Printer Friendly
The Free Library
14,799,441 articles and books
Member login
User name  
Password 
 
Join us Forgot password?

Hubble eyes the Cartwheel.


Millions of years ago, a small, energetic galaxy plowed through the core of a large, quiescent quiescent

at rest; latent; the G0 stage of the cell cycle.
 one. Luckily for astronomers, this changed the dormant galaxy in dramatic fashion.

Like a pebble cast into a pond, the tiny intruder An attacker that gains, or tries to gain, unauthorized access to a system. See attacker, intrusion and IDS.  generated a ripple of energy that expanded outward from the center of the big galaxy. Traveling at about 320,000 kilometers per hour, the wave compressed gas and dust in front of it and ignited rings of star birth in its wake. This process has so far lasted for some 200 million years. At the forefront of the wave lies the bluest, newest batch of stars; closer to the core reside redder, older stars.

That's how astronomers believe the Cartwheel, a striking, ring-shaped galaxy complete with spokes and a brilliant, bulls-eye core, got its shape (SN: 4/18/92, p.248). Images recently taken by the Hubble Space Telescope Hubble Space Telescope (HST), the first large optical orbiting observatory. Built from 1978 to 1990 at a cost of $1.5 billion, the HST (named for astronomer E. P. Hubble) was expected to provide the clearest view yet obtained of the universe.  depict with unprecedented clarity the Cartwheel's highly organized structure. The pictures also provide new clues to what the Cartwheel, located 500 million light-years from Earth, may have looked like before the fateful collision.

Hubble's pictures reveal hundreds of bright blue knots -- individual clusters of newborn stars -- that the expanding wave generated. Huge loops and bubbles indicate where massive stars, also formed in the aftermath of the collision, exploded as supernovas, hurling hurling, outdoor ball and stick game similar to field hockey (see hockey, field). The national pastime of Ireland, it was played for many centuries before the Gaelic Athletic Association standardized the rules in 1884.  their contents into space. In addition, the images show in new detail the galaxy's true colors -- its red center and blue outskirts -- notes Kirk D. Borne of the Space Telescope Science Institute The Space Telescope Science Institute (STScI) is the science operations center for the Hubble Space Telescope (HST; in orbit since 1990) and for the James Webb Space Telescope (JWST; scheduled to be launched in 2013).  in Baltimore.

"This is a chronometer chronometer (krənŏm`ətər), instrument for keeping highly accurate time, used especially in navigation. Before the advent of radio time signals it was the only device that provided the time accurately enough for a ship at sea to  on the galactic ga·lac·tic
adj.
1. Relating to milk.

2. Promoting the flow of milk.



galactic

1. pertaining to milk.

2. galactagogue.
 scale," he says. "We see old and new stars separated in space."

Borne and his collaborators note that the galaxy's interior contains so little dust that Hubble's wide-field and planetary camera saw right through it, imaging a more distant galaxy that lies directly behind the Cartwheel.

This lack of dust suggests that before the collision, the Cartwheel was merely an immense cloud of hydrogen gas or a galaxy with a very low density of stars. If so, the collision awoke a sleeping giant Sleeping Giant may refer to:

In geology:
  • Sleeping Giant (Connecticut), trap rock ridge system located in the Mount Carmel neighborhood of Hamden, Connecticut
, setting the Cartwheel ablaze with stars millions of years before the galaxy would otherwise have created them. "We see no evidence for a pristine population of stars underlying the pattern [of those generated by the interloper]," says Borne.

Although scientists had hoped the Hubble images might unveil the identity of the intruding galaxy, the pictures haven't narrowed the list of suspects. The lower of the two small galaxies to the right of the Cartwheel appears distorted and recently experienced a burst of star formation, features that make it a likely candidate. On the other hand, the top galaxy contains little gas, so the missing material may have been stripped as this galaxy passed through the Cartwheel.

A third galaxy, not shown in the accompanying image, also go remains a suspect.
COPYRIGHT 1995 Science Service, Inc.
No portion of this article can be reproduced without the express written permission from the copyright holder.
Copyright 1995, Gale Group. All rights reserved. Gale Group is a Thomson Corporation Company.

 Reader Opinion

Title:

Comment:



 

Article Details
Printer friendly Cite/link Email Feedback
Title Annotation:Hubble Space Telescope images the ring-shaped galaxy Cartwheel
Author:Cowen, Ron
Publication:Science News
Article Type:Brief Article
Date:Jan 21, 1995
Words:472
Previous Article:A glass melange: new options for hazardous waste? (vitrification of toxic wastes)
Next Article:Homosexual parents: all in the family. (emotional development of children of homosexual parents)
Topics:



Related Articles
Within a galaxy and outside a supernova.
Orbiting Hubble eyes active galaxy's disk. (Hubble Space Telescope)
Hubble eyes the shape of distant galaxies. (Hubble Space Telescope's wide-field and planetary camera) (Brief Article)
Fooled by gravity. (gravitational lense made galaxy FSC 10214+4724 appear brighter than it actually is)(Brief Article)
Hubble's deep view of the universe. (Hubble Space Telescope views one site for 10 days)(Science News of the Week)
Distant galaxies dazzle in the infrared. (Infrared Space Observatory detects supergalaxies that were birthplaces of stars)(Brief Article)
After Hubble: the Next Generation: probing the final frontier.(plans for Next Generation Space Telescope)
Dust buster eyes fireworks in nearby galaxy.(images from Hubble Space Telescope show inner disk-shaped galaxy in Centaurus A)(Brief Article)
Hubble gets multiple views of distant galaxy.(Brief Article)
Image reveals galaxy's violent past. (Starry View).(Andromdeda)

Terms of use | Copyright © 2010 Farlex, Inc. | Feedback | For webmasters | Submit articles