Mission type | Infrared astronomy | ||||||
---|---|---|---|---|---|---|---|
Operator | ESA / JAXA | ||||||
Website | jaxa.jp/SPICA | ||||||
Mission duration | 3 years (science mission) 5 years (design goal) [1] [2] | ||||||
Spacecraft properties | |||||||
Launch mass | 3650 kg [3] | ||||||
Payload mass | 600 kg | ||||||
Dimensions | 5.9 x 4.5 m [3] | ||||||
Power | 3 kW from a 14 m2 solar array [3] | ||||||
Start of mission | |||||||
Launch date | 2032 [4] | ||||||
Rocket | H3 [3] | ||||||
Launch site | Tanegashima, LA-Y | ||||||
Contractor | Mitsubishi Heavy Industries | ||||||
Orbital parameters | |||||||
Reference system | Sun–Earth L2 | ||||||
Regime | Halo orbit | ||||||
Epoch | Planned | ||||||
Main telescope | |||||||
Type | Ritchey-Chrétien | ||||||
Diameter | 2.5 m | ||||||
Collecting area | 4.6 m2 [5] | ||||||
Wavelengths | From 12 μm (mid-infrared) to 230 μm (far-infrared) [1] [2] | ||||||
Instruments | |||||||
| |||||||
The Space Infrared Telescope for Cosmology and Astrophysics (SPICA), was a proposed infrared space telescope, follow-on to the successful Akari space observatory. It was a collaboration between European and Japanese scientists, which was selected in May 2018 by the European Space Agency (ESA) as a finalist for the next Medium class Mission 5 (M5) of the Cosmic Vision programme, to launch in 2032. [6] At the time the other two finalists were THESEUS and EnVision, with the latter that was eventually selected for further development. [7] SPICA would have improved on the spectral line sensitivity of previous missions, the Spitzer and Herschel space telescopes, between 30 and 230 μm by a factor of 50—100. [8]
A final decision was expected in 2021, [4] but in October 2020, it was announced that SPICA was no longer being considered as a candidate for the M5 mission. [9] [10]
In Japan, SPICA was first proposed in 2007, initially called HII-L2 after the launch vehicle and orbit, as a large Strategic L-class mission, [11] [12] [13] and in Europe it was proposed to ESA's Cosmic Vision programme (M1 and M2), [11] but an internal review at ESA at the end of 2009 suggested that the technology readiness for the mission was not adequate. [14] [15] [16]
In May 2018, it was selected as one of three finalists for the Cosmic Vision Medium Class Mission 5 (M5) for a proposed launch date of 2032. [4] Within ESA, SPICA was part of the Medium Class-5 (M5) mission competition, with a cost cap of 550M Euros. [17]
It stopped being a candidate for M5 in October 2020 due to financial constraints. [9]
The concept was a collaboration between the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA). If funded, the telescope would have been launched on JAXA's H3 launch vehicle.
The Ritchey–Chrétien telescope's 2.5-metre mirror (smaller in size to the mirror of the Herschel Space Observatory) would have been made of silicon carbide, possibly by ESA given their experience with the Herschel telescope. The main mission of the spacecraft would have been the study of star and planetary formation. It would have been able to detect stellar nurseries in galaxies, protoplanetary discs around young stars, and exoplanets, helped by its own coronograph for the latter two types of objects.
The observatory would have featured a far-infrared spectrometer and was proposed to be deployed in a halo orbit around the L2 point. The design featured V-groove radiators and mechanical cryocoolers rather than liquid helium to cool the mirror to below 8 K (−265.15 °C) [2] (versus the 80 K or so of a mirror cooled only by radiation like Herschel's) which provides substantially greater sensitivity in the 10–100 μm infrared band (IR band); the telescope was intended to observe infrared light at longer wavelengths than the James Webb Space Telescope. Its sensitivity would have been more than two orders of magnitude over both the Spitzer and Herschel space telescopes. [2]
SPICA would have employed a 2.5 m diameter Ritchey–Chrétien telescope with a field of view of 30 arc minutes. [18]
As in the name, the main objective was to make advancement in the research of cosmology and astrophysics. Specific research fields include:
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.
Far-infrared astronomy is the branch of astronomy and astrophysics that deals with objects visible in far-infrared radiation.
The W. M. Keck Observatory is an astronomical observatory with two telescopes at an elevation of 4,145 meters (13,600 ft) near the summit of Mauna Kea in the U.S. state of Hawaii. Both telescopes have 10 m (33 ft) aperture primary mirrors, and, when completed in 1993 and 1996, they were the largest optical reflecting telescopes in the world. They are currently the third and fourth largest.
The Spitzer Space Telescope, formerly the Space Infrared Telescope Facility (SIRTF), was an infrared space telescope launched in 2003, that was deactivated when 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 Infrared Space Observatory (ISO) was a space telescope for infrared light designed and operated by the European Space Agency (ESA), in cooperation with ISAS and NASA. The ISO was designed to study infrared light at wavelengths of 2.5 to 240 micrometres and operated from 1995 to 1998.
