now and Aditya L-1 Launch will take place on 2nd September 2023.


πŸ•›11:50 Hrs. IST from Sriharikota


The mission aims to provide crucial insights into various aspects of solar activities and their influence on space weather. It will carry seven payloads to observe the photosphere, chromosphere, and the outermost layers of the Sun, the corona, in different wavebands.



Aditya-L1 is the first space-based observatory-class Indian solar mission to study the Sun. It is planned to be placed in a halo orbit around the Lagrangian point1 (L1) of the Sun-Earth system, which is about 1.5-million-km from Earth.


According to ISRO, the spacecraft will be placed in a halo orbit around the Lagrange point 1 (L1) of the Sun-Earth system, which is about 1.5 million km from the Earth.





Science Objectives:

The major science objectives of Aditya-L1 mission are:


Study of Solar upper atmospheric (chromosphere and corona) dynamics.

Study of chromospheric and coronal heating, physics of the partially ionized plasma, initiation of the coronal mass ejections, and flares

Observe the in-situ particle and plasma environment providing data for the study of particle dynamics from the Sun.

Physics of solar corona and its heating mechanism.

Diagnostics of the coronal and coronal loops plasma: Temperature, velocity and density.

Development, dynamics and origin of CMEs.

Identify the sequence of processes that occur at multiple layers (chromosphere, base and extended corona) which eventually leads to solar eruptive events.

Magnetic field topology and magnetic field measurements in the solar corona .

Drivers for space weather (origin, composition and dynamics of solar wind .








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