The Sun's Closest Twins
At the American Astronomical Society meeting, Edward Guinan described an ongoing program called "The Sun In Time" that is identifying and studying solar analogues. Working at every wavelength, from radio to X-rays, the group is researching stars that have sizes, masses, temperatures, and heavy-element contents that are similar to those of the present-day Sun as well as solar-twin stars at every age from birth onward.
Perhaps the greatest difference between young solar-type stars and old ones is their surface activity flares, spots, ultraviolet and X-ray outbursts, and other byproducts of magnetic turmoil. Stars are generally born spinning fast, revolving once in a day or two (compared to the Sun's 27-day rotation period). A fast spin results in a powerful dynamo effect inside the star, which produces strong magnetism and high-energy surface explosions. "These stars are on fire," says Guinan. Over time their spins slow down (due to magnetic braking via stellar winds), and their surface activity declines accordingly. The relation between age and spin is very tight. "If you tell me the rotation period of a G star, I'll tell you its age," Guinan says. This has allowed the group to assemble a zoo of solar analogues at different points along the Sun's lifeline.
One result of this work is an appreciation of just how badly our violent young Sun treated its inner planets. Extreme-ultraviolet radiation and particle winds may have eroded most of Mercury away, leaving just its dense inner portions as the "iron planet" we see today. Venus should have at least lost its atmosphere, meaning that the massive atmosphere it has now must have arrived later, perhaps by volcanism. Earth has always had a magnetic field protecting it from the worst of the particle winds, but the intense far-ultraviolet radiation of the young Sun must have had important photochemical effects, perhaps producing or destroying molecules involved with the origin of life. Mars was protected by a magnetic field for a while and then lost it, which may be why it lost most of its atmosphere.






