Wide Field and Planetary Camera
The Wide Field/Planetary Camera (WFPC) (pronounced as wiffpick) was a camera installed on the Hubble Space Telescope 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 bright astronomical objects, allowing for a number of discoveries to be made by HST even in its aberrated condition.
WFPC was proposed by James A. Westphal, a professor of planetary science at Caltech, and was designed, constructed, and managed by JPL. At the time it was proposed, 1976, CCDs had barely been used for astronomical imaging, though the first KH-11 KENNAN 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 Hubble Space Telescope instrumentation.
This first WFPC consisted of two separate cameras, each comprising 4 800x800 pixel Texas Instruments CCDs arranged to cover a contiguous field of view. The Wide Field camera had a 0.1 arcsecond pixel scale and was intended for the panoramic observations of faint sources at the cost of angular resolution. The Planetary Camera had a 0.043 arcsecond pixel scale and was intended for high-resolution observations. Selection between the two cameras was done with a four-facetted pyramid that rotated by 45 degrees.
As part of the corrective service mission (STS-61 in December 1993) the WFPC was swapped out for a replacement version. The Wide Field and Planetary Camera 2 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.
- Detection range, light wavelengths 115 to 1000 nm
- For the Wide Field Camera
- Field of View 2.6 x 2.6 arcminutes
- For the Planetary Camera
- Field of View 66 x 66 arcseconds
- Smallest pixel scale 0.043 arcsecond (unit of degree)
First light image
Although there was nothing known to be wrong with this instrument, the HST mirror problem meant a reduction in performance for the first few years until COSTAR was added. However, when COSTAR was added, which could correct the mirror problem WFPC was also replaced.
WFPC was replaced by the Wide Field and Planetary Camera 2, which was itself replaced by the Wide Field Camera 3 in 2009, While WFPC2 was returned to Earth, WFPC was disassembled and its parts cannibalized to make WFC3
- Wide Field and Planetary Camera 2
- Wide Field Camera 3
- Cosmic Origins Spectrograph
- Advanced Camera for Surveys
- Near Infrared Camera and Multi-Object Spectrometer
- Faint Object Camera