1999
Images
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1999
Spacepics: Please note that images are chronicled by date
- most recent listed first.
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ON
THE DAY THE SOLAR WIND DISAPPEARED,
SCIENTISTS SAMPLE PARTICLES DIRECTLY
FROM THE SUN
From
May 10-12, 1999, the solar wind that blows constantly from the Sun
virtually disappeared -- the most drastic and longest-lasting decrease
ever observed.
Dropping to a fraction of its normal density and to half its normal
speed, the solar wind died down enough to allow physicists to observe
particles flowing directly from the Sun's corona to Earth. This
severe change in the solar wind also changed the shape of Earth's
magnetic field and produced an unusual auroral display at the North
Pole.
Data
visualization of the X ray emissions over the North Pole during
the "polar rain" of electrons on May 11, 1999. The emissions
were detected by the PIXIE instrument on NASA's Polar spacecraft.
GSFC
Press Release 99-145
EDITOR'S NOTE: Images, movies, captions, and more detailed background
information associated with this release are available on the Internet
at:
http://www-spof.gsfc.nasa.gov/istp/news/9912
13
December 1999
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Data
From Goddard's Mars Orbiter Laser Altimeter (MOLA) Plays A Key Role
In Helping Scientists Determine The Primary Landing Site
Data
from Goddard's Mars Orbiter Laser Altimeter (MOLA) played a key
role in helping scientists determine the primary landing site for
the Mars Polar Lander. Engineers are aiming for a 200 kilometers
(125 miles) long and 20 kilometers (12-1/2 miles) wide strip of
gentle, rolling plains. Launched on January 3, 1999, Mars
Polar Lander will study the soil and look for ice beneath the surface
of the Martian south pole.
Landing Site Preview
Scientists used data from MOLA to learn about elevation changes
within the primary landing site (marked with an oval.) Colors in
the inset image correspond to changes in elevation. White colors
indicate elevations in excess of 3012 meters, red shows elevations
between 2500m - 3012m, yellow shows elevations 2450m - 2500m, dark
cyan shows elevations 2150m-2450m, dark violet shows elevations
from 320m - 2150m. The topography in these images is vertically
exaggerated by a factor of 5.
More
information visit our Mars page
02
December 1999
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Image Credit: NASA and The Hubble Heritage Team (STScI)
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Hubble
Telescope Reveals Swarm of Glittering Stars in Nearby Galaxy
NASA's
Hubble Space Telescope has peered at a small area within the Large
Magellanic Cloud (LMC) to provide the deepest color picture ever
obtained in that satellite galaxy of our own Milky Way.
Over
10,000 stars can be seen in the photo, covering a region in the
LMC about 130 light-years wide. The faintest stars in the picture
are some 100 million times dimmer than the human eye's limit of
visibility. Our Sun, if located in the LMC, would be one of the
faintest stars in the photograph, indistinguishable from the swarm
of other similar stars.
Also
visible in the image are sheets of glowing gas, and dark patches
of interstellar dust silhouetted against the stars and gas behind
them.
The
LMC is a small companion galaxy of our own Milky Way, visible only
from Earth's southern hemisphere. It is named after Ferdinand Magellan,
one of the first Europeans to explore the world's southern regions.
The LMC attracts the attention of modern-day astronomers because,
at a distance of only 168,000 light-years, it is one of the nearest
galaxies. (Details)
Image
files are available on the Internet at:
http://heritage.stsci.edu
http://oposite.stsci.edu/pubinfo/pr/1999/44
or via links in
http://oposite.stsci.edu/pubinfo/latest.html
and
http://oposite.stsci.edu/pubinfo/pictures.html
Higher
resolution digital versions (300 dpi JPEG and TIFF) are available
at:
http://oposite.stsci.edu/pubinfo/pr/1999/44/pr-photos.html
02
December 1999
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A
MINUET OF GALAXIES
This
troupe of four galaxies, known as Hickson Compact Group 87 (HCG
87), is performing an intricate dance orchestrated by the mutual
gravitational forces acting between them. The dance is a slow, graceful
minuet, occurring over a time span of hundreds of millions of years.
The
Wide Field and Planetary Camera 2 on NASA's Hubble Space Telescope
(HST) provides a striking improvement in resolution over previous
ground-based imaging. In particular, this image reveals complex
details in the dust lanes of the group's largest galaxy member (HCG
87a), which is actually disk-shaped, but tilted so that we see it
nearly edge-on. Both 87a and its elliptically shaped nearest neighbor
(87b) have active galactic nuclei which are believed to harbor black
holes that are consuming gas.
