Hubble Spies Curious Galaxy Moving a Little Closer
This Hubble image stars Messier 90, a beautiful spiral galaxy located roughly 60 million light-years from the Milky Way in the constellation of Virgo (the Virgin). The galaxy is part of the Virgo Cluster, a gathering of galaxies that is over 1,200 strong.
Chandra :: Photo Album :: SN 1006 :: July 01, 2008
Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world.
Chandra :: Photo Album :: G292.0+1.8 :: October 23, 2007
The aftermath of the death of a massive star is shown in beautiful detail in this composite image of G292.0+1.8. In color is the Chandra X-ray Observatory image - easily the deepest X-ray image ever obtained of this supernova remnant - and in white is optical data from the Digitized Sky Survey. Although considered a "textbook" case of a supernova remnant, the intricate structure shown here reveals a few surprises.
Chandra :: Photo Album :: N132D :: 04 Oct 05
This beautiful image shows a glowing horseshoe-shaped cloud of hot gas against a backdrop of thousands of stars in the Large Magellanic Cloud, a nearby galaxy. Observations with Chandra (X-ray/blue) and Hubble (optical/pink & purple) were used to make this composite image of N132D, a supernova remnant that was produced by the explosion of a massive star.
Chandra :: Photo Album :: NGC 6543 :: July 30, 2008
This composite of data from NASA's Chandra X-ray Observatory and Hubble Space Telescope is a new look for NGC 6543, better known as the Cat's Eye nebula. This famous object is a so-called planetary nebula that represents a phase of stellar evolution that the Sun should experience several billion years from now.
Chandra :: Photo Album :: G352.7-0.1 :: April 10, 2014
Supernova remnants are created when a massive star explodes and its remains are hurled into space. Astronomers have found a supernova remnant that it is sweeping up a remarkable amount of material—equivalent to 45 times the mass of the Sun—as it expands. This supernova remnant is called G352.7-0.1 and is seen in this composite image containing X-rays from Chandra (blue), radio waves from the VLA (pink), infrared data from Spitzer (orange), and optical data from the DSS (white).