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FRI · 2026-08-14 · 02:13 GMTBRIEF NSR-2026-0814-102163
News/Indian solar mission's new findings throw light on enduring …
NSR-2026-0814-102163News Report·EN·Technology

Indian solar mission's new findings throw light on enduring Sun mysteries

India's Aditya-L1 solar mission has provided crucial clues to understanding the Sun's corona, which is millions of degrees hotter than its surface, a long-standing mystery. Astrophysicists, led by Prof R Ramesh of the Indian Institute of Astrophysics, published findings in Astrophysical Journal Letters detailing temperature variations that defy conventional physics.

2 hours agoShareSaveAdd as preferred on GoogleGeeta PandeyBBC Correspondent, DelhiBBC News - WorldFiled 2026-08-14 · 02:13 GMTLean · CenterRead · 2 min
Indian solar mission's new findings throw light on enduring Sun mysteries
BBC News - WorldFIG 01
Reading time
2min
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357words
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10entities
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Briefing Summary

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India's Aditya-L1 solar mission has provided crucial clues to understanding the Sun's corona, which is millions of degrees hotter than its surface, a long-standing mystery. Astrophysicists, led by Prof R Ramesh of the Indian Institute of Astrophysics, published findings in Astrophysical Journal Letters detailing temperature variations that defy conventional physics. The corona, the Sun's outer atmosphere, reaches temperatures of around 2 million degrees Celsius, despite frequent energy-losing eruptions like coronal mass ejections (CMEs). These CMEs, while causing auroras, can also disrupt Earth's power grids and satellites. The continued high temperature of the corona, even after these massive energy releases, suggests an unknown replenishing mechanism is at play, preventing the Sun from cooling down.

Confidence 0.90Sources 1Claims 5Entities 10
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Article analysis

Model · rule-based
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Technology
Human Interest
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Key claims

5 extracted
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Coronal Mass Ejections (CMEs) cause auroras and can lead to geomagnetic storms affecting Earth's power grids and satellites.

factualProf R Ramesh
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1.00
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The corona's temperature is about 2 million C, sometimes reaching 40 million C, while the surface is about 5,500C.

statisticProf R Ramesh
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The Sun's outer atmosphere (corona) is millions of degrees hotter than its surface, a long-standing scientific mystery.

factual
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A mechanism must exist to maintain the corona's high temperature, as the Sun loses energy through CMEs.

factualProf R Ramesh
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0.90
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India's Aditya-L1 solar mission has provided vital clues to understanding the corona's high temperature.

factualAstrophysicists in India
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Full report

2 min read · 357 words
One of the most enduring mysteries that has been puzzling scientists forever is how the Sun's outer atmosphere - the corona - is millions of degrees hotter than its surface. And how does the corona continue to remain so hot despite frequent eruptions during which it loses huge amounts of energy?Astrophysicists in India now say the latest findings from Aditya-L1, the country's first solar observation mission in space, have provided them some vital clues to unlocking those mysteries. Their findings are revealed in a recent paper published in the prestigious Astrophysical Journal Letters.The temperature variations in different regions of the Sun defy the laws of physics, says leading Indian solar astrophysicist Prof R Ramesh of the Indian Institute of Astrophysics (IIA) who led the study.If you cut through the Sun's layers, deep inside is the core where the temperature is 15 million Celsius. Travel outwards to the surface or the photosphere - the part that we see from the Earth - it's about 5,500C. Far away from the core is the Sun's outermost layer or corona where the temperature is about 2 million C - it can sometimes go up to 40 million C.Prof Ramesh says the corona is where extreme weather events - such as solar flares and coronal mass ejections (CMEs) - originate, during which large amounts of energy is released by the Sun into space. The CMEs cause beautiful auroras, and they can also affect life on Earth by causing geomagnetic storms that can knock down power grids and affect weather and communication satellites.In normal or low-activity times, the Sun launches two to three CMEs a day. During the maximum solar activity cycle that comes every 11 years, there can be 10 or more in a single day."Now if the Sun is losing such huge amounts of energy with each CME and it's not replenished, the star at the centre of our solar system would lose all its energy and Earth would plunge into an irreversible deep freeze," Prof Ramesh says.But since that's not happening, it means there's a "mechanism" by which the corona is able to maintain its inexplicably high temperature, he says.
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Keywords & salience

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solar corona
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aditya-l1
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sun mysteries
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solar flares
0.80
coronal mass ejections
0.80
solar astrophysicist
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temperature variations
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energy loss
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astrophysical journal letters
0.40
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