CHIPS (satellite)

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CHIPS (Cosmic Hot Interstellar Plasma Spectrometer, also Explorer 82 or UNEX-2) was a NASA Explorer program satellite. It was launched on 12 January 2003 from Vandenberg Air Force Base aboard a Delta II with the larger satellite ICESat, and had an intended mission duration of one year. CHIPS was the second of NASA's University Explorer (UNEX) mission class. It performed spectroscopy from 90 to 250 Angstrom (9 to 26-nm) extreme ultraviolet (EUV) light.[2]

Cosmic Hot Interstellar Plasma Spectrometer
CHIPS 3D image
CHIPS (Explorer 82) satellite
NamesExplorer 82
UNEX-2
CHIPS
Mission typeExtreme ultraviolet research
OperatorNASA / Space Sciences Laboratory
COSPAR ID2003-002B Edit this at Wikidata
SATCAT no.27643
WebsiteCHIPS
Mission duration1 year (planned)
5 years, 3 months (achieved)
Spacecraft properties
SpacecraftExplorer LXXXII
Spacecraft typeCosmic Hot Interstellar Plasma Spectrometer
BusCHIPS
ManufacturerSpaceDev
Launch mass60 kg (130 lb)
Dimensions5 × 2.8 × 3.2 m (16.4 × 9.2 × 10.5 ft)
Start of mission
Launch date13 January 2003, 00:45:00 UTC
RocketDelta II 7320-10 (Delta 294)
Launch siteVandenberg, SLC-2W
ContractorBoeing Launch Services
Entered service2003
End of mission
Deactivated11 April 2008
Orbital parameters
Reference systemGeocentric orbit[1]
RegimeLow Earth orbit
Perigee altitude578 km (359 mi)
Apogee altitude594 km (369 mi)
Inclination94.05°
Period96.40 minutes
Explorer program
← RHESSI (Explorer 81)
GALEX (Explorer 83) →

Mission

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The primary objective of the science team, led by principal investigator Mark Hurwitz, was to study the million-degree gas in the local interstellar medium. CHIPS was designed to capture the first spectra of the faint, extreme ultraviolet glow that is expected to be emitted by the hot interstellar gas within about 300 light-years of the Sun, a region often referred to as the Local Bubble. Surprisingly, these measurements produced a null result, with only very faint EUV emissions detected, despite theoretical expectations of much stronger emissions. It was the first U.S. mission to use TCP/IP for end-to-end satellite operations control.

Spacecraft

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The University of California, Berkeley's Space Sciences Laboratory (SSL) served as CHIP's primary ground station and manufactured the CHIPS spectrograph, designed to perform all-sky spectroscopy. Other ground network support was provided by ground stations at Wallops Flight Facility (WFF), Virginia and Adelaide, Australia. CHIPS's satellite bus was manufactured by SpaceDev.

Launch

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CHIPS (Cosmic Hot Interstellar Plasma Spectrometer) is a NASA astrophysics spacecraft that was launched by a Delta II launch vehicle from Vandenberg Air Force Base at 00:45:00 UTC on 13 January 2003.[1] The 60 kg (130 lb), triaxially-stabilized spacecraft has a spectrograph covering the 9–26 nm wavelength band at a resolution of 0.1 nm, scanning the entire sky in chunks of 5° x 27° segments during each orbit. The targets are the hot and diffuse nebula at about a million degrees temperature. The band covers several strong emission lines.[3]

Solar observatory

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In September 2005, the spacecraft was converted to a solar observatory.[4] From 3 April 2006 to 5 April 2008, CHIPS performed 1458 observations of the Sun.[5]

End of mission

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Satellite operations were terminated in 11 April 2008 due to budget constraints.[6]

See also

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References

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  1. ^ a b "Trajectory: CHIPS (Explorer 82) 2003-002B". NASA. 28 October 2021. Retrieved 3 December 2021.   This article incorporates text from this source, which is in the public domain.
  2. ^ Cosmic Hot Interstellar Plasma Spectrometer Archived 2013-11-21 at the Wayback Machine
  3. ^ "Display: CHIPS (Explorer 82) 2003-002B". NASA. 28 October 2021. Retrieved 3 December 2021.   This article incorporates text from this source, which is in the public domain.
  4. ^ "CHIPS Latest News". Archived from the original on 18 August 2012. Retrieved 3 December 2021.
  5. ^ CHIPS Solar Science Archive Archived 2011-08-13 at the Wayback Machine
  6. ^ Sanders, Robert (2 June 2008). "06.02.2008 – Low-cost EUV satellite shut down". newsarchive.berkeley.edu. Retrieved 24 January 2024.
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