A frEGGS-plosion of Star Formation | Hubble
When a massive new star starts to shine while still within the cool molecular cloud from which it formed, its energetic radiation can ionize the cloud’s hydrogen and create a large, hot bubble of ionized gas. Amazingly, located within this bubble of hot gas around a nearby massive star are the frEGGs: dark compact globules of dust and gas, some of which are giving birth to low-mass stars. The boundary between the cool, dusty frEGG and the hot gas bubble is seen as the glowing purple/blue edges in this fascinating image.
Credit: European Space Agency (ESA)/Hubble & NASA, R. Sahai
Release Date: October 12, 2020
#NASA #ESA #Astronomy #Space #Hubble #StarFormation #StellarNursery #J0250277600849 #Nebulae #Globules #Cassiopeia #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education
No comments:
Post a Comment