Keplerian rotation tagged posts

Last year, the Dawn spacecraft spied organic material near Ernutet crater on the dwarf planet Ceres, largest denizen of the asteroid belt. A new analysis suggests those organics could be more plentiful than originally thought. Credit: NASA / Hannah Kaplan

New technique could find some of the youngest planets in our galaxy. Two independent teams of astronomers have uncovered convincing evidence that three young planets are in orbit around an infant star known as HD 163296. Using a new planet-finding strategy, the astronomers identified 3 discrete disturbances in a young star’s gas-filled disk: the strongest evidence yet that newly formed planets are in orbit there.

Over the past several years, ALMA has transformed our understanding of protoplanetary disks – the gas- and dust-filled planet f...

Artist’s impression of the baby star TMC-1A. The star is located in the center and surrounded by a rotating gas disk. Gas is infalling to the disk from the envelope further out. Credit: Image courtesy of National Astronomical Observatory of Japan

The first direct observations delineating the gas disk around a baby star from the infalling gas envelope has been made. This finding fills an important missing piece in our understanding of the early phases of stellar evolution. The baby star TMC-1A is 450 light years away in the constellation Taurus. TMC-1A is a protostar, a star still in the process of forming. Large amounts of gas still surround TMC-1A.

Stars form in dense gas clouds. Baby stars grow by taking in the surrounding gas. In this process, gas cannot flow directly into the star...