Science By Joshua Sokol 12/3/2018
When Earth was a mass of newly minted rock some 4.5 billion years ago, the solar system was a cold place. Physicists predict our young sun put out some 15% to 25% less energy than it does today—enough to freeze over Earth’s oceans and make Mars even colder. Yet ancient rocks suggest water flowed across both planets, posing a perplexing puzzle.
For years, climate modelers solved this so-called “faint young sun†paradox by proposing that ancient atmospheres on both planets had the right composition of greenhouse gases to insulate them and keep them above freezing. But if the young sun reached its current weight only after a diet—shedding perhaps 5% of its early mass in a stellar wind of escaping particles—it would have burned brighter in its past than predicted, resolving the paradox. The only problem with that hypothesis? Scientists have had no way of knowing whether this stellar slim-down happened.
Now, astronomers say they have come up with a potential “fingerprint†of the sun’s ancient mass—climate cycles preserved in bands of martian rocks. To find their marker, Christopher Spalding, a planetary astronomer at Yale University, geobiologist Woodward Fischer at the California Institute of Technology in Pasadena, and astronomer Gregory Laughlin of Yale started with an orbital cycle that both Earth and Mars experience. As the solar system’s planets revolve around the sun, their own gravity tweaks each other’s orbits.
More:
https://www.sciencemag.org/news/2018/12/did-our-ancient-sun-go-diet-bands-martian-rock-could-solve-faint-young-sun-paradox