The 2012 National Reconnaissance Office space telescope donation to NASA was the declassification and donation to NASA of two identical space telescopes by the United States National Reconnaissance Office. The donation has been described by scientists as a substantial improvement over NASA's current Hubble Space Telescope.[ citation needed ] Although the telescopes themselves were given to NASA at no cost, the space agency must still pay for the cost of instruments and electronics for the telescopes, as well as the satellites to house them and the launch of the telescopes. On February 17, 2016, the Nancy Grace Roman Space Telescope (then known as the Wide Field Infrared Survey Telescope or WFIRST) was formally designated as a mission by NASA, predicated on using one of the space telescopes. [1]
While the Hubble Space Telescope of the National Aeronautics and Space Administration (NASA) has collected a large amount of astronomical data, has outlived all expectations, and has been described as one of the space agency's most successful missions, the facility will eventually succumb to the extreme environment of space. [2] In addition, with the James Webb Space Telescope costing at least US$9 billion, the agency's astrophysics budget is strained. As a result, NASA's other astrophysics missions have been delayed until funding becomes available. [3]
In January 2011 the National Reconnaissance Office (NRO) revealed to NASA the existence of two unneeded telescope optical systems, originally built to be used in reconnaissance satellites, and available to the civilian agency. NASA accepted the offer in August 2011 and announced the donation on 4 June 2012. [4] The instruments were constructed between the late 1990s and early 2000s, reportedly for NRO's unsuccessful Future Imagery Architecture program; [5] in addition to the two completed telescopes, a primary mirror and other parts for a third also exist. [6]
While NRO considers them to be obsolete, the telescopes are nevertheless new and unused. All charged couple devices (CCDs) and electronics have been removed, however, and NASA must add them at its own expense. When the telescopes' specifications were presented to scientists, large portions were censored due to national security. An unnamed space analyst stated that the instruments may be a part of the KH-11 Kennen line of satellites which have been launched since 1976, but which have now been largely superseded by newer telescopes with wider fields of view than the KH-11. The analyst stated, however, that the telescopes have "state-of-the-art optics" despite their obsolescence for reconnaissance purposes. [3]
The early consensus for the usage of the telescopes was to follow the NASA Astronomy and Astrophysics Decadal Survey of 2010, which lists the Wide Field Infrared Survey Telescope (now renamed the Nancy Grace Roman Space Telescope) as its highest priority. [2] [6] Observing in the infrared section of the electromagnetic spectrum, the Nancy Grace Roman Space Telescope will be used to study the role of dark energy in the Universe, as well as to directly image Jupiter-sized extrasolar planets. [7]
The NRO telescope design has several features which make it useful for Roman/WFIRST and superior to the Hubble. The NRO instrument's 2.4-meter (94 in) primary mirror is the same size and quality as the Hubble's. [3] [6] With double the mirror diameter of the original WFIRST design, it allows for up to twice the image resolution and gathers four times the light. [7] Unlike civilian telescopes, the NRO instrument also has a steerable secondary mirror for additional precision. [3] The telescope has a much wider field of view than Hubble due to its shorter focal length, allowing it to observe about 100 times the area at any given time as Hubble can. [4] This has led to the donated telescopes' characterization as "Stubby Hubbles". [7] Their obstructed design, however, may make imaging extrasolar planets more challenging, [8] and would be unsuitable for imaging the most distant galaxies at its longest infrared wavelengths, which requires cooling beyond the original NRO design temperature range. [6]
Whether using the NRO telescopes would save NASA money is unclear. While each is worth at least $250 million, their larger size compared to the proposed WFIRST design would require a larger rocket and camera. According to one NASA estimate using an NRO telescope would raise the cost of WFIRST by $250 million above its $1.5 billion budget. [6] Another estimate states that NASA would save up to $250 million. The agency's deputy acting director for astrophysics Michael Moore states that using both telescopes may ultimately save NASA $1.5 billion. [9] David Spergel estimated that using an NRO telescope would add about $100 million to WFIRST's cost, but would prefer to spend another $200 million for a coronagraph to improve its direct-imaging capability. [6]
Due to the budgetary constraints arising from the continued construction of the James Webb Space Telescope, NASA has stated that Roman/WFIRST may not be launched until 2024 at the earliest, [9] despite early speculation that by using an NRO telescope the mission might launch by roughly 2020, at about the same time as the European Space Agency's Euclid. [6] In addition, the availability of a telescope is believed to increase the probability that the mission will be launched at all. [4]
While the first telescope is now in use as the basis for Roman/WFIRST, [10] NASA currently does not have plans or funding for the usage of the second. [4] Astronomers had studied possible additional uses, [11] and NASA considered dozens of proposals; [12] the only prohibition is Earth observation, a condition of the NRO donation. [13] Possibilities include observing Earth's aurora and ionosphere, or asteroids and other faint objects within the Solar System. [6] NASA has also suggested that the telescope could be sent to Mars, photographing the surface with a resolution about four times finer than the current Mars Reconnaissance Orbiter's HiRISE instrument. From Martian orbit the telescope could also view the outer Solar System and the asteroid belt. [14]
The Hubble Space Telescope 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 versatile, renowned both as a vital research tool and as a public relations boon for astronomy. The Hubble telescope is named after astronomer Edwin Hubble and is one of NASA's Great Observatories. The Space Telescope Science Institute (STScI) selects Hubble's targets and processes the resulting data, while the Goddard Space Flight Center (GSFC) controls the spacecraft.
Infrared astronomy is a sub-discipline of astronomy which specializes in the observation and analysis of astronomical objects using infrared (IR) radiation. The wavelength of infrared light ranges from 0.75 to 300 micrometers, and falls in between visible radiation, which ranges from 380 to 750 nanometers, and submillimeter waves.