HCG
87 was selected for Hubble imaging by members of the public who
visited the Hubble Heritage website (http://heritage.stsci.edu)
during the month of May and registered their votes. The HST exposures
of the winning target were then acquired in July 1999 by the Hubble
Heritage Team and guest astronomers Sally Hunsberger (Lowell Observatory,
Flagstaff, Arizona) and Jane Charlton (Pennsylvania State University).
Image
Credit: The Hubble Heritage Team (AURA/STScI/NASA).
NOTE
TO EDITORS: For additional information, please contact Lisa Frattare,
STScI, 3700 San Martin Drive, Baltimore, MD 21218, (phone) 410-338-4724,
(fax) 410-338-4579, (e-mail) frattare@stsci.edu.
Image
files are available on the Internet at:
http://heritage.stsci.edu/
http://oposite.stsci.edu/pubinfo/pr/1999/31
or via links in
http://oposite.stsci.edu/pubinfo/latest.html
and
http://oposite.stsci.edu/pubinfo/pictures.html
Higher
resolution digital versions (300 dpi JPEG and TIFF)
are
available at:
http://oposite.stsci.edu/pubinfo/pr/1999/31/pr-photos.html
02
September 1999
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NASA
SELECTS MINIATURE SPACECRAFT TO TEST SPACE TECHNOLOGY
They're
each about the size of a large birthday cake, weigh about as much
as a desktop computer, and are smart enough to fly in formation
far from Earth while they test new technologies. They are three
very small satellites, called the Nanosat Constellation Trailblazer
mission, and today NASA selected them as the agency's latest New
Millennium mission. The mission will validate methods of operating
several spacecraft as a system, and test eight technologies in the
harsh space environment near the boundary of Earth's protective
magnetic field, or magnetosphere.
HQ
Press Release 99-095
19
August 1999
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MATTER'S
FINAL PLUNGE ON BLACK HOLE ROLLER COASTER DETECTED
The
final cry from material streaming toward a black hole at more than
6 million miles per hour -- possibly the first evidence of matter
actually falling into a black hole -- was detected by scientists
at NASA's Goddard Space Flight Center in Greenbelt, Md. This is
distinct from the readily observed phenomena of matter swirling
around or away from a black hole. The result, gathered from the
evidence of X-ray signatures from hot gas in a galaxy 100 million
light years away, appears in an upcoming article in Astrophysical
Journal Letters.
Resembling
a gigantic hubcap in space, a 3,700 light-year-diameter dust disk
encircles a 300 million solar-mass black hole in the center of the
elliptical galaxy NGC 7052.
GSFC Press Release 99-089
Related
Links:
Information about black holes is at:
http://imagine.gsfc.nasa.gov/docs/introduction/black_holes.html
More pictures and info is at:
http://antwrp.gsfc.nasa.gov/htmltest/rjn_bht.html
The Hubble Space Telescope photographed gas and dust swirling around
a massive black hole in a nearby galaxy:
http://oposite.stsci.edu/pubinfo/pr/1998/22/
16 August 1999
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Eclipse
99
On
Wednesday, August 11, 1999, a total eclipse of the Sun will be visible
from within a narrow corridor that traverses the Eastern Hemisphere.
The path of the Moon's umbral shadow begins in the Atlantic and
crosses Central Europe, the Middle East, and India where it ends
at sunset in the Bay of Bengal. A partial eclipse will be seen within
the much broader path of the Moon's penumbral shadow, which includes
Northeastern North America, all of Europe, Northern Africa and the
western half of Asia. This event is the last total solar eclipse
of the 20th century, and it will benefit formal and informal education
communities alike.
Eclipse 99 Website - fact-filled
website on this eclipse, a history of eclipses and future eclipses.
Visit this site for images and movies from the Aug. 11 Eclipse.
11
August 1999
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Caption
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STIFF
SOLAR ATMOSPHERE CANCELS DANCE AND GETS HOT
Coronal
loops, immense coils of hot gas on the surface of the Sun, vibrate
wildly after the blast wave from a solar flare hits them. However,
their dance is quickly squelched by resistance from the Sun's outer
atmosphere (corona). The corona restricts motion due to internal
friction hundreds of millions of times greater than expected, according
to recent observations from NASA's Transition Region and Coronal
Explorer (TRACE) spacecraft.
