Hubble's Constant And The Expanding Universe (II)
Explanation:
In this century, the discovery that the Universe is
expanding has produced a revolution in
human thought about the Cosmos.
American astronomer
Edwin Hubble
played a major role in this profound discovery, coining
the "Hubble constant". This single number describes the rate of the cosmic
expansion, relating the apparent recession velocities of external galaxies to
their distance.
Two groups of astronomers
trying to measure this fundamental constant
using the Hubble Space Telescope (HST) are continuing to report
conflicting results.
One group, led by astronomer Allan Sandage,
measures distances to galaxies using pulsating
Cepheid variable stars and
supernovae observed in galaxies like the
Virgo Cluster spiral galaxy, NGC4639, shown above. This galaxy
is the most distant one to which Cepheid-based determinations have been made
and was also the site of a well-studied 1990 supernova.
Their results favor a relatively small Hubble constant (slow expansion rate)
of about 55 kilometers per second per megaparsec which means that galaxies
one megaparsec (3 million lightyears) distant appear to recede from
us at a speed of 55 kilometers per second.
A substantially faster expansion rate (larger Hubble constant)
is being reported by astronomer Wendy Freedman and collaborators, also
based on HST data.
The value of Hubble's constant was recently the subject of a popular
public debate titled
"The Scale of the Universe 1996: The Value of Hubble's Constant".
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
