Goddard Space Flight Center
June 4, 2000
As planned, pieces of the observatory that survived the re-entry landed in the Pacific Ocean approximately 2,400 miles (3,862 km) southeast of Hawaii.
The fourth and final burn needed to re-enter NASA's Compton Gamma Ray Observatory was initiated at 1:22 a.m. EDT on June 4. Compton's Attitude Control thrusters and Orbit Adjust thrusters were fired for 30 minutes.
After the failure of one of Compton's three gyroscopes, NASA decided to bring the satellite back via a controlled reentry. NASA determined that it was much safer to bring the satellite back now to safe guard against further system failures in the spacecraft that might hinder a controlled reentry.
"This was a bittersweet day for NASA," said Al Diaz, Director of the Goddard Space Flight Center. "The end of the Compton Gamma Ray
Observatory mission marks the end of a remarkable spacecraft. Compton left a legacy of outstanding science and revolutionized our knowledge of the gamma ray sky. And while no one at NASA is ever happy to see the end of a science mission, prolonging this mission would have posed an unacceptable and increasing risk to human life. This was an extraordinarily complex task, involving both operations and engineering proficiency. I'm proud of this team and the job they did. They understood the significance of this task, and they performed it flawlessly."
Compton spent nine productive years in orbit. Engineers began planning for the Observatory's reentry in April 1999 when gyroscope #3 first began experiencing problems. By the time the gyro actually failed in December 1999, engineers had devised a number of deorbit scenarios. Engineers at Goddard, assisted by their counterparts at the Johnson Space Center in Houston, spent the past five months designing a reentry plan to safely deorbit the CGRO spacecraft.
A total of four burns were used to gradually lower the spacecraft's orbit. The first re-entry burn was conducted on May 30, and a second burn on May 31. At midnight on June 4, controllers fired CGRO's primary thrusters for a third time bringing spacecraft's low point to within 92miles (148 km) of the Earth's surface.
NASA and international space agencies plan several upcoming missions to continue where Compton left off. The Gamma-ray Large Area Space Telescope (GLAST) is a proposed new high-energy gamma-ray mission to identify and study nature's highest energy particle accelerators. GLAST will be 30 times more sensitive than the Energetic Gamma Ray Experiment Telescope (EGRET) onboard the Compton Gamma Ray Observatory. Swift will be the first mission to focus on studying the newly-discovered afterglow from gamma ray bursts. Swift's rapid repointing capability will enable high-precision X-ray and optical positions to be determined and relayed to the ground for use by a network of dedicated observers at large telescopes.
The Compton Gamma Ray Observatory was the second of NASA's Great Observatories and the gamma-ray equivalent to the Hubble Space Telescope and the Chandra X-ray Observatory. Compton was launched aboard the Space Shuttle Atlantis in April 1991, and at 17 tons, was the largest astrophysical payload ever flown at that time.
NEWSALERT: Saturday, June 3, 2000 @ 0851 GMT
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June 2nd, 2000 - Issue #248
=========================================================== SKY & TELESCOPE'S NEWS BULLETIN - JUNE 2, 2000 =========================================================== For images and Web links for these items, visit http://www.skypub.com =========================================================== In collaboration with key organizations of amateur and professional astronomers, SKY & TELESCOPE has established the AstroAlert e-mail news service to alert small-telescope users to significant happenings in the sky -- those that involve especially rare events or require immediate follow-up observations worldwide. To find out more, visit http://www.skypub.com/news/astroalert/astroalert.html. ===========================================================
Flight controllers are bringing down the satellite in steps, using four engine firings to lower the spacecraft's orbit until its closest point is within the atmosphere. The first two burns occurred on May 30th and 31st. The final two will happen on the day of reentry. Impact is expected at 6:20 Universal Time (2:20 a.m. EDT) Sunday.
The satellite is being destroyed because mission guidelines dictate that, should one of the spacecraft's three gyroscopes fail, as happened last December 19th, the mission would be terminated. The spacecraft could still be controlled with two gyroscopes but would be uncontrollable should a second unit fail. In March, Edward J. Weiler, NASA's Associate Administrator for the Office of Space Science, explained that there was a 10 percent chance that a second gyro would fail during the next three years. If the spacecraft were to plummet to Earth out of control, it would pose a 1-in-1,000 chance of causing a human fatality.
