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Wide Field and Planetary Camera

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launched in April 1990 and operated until December 1993. It was one of the instruments on Hubble at launch, but its functionality was severely impaired by the defects of the main mirror optics which afflicted the telescope. However, it produced uniquely valuable high resolution images of relatively
105:. The Planetary Camera had a 0.043 arcsecond per pixel resolution and was intended for high-resolution observations. Selection between the two cameras was done with a four-facetted pyramid that rotated by 45 degrees. 89:
reconnaissance satellite equipped with CCDs for imaging was launched in December 1976. The high sensitivity offered such promise that many astronomers strongly argued that CCDs should be considered for
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CCDs arranged to cover a contiguous field of view. The Wide Field camera had a 0.1 arcsecond per pixel resolution and was intended for the panoramic observations of faint sources at the cost of
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improved on its predecessor and incorporated corrective optics needed to overcome the main mirror defect. To avoid potential confusion, the WFPC is now most commonly referred to as WFPC1.
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The instrument had two different cameras within, the Wide Field and the Planetary Camera. The Wide Field camera had a wider field of view compared to the Planetary Camera.
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Although there was nothing known to be wrong with this instrument, the spherical aberration in HST's mirror severely limited the performance. WFPC was replaced by the
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Astronauts practice replacing the WFPC on Earth in water tank to simulate working in space in 1993. The model being used is a full-scale training version of the WFPC
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image for the Wide Field and Planetary Camera of HST, taken in May 1990; this view is near star HD96755 in the open cluster
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The Wide Field and Planetary Camera in space while it was being exchanged for Wide Field and Planetary Camera 2 during
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bright astronomical objects, allowing for a number of discoveries to be made by HST even in its aberrated condition.
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in 2009. After return to Earth, WFPC was disassembled and its parts cannibalized to make WFC3.
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in November 1993, next to an image by its replacement instrument with corrected optics
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This first WFPC consisted of two separate cameras, each comprising 4 800x800 pixel
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On its return to Earth, the WFPC was disassembled and parts of it were used in
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which included its own internal corrective optics. WFPC2 was replaced by the
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in December 1993) the WFPC was swapped out for a replacement version. The
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had barely been used for astronomical imaging, though the first
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Corrective Optics Space Telescope Axial Replacement (COSTAR)
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Near Infrared Camera and Multi-Object Spectrometer (NICMOS)
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Detection range, light wavelengths 115 to 1000 nm
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Wide Field and Planetary Camera view of Jupiter, 1991
