Ghost Light from Dead Galaxies Sheds Light on Ancient Galaxy Interactions

Ghost Light from Dead Galaxies Sheds Light on Ancient Galaxy Interactions Did you know that astronomers can learn about galaxies that died long ago? Thats part of the story of the cosmos that the  deep cosmos-gazing  Hubble Space Telescope  was built to tell. Along with other telescopes on the ground and on orbit, it fills in the story of the universe as it peers out at distant objects. Some of its most fascinating objects are galaxies, including some that formed in the infancy of the universe and are now long gone from the cosmic scene. What stories do they tell?   What Hubble Found Studying long-dead galaxies sounds like it would be impossible. In a way, it is. Theyre no longer around, but it turns out, some of their stars are. To learn more about early galaxies that no longer exist, Hubble observed dim  light from orphaned stars that lie some 4 billion light-years away from us. They were born billions of years ago and somehow were ejected at high speed from their original galaxies, which themselves are long gone. It turns out some kind of galactic mayhem sent these stars reeling across space. They belonged to a galaxies in a massive galaxy called Pandoras Cluster. The light from those far-flung stars provided clues to a crime scene of truly galactic proportions: as many as six galaxies were somehow torn to pieces within the cluster. How could this happen? Gravity Explains a Lot Each galaxy has a gravitational pull. Its the combined gravity of all the stars, clouds of gas and dust, black holes, and dark matter that exist in the galaxy.  In a cluster, you get the combined gravitational pull of all the galaxies, and that affects all of the members of the cluster. That gravity is pretty strong. In addition, galaxies tend to move around within their clusters, which affects the motions and interacts of their cluster-mates. Add those two effects together and you set the scene  for the destruction of some not-so-lucky small galaxies that happen to get caught in the action.  They get stuck in a squeeze play between their larger neighbors as they travel, Eventually, the strong gravity of the bigger galaxies pulls the smaller ones apart.   Astronomers found clues to this destructive shredding of galaxies by studying the light from stars scattered by the action.That light would be detectable long after the galaxies were destroyed. However, this predicted intracluster glow of stars is very faint and is quite a challenge to observe.These are extremely faint stars and they are brightest in infrared wavelengths of light. This is where Hubble comes in. It has very sensitive detectors to capture that faint glow from the stars. Its observations helped scientists study the combined light of about 200 billion stars that were cast out from interacting galaxies. Its measurements showed that the scattered stars are rich in heavier elements like oxygen, carbon, and nitrogen. This means they are not the first-ever stars formed. The first stars consisted mainly of hydrogen and helium, and forged heavier elements in their cores. When those earliest ones died, all the elements were cast into space and into nebulae of gas and dust. Later generations of stars formed from those clouds and show higher concentrations of heavy elements. It is the enriched stars that Hubble studied in an effort to track what happened to their galactic homes.   Future Studies Zero in on More Orphan Stars Theres still a lot to figure out about the earliest, most distant galaxies and their interactions. Everywhere Hubble looks, it finds more and more distant galaxies. The farther out it  peers, the further back in time it looks. Each time it makes a deep field observation, this telescope shows astronomers fascinating things about the earliest times in the cosmos. Thats all part of the study of cosmology, the origin and evolution of the universe.