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Conference 7.286::space

Title:Space Exploration
Notice:Shuttle launch schedules, see Note 6
Moderator:PRAGMA::GRIFFIN
Created:Mon Feb 17 1986
Last Modified:Thu Jun 05 1997
Last Successful Update:Fri Jun 06 1997
Number of topics:974
Total number of notes:18843

739.0. "IRAS reveals most luminous object ever seen in space" by PRAGMA::GRIFFIN (Dave Griffin) Fri Jun 28 1991 14:00

RELEASE:  91-98    (6/27/91)


     Astronomers studying very faint objects originally detected by
the Infrared Astronomical Satellite (IRAS) have discovered a new,
very distant object which they say is the most luminous object ever
seen in the universe.

     The observations, published today in the British science
journal Nature, show that this luminous object is a massive dust
cloud which radiates 99 percent of its light in the infrared part
of the spectrum.

     The team of astronomers believe that this mysterious cloud may
be a massive galaxy in the process of formation -- or,
alternatively, a quasar embedded in the dust of a massive galaxy.

     Infrared light -- or, more simply, heat radiation --  is
invisible to the human eye but can be detected by electronic
sensors such as those on the IRAS satellite.  IRAS discovered
hundreds of thousands of infrared objects that astronomers are now
observing more closely in order to determine what they are.  Often
these sources turn out to be dusty objects, because dust particles
are very efficient emitters of
infrared radiation.

    Astronomers define the luminosity of an object as  the total
amount of energy emitted at all wavelengths.  The luminosity of
this newly found object is an incredible 300 trillion times that of
the sun, or 30,000 times that of the entire Milky Way galaxy, which
itself consists of hundreds of billions of stars like the sun.
This tremendous energy output is greater even than the most
luminous known quasars, which were discovered in visible or
ultraviolet light.  Quasars are thought to derive their immense
power from the presence of massive black holes in their centers.

     Unlike typical quasars, this new source is emitting most of
its light in the infrared region of the electromagnetic spectrum.
The dust cloud, which the team believes is responsible for the far-
infrared radiation, has a mass of between 400 million and 1 billion
times that of the sun.  The lower figure exceeds the mass of
interstellar dust in any previously known galaxy. The higher figure
is comparable to the whole mass of heavy elements in the Milky Way
Galaxy, most of which today is locked up in stars.

     The object, in the constellation of Ursa Major, is
approximately 16 billion light-years from Earth.  When astronomers
study distant objects they are essentially looking back in time.
In this case the object is seen as it was 16 billion years ago, or
more than 80 percent of the way back in time to when the universe
is thought to have originated in the Big Bang.

     The team of astronomers, from four British universities and
two U.S. institutions, is led by Professor Michael Rowan-Robinson
of Queen Mary and Westfield College, London.  The team first
observed the mystery object as part of a program to identify
infrared sources detected by IRAS.

     The luminous dust cloud was discovered when the team was
trying to locate a visible light counterpart for one of the new
faint IRAS sources (the luminous source appears faint due to its
tremendous distance from Earth) at the United Kingdom's 4.2-meter
(13.7-foot) William Herschel telescope in the Canary Islands.
Using a spectrometer, they were able to detect the signatures of
elements such as carbon and hydrogen in the faint mystery source.

     The redshift -- or shift of the characteristic element lines
towards the red end of the spectrum caused by the expansion of the
universe -- is 2.236, showing the object to be a very distant
galaxy.  (The universal expansion causes more distant parts of the
universe to appear to be receding from Earth more rapidly; thus,
the more distant  the object, the larger the measured redshift of
the spectral lines.)

     More detailed images and spectra were obtained later at
Caltech's 200-inch telescope at Palomar Observatory near San Diego
and the William Herschel Telescope.

      The powerhouse that heats the massive dust cloud and causes
it to glow so brightly in infrared light is hidden from view, but
the astronomers theorize that it may be due to about a billion
extremely hot, luminous young stars formed in the early stages of
the birth of a galaxy.  If their theory is correct, this discovery
marks the first time astronomers have witnessed the birth of a
galaxy.

     An alternate theory is that the powerhouse is itself a quasar,
more luminous than ever seen before, shrouded from our view by the
cloud of dust.  Astronomers from other observatories around the
world have begun to train their telescopes on the new object to
shed further light on how galaxies and quasars formed during the
early history of the universe.