The Space Telescope Science Institute (STScI) is the science operations center for the Hubble Space Telescope (HST), science operations and mission operations center for the James Webb Space Telescope (JWST), and science operations center for the Nancy Grace Roman Space Telescope. STScI was established in 1981 as a community-based science center that is operated for NASA by the Association of Universities for Research in Astronomy (AURA). STScI's offices are located on the Johns Hopkins University Homewood Campus and in the Rotunda building in Baltimore, Maryland.
In astronomy, first light is the first use of a telescope to take an astronomical image after it has been constructed. This is often not the first viewing using the telescope; optical tests will probably have been performed to adjust the components.
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, following IRAS (1983) and ISO (1995–1998). It was the first spacecraft to use an Earth-trailing orbit, later used by the Kepler planet-finder.
The Goddard Space Flight Center (GSFC) is a major NASA space research laboratory located approximately 6.5 miles (10.5 km) northeast of Washington, D.C. in Greenbelt, Maryland, United States. Established on May 1, 1959 as NASA's first space flight center, GSFC employs approximately 10,000 civil servants and contractors. Named in recognition of American rocket propulsion pioneer Robert H. Goddard, it is one of ten major NASA field centers. GSFC is partially within the former Goddard census-designated place; it has a Greenbelt mailing address.
The National Reconnaissance Office (NRO) is a member of the United States Intelligence Community and an agency of the United States Department of Defense which designs, builds, launches, and operates the reconnaissance satellites of the U.S. federal government, and provides satellite intelligence to several government agencies, particularly signals intelligence (SIGINT) to the NSA, imagery intelligence (IMINT) to the NGA, and measurement and signature intelligence (MASINT) to the DIA. The NRO announced in 2023 that it plans within the following decade to quadruple the number of satellites it operates and increase the number of signals and images it delivers by a factor of ten.
The James Webb Space Telescope (JWST) is a space telescope designed to conduct infrared astronomy. Its high-resolution and high-sensitivity instruments allow it to view objects too old, distant, or faint for the Hubble Space Telescope. This enables investigations across many fields of astronomy and cosmology, such as observation of the first stars and the formation of the first galaxies, and detailed atmospheric characterization of potentially habitable exoplanets.
The KH-11 KENNEN is a type of reconnaissance satellite first launched by the American National Reconnaissance Office (NRO) in December 1976. Manufactured by Lockheed in Sunnyvale, California, the KH-11 was the first American spy satellite to use electro-optical digital imaging, and so offer real-time optical observations.
NASA's series of Great Observatories satellites are four large, powerful space-based astronomical telescopes launched between 1990 and 2003. They were built with different technology to examine specific wavelength/energy regions of the electromagnetic spectrum: gamma rays, X-rays, visible and ultraviolet light, and infrared light.
The Wide Field/Planetary Camera (WFPC) was a camera installed on the Hubble Space Telescope launched in April 1990 and operated 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.
Future Imagery Architecture (FIA) was a program awarded to Boeing to design a new generation of optical and radar imaging US reconnaissance satellites for the National Reconnaissance Office (NRO). In 2005 NRO director Donald Kerr recommended the project's termination, and the optical component of the program was finally cancelled in September 2005 by Director of National Intelligence John Negroponte. FIA has been called by The New York Times "perhaps the most spectacular and expensive failure in the 50-year history of American spy satellite projects." Despite the optical component's cancellation, the radar component, known as Topaz, has continued, with four satellites in orbit as of February 2016.
The Wide Field Camera 3 (WFC3) is the Hubble Space Telescope'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 during the first spacewalk of Space Shuttle mission STS-125 on May 14, 2009.
Cornelis A. "Neil" Gehrels was an American astrophysicist specializing in the field of gamma-ray astronomy. He was Chief of the Astroparticle Physics Laboratory at NASA's Goddard Space Flight Center (GSFC) from 1995 until his death, and was best known for his work developing the field from early balloon instruments to today's space observatories such as the NASA Swift mission, for which he was the principal investigator. He was leading the WFIRST wide-field infrared telescope forward toward a launch in the mid-2020s. He was a member of the National Academy of Sciences and the American Academy of Arts and Sciences.
The Joint Dark Energy Mission (JDEM) was an Einstein probe that planned to focus on investigating dark energy. JDEM was a partnership between NASA and the U.S. Department of Energy (DOE).
The Nancy Grace Roman Space Telescope is a NASA infrared space telescope in development and scheduled to launch by May 2027.
Bertram Raoul Bulkin was an American aeronautical engineer who participated in the first United States photo-reconnaissance satellite programs and is best known for his role in building the Hubble Space Telescope.
Michael Logan Lampton was an American astronaut, scientist, and founder of the optical ray tracing company Stellar Software. He was also known for his paper on electroacoustics with Susan M Lea, The theory of maximally flat loudspeaker systems.
The NIRSpec is one of the four scientific instruments flown on the James Webb Space Telescope (JWST). The JWST is the follow-on mission to the Hubble Space Telescope (HST) and is developed to receive more information about the origins of the universe by observing infrared light from the first stars and galaxies. In comparison to HST, its instruments will allow looking further back in time and will study the so-called Dark Ages during which the universe was opaque, about 150 to 800 million years after the Big Bang.
The Large Ultraviolet Optical Infrared Surveyor, commonly known as LUVOIR, is a multi-wavelength space telescope concept being developed by NASA under the leadership of a Science and Technology Definition Team. It is one of four large astrophysics space mission concepts studied in preparation for the National Academy of Sciences 2020 Astronomy and Astrophysics Decadal Survey.