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Ask An Astronomer: How ISRO's Aditya–L1 Mission Plans to Explore Sun's Mysteries
Thursday, February 6, 2020 IST
Ask An Astronomer: How ISRO

The year 2020 is already showing clear signs of becoming the year of solar physics. In January, space enthusiasts were treated with the most detailed images of the Sun ever taken, as the US-based National Science Foundation's Inouye Solar Telescope released its first images. On February 7, a new solar orbiter is set to take off to snap the first pictures of the Sun's north and south poles. The mission is being carried out by the US space agency NASA in collaboration with the European Space Agency (ESA).
 

 
 

Remember, NASA already has a solar probe, named Parker, providing incredible insights about the outer layer of the Sun. Launched in August 2018, Parker is now the closest spacecraft to the Sun. Now, the Indian Space Research Organisation (ISRO) has planned its solar mission, Aditya – L1, to be launched by the end of 2020. Looking at the scientific focus on the Sun across the globe, one may wonder why it is important to study this yellow dwarf star.
 
To answer this and understand more about ISRO's solar mission, we spoke to Dr. Abhay Deshpande, a Senior Scientist (Physicist) working for the Government of India as well as the Honorary Secretary of Khagol Mandal, a non-profit collective of astronomy enthusiasts who organise various sky observation programmes, lectures and study tours.
 
Apart from the heat and light that makes life possible on Earth, what are a few lesser-known impacts of the Sun on our daily life?
 
Although our parent star, the Sun, seems the brightest object for us, it is an average star in the astronomical sense. It is moderate in size and not one of the brightest stars in our galaxy. Moreover, it is at the edge of the galaxy and not the centre. All these features of the Sun make life possible on our planet Earth.
 
The Sun also shields us from several Gigantic Comets that may have the potential to hit Earth. The tremendous gravity of the Sun attracts all big incoming objects and thus keeps Earth safe.
 
Life on Earth depends on the energy that we get from the Sun. The Sun emits a large number of particles every second. The luminosity is 0.4 Billion Billion Billion (4 followed by twenty-six zeroes) Watts! Compare this common 10 Watt LED light we use at our homes. We receive such massive amounts of light consistently free of cost.
 
However, this figure also may vary. The Sun is a magnetically active object, and the magnetic field varies to follow an 11-year cycle of solar minima and maxima. The energy and charged particles released during these phases vary considerably and can have a wide range of impacts from weather to our modern-day communication.
 
What are solar maxima and minima?
 
Before we proceed, let us get familiar with Sun Spots, Sun Flare and Solar Wind.
 
On Sun, due to intense magnetic interactions, some regions get relatively cooled. These are the regions where Solar Plasma is trapped, and the temperature is around 4000°C as against the average temperature of 6000°C. Hence these regions appear darker and are called Sun Spots.
 
 
Near such intense magnetic regions, usually, there are sudden eruptions of Solar Flares. As the name suggests, these are bright flares coming out of the surface of the Sun known as photosphere. This results in the release of charged particles in space and some of such highly energised particles can travel and reach Earth. Such particles can heat up and change the weather patterns on Earth.
 
Fortunately, we have a magnetic field which is like a shield and this special shield divert most of the particles towards North or South Poles. These particles then ionise the upper layers and cause Arora Borealis in North and Arora Australis in the South region.
 
As mentioned earlier, the Sun exhibits a unique 11-year magnetic variation cycle. In this time the Magnetic Field changes and attends maxima and minima—due to the gradual flipping of magnetic axis of Sun in this period. The North and South Pole of the Sun flips in this time.
 
During maxima, Sun is very active and emits more charges particles. These particles can have severe effects on Earth! The minima are times when the Sun is "quiet" which means not much activity is there on Sun. The Sun Spots are rare or not seen at all. The emission of Solar Wind is minimum.
 
Tell us more about ISRO's Aditya-L1. What are the scientific objectives behind the mission?
 
Aditya-1 is India's first attempt to have Solar Observatory in space. Originally it was planned to place Aditya at 800 km height above Earth. But then an ambitious proposal was made, and now, the plan is to place Aditya near the Lagrangian Point L1. Hence we call this mission as Aditya-L1. The main objective of the mission is to observe the solar corona.

 
 

What do you mean by the Lagrangian Point L1?
 
