This radar image of 2007 TU24 was obtained on 28 January 2008
This radar image of 2007 TU24 was obtained on 28 January 2008, about 12 hours before the asteroid's 1.4-lunar-distance pass by the Earth. The Arecibo Observatory in Puerto Rico and the Greenbank Telescope in West Virginia were used to take this image. (c) NASA/JPL
Where am I? > Home > News > Astronomy

Asteroid 2007 TU24 zooms by Earth

Science Centric | 30 January 2008 09:28 GMT
Printable version A clip for your blog or website E-mail the story to a friend
Bookmark or share the story on your social network Vote for this article Leave a comment Decrease text size Increase text size
DON'T MISS —
Ghostly 'spokes' puff out from Saturn's ring's
Ghostly 'spokes' puff out from Saturn's ring's — [15 Nov 2009] — Massive, bright clouds of tiny ice particles hover above the darkened rings of Saturn in an image captured by the Cassini...
Exoplanets clue to sun's curious chemistry
Exoplanets clue to sun's curious chemistry — [12 Nov 2009] — 'For almost 10 years we have tried to find out what distinguishes stars with planetary systems from their barren cousins,'...
Opening up a colourful cosmic jewel box
Opening up a colourful cosmic jewel box — [29 Oct 2009] — Star clusters are among the most visually alluring and astrophysically fascinating objects in the sky. One of the most spectacular...
32 new exoplanets found
32 new exoplanets found — [20 Oct 2009] — 'HARPS is a unique, extremely high precision instrument that is ideal for discovering alien worlds,' says Stephane Udry,...
More Astronomy...

As expected, asteroid 2007 TU24 made its closest approach to Earth at 12:33 AM yesterday, 29 January, and is now headed away from our planet. At its closest point, the asteroid was 554,209 kilometres (344,370 miles) from Earth, or roughly 1.4 times the distance between the moon and Earth.

Scientists at NASA's Jet Propulsion Laboratory in Pasadena, Calif. had tracked the asteroid in advance and determined that there was no possibility of an impact. The rare close approach is providing a bonanza for scientists, who plan to scrutinise images and data gathered in hopes of learning more about our solar system's closest neighbours - near-Earth asteroids. More observations are planned for 1 February through 4 using the Arecibo Observatory in Puerto Rico. The observatory is operated by Cornell University, Ithaca, N.Y., for the National Science Foundation.

Source: Jet Propulsion Laboratory, NASA

This image shows an artist's conception of the bubble around our solar system moving through the interstellar medium, the matter that fills the local region of our galaxy. New observations from the Cassini spacecraft orbiting Saturn suggest the shape resembles something like a slippery ball moving through smoke, (c) NASA/JPL-Caltech/JHUAPLCassini data help redraw shape of solar system

— 16 October 2009

Images from the Ion and Neutral Camera on NASA's Cassini spacecraft suggest that the heliosphere, the region of the sun's influence, may not have the comet-like shape predicted by existing... — full story

Astronomers obtained this portrait of Barnard's Galaxy using the Wide Field Imager attached to the 2.2-metre MPG/ESO telescope at ESO's La Silla Observatory in northern Chile. Also known as NGC 6822, this dwarf irregular galaxy is one of the Milky Way's galactic neighbours. The dwarf galaxy has no shortage of stellar splendour and pyrotechnics. Reddish nebulae in this image reveal regions of active star formation, wherein young, hot stars heat up nearby gas clouds. Also prominent in the upper left of this new image is a striking bubble-shaped nebula. At the nebula's centre, a clutch of massive, scorching stars send waves of matter smashing into surrounding interstellar material, generating a glowing structure that appears ring-like from our perspective. Other similar ripples of heated matter thrown out by feisty young stars are dotted across Barnard's Galaxy, (c) ESOThe Milky Way's tiny but tough galactic neighbour

— 14 October 2009

In the new ESO image, Barnard's Galaxy glows beneath a sea of foreground stars in the direction of the constellation of Sagittarius (the Archer). At the relatively close distance of... — full story

Not surprisingly, interacting galaxies have a dramatic effect on each other. Studies have revealed that as galaxies approach one another massive amounts of gas are pulled from each galaxy towards the centre of the other, until ultimately, the two merge into one massive galaxy. NGC 2623 is in the late stages of the merging process, with the centres of the original galaxy pair now merged into one nucleus, but stretching out from the centre are two tidal tails of young stars, a strong indicator that a merger has taken place. During such a collision, the dramatic exchange of mass and gases initiates star formation, seen here in both the tails. The prominent lower tail is richly populated with bright star clusters - 100 of them have been found in these observations. These star clusters may have formed as part of a loop of stretched material associated with the northern tail, or they may have formed from debris falling back onto the nucleus. In addition to this active star-forming region, both galactic arms harbour very young stars in the early stages of their evolutionary journey, (c) NASA, ESA and A. Evans (Stony Brook University, New York)Sky merger yields sparkling dividends

— 13 October 2009

A recent NASA/ESA Hubble Space Telescope image captures what appears to be one very bright and bizarre galaxy, but is actually the result of a pair of spiral galaxies that resemble... — full story

This artist's conception shows a nearly invisible ring around Saturn - the largest of the giant planet's many rings. It was discovered by NASA's Spitzer Space Telescope, (c) NASA, JPL-Caltech, KeckSpitzer discovers an enormous ring around Saturn

— 8 October 2009

NASA's Spitzer Space Telescope has discovered an enormous ring around Saturn - by far the largest of the giant planet's many rings. The new belt lies at the far reaches of the Saturnian... — full story


Popular tags in Astronomy: Cassini · galaxies · Hubble · Mars