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Mahesh

07/01/24 06:32 AM IST

Aditya L1 journey

In News
  • Aditya-L1 was launched by ISRO on September 2, 2023 with the mission of observing, and helping us better understand the Sun.
  • It arrives at its destination, L1 or the first Sun-Earth Lagrangian point recently.
Study of Sun
  • The Sun produces energy through nuclear fusion in its interior, and emits it from its outer layers.
  • The photosphere, a 6,000-degree Celsius layer, emits all visible and infrared light, crucial for life. Above is the chromosphere, and higher still is the million-degree Celsius hot corona.
  • Interestingly, the corona is much hotter than the inner layers of the Sun — there must be some energy source which provides this heat.
  • However, the processes involved in this are not yet fully understood.
  • Moreover, it also emits ultraviolet and X-ray radiation which would be lethal to life on Earth, without the presence of the atmosphere which absorbs most harmful radiation.
  • The Sun also continuously streams electrically charged particles — a stream known as the Solar wind.
  • These charged particles produce the spectacular aurorae, known as the Northern and Southern Lights, seen close to the north and south poles of the Earth.
  • There are also sudden bursts and ejections of charged particles from the Sun into interplanetary space, known as Solar flares and coronal mass ejections.
  • These directly affect space weather, space-reliant technologies like satellite communication networks, and can produce electric power blackouts in Earth’s higher latitudes.
Aditya L1
  • Aditya-L1 is located outside the Earth’s atmosphere, its instruments can observe the ultraviolet radiation from the corona, and in the process, better understand its workings.
  • Moreover, we need to monitor the Solar atmosphere and the corona continuously to monitor eruptions on the Sun, and study the properties of charged particles in the Solar wind.
  • Crucially, this task has to be carried out from outside Earth’s atmosphere, and as close to the Sun as possible.
  • This will then help provide early warning of Solar eruptions, and allow us to initiate actions to minimise the disruption they may cause.
  • Aditya-L1 has seven instruments for the observation of all the radiation and charged particles.
  • Its location, 1.5 million km away from Earth towards the Sun (more on that next), allows uninterrupted observations.
Location of Aditya L1
  • L1 stands for the first Lagrangian point— there are five such points, L1 to L5, associated with the motion of one astronomical body around another one, in Aditya’s case, Earth and the Sun.
  • These points were theoretically discovered by the Swiss mathematician Leonhard Euler and the Italian-French mathematician Joseph-Louis Lagrange in the 19th century.
  • When a spacecraft is in orbit around Earth, it is affected by the gravitational force exerted on it by the planet.
  • Yet it does not fall to Earth’s surface because effectively, Earth’s gravity is balanced by a centrifugal force which arises due to the motion of the spacecraft around the Earth.
  • L1 is the sweet spot between Earth and the Sun, where the gravitational force exerted on a spacecraft by the two celestial bodies, and the centrifugal force cancel each other.
  • As a result, once placed exactly at L1, Aditya would always continue to remain there without expending any energy.
Point L1
  • L1 is on the line joining the Sun and the Earth. As Earth rotates round the Sun, L1 goes round the Sun too, while always remaining on the same line.
  • Thus, rather than being at the same point in space, Aditya will remain at the same position, relative to the Sun and Earth.
  • In fact, the L1 point itself is fundamentally unstable — a tiny pull or push can send the spacecraft hurtling away in some other direction. To avoid this, Aditya is placed in an orbit around L1.
  • A complex orbit nearly perpendicular to the line joining the Sun and Earth, it will take the spacecraft about 178 days to complete one full orbit.
Why L1?
  • Aditya is meant to act as an early warning system for solar flares and coronal mass ejections,is necessary to have an uninterrupted view of the Sun.
  • When Aditya is at L1, the Earth is always on one side of it, and the Sun on the other side.
  • Thus, the spacecraft’s instruments can be pointed towards the Sun for a completely uninterrupted view.
  • Even though placing the spacecraft at an orbit around L1 is complex, the benefits of having an uninterrupted view of the Sun at all times is well worth the effort, risk, and expense.
  • A few space missions are already parked around the L1 point, including the LISA Pathfinder, and Solar and Heliospheric Observatory (SOHO), both collaborative missions of NASA and European Space Agency.
L2 point
  • While the L1 is the ideal point to observe the Sun, L2 is a very useful staging point for spacecraft to be used for observing the distant Universe.
  • L2 also is along the line joining the Sun and Earth, but it is on the opposite side of the Earth, at about 1.5 million kilometres.
  • So, a spacecraft in a halo orbit around L2 can have all its instruments pointing away from the Earth, to get an uninterrupted view of the deep space.
  • The James Webb Space Telescope (JWST), Gaia and Euclid are some of the important astronomical probes which are presently in orbit around L2.
  • The Planck mission, which carried out path breaking observations of the cosmic microwave background radiation was also located there.
Source- Indian Express

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