NGC 4762

ngc 4762This is a disk galaxy seen almost perfectly edge on. The image from the Hubble Space Telescope shows us just how thin disk galaxies can be. NGC 4762, a galaxy in the nearby Virgo Cluster of Galaxies, is so thin that it is actually difficult to determine what type of disk galaxy it is. Its lack of a visible dust lane suggests that it is probably a low-dust lenticular galaxy, but it is still possible that a view from another angle would reveal spiral structure. The galaxy spans about 100,000 light years from end to end, with its center showing a slight bulge of stars. Most galaxies don’t appear this thin because our point of view from Earth doesn’t line up well enough with the planes of their thin galactic disks. However, galaxies this thin are common. Indeed, our own Milky Way Galaxy is thought to have roughly the same overall dimensions as NGC 4762.

Image Credit: NASA / ESA

The Cone Nebula

Cone NebulaThe cone’s shape comes from a dark absorption nebula consisting of cold molecular hydrogen and dust in front of a faint emission nebula containing hydrogen ionized by S Monocerotis, the brightest star of NGC 2264. The faint nebula is approximately 2,700 light-years from Earth.

Beldar was unavailable to confirm that this is the correct location for his home planet Remulak.

Image Credit: NASA

The Eye of Jupiter

jupitereye_0Not really. The trick is that the planet seems to be looking back at us because Hubble happened to catch the shadow of Ganymede, Jupiter’s largest moon, as it moved across the Giant Red Spot. Hubble was monitoring changes in that huge storm last April when the moon’s shadow moved across the center of the storm. For a moment, Jupiter became Cyclops.

Image Credit: NASA

Blue Whisps

Turquoise-tinted plumes in the Large Magellanic CloudThis Hubble image shows part of the outskirts of the Tarantula Nebula in the Large Magellanic Cloud. The colors seen in this picture are different from what we normally see in the images of the Large Magellanic Cloud  because an unusual set of filters was used. The customary R filter, which passes red light, was replaced by a filter letting through the near-infrared light. Hydrogen gas normally appears pink because it shines most brightly in the red. In this case, however, other less prominent emission lines dominate in the blue and green filters.

Image Credit: NASA

NGC 3310

NGC 3310NGC 3310 is a grand design spiral galaxy in the constellation Ursa Major. It is also a starburst galaxy. (Starburst galaxies are undergoing an exceptionally high rate of star formation.) NGC 3310 probably collided with one of its satellite galaxies about 100 million years ago, triggering widespread star formation. The ring clusters of NGC 3310 have been undergoing starburst activity for at least the last 40 million years.

Image Credit: NASA