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flight on the space shuttle and flew on the
Spacelab 1 mission as a joint effort between the Laboratoire d'Astronomie Spatiale and the University of California, Berkeley. The prime experiment objective of this telescope is to observe faint astronomical sources in the far ultraviolet with sensitivities far higher than previously available. The experiment will cover the 1300 to 1800 A band, which is inaccessible to observers on earth. The observing program during the mission consists of obtaining deep sky images during spacecraft nighttime. The targets will include hot stars and nebulae in our own galaxy, faint diffuse galactic features similar to the cirrus clouds seen by the Infrared Astronomical Satellite (IRAS), large nearby galaxies, nearby clusters of galaxies, and objects of cosmological interest such as quasars and the diffuse far ultraviolet background.
307:, a NASA explorer class satellite mission, was launched on June 7, 1992 and it operated till January 31, 2001. EUVE is entirely dedicated to observations in the wavelength range from 70 to 760 Ă…. The first phase of the mission (six months) was dedicated to an all-sky survey using the imaging instruments. The second phase instead is dedicated to pointed observations with mainly the spectroscopic instruments.
145:
140:
31:
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The Far
Ultraviolet Space Telescope is a compact, wide field-of-view, far ultraviolet instrument designed for observations of extended and point sources of astronomical interest. It was originally used in sounding rocket work by both French and American investigators. The instrument was modified for
271:
were awarded the 2006 Nobel prize in physics. The SNAP was superseded by the Wide Field InfraRed Survey
Telescope (WFIRST)., and now the Nancy Grace Roman Space Telescope – or Roman Space Telescope, – a NASA observatory designed to settle essential questions in the areas of dark energy, exoplanets,
247:
project. SNAP, the
Supernova/Acceleration Probe, was to study exploding stars called supernovae, as well as the gentle smearing of the light from distant galaxies due to gravity — called weak gravitational lensing — and put limits on what may or may not be the force driving the outward pull on the
638:
Tie, Suk Sien; Kirkby, David; Martini, Paul; Poppett, Claire; Pappalardo, Daniel; Schlegel, David; Shover, Jonathan; Guy, Julien; Fanning, Kevin; Honscheid, Klaus; Lampton, Michael; Jelinsky, Patrick; Besuner, Robert; Zhang, Kai; Brooks, David; Doel, Peter; Duan, Yutong; Gastañaga, Enrique; Kehoe,
339:
actionable information that has vastly higher spatial resolution and is updated more frequently than is currently available. We envision that the imagery and notifications from FUEGO will feed into an integrated fire information and management system to help limit the destruction from wildfires.
338:
The Fire
Urgency Estimator in Geostationary Orbit (FUEGO) Mission will continuously observe a large area of the Earth (primarily the western US) to rapidly identify the ignition of wildland fires and track their motions. FUEGO provides agencies and fire fighters on the ground with real-time
287:
The Dark Energy
Spectroscopic Instrument (DESI) will measure the effect of dark energy on the expansion of the universe. It will obtain optical spectra for tens of millions of galaxies and quasars, constructing a 3D map spanning the nearby universe to 11 billion light years.
272:
and infrared astrophysics. The telescope was initially developed as the WFIRST, and renamed in 2020 to honor Nancy Grace Roman, NASA's first Chief of
Astronomy. Roman has been called the “mother” of NASA's Hubble Space Telescope.
639:
Robert; Landriau, Martin; Levi, Michael; Prada, Francisco; Tarle, Gregory (2020). "The DESI sky continuum monitor system". In Evans, Christopher J.; Bryant, Julia J.; Motohara, Kentaro (eds.).
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Pennypacker, Carlton; Jakubowski, Marek; Kelly, Maggi; Lampton, Michael; Schmidt, Christopher; Stephens, Scott; Tripp, Robert (2013).
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161:(March 1, 1941 – June 9, 2023) was an American astronaut, scientist, and founder of the optical ray tracing company
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selected as payload specialist (the same mission as STS-61K—but renamed), replaced by backup payload specialist
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graduate professor and theoretical astrophysicist, Susan M. Lea,. They had one daughter, Jennifer Lea
Lampton.
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903:
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867:
770:"FUEGO — Fire Urgency Estimator in Geosynchronous Orbit — A Proposed Early-Warning Fire Detection System"
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Universe. SNAP was to investigate over one thousand square degrees of sky with a 500 megapixel camera.
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Lampton, M; Collaboration, SNAP (2002). "[astro-ph/0209549] The SNAP Telescope".
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Lea, S.; Lampton, M. (1972). "The theory of maximally flat loudspeaker systems".
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selected as payload specialist (mission cancelled after the
Challenger accident)
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selected as payload specialist (mission cancelled after the technical problems)
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868:"NASA - ATLAS-1: The First Atmospheric Laboratory for Applications and Science"
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30:
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he was one of the "Fiendish
Fourteen", 14 students responsible for the
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from 1978 to 1992. Below is a list of the missions he was a part of.
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Fire Urgency Estimator in Geostationary Orbit (FUEGO) Project
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Ground-based and Airborne Instrumentation for Astronomy VIII
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256:
719:"Results from the Far Ultraviolet Space Telescope (FAUST)"
717:
Sasseen, T.P.; Bowyer, S.; Lampton, M.; Wu, X. (1993).
637:
627:
https://www.space.com/nancy-grace-roman-space-telescope
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546:
276:
Dark Energy Spectroscopic Instrument (DESI) Project
377:selected and served as backup payload specialist
181:Michael Logan Lampton was born March 1, 1941, in
885:
171:The theory of maximally flat loudspeaker systems
625:What is the Nancy Grace Roman Space Telescope?
