University of California, Berkeley | 2017 Jun 13
[img3="Radio image of a very young binary star system, less than about 1 millionDid our sun have a twin when it was born 4.5 billion years ago?
years old, that formed within a dense core (oval outline) in the Perseus
molecular cloud. All stars likely form as binaries within dense cores.
SCUBA-2 survey image by Sarah Sadavoy, CfA."]https://news.berkeley.edu/wp-content/up ... _5_350.jpg[/img3][hr][/hr]
Almost certainly yes — though not an identical twin. And so did every other sunlike star in the universe, according to a new analysis by a theoretical physicist from the University of California, Berkeley, and a radio astronomer from the Smithsonian Astrophysical Observatory at Harvard University.
Many stars have companions, including our nearest neighbor, Alpha Centauri, a triplet system. Astronomers have long sought an explanation. Are binary and triplet star systems born that way? Did one star capture another? Do binary stars sometimes split up and become single stars?
Astonomers have even searched for a companion to our sun, a star dubbed Nemesis because it was supposed to have kicked an asteroid into Earth’s orbit that collided with our planet and exterminated the dinosaurs. It has never been found.
The new assertion is based on a radio survey of a giant molecular cloud filled with recently formed stars in the constellation Perseus, and a mathematical model that can explain the Perseus observations only if all sunlike stars are born with a companion. ...
Embedded Binaries and Their Dense Cores - Sarah I. Sadavoy, Steven W. Stahler
- Monthly Notices of the RAS 469(4):3881 (Aug 2017) DOI: 10.1093/mnras/stx1061
arXiv.org > astro-ph > arXiv:1705.00049 > 28 Apr 2017