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 Herschel Space Observatory was a space observatory built and operated by the European Space Agency (ESA). It was active from 2009 to 2013, and was the largest infrared telescope ever launched until the launch of the James Webb Space Telescope in 2021. Herschel carries a 3.5-metre (11.5 ft) mirror and instruments sensitive to the far infrared and submillimetre wavebands (55–672 μm). Herschel was the fourth and final cornerstone mission in the Horizon 2000 programme, following SOHO/Cluster II, XMM-Newton and Rosetta.
The Constellation-X Observatory was a mission concept for an X-ray space observatory to be operated by NASA; in 2008 it was merged with ESA and JAXA efforts in the same direction to produce the International X-ray Observatory project, announced on 24 July 2008.
Planck was a space observatory operated by the European Space Agency (ESA) from 2009 to 2013. It was an ambitious project that aimed to map the anisotropies of the cosmic microwave background (CMB) at microwave and infrared frequencies, with high sensitivity and angular resolution. The mission was highly successful and substantially improved upon observations made by the NASA Wilkinson Microwave Anisotropy Probe (WMAP).
Submillimetre astronomy or submillimeter astronomy is the branch of observational astronomy that is conducted at submillimetre wavelengths of the electromagnetic spectrum. Astronomers place the submillimetre waveband between the far-infrared and microwave wavebands, typically taken to be between a few hundred micrometres and a millimetre. It is still common in submillimetre astronomy to quote wavelengths in 'microns', the old name for micrometre.
The Great Observatories Origins Deep Survey, or GOODS, is an astronomical survey combining deep observations from three of NASA's Great Observatories: the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory, along with data from other space-based telescopes, such as XMM Newton, and some of the world's most powerful ground-based telescopes.
The Exoplanet Characterisation Observatory (EChO) was a proposed space telescope as part of the Cosmic Vision roadmap of the European Space Agency, and competed with four other missions for the M3 slot in the programme. On 19 February 2014 the PLATO mission was selected in place of the other candidates in the programme, including EChO.
The SAFARI imaging spectrometer was the European image sensor of Japanese infrared telescope SPICA and is being developed under the leadership of SRON Netherlands Institute for Space Research. SAFARI is an infrared camera with about 6,000 pixels that can make real ‘photos’ of the sky in three adjacent wavelength areas. Fourier transform spectroscopy (FTS) obtains detailed spectral information, allowing astronomers to determine the chemical composition of the observed celestial sources. The Netherlands Organisation for Applied Scientific Research (TNO) is developing the mechanism of this FTS.
SAFIR is a proposed NASA space observatory for far-infrared light. The plan calls for a single large mirror 5–10 meters (16–33 ft) in diameter, cryogenically cooled to 5 kelvins. This would feed detector arrays sensitive from 5 to 1000 μm. The possibility of servicing such a telescope in space has been evaluated.
The Habitable Exoplanet Observatory (HabEx) is a space telescope concept that would be optimized to search for and image Earth-size habitable exoplanets in the habitable zones of their stars, where liquid water can exist. HabEx would aim to understand how common terrestrial worlds beyond the Solar System may be and determine the range of their characteristics. It would be an optical, UV and infrared telescope that would also use spectrographs to study planetary atmospheres and eclipse starlight with either an internal coronagraph or an external starshade.
Origins Space Telescope (Origins) is a concept study for a far-infrared survey space telescope mission. A preliminary concept in pre-formulation, it was presented to the United States Decadal Survey in 2019 for a possible selection to NASA's large strategic science missions. Origins would provide an array of new tools for studying star formation and the energetics and physical state of the interstellar medium within the Milky Way using infrared radiation and new spectroscopic capabilities.
Transient High-Energy Sky and Early Universe Surveyor (THESEUS) is a space telescope mission proposal by the European Space Agency that would study gamma-ray bursts and X-rays for investigating the early universe. If developed, the mission would investigate star formation rates and metallicity evolution, as well as studying the sources and physics of reionization.
The Science Programme of the European Space Agency is a long-term programme of space science and space exploration missions. Managed by the agency's Directorate of Science, The programme funds the development, launch, and operation of missions led by European space agencies and institutions through generational campaigns. Horizon 2000, the programme's first campaign, facilitated the development of eight missions between 1985 and 1995 including four "cornerstone missions" – SOHO and Cluster II, XMM-Newton, Rosetta, and Herschel. Horizon 2000 Plus, the programme's second campaign, facilitated the development of Gaia, LISA Pathfinder, and BepiColombo between 1995 and 2005. The programme's current campaign since 2005, Cosmic Vision, has so far funded the development of ten missions including three flagship missions, JUICE, Athena, and LISA. The programme's upcoming fourth campaign, Voyage 2050, is currently being drafted. Collaboration with agencies and institutions outside of Europe occasionally occur in the Science Programme, including a collaboration with NASA on Cassini–Huygens and the CNSA on SMILE.
Cosmic Vision is the third campaign of space science and space exploration missions in the Science Programme of the European Space Agency (ESA). Formulated in 2005 as Cosmic Vision: Space Science for Europe 2015–2025, the campaign succeeded the Horizon 2000 Plus campaign and envisioned a number of missions in the fields of astronomy and solar system exploration beyond 2015. Ten missions across four funding categories are planned to be launched under Cosmic Vision, with the first being CHEOPS in December 2019. A mission to the Galilean moons (JUICE), the first deep space mission with an opportunistic target, and one of the first gravitational-wave space observatories (LISA), are planned for launch as part of the Cosmic Vision campaign.