12 August 2022
Our Solar is doomed. Billions of years from now, the Solar will deplete its hydrogen gasoline and swell to a purple big earlier than turning into a white dwarf. It’s a widely known story, and one astronomers have understood for many years. Now, due to the newest information from Gaia, we all know the Solar’s future in a lot better element.
The timeline of human civilization is a mere blip within the lifetime of a star. We haven’t been round lengthy sufficient to observe a star’s delivery, life, and dying. However we are able to perceive stellar evolution by observing different stars which may be older or youthful than the Solar. It’s just like the way in which you would possibly perceive how people dwell and die by taking a look at a assortment of images all taken on the similar time on a single day. One of many first snapshots of stellar evolution was performed within the early 1900s. First as a knowledge desk by Ejnar Hertzsprung in 1905, however extra famously performed as a diagram by Henry Norris Russell in 1914. Now generally known as Hertzsprung-Russell diagrams, or HR diagrams, they plot the colour or spectral class of a star versus its absolute magnitude. Colour is a measure of a star’s temperature, and absolute magnitude is a gauge of its dimension.
The early HR diagrams solely had information for about 300 stars, however even then it was clear most stars lay alongside a linear path generally known as the primary sequence. Since most stars are inside the primary sequence, it stands to purpose that stars spend most of their lives as most important sequence stars. Small stars shine at cool temperatures, whereas bigger extra huge stars burn hotter. The HR diagrams confirmed that some stars similar to purple giants have been massive however cool, and others generally known as white dwarfs have been small and sizzling, however these have been the exceptions. As astronomers gathered extra information, they might see how bigger most important sequence stars entered a large stage earlier than turning into white dwarfs or neutron stars. By and huge, the mass of a star determines its lifetime and destiny.
We now know that whereas the mass of a star is a vital facet of stellar evolution, its chemical composition additionally performs an essential position. Two stars related in mass however completely different in composition can have very completely different lifetimes. That is the place the Gaia survey is available in. Whereas early stellar surveys had lots of or hundreds of stars, Gaia has greater than a billion. Within the newest information launch, the Gaia staff created an HR diagram of greater than 4 million stars inside 5,000 light-years of Earth. For these stars, we all know not solely their dimension and spectral temperature but in addition know their chemical composition. This implies the Gaia staff may create an HR diagram of stars with an analogous mass and composition to the Solar. The end result traces the evolutionary path of Solar-like stars from the primary sequence to the purple giants. Based mostly on the information, the Solar will attain its most temperature at an age of 8 billion years, then shift towards the purple big part earlier than lastly dying at round 11 billion years previous.
The Gaia staff additionally discovered almost 6,000 stars which are close to twins of the Solar, having related mass, temperature, composition, and age. By observing these stars, astronomers will get a greater understanding of whether or not our Solar is typical. For instance, do these different stars have photo voltaic cycles just like the Solar? Do some have intervals of intense photo voltaic flares or are they pretty secure just like the Solar?
With a lot gathered information, Gaia is revealing new particulars about our personal star, the way it could behave within the close to future, and the way it will die within the far future. We’ve lengthy recognized the top is nigh for the Solar, however we’re starting to be taught simply how and when the top will come.