    A joint mission between the United States, Netherlands and
United Kingdom, IRAS was launched by NASA in 1983.  For 10 months
it surveyed the entire sky, providing our first ever comprehensive
view of the universe at four different infrared wavelengths.

      In 1985 the U.S. Infrared Processing and Analysis Center
(IPAC), funded by NASA and based at the Jet Propulsion Laboratory
and the California Institute of Technology, produced a catalog of
sources detected by IRAS.  From 1985-1988 IPAC re-analyzed the
satellite data to produce a more sensitive catalog of infrared
sources.

     Joining Rowan-Robinson on the team of astronomers involved in
the discovery are Dr. Tom Broadhurst, Dr. Andy Lawrence, Seb Oliver
and Andy Taylor of Queen Mary and Westfield College, London; Dr.
Richard McMahon of the Institute of Astronomy, Cambridge, England;
Dr. Carol Lonsdale, Dr. Perry Hacking and Tim Conrow of the
JPL/Caltech Infrared Processing and Analysis Center (IPAC); Prof.
George Efstathiou and Dr. Will Saunders of  the University of
Oxford, England; Prof. Richard Ellis of University of Durham; and
Dr. Jim Condon of the National Radio Astronomy Observatory,
Charlottesville, Virginia.

     JPL's contributions to  the project, as well as the U.S.
T.RTitleUserPersonal
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739.1IRAS CD-ROMs availableVERGA::KLAESAll the Universe, or nothing!Thu Feb 27 1992 12:2248
Article: 388
From: [email protected] (Ron Baalke)
Newsgroups: sci.space.news
Subject: IRAS CD-ROMs Now Available
Date: 26 Feb 92 05:19:16 GMT
Sender: [email protected] (Usenet)
Organization: Jet Propulsion Laboratory
 
                           ====================
                               IRAS CD-ROMs
                             February 25, 1992
                           ====================
 
     The first release of the IRAS Sky Survey Atlas is now available to the
public on four CD-ROMs.  The Infrared Astronomical Satellite (IRAS) was
launched in 1983 into low Earth orbit to scan the entire sky in search of
infrared radiation from galaxies, dust clouds, stars, solar system objects,
and previously unknown objects.  From January to November 1983, IRAS conducted
a survey of 98% of the sky in four wavelengths centered at 12, 25, 60 and
100 microns.  IRAS was a joint mission between JPL, the United Kingdom and 
the Netherlands.
 
     The four CD-ROMs in this release covers the high ecliptic latitudes
from 50 to 90 degrees and from -50 to -90 degrees, which comprises 38% of the
sky.  The images on these CD-ROMs are 500x500 pixel resolution FITS images,
and consists of 16 bit and 32 bit images.  The images have been processed by
the Infrared Processing and Analysis Center (IPAC) at Caltech/JPL to improve
the calibration and to remove zodiacal emission.  The second set of CD-ROMs of
the IRAS Sky Survey which will cover the entire sky will be released later
this year.
 
     The IRAS CD-ROMs along with display software can be obtained from the 
National Space Science Data Center (NSSDC) for a small fee of $38.  You can
contact NSSDC at:
 
        National Space Science Data Center
	Goddard Space Flight Center
	Greenbelt, Maryland 20771
	Telephone: (301) 286-6695
        Email address:  [email protected]
 
     ___    _____     ___
    /_ /|  /____/ \  /_ /|     Ron Baalke         | [email protected]
    | | | |  __ \ /| | | |     Jet Propulsion Lab |
 ___| | | | |__) |/  | | |__   M/S 525-3684 Telos | In the middle of difficulty
/___| | | |  ___/    | |/__ /| Pasadena, CA 91109 | lies opportunity  --
|_____|/  |_|/       |_____|/                     | Albert Einstein

739.2Tenth anniversary of IRASVERGA::KLAESLife, the Universe, and EverythingTue Feb 09 1993 11:48102
From:	DECWRL::"[email protected]" "Ron Baalke" 30-JAN-1993 
To:	[email protected]
CC:	
Subj:	IRAS - 10 Years Ago

From the "JPL Universe"
January 29, 1993

IRAS: 10 years ago, infrared widened our eyes
By Mary Hardin

     Ten years ago this week, the launch of the Infrared
Astronomical Satellite (IRAS) made history as the first
spacecraft designed specifically to study the universe at
infrared wavelengths.

