The star system V664 Cassiopeia is leaving "bread crumbs" as it races through the galaxy: a trail of gas and dust that may span several light-years. The system consists of two stars in a very tight orbit. One of the stars recently blew its outer layers into space, and the motion of the companion star kicked the material farther into space, forming a colorful bubble around the system. Some of the material piles up in front of the stars like water in front of a ship. [T.A. Rector (Univ. Alaska Anchorage)/H. Schweiker (WIYN/NOAO/AURA/NSF)]
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V664 Cassiopeia is complicated. It consists of two stars that are so close together they’re almost touching. It’s ramming into clouds of gas and dust like a cosmic fist. And it’s leaving behind a trail of breadcrumbs that may span several light-years.
The system is in Cassiopeia, the queen, which is low in the north-northeast at nightfall right now. V664 is to the left of the “W” formed by Cassiopeia’s brightest stars, although it’s too faint to see with the eye alone.
But a telescope sees a remarkable sight — a structure that looks something like a jellyfish squirting across the sky, or perhaps a fist jabbing a pool of water.
The system consists of a “dead” star known as a white dwarf, plus a second star that resembles the Sun. Not long ago, the white dwarf was also a “normal” star like the Sun. But it puffed up to giant proportions, engulfing its companion.
As the companion swirled through the star’s outer layers, it stole some of the hot gas for its own, but kicked most of the gas away, forming a colorful bubble around the two stars.
The system is moving fast, so the bubble piles up material in front of it like water in front of a ship. At the same time, some of the gas in the bubble gets left behind like a trail of breadcrumbs. The system has been leaving that trail for a hundred thousand years, so the trail could stretch across several light-years.
And V664 Cas is likely to get a lot more interesting. More about that tomorrow.
Script by Damond Benningfield, Copyright 2015