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.

Briefing Summary
AI-generatedIndia'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.
Article analysis
Model · rule-basedKey claims
5 extractedCoronal Mass Ejections (CMEs) cause auroras and can lead to geomagnetic storms affecting Earth's power grids and satellites.
The corona's temperature is about 2 million C, sometimes reaching 40 million C, while the surface is about 5,500C.
The Sun's outer atmosphere (corona) is millions of degrees hotter than its surface, a long-standing scientific mystery.
A mechanism must exist to maintain the corona's high temperature, as the Sun loses energy through CMEs.
India's Aditya-L1 solar mission has provided vital clues to understanding the corona's high temperature.