GSFC Press Release 99-088
05
August 1999
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SUPER-SHARP
VIEW OF THE DOOMED STAR ETA CARINAE
A
huge, billowing pair of gas and dust clouds are captured in this
stunning NASA Hubble Space Telescope image of the supermassive star
Eta Carinae.
Using
a combination of image processing techniques (dithering, subsampling
and deconvolution), astronomers created one of the highest resolution
images of an extended object ever produced by Hubble Space Telescope.
The resulting picture reveals astonishing detail.
Even
though Eta Carinae is more than 8,000 light-years away, structures
only 10 billion miles across (about the diameter of our solar system)
can be distinguished. Dust lanes, tiny condensations, and strange
radial streaks all appear with unprecedented clarity.
Eta
Carinae was observed by Hubble in September 1995 with the Wide Field
Planetary Camera 2 (WFPC2). Images taken through red and near-ultraviolet
filters were subsequently combined to produce the color image shown.
A sequence of eight exposures was necessary to cover the object's
huge dynamic range: the outer ejecta blobs are 100,000 times fainter
than the brilliant central star.
Eta
Carinae was the site of a giant outburst about 150 years ago, when
it became one of the brightest stars in the southern sky. Though
the star released as much visible light as a supernova explosion,
it survived the outburst. Somehow, the explosion produced two polar
lobes and a large thin equatorial disk, all moving outward at about
1.5 million miles per hour.
The
new observation shows that excess violet light escapes along the
equatorial plane between the bipolar lobes. Apparently there is
relatively little dusty debris between the lobes down by the star;
most of the blue light is able to escape. The lobes, on the other
hand, contain large amounts of dust which preferentially absorb
blue light, causing the lobes to appear reddish.
Estimated
to be 100 times more massive than our Sun, Eta Carinae may be one
of the most massive stars in our Galaxy. It radiates about five
million times more power than our Sun. The star remains one of the
great mysteries of stellar astronomy, and the new Hubble images
raise further puzzles. Eventually, this star's outburst may provide
unique clues to other, more modest stellar bipolar explosions and
to hydrodynamic flows from stars in general.
Photo
Credit: Jon Morse (University of Colorado), and
NASA
Investigating Team: Kris Davidson (University of Minnesota), Bruce
Balick (University of Washington), Dennis Ebbets (Ball Aerospace),
Adam Frank (University of Minnesota), Fred Hamann (University of
California - San Diego), Roberta Humphreys (University of Minnesota),
Sveneric Johansson (Lund Observatory), Jon Morse (University of
Colorado), Nolan Walborn (Space Telescope Science Institute), Gerd
Weigelt (Max Planck Inst. for Radio Astronomy, Bonn), and Richard
White (Space Telescope Science Institute)
Image
files in GIF and JPEG format and captions may be accessed on Internet
via anonymous ftp from oposite.stsci.edu in /pubinfo.
GIF
JPEG PRC96-23a Eta Carinae color gif/EtaCarC.gif jpeg/EtaCarC.jpg
Higher resolution digital versions (300dpi JPEG) of the release
photographs will be available temporarily in /pubinfo/hrtemp: 96-23a.jpg
(color), 96-23abw.jpg (black/white).
GIF
and JPEG images, captions and press release text are available via
World Wide Web at: http://www.stsci.edu/pubinfo/PR/96/23.html
and via links in: http://www.stsci.edu/pubinfo/latest.html
or http://www.stsci.edu/pubinfo/pictures.html
.
GSFC
Press Release
Images
and Captions
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ETA
CARINAE SPECTRA
These
are spectra of light emitted by hydrogen atoms in Eta Carinae and
its surrounding nebula. The spectra were taken by the Space Telescope
Imaging Spectrograph (STIS) instrument on board the Hubble Space
Telescope. A spectrograph separates light into its component colors,
which correspond to different wavelengths. This is similar to the
way a prism separates white light into a rainbow of distinct colors.
By analyzing light this way, astronomers learn a great deal about
the object emitting the light, such as its temperature, chemical
composition, and motion. The light used by STIS for this graph corresponds
to hydrogen alpha emission, which appears red to the human eye.
