The Wide Field Camera 3 (WFC3) is the
Hubble Space Telescope
The Hubble Space Telescope (often referred to as HST or Hubble) is a space telescope that was launched into low Earth orbit in 1990 and remains in operation. It was not the first space telescope, but it is one of the largest and most versa ...
's last and most technologically advanced instrument to take images in the visible spectrum. It was installed as a replacement for the
Wide Field and Planetary Camera 2
The Wide Field and Planetary Camera 2 (WFPC2) is a camera formerly installed on the Hubble Space Telescope. The camera was built by the Jet Propulsion Laboratory and is roughly the size of a baby grand piano. It was installed by servicing missio ...
during the first spacewalk of Space Shuttle mission
STS-125
STS-125, or HST-SM4 (Hubble Space Telescope Servicing Mission 4), was the fifth and final Space Shuttle mission to the Hubble Space Telescope (HST) and the last solo flight of the Space Shuttle Atlantis, Space Shuttle ''Atlantis''.
The launch of ...
(Hubble Space Telescope Servicing Mission 4) on May 14, 2009.
WFC3 was still operating.
Specifications
The instrument is designed to be a versatile
camera
A camera is an Optics, optical instrument that can capture an image. Most cameras can capture 2D images, with some more advanced models being able to capture 3D images. At a basic level, most cameras consist of sealed boxes (the camera body), ...
capable of imaging astronomical targets over a very wide wavelength range and with a large field of view. It is a fourth-generation instrument for Hubble.
The instrument has two independent light paths: a UV and optical channel that uses a pair of
charge-coupled device
A charge-coupled device (CCD) is an integrated circuit containing an array of linked, or coupled, capacitors. Under the control of an external circuit, each capacitor can transfer its electric charge to a neighboring capacitor. CCD sensors are a ...
s (CCD) to record images from 200 to 1000
nm; and a near infrared detector array that covers the wavelength range from 800 to 1700 nm.
The UV/optical channel has two CCDs, each 2048×4096
pixel
In digital imaging, a pixel (abbreviated px), pel, or picture element is the smallest addressable element in a raster image, or the smallest point in an all points addressable display device.
In most digital display devices, pixels are the smal ...
s, while the IR detector is 1024×1024.
The focal planes of both channels were designed specifically for this camera. The optical channel has a field of view of 164 by 164 arcsec (2.7 by 2.7 arcminute, about 8.5% of the diameter of the full moon as seen from Earth) with 0.04 arcsec pixels. This view is comparable to the
Wide Field and Planetary Camera 2
The Wide Field and Planetary Camera 2 (WFPC2) is a camera formerly installed on the Hubble Space Telescope. The camera was built by the Jet Propulsion Laboratory and is roughly the size of a baby grand piano. It was installed by servicing missio ...
and is slightly smaller than that of the
Advanced Camera for Surveys
The Advanced Camera for Surveys (ACS) is a third-generation axial instrument aboard the Hubble Space Telescope (HST). The initial design and scientific capabilities of ACS were defined by a team based at Johns Hopkins University. ACS was assembl ...
. The near infrared channel has a field of view of 135 by 127 arcsec (2.3 by 2.1 arcminutes) with 0.13 arcsec pixels, and has a much larger field of view than
Near Infrared Camera and Multi-Object Spectrometer
The Near Infrared Camera and Multi-Object Spectrometer (NICMOS) is a scientific instrument for infrared astronomy, installed on the Hubble Space Telescope (HST), operating from 1997 to 1999, and from 2002 to 2008. Images produced by NICMOS contain ...
, which it was designed to largely replace.
The near infrared channel is a pathfinder for the future
James Webb Space Telescope
The James Webb Space Telescope (JWST) is a space telescope which conducts infrared astronomy. As the largest optical telescope in space, its high resolution and sensitivity allow it to view objects too old, distant, or faint for the Hubble Spa ...
.
Both channels have a variety of broad and narrow-band filters, as well as
prisms and
grisms, which enable wide-field, very-low-resolution spectroscopy that is useful for surveys.
The optical channel covers the visible spectrum (380 nm to 780 nm) with high efficiency, and is also able to see into the near ultraviolet (down to 200 nm).
The IR channel is designed to lack sensitivity beyond 1700 nm (as compared with the 2500 nm limit for NICMOS) to avoid being swamped by thermal background coming from the relatively warm HST structure. This allows WFC3 to be cooled using a
thermoelectric cooler instead of carrying a consumable cryogen to cool the instrument.
