NASA's Hubble Space Telescope has provided astronomers with what may be their first direct view of an immense ring of dust which fuels a massive black hole at the heart of the spiral galaxy M51, located 20 million light-years away. Surprisingly, they found that the ring is standing almost perpendicularly to the relatively flat spiral galaxy, like a top spinning on its side with respect to the floor. Even more surprising is the discovery of a secondary ring or dust lane which is contrary to all expectations.

NASA's Hubble Space Telescope (HST) has revealed a new class of object in the universe -- a grouping of gigantic star clusters produced by the collision of galaxies. Images of the core of the peculiar galaxy Arp 220 show that stars are produced at a furious rate from the dust and gas supplied by the interaction of two galaxies.

Imagine turning your home computer into the equivalent of a professional telescope which can display millions of stars and galaxies located anywhere in the sky.. Astronomers as well as educators will soon be able to have the sky at their fingertips thanks to an ambitious effort now being funded by NASA and being carried out by the Space Telescope Science Institute (STScI) in Baltimore, Maryland.

NASA's Hubble Space Telescope has revealed an unusual and fascinating new optical jet in the nucleus of the elliptical galaxy NOC 3862.

Astronomers report that they have found new evidence that a black hole weighing 3 million times the mass of the Sun exists at the center of the nearby elliptical galaxy M32, based on images obtained with NASA's Hubble Space Telescope (HST). The images show that the stars in M32 become extremely concentrated toward the nucleus. This central structure resembles the gravitational "signature" of a massive black hole. The presence of a black hole in an ordinary galaxy like M32 may mean that inactive black holes are common to the centers of galaxies. The new HST images show that M32 is an interesting... Read more

The NASA Hubble Space Telescope (HST) has imaged N66, a planetary nebula in the Large Magellanic Cloud (a satellite galaxy of our own Milky Way galaxy). The image was obtained at 10:41 p.m. EDT on June 26, 1991, using the European Space Agency's Faint Object Camera.

The image at top right shows Jovian aurora observed on February 8, 1992, by the European Space Agency's Faint Object Camera (FOC) aboard NASA's Hubble Space Telescope (HST). This is the first direct image of the aurora taken in ultraviolet light (1600 Angstroms) and the best auroral images ever. An earlier image of Jupiter's full disk (lower left), obtained by HST's Wide Field/Planetary Camera, shows the location of the northern aurora (box) with respect to the rest of the planet.

This photograph from the NASA Hubble Space Telescope presents the first clear view of one of the hottest known stars, the central star of nebula NGC 2440 in our Milky Way galaxy. The superhot star, called "the NGC 2440 nucleus" is the bright white dot in the center of this photograph.

A new image processing technique has yielded the clearest view yet of an extraordinary star cluster located about 169,000 light years from Earth. The new technique, called photometric reconstruction, was applied to a photograph of the star cluster Rl36 that was obtained with the Planetary Camera onboard the NASA Hubble Space Telescope. It reveals that there are at least 47 stars located within an area 1.6 light years across in Rl36. (One light year is approximately 5.8 trillion miles long.) In contrast, the Sun is about 4 light years from the nearest known star, Proxima Centauri.

A NASA Hubble Space Telescope (HST) view of a 4,000 light-year long jet of plasma emanating from the bright nucleus of the giant elliptical galaxy M87. This ultraviolet light image was made with the European Space Agency's Faint Object Camera (FOC), one of two imaging systems aboard HST.