Search results
11 maj 2023 · The temperature of the sun varies from around 27 million degrees Fahrenheit (15 million degrees Celsius) at the core to only about 10,000 degrees F (5,500 degrees C) at the surface,...
- Curious Kids
The temperature of the sun. Heat is created in the very...
- Hydrogen and Helium
In the sun's core, gravitational forces create tremendous...
- How Was the Sun Formed
The Sun: Our Perfectly Average Middle Aged Star (Image...
- When Will the Sun Die
That's when the sun will become a red giant, which it will...
- Parker Solar Probe
NASA's Parker Solar Probe is on a mission to study the sun...
- Gravity
Gravity can be described in a variety of ways. Here's how...
- NASA's Lucy Asteroid-Hopping Probe Captures 1st Snapshot of Space Rock 'Dinky' (Photo)
NASA's Lucy spacecraft just sent home an impressive glimpse...
- James Webb Space Telescope Deepens Major Debate Over Universe's Expansion Rate
According to most models, the Hubble constant should equal...
- Curious Kids
13 gru 2023 · From the fiery depths of its core to the outermost reaches of its corona, here are the temperatures, from millions of degrees in Kelvin to the more comprehensible Celsius and Fahrenheit scales. The hottest part of the Sun is the core: 15 million K; ~15 million ° C; 27 million ° F.
The temperature in the Sun's core is about 27 million degrees Fahrenheit (15 million degrees Celsius) – hot enough to sustain nuclear fusion. This creates outward pressure that supports the star's gigantic mass, keeping it from collapsing.
The Sun is gradually becoming hotter in its core, hotter at the surface, larger in radius, and more luminous during its time on the main sequence: since the beginning of its main sequence life, it has expanded in radius by 15% and the surface has increased in temperature from 5,620 K (9,660 °F) to 5,772 K (9,930 °F), resulting in a 48% ...
7 paź 2019 · The temperature in the core is around 15 million degrees Celsius. This, combined with the huge pressure and density of the plasma force hydrogen nuclei to fuse together, creating helium and releasing vast quantities of energy in the process.
10 paź 2012 · The temperature in the chromosphere varies between about 4000 K at the bottom (the so-called temperature minimum) and 8000 K at the top (6700 and 14,000 degrees F, 3700 and 7700 degrees C), so in this layer (and higher layers) it actually gets hotter if you go further away from the Sun, unlike in the lower layers, where it gets hotter if you go ...
Model values at center of Sun: Central pressure: 2.477 x 10 11 bar (2.477 x 10 17 g/cm s 2) Central temperature: 1.571 x 10 7 K Central density: 1.622 x 10 5 kg/m 3 (1.622 x 10 2 g/cm 3)
