In short, the group found that the sun will reach its maximum temperature level at around 8 billion years of age, after which itll cool down but continue to increase in size. A visual representation of the suns lifetime can be seen listed below. Keep in mind how, as the video advances, the suns path begins to intensify.
ESA/Gaia/DPAC.
This version of a Hertzsprung-Russell diagram was gotten with a selection of stars from Gaias 2nd release brochure. Its the most detailed to date made by mapping stars over the whole sky, according to ESA.
ESA/Gaia/DPAC.
The method the team obtained this information was sort of by casting an ultra-wide net throughout all the Gaia information obtained of the Milky Way so far, then recognizing stars with temperatures, surface gravities, chemical structures, masses and radii that are similar to those of the sun. While browsing for these candidates, the group made sure to select out stars comparable to our sun yet various in age, so a comprehensive timeline could be constructed. Going forward, according to the Gaia collaboration, not only will this be helpful for establishing a clear sun trajectory, but itll likewise be useful for researchers who have other solar questions, such as “do all solar analogues have planetary systems similar to ours?
Between 5 billion and 7 billion years from now, our sun will reach the end of its life. At present, our sun is considered to be in the prime of its life. We might anticipate our host star to be the most convenient of its kind to study, its actually a lot harder to evaluate than stars further away because its so utterly intense due to its proximity.
Between 5 billion and 7 billion years from now, our sun will reach the end of its life. In brief, the group discovered that the sun will reach its maximum temperature level at roughly 8 billion years of age, after which itll cool down however continue to increase in size. The way the team obtained this info was sort of by casting an ultra-wide net throughout all the Gaia data retrieved of the Milky Way so far, then identifying stars with temperature levels, surface gravities, chemical compositions, masses and radii that are similar to those of the sun. While browsing for these candidates, the team made sure to pick out stars similar to our sun yet different in age, so an in-depth timeline might be constructed. Going forward, according to the Gaia partnership, not only will this be beneficial for developing a clear sun trajectory, however itll likewise be useful for scientists who have other solar questions, such as “do all solar analogues have planetary systems comparable to ours?