HST SM4 COS Installation EVA
Cosmic Origins Spectrograph (COS) will be the most sensitive ultraviolet spectrograph ever flown on Hubble. COS will probe the "cosmic web" - the large-scale structure of the universe whose form is determined by the gravity of dark matter and is traced by galaxies and intergalactic gas. COS will explore how the "cosmic web" evolved from ancient times. COS will also sample the chemical content and physical state of gas in distant galaxy halos, providing important insight into the building process of early galaxies and the production of elements heavier than hydrogen and helium over cosmic time. Required to accomplish these goals is the extraordinary sensitivity of COS's far-ultraviolet channel—a factor more than 30 times greater than that of previous spectroscopic instruments for the detection of extremely low light levels. A two-fold enhancement will be offered by COS's near-ultraviolet channel. To install the COS instrument into the Hubble Space Telescope, he Servicing Mission 4 astronauts will remove the Corrective Optics Space Telescope Axial Replacement (COSTAR) instrument (installed during Servicing Mission 1 in 1993, to correct for Hubble's spherical aberration) and then install COS in its place.
HST SM4 COS Installation EVA completed and edited animation sequence.
Animated sequence depicting the removal of the Corrective Optics Space Telescope Axial Replacement (COSTAR) instrument and the installation of the Cosmic Origins Spectrograph (COS) during Hubble Space Telescope Servicing Mission 4.
Animated sequence depicting the removal of the Corrective Optics Space Telescope Axial Replacement (COSTAR) instrument and the installation of the Cosmic Origins Spectrograph (COS) during Hubble Space Telescope Servicing Mission 4.
Animated sequence depicting the removal of the Corrective Optics Space Telescope Axial Replacement (COSTAR) instrument and the installation of the Cosmic Origins Spectrograph (COS) during Hubble Space Telescope Servicing Mission 4.
Animated sequence depicting the removal of the Corrective Optics Space Telescope Axial Replacement (COSTAR) instrument and the installation of the Cosmic Origins Spectrograph (COS) during Hubble Space Telescope Servicing Mission 4.
Animated sequence depicting the removal of the Corrective Optics Space Telescope Axial Replacement (COSTAR) instrument and the installation of the Cosmic Origins Spectrograph (COS) during Hubble Space Telescope Servicing Mission 4.
Animated sequence depicting the removal of the Corrective Optics Space Telescope Axial Replacement (COSTAR) instrument and the installation of the Cosmic Origins Spectrograph (COS) during Hubble Space Telescope Servicing Mission 4.
Credits
Please give credit for this item to:
NASA Goddard Space Flight Center
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Animator
- Bob Sauls (Frassanito and Associates)
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Producer
- Michael McClare (HTSI)
Release date
This page was originally published on Friday, August 22, 2008.
This page was last updated on Wednesday, May 3, 2023 at 1:55 PM EDT.
Series
This page can be found in the following series:Datasets used
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[HST: WFPC2]
ID: 655Wide-Field Planetary Camera 2 (WFPC2) was installed in Dec 1993 and used to obtain high resolution images of astronomical objects. This camera was removed in the last servicing mission so it is no longer in service.
This dataset can be found at: http://www.stsci.edu/hst/wfpc2/wfpc2_diag.html
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Note: While we identify the data sets used on this page, we do not store any further details, nor the data sets themselves on our site.