Washington, July 2 (ANI): Two University of Hawaii astronomers have found a binary star-disk system in which each star is surrounded by the kind of dust disk that is frequently the precursor of a planetary system, which makes them solar systems in the making.
The astronomers in question are doctoral student Rita Mann and Dr. Jonathan Williams, who used the Submillimeter Array on Mauna Kea, Hawaii, to make the observations.
A binary star system consists of two stars bound together by gravity that orbit a common center of gravity.
Most stars form as binaries, and if both stars are hospitable to planet formation, it increases the likelihood that scientists will discover Earth-like planets.
This binary system, 253-1536, stands out as the first known example of two optically visible stars, each surrounded by a disk with enough mass to form a planetary system like our own.
It lies 1,300 light-years from Earth, in the famous Orion Nebula, the kind of rich cluster of stars that is a common birth environment for most stars in our Milky Way galaxy, including our Sun.
One of the disks was discovered in an image taken with the Hubble Space Telescope, but the other disk was hidden in the glare of the star.
Hubble saw only the disk shadow, so the amount of material and its capability for planet formation was unknown until the UH team made the SMA observations.
The two stars are 400 times farther from each other than Earth is from the Sun.
They would take 4,500 years, or about the length of human recorded history, to complete one orbit around their common center.
Both stars are only about a third the mass of our Sun and are much cooler and redder in color.
The larger disk in 253-1536 is also the most massive found in the Orion Nebula so far.
The discovery of this massive disk and the binary disk system improve our understanding of how common planet formation is in our Galaxy and place our Solar System in context. (ANI)