     "IRAS opened the entire Milky Way to our view, revealing
previously unsuspected phenomena and providing new probes of the
structure of the galaxy," said Dr. Charles Beichman, director of
JPL's Infrared Processing and Analysis Center (IPAC) and a member
of the IRAS science team.

     The satellite was an international project involving The
Netherlands, the United Kingdom and the United States, but its
early life was so full of problems it almost didn't get off the
ground. To begin with, the project was two years and tens of
millions of dollars over budget due to problems with the
detectors, the telescope and the cryogenic valves. There were
also some fears that the cover would not come off the telescope,
and if it did, that the mirror would be covered with nitrogen
frost. Despite these concerns, the spacecraft was launched, and
after a troubled start, it began producing a steady stream of data.

     To ensure that the satellite was sensitive to the infrared
heat coming from deep space, the spacecraft carried 700 liters of
superfluid helium to cool the telescope and detectors to a
temperature of 2 degrees Celsius above absolute zero. After 10
months in orbit, the helium evaporated and the data-taking
portion of the mission was over.

     But the data-analysis phase was just beginning. From its
vantage point above the glare of Earth's atmosphere, IRAS
produced more than 600,000 individual objects and more than 1,600
images of the entire sky. All told, the IRAS mission has helped
astronomers make many startling discoveries.

     "IRAS found more evidence for planet building among mature
stars," Beichman said. "One of the great surprises of the mission
was that Vega, one of the brightest visible stars in the sky, was
10 times brighter in the infrared than predicted. The infrared
radiation coming from Vega, and similar stars, is consistent with
a ring or disk of solid material orbiting the central star. IRAS
found that one-quarter of all stars have this same phenomenon."

     Another surprise was the number of galaxies it revealed. "No
one expected IRAS to find more than 1,000 galaxies, but we found
60,000," Beichman exclaimed. "These galaxies have been used to
probe the overall structure of the universe. One IRAS object may
be a galaxy captured in the process of formation.

     "IRAS was also a prolific comet finder, having detected
about 25 of them," he continued.

     Observations of these objects have changed the way
scientists think about comets. Prior to IRAS, astronomers thought
comets were large balls of ice hurtling through space. IRAS
showed that comets are made of mostly dirt and rock, with an icy
covering.

     The wealth of data produced by IRAS is used in ongoing
research by astronomers from around the world.

     "IRAS revealed the infrared sky to us in the way people will
be looking at it for a long time," Beichman said. "It is our
first and only view of what's out there until somebody does it
better. And it's not going to be easy to do it much better than
we did."

     That opportunity to follow up on many of the IRAS
discoveries will come sometime after the turn of the century,
when JPL's Space Infrared Telescope Facility (SIRTF) is launched
into solar orbit. SIRTF will take advantage of the enormous
technical advances in infrared detector arrays that have been
made over the last decade, making it 1,000 times more sensitive
than IRAS.

     However, SIRTF may lack a bit of magic that came with its
predecessor. "After all, one can open one's eyes to the night sky
for the first time only once," Beichman concluded. That honor
will forever belong to IRAS.

     ___    _____     ___
    /_ /|  /____/ \  /_ /|     Ron Baalke         | [email protected]
    | | | |  __ \ /| | | |     Jet Propulsion Lab |
 ___| | | | |__) |/  | | |__   M/S 525-3684 Telos | Every once in a while,
/___| | | |  ___/    | |/__ /| Pasadena, CA 91109 | try pushing your luck.
|_____|/  |_|/       |_____|/                     |

% ====== Internet headers and postmarks (see DECWRL::GATEWAY.DOC) ======
% From: [email protected] (Ron Baalke)
% Subject: IRAS - 10 Years Ago

739.3ISSA - Infrared Sky Survey AtlasMTWAIN::KLAESKeep Looking UpTue Jun 21 1994 14:0341
From:	US4RMC::"ASTRO%[email protected]" "Astronomy Discussion 
        List" 20-JUN-1994 17:41:01.83
To:	Multiple recipients of list ASTRO <ASTRO%[email protected]>
CC:	
Subj:	Re: ISSA

>Could anyone teel me were I can get the complete ISSA images for the
>entire sky. It was to be released in 1992.  [email protected]

The ISSA Postage Stamp Service is maintained by
    
Dave Van Buren [email protected]
Rick Ebert [email protected]
Daniel Egret [email protected]

ISSA is the Infrared Sky Survey Atlas, an all-sky survey made by the
IRAS (Infrared Astronomical Satellite) at wavelengths of 12, 25, 60
and 100 microns. All but a few percent of the sky are covered with 1.5
arcminute pixels. These data are also available on CD ROM from the
National Space Science Data Center at NASA's Goddard Space Flight Center. 