The
spectra are from different times during the star's recent doubling
of brightness; December 1997 (top left), November 1998 (top right),
March 1998 (bottom left), February 1999 (bottom right). The horizontal
axis of each spectrum displays the wavelength, or color, of the
light. Shorter wavelengths (more blue) are on the left and longer
wavelengths (more red) are on the right. The vertical axis measures
the brightness (intensity) of the light. The diagonal axis is the
area around Eta Carinae imaged by STIS. The peak is light from Eta
Carinae, and smaller peaks in the foreground are light from the
surrounding nebula.
A
wide "canyon" is especially prominent on the left side
of the December 1997 and March 1998 spectra. This is due to the
blocking of light, called an absorption feature, that probably results
from an extended atmospheric "wind" of gas being blown
from the surface of Eta Carinae. Note that in the spectra on the
right, this canyon grows smaller and almost disappears in the February
1999 spectrum. This indicates that the wind varies with time and
has recently changed substantially.
A
narrow canyon can also be seen on the left side of the peaks closer
to the top. This newly discovered feature indicates high density
gas between the star and the observer. Its depth also changes with
time. One explanation is that a rotating disk of gas surrounding
Eta Carinae alternately brings high and low density regions into
view, with the dense regions blocking more light when they rotate
between us and Eta Carinae.
Image
Credit: NASA/STScI/ Ted Gull / Phil Plait
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TROUBLE
BREWING IN ETA CARINAE
GSFC
Press Release
Images
and Captions
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GSFC
Press Release
Images
and Captions
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SUPER-SHARP
VIEW OF THE DOOMED STAR ETA CARINAE
GSFC
Press Release
Images
and Captions
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HUBBLE
COMPLETES EIGHT-YEAR EFFORT TO MEASURE EXPANDING UNIVERSE
The
Hubble Space Telescope Key Project Team today announced that it
has completed efforts to measure precise distances to far-flung
galaxies, an essential ingredient needed to determine the age, size
and fate of the universe.
"Before
Hubble, astronomers could not decide if the universe was 10 billion
or 20 billion years old," said team leader Wendy Freedman of
the Observatories of the Carnegie Institution of Washington. "The
size scale of the universe had a range so vast that it didn't allow
astronomers to confront with any certainty many of the most basic
questions about the origin and eventual fate of the cosmos. After
all these years, we are finally entering an era of precision cosmology.
Now we can more reliably address the broader picture of the universe's
origin, evolution and destiny."
See
the HQ Press Release for further details.
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The
Ni-59 produced by a supernova changes into Co-59 as time passes. When
these particles are accelerated up to high energies (become cosmic
rays), the hourglass breaks (the orbiting electrons are lost) and
no more Ni-59 changes. New measurements from the ACE spacecraft show
that nearly all the Ni-59 has changed before the particles are accelerated,
indicating that more than a hundred thousand years pass between production
and acceleration (and maybe much more). -- image credit: Eric Christian,
NASA
NEW
FINDINGS NARROW THEORIES ON COSMIC RAY ORIGIN
Where
do those fast-flying atoms that pelt the Earth come from? Scientists
catching cosmic rays with a NASA spacecraft have tightened the constraints
on the evolving theory of how atoms travelling at nearly the speed
of light are produced in stars and are strewn across the Universe
through star explosions, or supernovae.
Cosmic
rays bombard the Earth's atmosphere constantly. These highly energetic
particles are not "rays," however, but rather atoms that
were stripped of their electrons when they were accelerated to enormous
speeds. While many scientists agree that the energy of supernovae
is needed to produce cosmic rays, debates rage over the "seed
particles," or the actual atoms that are being accelerated.
Are the particles accelerated directly from a supernova, like shrapnel
in an explosion? Or are they from dust and gas already present in
the region between stars, bumped to high speeds by the blast wave
of a supernova explosion?
Results
from NASA's Advanced Composition Explorer (ACE) suggest that cosmic
rays are not accelerated directly from supernovae, as some current
models predict. Rather, it is material that has been sitting around
for hundreds of thousands of years that gets accelerated by the
shock wave of a supernova explosion.
Dr.
Paul Hink of Washington University in St. Louis (WUSL) and a team
of scientists from WUSL, California Institute of Technology, NASA's
Jet Propulsion Laboratory and NASA's Goddard Space Flight Center
present these results from the ACE Cosmic Ray Isotope Spectrometer
(CRIS) at the Centennial Meeting of the American Astronomical Society
in Chicago on May 31, 1999. See the GSFC Press Release for further details.