CGRO's mission was nominally for 5 years, but it has provided valuable data for nearly 9 years. See the July issue of Sky & Telescope (page 48) for an overview of the spacecraft's mission and scientific findings.
SPACE.com News
Friday 02 June 2000
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June 1st, 2000 - Issue #247
NASA Headquarters, Washington, DC
Goddard Space Flight Center, Greenbelt, MD
May 26, 2000
NASA controllers will fire CGRO's thrusters four times to lower the observatory's orbit. After each burn, mission trackers at Goddard Space Flight Center, Greenbelt, MD, will determine the observatory's exact position and, if necessary, adjust the descent. The engine burns will occur at:
Recorded status reports will be available after each burn on the Goddard Audio News Service (301/286-NEWS). Status reports will be posted the following morning to:
http://www.nasa.gov/hqpao/status_index.html
Live coverage on NASA Television of the deorbit activities will begin at 1 a.m. EDT June 4 and conclude at the close of the 6 a.m. briefing.
NASA Television coverage will include science highlights, re- entry animation and commentary on the re-entry activities by Dr. Neil Gehrels, CGRO project scientist. A NASA fact sheet on the re-entry can be found at:
Unlike most satellites, Compton is too large to burn up entirely in the atmosphere during re-entry. More than 6 tons (12,400 pounds) of metal debris is expected to fall to the Earth's surface. The debris fragments will range in size from the size of a small stone to several hundred pounds or kilograms.
To ensure the safety of aircraft and surface vessels in or near the target impact area, Debris Hazard Warning Areas were established well away from land. Shipping and air traffic in the area have been notified to ensure that craft will not be in the vicinity of the impact area.
NASA decided before Compton was launched that, due to the observatory's size, it would be returned to Earth by controlled re-entry when the mission was over. Extensive research showed that it was significantly safer to perform a controlled re-entry than any other method of dealing with the satellite.
NASA Television is broadcast on GE-2, transponder 9C located at 85 degrees West longitude, with vertical polarization. Frequency is on 3880.0 MHz, with audio on 6.8 MHz.
30 mei 2000
Het heelal straalt ons toe in een breed spectrum, van de laag energetische radiostraling, tot de hoog energetische Röntgen- en gammastraling. Slechts een deel van de straling dringt door onze dampkring en daar weer een klein deel van kunnen wij detecteren met onze ogen, het zichtbare licht. Om gammastraling uit het heelal waar te nemen moeten we onze toevlucht nemen tot satellieten als het Compton-observatorium.
COMPTEL is ontworpen voor het waarnemen van gammastraling met een energie van mega-elektronvolts. Deze straling ontstaat bij de meest gewelddadige gebeurtenissen in het universum, zoals supernova's, het verdwijnen van materie in zwarte gaten, de raadselachtige 'gamma-ray bursts' en de vorming van de elementen.
Tijdens haar dienst op het Compton-observatorium heeft COMPTEL de hemel in kaart gebracht in een voorheen grotendeels onontgonnen deel van het spectrum. Onderzoekers van SRON hebben bijgedragen aan alle facetten van het onderzoek, waaronder het opsporen van gammastralende radioactieve atoomkernen in het heelal, zoals aluminium-26, titanium-44 en kobalt-56. Deze ontstaan in zware sterren en komen vrij bij supernova-explosies. De gammastraling van de radioactieve atoomkernen vormt een directe vingerafdruk van de zogenaamde nucleosynthese, de vorming van de elementen in het heelal.
Met het in zee storten van het Compton-observatorium eindigen negen jaren vruchtbaar onderzoek in het meest variabele stralingsgebied van het spectrum. Dat is vier jaar langer dan oorspronkelijk gepland. Astrofysici zullen het nu twee jaar moeten stellen zonder 'gamma-ogen'. In 2002 wordt de draad weer opgepakt door de Europese gamma-satelliet Integral.
Stichting Ruimte Onderzoek Nederland (SRON) is een instituut van de Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) en initieert, ontwikkelt, bouwt en gebruikt instrumenten voor wetenschappelijk onderzoek in en vanuit de ruimte.
SPACE.com Today
25 May 2000
Scientists Prepare to De-Orbit Compton Satellite
NASA's ground-control team is expected to decide this week to
bring down the spacecraft into the eastern Pacific Ocean.
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May 25th, 2000 - Issue #243