SPICA (spacecraft)
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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 , owners = , headquarters = Paris, Île-de-France, France , coordinates = , spaceport = Guiana Space Centre , seal = File:ESA emblem seal.png , seal_size = 130px , image = Views in the Main Control Room (1205 ...
(ESA) as a finalist for the next Medium class Mission 5 of the Cosmic Vision programme, to launch in 2032. At the time the other two finalists were THESEUS and EnVision, with the latter that was eventually selected for further development. 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. A final decision was expected in 2021, but in October 2020, it was announced that SPICA was no longer being considered as a candidate for the M5 mission.


History

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,Cosmic Vision programme (M1 and M2), but an internal review at ESA at the end of 2009 suggested that the technology readiness for the mission was not adequate. 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. Within ESA, SPICA was part of the Medium Class-5 (M5) mission competition, with a cost cap of 550M Euros. It stopped being a candidate for M5 in October 2020 due to financial constraints.


Overview

The concept was a collaboration between the
European Space Agency , owners = , headquarters = Paris, Île-de-France, France , coordinates = , spaceport = Guiana Space Centre , seal = File:ESA emblem seal.png , seal_size = 130px , image = Views in the Main Control Room (1205 ...
(ESA) and the
Japan Aerospace Exploration Agency The is the Japanese national air and space agency. Through the merger of three previously independent organizations, JAXA was formed on 1 October 2003. JAXA is responsible for research, technology development and launch of satellites into orb ...
(JAXA). If funded, the telescope would have been launched on JAXA's H3 launch vehicle. The
Ritchey–Chrétien telescope A Ritchey–Chrétien telescope (RCT or simply RC) is a specialized variant of the Cassegrain telescope that has a hyperbolic primary mirror and a hyperbolic secondary mirror designed to eliminate off-axis optical errors (coma). The RCT has a wi ...
's 2.5-metre mirror (similar in size to the mirror of the
Herschel Space Observatory 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 Telesc ...
) 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 A star is an astronomical object comprising a luminous spheroid of plasma (physics), plasma held together by its gravity. The List of nearest stars and brown dwarfs, nearest star to Earth is the Sun. Many other stars are visible to the naked ...
and
planetary formation The nebular hypothesis is the most widely accepted model in the field of cosmogony to explain the formation and evolution of the Solar System (as well as other planetary systems). It suggests the Solar System is formed from gas and dust orbiting t ...
. It would have been able to detect stellar nurseries in
galaxies A galaxy is a system of stars, stellar remnants, interstellar gas, dust, dark matter, bound together by gravity. The word is derived from the Greek ' (), literally 'milky', a reference to the Milky Way galaxy that contains the Solar System. ...
, protoplanetary discs around young stars, and exoplanets, helped by its own coronograph for the latter two types of objects.