444:IEEE Transactions on Audio and Electroacoustics
311:Far Ultraviolet Space Telescope (FAUST) Project
615:https://astrobiology.nasa.gov/missions/wfirst/
333:Fire urgency estimator in geosynchronous orbit
471:
469:
835:
757:https://ntrs.nasa.gov/citations/19890020055
292:Extreme Ultraviolet Explorer (EUVE) Project
239:SuperNova Acceleration Probe (SNAP) Project
692:"The Extreme Ultraviolet Explorer Mission"
475:
441:
29:
914:California Institute of Technology alumni
909:University of California, Berkeley alumni
793:
648:
586:
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499:https://physics.sfsu.edu/people/susan-lea
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342:
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185:. In 1961, while Lampton was attending
919:People from Williamsport, Pennsylvania
886:
478:"Astronaut Biography: Michael Lampton"
315:Lampton was heavily involved with the
296:Lampton was heavily involved with the
280:Lampton was heavily involved with the
255:(JDEM), a cooperative venture between
243:Lampton was heavily involved with the
860:
761:
755:The Far Ultraviolet Space Telescope:
710:
204:, on June 9, 2023, at the age of 82.
165:. He was also known for his paper on
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683:
631:
540:
282:Dark Energy Spectroscopic Instrument
613:Nancy Grace Roman Space Telescope:
435:
13:
14:
930:
845:. astronautix.com. Archived from
594:"The Nobel Prize in Physics 2006"
232:University of California-Berkeley
643:. Vol. 11447. p. 187.
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143:
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810:https://fuego.ssl.berkeley.edu/
802:
749:
619:
511:https://drsusanlea.com/bio.html
317:Far Ultraviolet Space Telescope
696:Large-Scale Surveys of the Sky
607:
561:
515:
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195:San Francisco State University
16:American astronaut (1941–2023)
1:
429:
743:10.1016/0273-1177(93)90174-A
497:SFSU | Dr. Susan Lea :
331:Lampton participated in the
305:Extreme Ultraviolet Explorer
298:Extreme Ultraviolet Explorer
207:
7:
509:Dr. Susan Lea's biography:
10:
935:
723:Advances in Space Research
183:Williamsport, Pennsylvania
52:Williamsport, Pennsylvania
822:"home/hqnews/1990/90-072"
690:Lampton, Michael (1990).
402:/Spacelab EOM 1-2 mission
261:U.S. Department of Energy
253:Joint Dark Energy Mission
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131:
117:
107:
100:
95:Space Sciences Laboratory
86:
78:
59:
37:
28:
21:
460:10.1109/TAU.1972.1162374
423:due to medical problems
200:Michael Lampton died in
523:"Michael Logan Lampton"
388:/Spacelab EOM 1 mission
343:NASA Astronaut Program
263:. SNAP collaborators
251:SNAP was part of the
159:Michael Logan Lampton
230:in Physics from the
193:. He was married to
191:Great Rose Bowl Hoax
904:American astronauts
786:2013RemS....5.5173P
735:1993AdSpR..13l.631S
704:1990lsss.conf..137L
659:2020SPIE11447E..85T
347:Lampton was a NASA
214:Bachelor of Science
202:Oakland, California
71:Oakland, California
667:10.1117/12.2561436
349:payload specialist
335:(FUEGO) project.
169:with Susan M Lea,
112:Payload Specialist
23:Michael L. Lampton
849:on April 15, 2002
795:10.3390/rs5105173
780:(10): 5173–5192.
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843:"flights/sts61k"
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571:. Archived from
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167:electroacoustics
163:Stellar Software
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133:Mission insignia
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729:(12): 631–634.
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48:March 1, 1941
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872:. Retrieved
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851:. Retrieved
847:the original
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826:. Retrieved
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598:. Retrieved
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573:the original
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482:. Retrieved
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421:Dirk Frimout
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269:George Smoot
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102:Space career
101:
65:(2023-06-09)
63:June 9, 2023
899:2023 deaths
894:1941 births
454:: 200–203.
265:John Mather
109:UC Berkeley
79:Nationality
888:Categories
874:2016-07-22
870:. nasa.gov
853:2016-07-22
828:2016-07-22
824:. nasa.gov
650:2101.11736
600:2016-07-22
579:2013-07-03
532:1 December
484:2016-07-22
430:References
319:project.
300:project.
284:project.
216:degree in
44:1941-03-01
374:/Columbia
363:Position
208:Education
91:Physicist
416:/ATLAS-1
400:STS-61-K
386:STS-51-H
259:and the
118:Missions
82:American
808:FUEGO:
782:Bibcode
731:Bibcode
700:Bibcode
698:: 137.
655:Bibcode
360:Mission
222:Caltech
218:Physics
187:Caltech
673:
569:"SNAP"
414:STS-45
234:, 1967
224:, 1962
126:STS-45
73:, U.S.
54:, U.S.
645:arXiv
549:arXiv
450:(3).
372:STS-9
228:Ph.D.
220:from
122:STS-9
671:ISBN
534:2023
452:IEEE
410:1989
396:1986
382:1985
368:1983
357:Year
303:The
267:and
257:NASA
245:SNAP
60:Died
38:Born
790:doi
739:doi
663:doi
456:doi
890::
788:.
776:.
772:.
737:.
727:13
725:.
721:.
694:.
669:.
661:.
653:.
525:.
468:^
448:20
446:.
173:.
124:,
93:,
877:.
856:.
831:.
798:.
792::
784::
778:5
745:.
741::
733::
706:.
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679:.
665::
657::
647::
603:.
582:.
557:.
551::
536:.
487:.
462:.
458::
46:)
42:(
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.