On the WWW, the URL is
http://brando.ipac.caltech.edu:8888/ISSA-PS

Good Luck
------------------------------------------------------------------------
Dave Meriwether
EUVE Science Operations Center

email: [email protected]
web: http://cea-ftp.cea.berkeley.edu/~davem/

% ====== Internet headers and postmarks (see DECWRL::GATEWAY.DOC) ======
% Date:         Sat, 18 Jun 1994 13:30:12 -0700
% Reply-To: Astronomy Discussion List <ASTRO%[email protected]>
% Sender: Astronomy Discussion List <ASTRO%[email protected]>
% From: Dave Meriwether <[email protected]>
% Subject:      Re: ISSA
% X-To:         Astronomy Discussion List <[email protected]>
% To: Multiple recipients of list ASTRO <ASTRO%[email protected]>

739.4IRAS data shows cosmic dust ring around SunMTWAIN::KLAESHouston, Tranquility Base here...Wed Jul 06 1994 18:0168
From:	US2RMC::"[email protected]" "MAIL-11 Daemon"  6-JUL-1994 
To:	[email protected]
CC:	
Subj:	Cosmic Dust Ring Detected

Cosmic dust may explain life on earth
6/30/94
 
   GAINESVILLE, Fla., June 30 (UPI) -- A ring of cosmic dust around
the sun may have supplied the carbon essential to the beginning of
life, University of Florida scientists said Thursday. 

   Stanley F. Dermott, professor and chairman of the university's
astronomy department, said discovery of the dust, which originates in
the asteroid belt, may help to unravel some mysteries on the origin of
life. 

   "This dust is largely carbonaceous material -- the material from
which life could form," Dermott reported in a June 30 cover story in
the British journal Nature. "This ring may act as a kind of funnel and
may have been the means of getting this life-forming material onto the
Earth after the planet formed." 

   Asteroids collide to form dust that collects in a gigantic ring
around the sun. The Earth's orbit is inside the ring, and the Earth's
gravity may pull much of the dust into the atmosphere and onto the
planet's surface, added Dermott, who is working to confirm this part
of the theory. 

   "The ring's existence will come as a surprise to astronomers,"
Dermott said. "Nothing like this has been found before -- that the
planets themselves are in rings that extend around the sun." 

   The cloud's existence was confirmed by observations from NASA's
Infrared Astronomical Satellite and computer experiments at UF, said
Dermott, who did the research with graduate student Sumita Jayaraman. 

   Dermott said he became suspicious when NASA's infrared, or heat-
sensitive, satellite detected heat from the dust. Seven years ago, he
said, he and Philip Nicholson of Cornell University discovered that
the half of the sky behind the Earth in its orbit was consistently
brighter than the other half, not realizing then that the cause was
the dust cloud trailing the Earth. 

   According to Dermott, one other development is the potential for
astronomers to study asteroidal material in their own back yard. 

   "People think of getting a sample of extra-terrestrial body off a
spacecraft. We now realize that bits of these particles collide with
the Earth and can be collected here for scientific study," he said. 

   The ring's discovery gives scientists a new way of thinking about
age-old questions, said Dermott. "Now that we've found this ring, we
can start to work on its implications for the mysteries of the origin
of life." 

   (Written by Jeff Bray in Miami, Edited by Larry Schuster, UPI
Science and Technology Editor in Washington) 

% ====== Internet headers and postmarks (see DECWRL::GATEWAY.DOC) ======
% Date: Tue, 5 Jul 1994 17:58:05 GMT
% From: Ron Baalke <[email protected]>
% To: [email protected]
% Message-Id: <[email protected]>
% Subject: Cosmic Dust Ring Detected
% Sender: [email protected]
% Reply-To: [email protected]