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Sun radius
700,000 km
Photosphere temperature
5800 K
Core temperature
15 million K
Luminosity of the Sun
4 × 10²⁶ W
Solar constant
1400 W/m²
Equatorial rotation period of the Sun
25 days
Sunspot cycle duration
11 years
Full magnetic cycle duration
22 years
Corona temperature
Approximately 3 million K
Solar wind speed
Approximately 500 km/s (up to 800 km/s from coronal holes)
Core
The center of the Sun where nuclear fusion occurs converting hydrogen to helium.
Proton-Proton chain
The primary fusion process in the Sun that combines four hydrogen nuclei into one helium nucleus.
E=mc²
Equation describing the mass-energy equivalence used in nuclear fusion.
Helioseismology
The study of solar vibrations used to learn about the Sun's interior.
Granules
Small, bright features on the Sun's surface caused by convection, about 1000 km across.
Spicules
Jets of gas in the chromosphere, approximately 100 km/s, lasting a few minutes.
Coronal holes
Regions of lower density in the corona where solar wind primarily escapes.
Sunspots
Dark spots on the photosphere caused by cooler temperatures due to strong magnetic fields.
Maunder Minimum
Period from 1645–1715 with almost no observed sunspots, associated with colder climate.
Solar flares
Explosions on the Sun that can produce X-rays and UV radiation.
Coronal Mass Ejection (CME)
A huge bubble of magnetized gas ejected into space capable of affecting Earth.
Neutrinos
Tiny particles produced during fusion with almost no interaction with matter.
Neutrino oscillation
The phenomenon of neutrinos changing type while traveling, discovered during the solar neutrino problem.
Granulation
The pattern of bright centers (hot gas rising) and dark edges (cool gas sinking) seen on the Sun's surface.
Differential rotation
The Sun's rotation varies with latitude; equator rotates faster than poles.
Solar activity impact on Earth
Can cause auroras, satellite disruptions, GPS issues, radio communication problems, and power outages.