·The Hindu·15 marks·250–350 wordsS&T

Discuss the scientific objectives of Aditya-L1 and explain why the Sun–Earth L1 point is an ideal vantage point for solar observation.

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In this answer
  1. Scientific objectives
  2. Why L1 is an ideal vantage point

Aditya-L1, India's first solar mission, was launched on PSLV-C57 on 2 September 2023. It was placed in a halo orbit around the Sun–Earth Lagrange point L1 on 6 January 2024 [1]. Its purpose is to study the Sun as the source of space weather, and L1 is the position that makes this study possible.

Scientific objectives

  • Coronal heating: to find out why the Sun's outer atmosphere, the corona, is far hotter than its surface [2].
  • Solar eruptions: to study pre-flare and flare activity and coronal mass ejections (CMEs), including their origin, characteristics and dynamics [2].
  • Space-weather drivers: to track how particles and fields move through the interplanetary medium [2].
  • Instruments: the spacecraft carries 7 payloads. Four are remote-sensing instruments that look at the Sun: VELC, SUIT, SoLEXS and HEL1OS. Three are in-situ instruments that measure conditions at L1: ASPEX, PAPA and MAG [1].
  • Early results: PAPA recorded the impact of CMEs on the solar wind in February 2024 [3]. In 2026, Indian Institute of Astrophysics (IIA) scientists used VELC data to make Doppler velocity images of the corona. These images can show whether a CME is moving along the Sun–Earth line [4].

Why L1 is an ideal vantage point

 SUN ●───────────────────────────●─────────● EARTH
                          Aditya-L1 (L1)
                          ~1.5 million km from Earth

Fig.: L1 lies on the Sun–Earth line, about 1% of the way to the Sun

  • Continuous view: a halo orbit gives a view of the Sun free from eclipses or occultation [1]. This allows round-the-clock observation.
  • Stable position: at L1, the gravity of the Sun and Earth balances the spacecraft's orbital motion. It therefore keeps pace with Earth and needs little fuel to stay in place.
  • Sampling the solar wind before it reaches Earth: L1 is about 1.5 million km away, roughly 4 times the Earth–Moon distance [5]. This is beyond Earth's magnetic shield, so in-situ payloads measure the solar wind before it reaches Earth [3].
  • Head-on view of threats: because L1 sits on the Sun–Earth line, VELC's Doppler images can show whether a CME is heading towards Earth. Ordinary coronagraph images cannot show this [4].

Aditya-L1 links its scientific goals with an ideal observing position: it watches the Sun without interruption and measures what reaches Earth's neighbourhood. Next, ISRO and IIA should check VELC's direction readings against the spacecraft's own in-situ data. They should then turn these results into routine warnings that protect satellites, NavIC and power grids. That would support SDG 9 (resilient infrastructure) and confirm the value of India's position at L1.

Sources

  1. 1ADITYA-L1 — ISRO: launch and orbit-insertion dates, halo orbit, view free from eclipses and occultation, 7 payloads (4 remote-sensing + 3 in-situ)
  2. 2Aditya-L1 booklet — ISRO: science objectives (coronal heating, flares, CMEs, space-weather dynamics, particles and fields)
  3. 3PAPA payload aboard Aditya-L1 detects solar wind impact of Coronal Mass Ejections — ISRO: in-situ detection of CME impacts, February 2024
  4. 4"Aditya-L1 mission offers new insights into the direction of solar eruptions", The Hindu, 21 Oct 2026 (news report): IIA's VELC Doppler velocity images showing CME motion along the Sun–Earth line
  5. 5Aditya-L1 booklet — ISRO, "1.5 million kilometres from the Earth, about 4 times farther than the Moon": distance of L1 from Earth
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