The core temperature of the Sun is estimated to be around 15 million °C, determined through models that align with observational data. Scientists analyze energy transport from the core to the surface, using the Sun's light emission to calculate necessary temperature and density gradients for stability. Another method involves comparing the known fusion rate to potential rates at various temperatures, allowing for estimates without prior knowledge of fusion processes. Fundamental principles like Newton's gravity and the ideal gas equation also contribute to determining the central pressure, density, and temperature. These approaches collectively provide a robust estimation of the Sun's core temperature.
#1
Murtuza Tipu
47
2
It was estimated that the heat inside the core of the Sun inside around 15 000 000 °C - this value is extremely enormous. How did scientists estimate this value?
In general: you make models of the sun, and then you see which one agrees with all observations, and check which temperature this model predicts for the core.
A very simple model that gives a good approximation: fusion happens within a small volume in the core, and a part of the released energy is transported to the surface afterwards until it can escape as light. We know how much light the sun emits, and you can calculate the necessary temperature and density gradients inside that is required to transport this power and to keep the sun stable. Work from the surface inwards and you get an estimate for the core temperature.
Another nice approach is the fusion rate - this is known from the total power as well, and it can be compared to the fusion rate the sun would have at different temperatures.
#3
Helios
267
63
It is not necessary to know anything about fusion to estimate the Sun's central temperature. Very good estimates were made even before fusion was ever understood. After all, the Sun is just a self-gravitating ball of gas. It's Newton's gravity and the ideal gas equation. Find the central pressure and density and the temperature is found by the IGE.
Partial solar eclipse from Twizel, South Isl., New Zealand ...
almost missed it due to cloud, didnt see max at 0710 NZST as it went back into cloud.
20250922, 0701NZST
Canon 6D II 70-200mm @200mm,
F4, 100th sec, 1600ISO
Makeshift solar filter made out of solar eclipse sunglasses
This thread is dedicated to the beauty and awesomeness of our Universe. If you feel like it, please share video clips and photos (or nice animations) of space and objects in space in this thread. Your posts, clips and photos may by all means include scientific information; that does not make it less beautiful to me (n.b. the posts must of course comply with the PF guidelines, i.e. regarding science, only mainstream science is allowed, fringe/pseudoscience is not allowed).
n.b. I start this...
Asteroid, Data - 1.2% risk of an impact on December 22, 2032. The estimated diameter is 55 m and an impact would likely release an energy of 8 megatons of TNT equivalent, although these numbers have a large uncertainty - it could also be 1 or 100 megatons.
Currently the object has level 3 on the Torino scale, the second-highest ever (after Apophis) and only the third object to exceed level 1. Most likely it will miss, and if it hits then most likely it'll hit an ocean and be harmless, but...