31
May 1999
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Astronomers
Detect Activity From "Quiet" Supermassive Black Holes
Astronomers
have heard the first shy words from seemingly quiet supermassive
black holes in the form of a unique type of X-ray light. These black
holes exist in the centers of the oldest, largest galaxies and have
a mass of about a billion suns, compressed into a region comparable
to the size of our solar system.
For
more detail, check these links:
GSFC Press Release 99-036
13
April 1999
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Astronomers
Discover "Middleweight" Black Holes
The
field of black holes, formerly dominated by heavyweights packing
the gravitational punch of a billion Suns and lightweights just
a few times heavier than our Sun, now has a new contender -- a just-discovered
mysterious class of "middleweight" black holes, weighing
in at 100 to 10,000 Suns.
For
more detail, check these links:
HQ Press Release 99-051
13
April 1999
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Find
First Observational Evidence For "Hypernova" Explosion
Astronomers
at Northwestern University and University of Illinois have detected
the first observational evidence for the remnants of a hypernova,
an explosion a hundred times more energetic than an exploding star
(supernova) and the possible source of powerful gamma ray bursts,
the most energetic events known in the Universe other than its creation
as a result of the Big Bang.
For
more detail, check these links:
GSFC Press Release 99-035
12
April 1999
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Astronomers
Solve The Case Of The Unknown Star Explosion, Discover Rare Coupling
Of Elements
Astronomers
have pieced together the scene of a crime that no one saw: a 700-year-old
star explosion nearly as bright as a full moon, undocumented by
early stargazers and unknown to modern-day astronomers until only
very recently. Clues came in the form of two radioactive elements
never before seen together in such explosions, a rare event that
offers a new avenue to test star explosion theories.
For
more detail, check this link:
GSFC Press Release 99-037
08
April 1999
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FUSE
Satellite Arrives In Florida For Launch Preparations
NASA's
Far Ultraviolet Spectroscopic Explorer (FUSE) satellite arrived
Thursday, April 1 at NASA Hangar AE on Cape Canaveral Air Station
to begin prelaunch processing for launch next month.
For
more detail, check these links:
KSC Press Release 23-99
FUSE Homepage
02
April 1999
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Solar
Structures Can Help Forecast
Largest Solar Blasts
"S"
marks the spot for scientists trying to forecast solar eruptions
that can damage satellites, disrupt communications networks and
cause power outages.
Using
the Japanese Yohkoh spacecraft, NASA-sponsored scientists have discovered
that an S-shaped structure often appears on the Sun in advance of
a violent eruption, called a coronal mass ejection, that is as powerful
as billions of nuclear explosions.
"Early
warnings of approaching solar storms could prove useful to power
companies, the communications industry and organizations that operate
spacecraft, including NASA," said Dr. George Withbroe, science
director for Sun-Earth Connection research at NASA Headquarters.
"This is a major step forward in understanding these tremendous
storms." (Details)
NOTE TO EDITORS: Images and supporting material can be found on
the Internet at: http://solar.physics.montana.edu/press/
http://www.isas.ac.jp/info/sat/yohkoh-e.html#Tag:0
http://solar.physics.montana.edu/YPOP/
15
March 1999
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Hubble
Finds More Evidence of Galactic Cannibalism
This
beautiful, eerie silhouette of dark dust clouds against the glowing
nucleus of the elliptical galaxy NGC 1316 may represent the aftermath
of a 100 million year old cosmic collision between the elliptical
and a smaller companion galaxy.
A
number of faint objects are scattered across the image, including
both reddish galaxies in the distant background and bluer, point-like
star clusters orbiting NGC 1316. These clusters, relatively loosely-knit
swarms containing a few thousand stars each, are smaller and fainter
than those found in other elliptical galaxies. These clusters are
too old to have been created in the collision which produced the
dusty debris we see today, and too young to have been torn apart
by galactic tidal forces. The clusters may have been born in the
course of a still earlier collision, or belonged to the galaxy which
most recently fell victim to NGC 1316.
The
picture was taken in April of 1996 with the Wide Field Planetary
Camera 2. The color rendition was constructed using separate images
taken in blue and red light. NGC 1316 is located 53 million light-years
away in the constellation Fornax. The field of view shown is about
12,000 light-years across.