294:Near Infrared Camera and Multi-Object Spectrometer 1497: 399: 397: 77:, and was designed, constructed, and managed by 547:Goddard High Resolution Spectrograph (GHRS/HRS) 208:. This view is 11 by 14 arcseconds of the sky. 16:Former instrument on the Hubble Space Telescope 887: 873: 446: 394: 496:Space Telescope Imaging Spectrograph (STIS) 244:On the left, an un-corrected WFPC image of 108:As part of the corrective service mission ( 880: 866: 460: 453: 439: 562:Wide Field and Planetary Camera 2 (WFPC2) 344:(Technical report). NASA. 1982. CP-2244. 239: 227: 195: 138: 40: 32: 1516:Space hardware returned to Earth intact 756:Great Observatories Origins Deep Survey 1498: 557:Wide Field and Planetary Camera (WFPC) 378: 376: 374: 332: 81:. At the time it was proposed, 1976, 73:, a professor of planetary science at 1018:Multi-angle imaging spectroradiometer 861: 434: 840: 299:Space Telescope Imaging Spectrograph 289:Goddard High Resolution Spectrograph 191: 45:WFPC image of Messier 100 (NGC 4321) 371: 13: 1506:Hubble Space Telescope instruments 1030:Tropospheric Emission Spectrometer 164:Field of View 2.6 x 2.6 arcminutes 14: 1527: 1420:Mars Astrobiology Explorer-Cacher 1367:Nancy Grace Roman Space Telescope 787:Space Telescope Science Institute 481:Cosmic Origins Spectrograph (COS) 476:Advanced Camera for Surveys (ACS) 419: 259:Wide Field and Planetary Camera 2 219:Wide Field and Planetary Camera 2 134: 114:Wide Field and Planetary Camera 2 1485:Space Flight Operations Facility 1277:Shuttle Radar Topography Mission 839: 828: 827: 515: 509: 319:"NRO review and redaction guide" 175:Field of View 66 x 66 arcseconds 1334:Wide Field and Planetary Camera 542:Faint Object Spectrograph (FOS) 341:The Space Telescope Observatory 349: 326:National Reconnaissance Office 311: 212: 26:in Rindge, New Hampshire, see 1: 1414:Astrobiology Field Laboratory 304: 1480:Near-Earth Asteroid Tracking 1340:Wide Field Infrared Explorer 1024:Soil Moisture Active Passive 927:Atmospheric infrared sounder 357:"WFC3 - Wide Field Camera 3" 7: 999:Mars Reconnaissance Orbiter 792:Goddard Space Flight Center 782:Great Observatories program 552:High Speed Photometer (HSP) 426:Jupiter image by WFPC, 1991 274:Cosmic Origins Spectrograph 269:Advanced Camera for Surveys 252: 181:Smallest pixel scale 0.043 51:Wide Field/Planetary Camera 10: 1532: 1457:Table Mountain Observatory 501:Wide Field Camera 3 (WFC3) 486:Fine Guidance Sensor (FGS) 346:, page 28. 40 MB PDF file. 161:For the Wide Field Camera 18: 1470: 1429: 1406: 1385: 1372:Near-Earth Asteroid Scout 1354: 1283:Solar Mesosphere Explorer 1065: 962:Large Binocular Telescope 895: 889:Jet Propulsion Laboratory 823: 774: 740:Hubble eXtreme Deep Field 670: 570: 537:Faint Object Camera (FOC) 524: 507: 468: 284:Faint Object Spectrograph 172:For the Planetary Camera 1462:Solar System Ambassadors 1289:Spaceborne Imaging Radar 1447:NASA Deep Space Network 1295:Spitzer Space Telescope 1215:Mars Exploration Rovers 1006:Mars Science Laboratory 933:Deep Space Atomic Clock 706:Hubble Ultra-Deep Field 698:Hubble Deep Field South 1012:Microwave limb sounder 462:Hubble Space Telescope 388:www.spacetelescope.org 249: 237: 209: 144: 92:Hubble Space Telescope 63:Hubble Space Telescope 46: 38: 1430:Related organizations 243: 231: 199: 142: 69:WFPC was proposed by 44: 36: 1475:JPL Science Division 1209:Mars Global Surveyor 1177:Mars Climate Orbiter 815:Hubble Origins Probe 714:Extended Groth Strip 525:Previous instruments 766:List of deep fields 748:Hubble Legacy Field 681:Pillars of Creation 469:Current instruments 279:Faint Object Camera 264:Wide Field Camera 3 223:Wide Field Camera 3 125:Servicing Mission 4 121:Wide Field Camera 3 811:(2010 documentary) 761:Anniversary images 250: 238: 210: 145: 103:angular resolution 47: 39: 1493: 1492: 1452:Goldstone Complex 1407:Canceled missions 1386:Proposed missions 1203:Mars Polar Lander 855: 854: 752: 744: 736: 726: 718: 710: 702: 694: 690:Hubble Deep Field 686: 663: 649: 635: 623: 611: 594: 324:(2006 ed.). 192:First light image 99:Texas Instruments 94:instrumentation. 71:James A. 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ESA 322:(PDF) 129:WFPC2 1437:NASA 1149:IRAS 1081:Dawn 1036:SWOT 951:Juno 797:NASA 365:2009 246:M100 178:f/30 83:CCDs 55:WFPC 49:The 79:JPL 1502:: 407:. 396:^ 386:. 373:^ 131:. 881:e 874:t 867:v 662:) 648:) 634:) 622:) 610:) 593:) 454:e 447:t 440:v 411:. 390:. 367:. 328:. 53:( 30:.

Index

low-power
radio station
WFPC-LP


camera
Hubble Space Telescope
James A. Westphal
Caltech
JPL
CCDs
KH-11 KENNEN
Hubble Space Telescope
Texas Instruments
angular resolution
STS-61
Wide Field and Planetary Camera 2
Wide Field Camera 3
Servicing Mission 4
WFPC2

arcsecond

first light
NGC 3532
Wide Field and Planetary Camera 2
Wide Field Camera 3

STS-61

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