Description

The observatory would have featured a far-infrared spectrometer and was proposed to be deployed in a
halo orbit A halo orbit is a periodic, three-dimensional orbit near one of the L1, L2 or L3 Lagrange points in the three-body problem of orbital mechanics. Although a Lagrange point is just a point in empty space, its peculiar characteristic is that it ca ...
around the
L2 point In celestial mechanics, the Lagrange points (; also Lagrangian points or libration points) are points of equilibrium for small-mass objects under the influence of two massive orbiting bodies. Mathematically, this involves the solution of th ...
. The design featured V-groove radiators and mechanical
cryocooler A refrigerator designed to reach cryogenic temperatures (below ) is often called a cryocooler. The term is most often used for smaller systems, typically table-top size, with input powers less than about 20 kW. Some can have input powers as lo ...
s rather than liquid helium to cool the mirror to below
like Herschel's) which provides substantially greater sensitivity in the 10–100
μm The micrometre ( international spelling as used by the International Bureau of Weights and Measures; SI symbol: μm) or micrometer (American spelling), also commonly known as a micron, is a unit of length in the International System of Unit ...
infrared band (IR band); the telescope was intended to observe infrared light at longer wavelengths than the
James Webb Space Telescope The James Webb Space Telescope (JWST) is a space telescope which conducts infrared astronomy. As the largest optical telescope in space, its high resolution and sensitivity allow it to view objects too old, distant, or faint for the Hubble Spa ...
. Its sensitivity would have been more than two orders of magnitude over both the Spitzer and Herschel space telescopes. ;Large-aperture Cryogenic Telescope SPICA would have employed a 2.5 m diameter
Ritchey–Chrétien telescope A Ritchey–Chrétien telescope (RCT or simply RC) is a specialized variant of the Cassegrain telescope that has a hyperbolic primary mirror and a hyperbolic secondary mirror designed to eliminate off-axis optical errors (coma). The RCT has a wi ...
with a field of view of 30 arc minutes. ;Focal-Plane Instruments * SMI (SPICA Mid-infrared Instrument): 12–36 μm ** SMI-LRS (Low-Resolution Spectroscopy): 17–36 μm. Its aim would have been the detection of PAH dust emission as a clue of distant galaxies and emission of minerals from planet formation regions around stars ** SMI-MRS (Mid-Resolution Spectroscopy): 18–36 μm. Its high sensitivity for line emission with a relatively high wavelength resolution (R=2000) would have enabled the characterization of distant galaxies and planet formation regions detected by SMI-LRS ** SMI-HRS (High-Resolution Spectroscopy): 12–18 μm. With its extremely high wavelength resolution (R=28000), SMI-HRS could study the dynamics of molecular gas in planet formation regions around stars *
SAFARI A safari (; ) is an overland journey to observe wild animals, especially in eastern or southern Africa. The so-called "Big Five" game animals of Africa – lion, leopard, rhinoceros, elephant, and Cape buffalo – particularly form an importa ...
(SPICA Far-infrared Instrument): 35–230 μm * B-BOP (B-BOP stands for "B-fields with BOlometers and Polarizers"): Imaging polarimeter operating in three bands, 100 μm, 200 μm and 350 μm. B-Bop would have enabled the polarimetric mapping of Galactic filamentary structures to study the role of magnetic fields in filaments and star formation.


Objectives

As in the name, the main objective was to make advancement in the research of cosmology and astrophysics. Specific research fields include: * The birth and evolution of galaxies * The birth and evolution of stars and planetary systems * The evolution of matter


Discovery science

* Setting constraints on the emission of ground state Н2 emission from the first (population III) generation of stars * The detection of biomarkers in the mid-infrared spectra of exo-planets and/or the primordial material in protoplanetary disks * The detection of Н2 haloes around galaxies in the local Universe * With sufficient technical development of coronagraphic techniques: the imaging of any planets in the habitable zone in the nearest few stars * The detection of the far infrared transitions of polycyclic aromatic hydrocarbons (PAHs) in the interstellar medium. The very large molecules thought to comprise the PAHs, and which give rise to the characteristic features in the near-infrared, have vibrational transitions in the far-infrared which are widespread and extremely weak * The direct detection of dust formation in super novae in external galaxies and the determination of the origin of the large amounts of dust in high redshift galaxies


See also

* Akari *
ALMA Alma or ALMA may refer to: Arts and entertainment * ''Alma'' (film), a 2009 Spanish short animated film * ''Alma'' (Oswald de Andrade novel), 1922 * ''Alma'' (Le Clézio novel), 2017 * ''Alma'' (play), a 1996 drama by Joshua Sobol about Alma ...
*
Herschel Space Observatory 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 Telesc ...
*
James Webb Space Telescope The James Webb Space Telescope (JWST) is a space telescope which conducts infrared astronomy. As the largest optical telescope in space, its high resolution and sensitivity allow it to view objects too old, distant, or faint for the Hubble Spa ...
* Origins Space Telescope


References


External links


SPICA mission homepage



Homepage at the European Space Agency

SPICA / SAFARI at JPL
* . JAXA
Sagamihara is a city in Kanagawa Prefecture, Japan. , the city has an estimated population of 723,470, with 334,812 households, and a population density of 1,220 persons per km2. The total area of the city is . Sagamihara is the third-most-populous city ...
{{DEFAULTSORT:SPICA telescope Infrared telescopes Japanese space probes Cosmic Vision Proposed space probes Spacecraft using halo orbits Artificial satellites at Earth-Sun Lagrange points