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As of my last knowledge update in September 2021, the Aditya-L1 mission was an upcoming Indian space mission by the Indian Space Research Organisation (ISRO) designed to study the Sun. Please note that mission details may have evolved since then, and I recommend checking the latest information on the ISRO website or other reliable sources for the most current details. However, here are the key details about the Aditya-L1 mission as of my last update:
The primary objective of the Aditya-L1 mission is to study the Sun, specifically focusing on its outermost layer, the solar corona. The mission aims to improve our understanding of the Sun’s behavior, which has a direct impact on space weather and can affect communication, navigation systems, and power grids on Earth.
The mission is planned to be launched using India’s Polar Satellite Launch Vehicle (PSLV). PSLV has a strong track record of launching a variety of satellites into different orbits.
Aditya-L1 is expected to carry a suite of scientific instruments to observe the Sun, including: Visible Emission Line Coronagraph (VELC): To study the outermost layer of the solar corona. Solar Ultraviolet Imaging Telescope (SUIT): To capture images and data in the ultraviolet (UV) region of the electromagnetic spectrum. Plasma Analyser Package for Aditya (PAPA): To study the composition and nature of solar wind and its properties. Solar Low-Energy X-ray Spectrometer (SoLEXS): To observe low-energy X-ray emissions from the Sun. Magnetometer: To measure the magnetic field on the Sun’s surface and its variations.
Aditya-L1 is intended to be placed in a halo orbit around the first Lagrange point (L1) of the Sun-Earth system. This unique orbit allows for continuous observation of the Sun without being blocked by the Earth. 5. Duration: The mission’s duration is expected to be several years, during which it will provide valuable data to enhance our understanding of solar phenomena and their impact on space weath
There are essentially seven payloads on the Aditya L-1. The main one is the Visible Emission Line Coronagraph (VLEC) to study the solar corona from the lowermost part upwards. The Solar Ultraviolet Imaging Telescope (SUIT) will capture the UV image of the solar photosphere and chromosphere. It will examine the variation in light energy emitted.
Meanwhile, the Solar Low Energy X-ray Spectrometer (SoLEXS) and High Energy L1 Orbiting X-ray Spectrometer (HEL1OS) will analyse X-ray flares. The Aditya Solar wind Particle Experiment (ASPEX) and Plasma Analyser Package for Aditya (PAPA) have been built to study the solar wind and energetic ions.
The points can be used as ‘parking spots’ for spacecraft in space to remain in a fixed position with minimal fuel consumption, according to NASA. They have been named after Italian-French mathematician Joseph-Louis Lagrange (1736-1813), who was the first one to find the positions. So, between the Earth and the Sun, a satellite can occupy any of five Lagrangian points. “Of the five Lagrange points, three are unstable and two are stable. The unstable Lagrange points – labelled L1, L2, and L3 – lie along the line connecting the two large masses. The stable Lagrange points – labelled L4 and L5 – form the apex of two equilateral triangles,” NASA explains. The L4 and L5 are also called Trojan points and celestial bodies like asteroids are found here.
for more – https://indianexpress.com/article/explained/explained-sci-tech/aditya-l-1-solar-mission-explained-8920110/
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