 |
 |
(617) 495-7462
Christine Pulliam
(617) 495-7463
pubaffairs@cfa
Release No.: 2005-17For Release: Tuesday, June 14, 2005
SMA Confirms Proto-Planetary Systems are Common in the Galaxy
SMA Confirms Proto-Planetary Systems are Common in the Galaxy
In this artist rendering, the proplyds appear as rapidly spinning stars surrounded by a dust disk around the middle and two stellar jets extending from the poles. Nestled inside a cocoon of gas, these jets slow down the angular momentum of the spinning star so that eventually, planets may form.
Credit: David Aguilar, CfA
High Resolution Image (jpg)
Low Resolution Image (jpg)
Credit: David Aguilar, CfA
High Resolution Image (jpg)
Low Resolution Image (jpg)
A Hubble Space Telescope view of a small portion of the Orion Nebula reveals five young stars. Four of the stars are surrounded by protoplanetary disks, or "proplyds," of gas and dust. These disks might evolve into solar systems like our own.
Credit: C.R. O'Dell/Rice University; NASA
Low Resolution Image (jpg)
Credit: C.R. O'Dell/Rice University; NASA
Low Resolution Image (jpg)
These are Hubble Space Telescope images of four newly discovered protoplanetary disks around young stars in the Orion nebula, located 1,500 light-years away. The red glow in the center of each disk is a young, newly formed star, roughly one million years old. Each image is 167 billion miles across (30 times the diameter of our own solar system). The disks range in size from two to eight times the diameter of our solar system.
Credit: M. McCaughrean (Max Planck Institute for Astronomy), C.R. O'Dell (Rice University), and NASA
Low Resolution Image (jpg)
Credit: M. McCaughrean (Max Planck Institute for Astronomy), C.R. O'Dell (Rice University), and NASA
Low Resolution Image (jpg)
|