The camera makes use of returned space hardware as the structure is built from the original
Wide Field and Planetary Camera
The Wide Field/Planetary Camera (WFPC) (pronounced as wiffpick (Operators of the WFPC1 were known as "whiff-pickers")) was a camera installed on the Hubble Space Telescope launched in April 1990 and operated until December 1993. It was one of ...
as well as the filter assembly.
These were switched for the
Wide Field and Planetary Camera 2
The Wide Field and Planetary Camera 2 (WFPC2) is a camera formerly installed on the Hubble Space Telescope. The camera was built by the Jet Propulsion Laboratory and is roughly the size of a baby grand piano. It was installed by servicing missio ...
by the servicing mission
STS-61
STS-61 was the first NASA Hubble Space Telescope servicing mission, and the fifth flight of the Space Shuttle ''Endeavour''. The mission launched on 2 December 1993 from Kennedy Space Center (KSC) in Florida. The mission restored the spacebor ...
in December 1993.
WFC3 was originally conceived as an optical channel only; the near infrared channel was added later. WFC3 is intended to ensure that
Hubble retains a powerful imaging capability through to the end of its lifetime.
History
WFC3 had been in the planning since the Spring of 1998. It was built by a team of highly experienced Hubble engineers and scientists drawn from many organizations, with leadership at
Goddard Space Flight Center
The Goddard Space Flight Center (GSFC) is a major NASA space research laboratory located approximately northeast of Washington, D.C. in Greenbelt, Maryland, United States. Established on May 1, 1959 as NASA's first space flight center, GSFC empl ...
in
Maryland
Maryland ( ) is a state in the Mid-Atlantic region of the United States. It shares borders with Virginia, West Virginia, and the District of Columbia to its south and west; Pennsylvania to its north; and Delaware and the Atlantic Ocean to ...
. WFC3 was constructed mostly at Goddard Space Flight Center and Ball Aerospace in Colorado.
Various parts were built by contractors across the United States and the United Kingdom.
The instrument was scheduled by
NASA
The National Aeronautics and Space Administration (NASA ) is an independent agency of the US federal government responsible for the civil space program, aeronautics research, and space research.
NASA was established in 1958, succeeding t ...
to launch with
STS-125
STS-125, or HST-SM4 (Hubble Space Telescope Servicing Mission 4), was the fifth and final Space Shuttle mission to the Hubble Space Telescope (HST) and the last solo flight of the Space Shuttle Atlantis, Space Shuttle ''Atlantis''.
The launch of ...
on 14 October 2008, but the mission was postponed due to additional repairs that were required. The mission launched on 11 May 2009 and the WFC3 was installed on 14 May. by astronauts
John M. Grunsfeld and
Andrew J. Feustel
Andrew Jay "Drew" Feustel (; born August 25, 1965) is an American/Canadian NASA astronaut and geophysicist. Following several years working as a geophysicist, Feustel was selected as an astronaut candidate by NASA in July 2000. He is the vetera ...
.
WFC3 Pillars of Creation
In celebration of the 25th anniversary since the launch of the Hubble Space Telescope, astronomers assembled a larger and higher-resolution photograph of the
Pillars of Creation
''Pillars of Creation'' is a photograph taken by the Hubble Space Telescope of elephant trunks of interstellar gas and dust in the Eagle Nebula, in the Serpens constellation, some from Earth. These elephant trunks had been discovered by Jo ...
, which was unveiled in January 2015 at the American Astronomical Society meeting in Seattle. The image was photographed by the Hubble Telescope's Wide Field Camera 3, installed in 2009, and produced using near-infrared and visible light exposure.
The 1995 version of this picture of part of the Eagle nebula was taken with WFPC2.
2015 onwards
On January 8, 2019, the instrument experienced a suspected hardware problem and the onboard computer suspended operations with the WFC3 while other instruments continued operation. NASA later stated that the issue was software related and brought the instrument to normal status on January 17, 2019.
Gallery
File:HH 901 and HH 902 in the Carina nebula (captured by the Hubble Space Telescope).jpg, WFC3 view of Mystic Mountain
''Mystic Mountain'' is a photograph and a term for a region in the Carina Nebula imaged by the Hubble Space Telescope. The view was captured by the then-new Wide Field Camera 3, though the region was also viewed by the previous generation inst ...
in the Carina Nebula
File:Pillars of creation 2014 HST WFC3-UVIS full-res denoised.jpg, A higher-resolution HST image of the Pillars of Creation in the Eagle Nebula
The Eagle Nebula (catalogued as Messier 16 or M16, and as NGC 6611, and also known as the Star Queen Nebula) is a young open cluster of stars in the constellation Serpens, discovered by Jean-Philippe de Cheseaux in 1745–46. Both the "Eagle" ...
