Illustration of a ring formed by planets around nearby star Fomalhaut.

Fomalhaut Disk Art with Labels

An artist’s conception of the disk of material in orbit around star Fomalhaut. Two planets shepherd the dust into a tight ring.

Illustration of two planets in protoplanetary disk feeding a young star.

Baby Planets Feed Their Mother Star

In this artist’s interpretation, baby planets forming around the young star HD 142527 are pulling streams of gas inward toward them as they grow. Much of the gas then overshoots the planets and continues inward to the portion of the disk close to the star, where it can eventually fall onto the star itself.

Illustration of the life cycle of massive stars.

Seeding Planets with Interesting Chemistry

The most massive stars in a cluster of stars have a tremendous impact on the formation and environment of the rest of the cluster, including the less-massive stars and their planets. The massive young stars are surrounded by “hot cores” that include copious organic material that later may be spewed into interstellar space by stellar winds and other processes. This can help “seed” star-forming regions with some of the chemicals found by the Green Bank Telescope (GBT) and other telescopes.

Diagram of the parallax technique, showing the Earth in different positions with respect to the sun at different times of years, and the subsequently different place on the sky that the Pleiades appears.
Artist impression of galaxy at the center of the Phoenix Cluster

The Center of the Phoenix Cluster

Artist impression of galaxy at the center of the Phoenix Cluster. Powerful radio jets from the supermassive black hole at the center of the galaxy are creating giant radio bubbles (blue) in the ionized gas surrounding the galaxy. ALMA has detected cold molecular gas (red) hugging the outside of the bubbles. This material could eventually fall into the galaxy where it could fuel future star birth and feed the supermassive black hole.

Artist's conception of particle acceleration in a solar flare.