|
Collection:
|
|
NASA Marshall Space Flight Center Collection
Collection
NASA Marshall Space Flight Center Collection
Collection
|
|
Name of Image:
|
|
Hubble Space Telescope Image
Name_of_Image
Hubble Space Telescope Image
Name of Image
|
|
Full Description:
|
|
A comparison image of the M100 Galactic Nucleus, taken by the Hubble Space Telescope (HST) Wide Field Planetary Camera-1 (WF/PC1) and Wide Field Planetary Camera-2 (WF/PC2). The HST was placed in a low-Earth orbit by the Space Shuttle Discovery, STS-31 mission, in April 1990. Two months after its deployment in space, scientists detected a 2-micron spherical aberration in the primary mirror of the HST that affected the telescope's ability to focus faint light sources into a precise point. This imperfection was very slight, one-fiftieth of the width of a human hair. During four spacewalks, the STS-61 crew replaced the solar panel with its flexing problems; the WF/PC1 with the WF/PC2, with built-in corrective optics; and the High-Speed Photometer with the Corrective Optics Space Telescope Axial Replacement (COSTAR), to correct the aberration for the remaining instruments. The purpose of the HST, the most complex and sensitive optical telescope ever made, is to study the cosmos from a low-Earth orbit for 15 years or more. The HST provides fine detail imaging, produces ultraviolet images and spectra, and detects very faint objects.
Full_Description
A comparison image of the M100 Galactic Nucleus, taken by the Hubble Space Telescope (HST) Wide Field Planetary Camera-1 (WF/PC1) and Wide Field Planetary Camera-2 (WF/PC2). The HST was placed in a low-Earth orbit by the Space Shuttle Discovery, STS-31 mission, in April 1990. Two months after its deployment in space, scientists detected a 2-micron spherical aberration in the primary mirror of the HST that affected the telescope's ability to focus faint light sources into a precise point. This imperfection was very slight, one-fiftieth of the width of a human hair. During four spacewalks, the STS-61 crew replaced the solar panel with its flexing problems; the WF/PC1 with the WF/PC2, with built-in corrective optics; and the High-Speed Photometer with the Corrective Optics Space Telescope Axial Replacement (COSTAR), to correct the aberration for the remaining instruments. The purpose of the HST, the most complex and sensitive optical telescope ever made, is to study the cosmos from a low-Earth orbit for 15 years or more. The HST provides fine detail imaging, produces ultraviolet images and spectra, and detects very faint objects.
Full Description
|
|
Date of Image:
|
|
1994-01-01
Date_of_Image
1994-01-01
Date of Image
|
|
Category:
|
|
History of Hubble Space Telescope (HST)
Category
History of Hubble Space Telescope (HST)
Category
|
|
term:
|
|
Hubble Space Telescope
Keywords
Hubble Space Telescope
term
|
|
term:
|
|
HST
|
|
term:
|
|
Wide Field Planetary Camera
Keywords
Wide Field Planetary Camera
term
|
|
term:
|
|
WF/PC
|
|
term:
|
|
M100
|
|
term:
|
|
Galactic Nucleus
Keywords
Galactic Nucleus
term
|
|
facet_what:
|
|
Earth
facet_what
Earth
facet_what
|
|
facet_what:
|
|
Space Shuttle Orbiter
facet_what
Space Shuttle Orbiter
facet_what
|
|
facet_what:
|
|
Hubble Space Telescope (HST)
facet_what
Hubble Space Telescope (HST)
facet_what
|
|
facet_where:
|
|
M100
facet_where
M100
facet_where
|
|
facet_where:
|
|
Marshall Space Flight Center (MSFC)
facet_where
Marshall Space Flight Center (MSFC)
facet_where
|
|
facet_when:
|
|
April 1990
facet_when
April 1990
facet_when
|
|
facet_when_year:
|
|
1990
facet_when_year
1990
facet_when_year
|
|
Reference Number:
|
|
MSFC-75-SA-4105-2C
Reference_Number
MSFC-75-SA-4105-2C
Reference Number
|
|
MIX #:
|
|
9408670
|
|
NIX #:
|
|
MSFC-9408670
|
|
MSFC Negative Number:
|
|
9408670
MSFC_Negative_Number
9408670
MSFC Negative Number
|
|
UID:
|
|
SPD-MARSH-9408670
UID
SPD-MARSH-9408670
UID
|
|
original url:
|
original_url
original url
|