, taken in 2014 as a tribute to the original photograph
File:Jupiter on 2010-06-07 (captured by the Hubble Space Telescope).jpg, Jupiter in 2010, by WFC3
See also
HST instruments :
*
Wide Field and Planetary Camera
The Wide Field/Planetary Camera (WFPC) (pronounced as wiffpick (Operators of the WFPC1 were known as "whiff-pickers")) was a camera installed on the Hubble Space Telescope launched in April 1990 and operated until December 1993. It was one of ...
*
Wide Field and Planetary Camera 2
The Wide Field and Planetary Camera 2 (WFPC2) is a camera formerly installed on the Hubble Space Telescope. The camera was built by the Jet Propulsion Laboratory and is roughly the size of a baby grand piano. It was installed by servicing missio ...
*
Advanced Camera for Surveys
The Advanced Camera for Surveys (ACS) is a third-generation axial instrument aboard the Hubble Space Telescope (HST). The initial design and scientific capabilities of ACS were defined by a team based at Johns Hopkins University. ACS was assembl ...
*
Cosmic Origins Spectrograph
The Cosmic Origins Spectrograph (COS) is a science instrument that was installed on the Hubble Space Telescope during Servicing Mission 4 ( STS-125) in May 2009. It is designed for ultraviolet (90–320 nm) spectroscopy of faint point sources ...
*
Faint Object Camera
The Faint Object Camera (FOC) was a camera installed on the Hubble Space Telescope from launch in 1990 until 2002. It was replaced by the Advanced Camera for Surveys. In December 1993, Hubble's vision was corrected on STS-61 by installing COST ...
*
Faint Object Spectrograph
The Faint Object Spectrograph (FOS) was a spectrograph installed on the Hubble Space Telescope. It was replaced by the Space Telescope Imaging Spectrograph in 1997, and is now on display in the National Air and Space Museum in Washington DC.
FO ...
*
Goddard High Resolution Spectrograph
The Goddard High Resolution Spectrograph (GHRS or HRS) was an ultraviolet spectrograph installed on the Hubble Space Telescope during its original construction, and it was launched into space as part of that space telescope aboard the Space Shuttl ...
*
Near Infrared Camera and Multi-Object Spectrometer
The Near Infrared Camera and Multi-Object Spectrometer (NICMOS) is a scientific instrument for infrared astronomy, installed on the Hubble Space Telescope (HST), operating from 1997 to 1999, and from 2002 to 2008. Images produced by NICMOS contain ...
*
Space Telescope Imaging Spectrograph
The Space Telescope Imaging Spectrograph (STIS) is a spectrograph, also with a camera mode, installed on the Hubble Space Telescope. Aerospace engineer Bruce Woodgate of the Goddard Space Flight Center was the principal investigator and creat ...
Other space telescopes and their instruments :
*
Spitzer Space Telescope
The Spitzer Space Telescope, formerly the Space Infrared Telescope Facility (SIRTF), was an infrared space telescope launched in 2003. Operations ended on 30 January 2020. Spitzer was the third space telescope dedicated to infrared astronomy, f ...
(Great Observatory for infrared, launched 2003)
**
Infrared Array Camera
The Infrared Array Camera (IRAC) was an infrared camera system on the ''Spitzer Space Telescope'' which operated in the mid-infrared spectrum. It was composed of four detectors that operated simultaneously at different wavelengths; all four were ...
(Spitzer near to mid infrared camera)
*
NIRCam
NIRCam (Near-InfraRed Camera) is an instrument aboard the James Webb Space Telescope. It has two major tasks, as an imager from 0.6 to 5 micron wavelength, and as a wavefront sensor to keep the 18-section mirrors functioning as one. In other wor ...
(Near IR camera under 5 micron light for JWST)
References
External links
* Th
WFC3 Web siteat th
Space Telescope Science Institute which includes a description of the instrument and a link that compares the capabilities of various Hubble instruments.
NASA.gov WF3
{{Hubble Space Telescope
Hubble Space Telescope instruments
Space imagers