National Aeronautics and Space Administration Logo
Follow this link to skip to the main content NASA Banner
Solar System Exploration
Missions
Spitzer Space Telescope
Missions to Our Solar System
 By Target   By Name   By Decade 
Beyond Our Solar System Our Solar System Sun Mercury Venus Moon Earth Mars Dwarf Planets Dwarf Planets Dwarf Planets Asteroids Comets Jupiter Saturn Uranus Neptune Kuiper Belt
 
 Past 
 Present 
 Future 
 Concepts 
Spitzer
Spitzer Space Telescope Mission to Our Solar System

Mission Type: Orbiter
Launch Vehicle: Delta II, Model 7920H
Launch Site: Pad 17-B, Cape Canaveral Air Force Station, Fla.
NASA Center: Jet Propulsion Laboratory
Spacecraft Mass: 865 kg at launch
Spacecraft Instruments: 1) Telescope; 2) Infrared array camera; 3) Infrared spectrograph; and 4) Multiband imaging photometer
Spacecraft Dimensions: 4.45 m long, 2.1 m in diameter
Spacecraft Power: Solar
Maximum Power: 400 watts
Program Manager: Lia LaPiana, NASA HQ
Project Manager: David Gallagher. Jet Propulsion Laboratory
Principal Scientists: Dr. Michael Werner, Jet Propulsion Laboratory; Dr. Jay Frogel, NASA HQ
Total Cost: $1.19 billion (including launch vehicle, observatory, mission operations and data analysis)
References:
Space Infrared Telescope Faciility Launch Press Kit, NASA, August 2003.


Spitzer Space Telescope, originally known as the Space Infrared Telescope Facility (SIRTF), was an orbiting observatory that studied the early universe, distant galaxies and newly forming stars and planets. It was also the fourth and final mission of NASA's Great Observatories, a series that has included the Hubble Space Telescope, the Chandra X-Ray Observatory and the Compton Gamma Ray Observatory.

The observatory consisted of an 85-centimeter-diameter (33.5-inch) telescope and three cryogenically cooled science instruments. The science instruments performed imaging and spectroscopy -- breaking light into different colors, like a prism, so the chemical composition of an object can be determined. Observations were conducted in the infrared to detect objects and processes in the universe that are either too cool or too dust-enshrouded to be seen otherwise. The observatory launched into an orbit that trailed Earth as it goes around the Sun. This unique orbit placed the observatory in deep space, far from the heat generated by Earth itself.

Spitzer also was unique in that it was smaller and lighter than past missions involving cryogenically cooled telescopes. In past missions, a vacuum shell surrounded the telescope like a thermos bottle, actively chilling the observatory and science instruments. On Spitzer, the vacuum shell surrounds only the instrument chamber and the liquid helium tank. Engineers refer to this configuration as a warm launch architecture. It means that much less coolant is needed, allowing for the use of a relatively smaller launch vehicle. The configuration allowed Spitzer to collect science data for more than five years -- twice the length of the longest previous infrared mission.

Spitzer was only one-third as long and one-eleventh the weight of its bigger sibling, the Hubble Space Telescope. The four-meter-tall (14.6-foot), 865-kilogram (1,907-pound) observatory enclosed a cryogenically cooled telescope and three science instruments - a multiband imaging photometer, an infrared spectrometer and an infrared-detector array camera - as well as all the required power, computer, communications and navigation equipment.

The telescope was cooled using extremely cold liquid helium. Over the course of the mission, this ultra-cold helium slowly leaked out into space. After five and a half years, all of the helium was lost and the spacecraft was reconfigured for an extended mission observing warmer targets.

The heart of Spitzer was an 85-centimeter-diameter (about 33.5-inch) telescope and three cryogenically cooled science instruments that performed imaging and spectroscopy at wavelengths from about 3 to 180 microns.

Like the Hubble Space Telescope, Spitzer was a Cassegrain design, named for the French sculptor Guillaume Cassegrain, who invented it in 1672. Light from distant objects in space enters the telescope and is reflected by a primary mirror at the telescope's rear. The light is then gathered onto a smaller secondary mirror suspended in the middle of the telescope near the front end. The light in turn reflects back toward the rear of the telescope, where it passes through a hole in the middle of the primary mirror. At the rear, behind the primary mirror, is the sensor that records the image. Spitzer's telescope weighed less than 50 kilograms (about 110 pounds).


Key Dates
25 Aug 2003:  Launch (01:35:39 EDT)
15 May 2009:  Extended Mission Begins
Status: Extended Mission in Progress
Fast Facts
Spitzer Facts Spitzer was the last of NASA's Great Observatories, which included Hubble Space Telescope, the Chandra X-Ray Observatory and the Compton Gamma Ray Observatory.

Instead of orbiting Earth like other space telescopes, Spitzer tagged along behind Earth as it orbits our Sun. This keeps it clear of Earth's heat and makes for better pictures.

Spizer saw every part of the sky at least every six months during its 5 1/2-year primary mission..
Science & Technology Features
People Spotlight
Edward Weiler Edward Weiler
Dr. Edward J. Weiler was named Associate Administrator of the Science Mission Directorate at NASA Headquarters in Washington, D.C. in May 2008. Read More...
Headlines
Links
Awards and Recognition   Solar System Exploration Roadmap   Contact Us   Site Map   Print This Page
NASA Official: Kristen Erickson
Advisory: Dr. James Green, Director of Planetary Science
Outreach Manager: Alice Wessen
Curator/Editor: Phil Davis
Science Writer: Autumn Burdick
Producer: Greg Baerg
Webmaster: David Martin
> NASA Science Mission Directorate
> Budgets, Strategic Plans and Accountability Reports
> Equal Employment Opportunity Data
   Posted Pursuant to the No Fear Act
> Information-Dissemination Policies and Inventories
> Freedom of Information Act
> Privacy Policy & Important Notices
> Inspector General Hotline
> Office of the Inspector General
> NASA Communications Policy
> USA.gov
> ExpectMore.gov
> NASA Advisory Council
> Open Government at NASA
Last Updated: 1 Dec 2010