A Baby Solar System Found by Hubble?
March 8, 2018
Credits: NASA/ESA/G. Schneider (Univ. of Arizona)
Hubble Et al. (see below): Astronomers have used NASAs Hubble Space Telescope to uncover a vast, complex dust structure, about 150 billion miles across, enveloping the young star HR 4796A. A bright, narrow, inner ring of dust is already known to encircle the star and may have been +69corralled by the gravitational pull of an unseen giant planet. This newly discovered huge structure around the system may have implications for what this yet-unseen planetary system looks like around the 8-million-year-old star, which is in its formative years of planet construction.
The debris field of very fine dust was likely created from collisions among developing infant planets near the star, evidenced by a bright ring of dusty debris seen 7 billion miles from the star. The pressure of starlight from the star, which is 23 times more luminous than the Sun, then expelled the dust far into space.
But the dynamics dont stop there. The puffy outer dust structure is like a donut-shaped inner tube that got hit by a truck. It is much more extended in one direction than in the other and so looks squashed on one side even after accounting for its inclined projection on the sky. This may be due to the motion of the host star plowing through the interstellar medium, like the bow wave from a boat crossing a lake. Or it may be influenced by a tidal tug from the stars red dwarf binary companion (HR 4796B), located at least 54 billion miles from the primary star.
The dust distribution is a telltale sign of how dynamically interactive the inner system containing the ring is, said Glenn Schneider of the University of Arizona, Tucson, who used Hubbles Space Telescope Imaging Spectrograph (STIS) to probe and map the small dust particles in the outer reaches of the HR 4796A system, a survey that only Hubbles sensitivity can accomplish.
More:
http://nineplanets.org/news/a-baby-solar-system-found-by-hubble/