Credit:
Carl Grillmair (California Institute of Technology) and NASA
The Space Telescope
Science Institute is operated by the Association
of Universities for Research in Astronomy, Inc. (AURA), for
NASA, under contract with the
Goddard Space Flight Center,
Greenbelt, MD. The Hubble Space Telescope is a project of international
cooperation between NASA and the
European Space Agency (ESA).
(
Full Story) (2/18/99)
18 February 1999
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SOHO
Spacecraft Detects Source Of High Speed "Wind" From The
Sun
Like
water gushing through cracks in a dam, scientists observed "fountains"
of electrified gas, called the solar wind, flowing around magnetic
regions on the Sun to begin a two million mile per hour rush into
space. Using the Solar and Heliospheric Observatory (SOHO) spacecraft,
American and European scientists observed solar wind flows coming
from the edges of honey-comb shaped patterns of magnetic fields
at the surface of the Sun. These observations are presented in the
Feb. 5 issue of SCIENCE magazine. The research will lead to better
understanding of the high speed solar wind, a stream of electrified
gas that affects the Earth's space environment.
For
more detail, check this link:
Press Release 99-020
04 February 1999
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Gamma
Ray Burst Imaged For First Time
Astronomers
racing the clock managed to take the first-ever optical images of
one of the most powerful explosions in the Universe -- a gamma ray
burst -- as it was occurring on Saturday, Jan. 23, 1999. Gamma ray
bursts produce more energy in a very short period than the rest
of the entire Universe combined. (Details)
01
February 1999
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Third
EGRET Catalog
Press
Release 99-002
An
online version of the
Third EGRET Catalog is available by clicking the link and will
be published in an upcoming issue of Astrophysical Journal Supplements.
Researchers
working with the Energetic Gamma Ray Experiment Telescope (EGRET)
on NASA's Compton Gamma Ray Observatory spacecraft have cataloged
the entire high-energy gamma-ray sky as we know it, from pulsars
in our own Galaxy to blazars at the farthest ends of the Universe.
This
Third EGRET Catalog, presented at the 193rd American Astronomical
Society Meeting in Austin, Texas, contains 271 gamma-ray sources
detected from 1991-1995, including the Large Magellanic Cloud, the
great solar flare of 1991, a probable radio galaxy, and 170 sources
yet unidentified.
"This
catalog includes all the high-energy gamma ray sources in the Universe
that could be detected by EGRET," said Dr. Robert Hartman,
an astrophysicist on the EGRET team at NASA's Goddard Space Flight
Center. "This is a huge step for gamma-ray astronomy from the
early days 25 years ago, yet in many ways the field is still in
its infancy."
19
January 1999
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Press
Release 99-003
Photo
Release 99-005P
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X-Ray
Pulsar With Companion Star Images
This
is an artist's conception of an X-ray pulsar in a binary star system:
Matter from a companion star, most likely a Red Giant, channels
onto a rapidly spinning neutron star at its magnetic poles. Magnetic
fields run in loops from pole to pole. Radiation in the form of
X-rays appears to pulse on and off as hot patches of gas are exposed
at the poles with the neutron star's rotation. (The axis of rotation
is different from the axis of the magnetic field.) The neutron star
-- more massive than the Sun yet with a diameter of only 10-15 kilometers
-- is extremely dense. Its strong gravitational force accelerates
infalling matter to high energies.
Art
Credit: Maggie Masetti, NASA
THE
ONLY KNOWN BURSTING PULSAR PROVIDES CLUES TO PULSAR NATURE
Astronomers
observing the unique "Bursting Pulsar" -- the only pulsar
known to generate both regular pulses and frequent enormous bursts
of radiation -- have characterized the relationship between the
two phenomena. This may shed light on the pulsing mechanism behind
other pulsars and how it is affected by magnetic fields, companion
stars and occasional bursts of radiation.
Dr.
Michael Stark, an astrophysicist with NASA's Goddard Space Flight
Center (GSFC) and the University of Maryland, College Park, and
Dr. Keith Jahoda, astrophysicist in the X-ray branch at GSFC, present
their findings at the 193rd American Astronomical Society Meeting
in Austin, Texas.
11
January 1999
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We
are interested in what you think, so please send us your comments.
Curator:
Lynn Jenner
Author:
Darlene A.
Ahalt
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