In any two-body system, like Earth-Sun, there are Five points called Lagrangian where the gravity seems to balance. These are positions where the gravitational pull of Sun and Earth is precisely equal to the centripetal force required for a small object to move with them. In other words, if we have an object placed near these points, it will not need much fuel to go around the Sun-Earth system. Hence, these points are considered the best locations to place observational telescopes and probes.
 
An earlier mission Wilkinson Microwave Anisotropy Probe (WMAP), for example, was placed at point L2 satellite Planck. Also, the much-awaited James Webb Space Telescope will be accommodated at L2. The Solar and Heliospheric Observatory of 1995 was also placed at L1.
 
 
What is Sun's Corona? What are the unanswered mysteries around it?
 
Hypothetically speaking, imagine we are standing on Solar surface is called the photosphere (there is no 'hard' surface on Sun. It is just boiling gas surface, and hence we cannot stand on it). Then we see Sun's atmosphere, which is called as the chromosphere. It is rich in elements and dense and gets the first hand shock due to continuous Solar Flares emissions. Beyond that, the Sun's outermost layer is spread over thousands of kilometres. This outer atmosphere is called the corona. It is full of plasma and glows continuously. Normally, it cannot be seen due to Sun's brightness. But during Total Solar Eclipse, we can easily see corona with the unaided eye. It is a mild and beautiful sight!
 
The mystery around corona is that its temperature is very high. Much higher than Photosphere or Chromosphere! Imagine a cold night and you put on heater in your home. As you go away from heater, you will get less warmth. Naturally, the farther an object from the source of heat, the colder it should be. But in the case of the corona, as we go away from Sun….the temperature is observed to increase! This was unsolved mystery for years and is not yet completely understood. The answer may be hiding somewhere in the magnetic field lines of the corona. The trapped gases may heat up due to various interactions. Understanding of Coronal Mass Ejection is even more crucial for us as it has a direct bearing on the Earth's weather.
 
ISRO's Aditya-L1 is a half-ton satellite with six payloads. The most crucial payload is the Visible Line Coronograph. Corona is 100,000 times dimmer than Sun. Hence, we cannot see it unless there is a total solar eclipse (TSE). We know that TSE is a rare phenomenon and can occur at the most twice a year.
 
Further, the maximum duration of TSE is just 7 min 29 sec. So, even if all TSE can be observed for the maximum duration, you can see corona for less than 15 min only in a year. Hence, Coronograph is designed to ensure we can block the Sun and observe corona round the year.
 
Why is studying the Sun important?
 
Sun is, scientifically, the most exciting star for us. Not only because life on Earth depends on it, but also because the Sun is the only star, at present, where humans can send Missions and collect lots of Data. Apart from the growing scientific curiosity, there are numerous practical implications of studying the Sun. Let me give you an example.
 
In 1905, Albert Einstein proposed the mechanism by which energy and mass can be interchanged. Subsequently, he came up with the General Theory of Relativity which is one of the most successful theories of the 20th Century. Questions like how the Sun operates, how it releases energy or what is the age of the Sun were unanswered for many years. Only after Einstein's theories, scientists were able to deduce that Sun's energy is an outcome of fusion reaction. Hydrogen converts to Helium and radiation are emitted during this reaction. It is this reaction which now Scientists are trying to optimise to generate large amounts of electricity reliably and safely! Thus studying the Sun could pave the way for a sustainable future.
 
In the past 100 years, we have understood Sun to an increased level of accuracy. Based on the same, physicists have found out how Stars are born, how they live, and how they will die. The knowledge is very important to understand the critical question of how we came into existence. Also, if we are looking to find life in space and become multiplanet species, we should know in great detail where and what we should be focusing. This is not possible without knowledge of the behaviour of Stars.

 
 
 
 
 

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Shibu Chandran
2 hours ago

Serving political interests in another person's illness is the lowest form of human value. A 70+ y old lady has cancer.

November 28, 2016 05:00 IST
Shibu Chandran
2 hours ago

Serving political interests in another person's illness is the lowest form of human value. A 70+ y old lady has cancer.

November 28, 2016 05:00 IST
Shibu Chandran
2 hours ago

Serving political interests in another person's illness is the lowest form of human value. A 70+ y old lady has cancer.

November 28, 2016 05:00 IST
Shibu Chandran
2 hours ago

Serving political interests in another person's illness is the lowest form of human value. A 70+ y old lady has cancer.

November 28, 2016 05:00 IST


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