Просмотр кода страницы Английская Википедия:Advanced Satellite for Cosmology and Astrophysics

{{Английская Википедия/Панель перехода}}
{{Use dmy dates|date=November 2016}}
{{Infobox spaceflight |auto=all
| name                  = Advanced Satellite for Cosmology and Astrophysics
| names_list            = ASTRO-D, Asuka
| image                 = ASCA.jpg
| image_caption         = 
| image_size            = 275px

| mission_type          = X-ray observatory
| operator              = [[Institute of Space and Astronautical Science|ISAS]]{{\}}[[NASA]]
| COSPAR_ID             = 1993-011A
| SATCAT                = 22521
| website               = http://heasarc.gsfc.nasa.gov/docs/asca/
| mission_duration      = Final: {{time interval|20 February 1993 02:20|2 March 2001 14:20|show=ymd|sep=,}}

| manufacturer          = [[NEC]]
| launch_mass           = {{convert|420|kg|lb|abbr=on}}
| dimensions            = {{convert|4.7|m|ft|abbr=on}} long
| power                 = <!--end-of-life power, in watts-->

| launch_date           = {{start-date|20 February 1993, 02:20}}&nbsp;UTC
| launch_rocket         = [[Mu (rocket family)|Mu-3SII]], mission M-3SII-7
| launch_site           = [[Kagoshima Space Center]], Japan
| launch_contractor     = ISAS

| disposal_type         = deorbited
| decay_date            = {{end-date|2 March 2001, 14:20}}&nbsp;UTC

| orbit_reference       = [[Geocentric orbit|Geocentric]]
| orbit_regime          = [[Low Earth orbit|Low Earth]]
| orbit_semimajor       = 
| orbit_eccentricity    = 0.01
| orbit_periapsis       = {{convert|523.6|km|mi|abbr=on}}
| orbit_apoapsis        = {{convert|615.3|km|mi|abbr=on}}
| orbit_inclination     = 31.1°
| orbit_period          = 96.09 minutes
| orbit_epoch           = 20 February 1993
| apsis                 = gee

| telescope_type        = [[Wolter telescope|Wolter]]
| telescope_diameter    = {{convert|1.2|m|ft|abbr=on}}
| telescope_focal_length= {{convert|3.5|m|ft|abbr=on}}
| telescope_area        = {{convert|1300|cm2|sqin|abbr=on}} @ 1 kev <br /> {{convert|600|cm2|sqin|abbr=on}} @ 7 keV
| telescope_wavelength  = [[X-ray]], SIS: 3–0.12&nbsp;[[nanometre|nm]] (0.4–10&nbsp;[[kiloelectronvolt|keV]])<ref>{{cite web| url=https://heasarc.gsfc.nasa.gov/docs/asca/asca_sis.html |date=2001-06-25 | access-date=2016-11-26 | title=Solid-state Imaging Spectrometers |quote= Energy Range: 0.4 keV to 10 keV keV  }}</ref> <br /> GIS: 1.8–0.12&nbsp;nm (0.7–10&nbsp;keV)<ref>{{cite web| url=https://heasarc.gsfc.nasa.gov/docs/asca/asca_gis.html |date=2005-04-01 | access-date=2016-11-26 |title=Gas Imaging Spectrometers | quote= Energy Range : 0.7 keV to 10 keV }}</ref>
| telescope_resolution  = 
| instruments_list      = {{Infobox spaceflight/Instruments
  | acronym1 = XRT | name1 = X-ray Telescope
  | acronym2 = SIS | name2 = Solid-State Imaging Spectrometer
  | acronym3 = GIS | name3 = Gas Imaging Spectrometer
 }}
}}

The '''Advanced Satellite for Cosmology and Astrophysics''' ('''ASCA''', formerly named '''ASTRO-D''') was the fourth cosmic X-ray astronomy mission by [[JAXA]], and the second for which the [[United States]] provided part of the scientific payload. The satellite was successfully launched on 20 February 1993. The first eight months of the ASCA mission were devoted to performance verification. Having established the quality of performance of all ASCA's instruments, the spacecraft provided science observations for the remainder of the mission. In this phase the observing program was open to [[astronomer]]s based at Japanese and U.S. institutions, as well as those located in member states of the [[European Space Agency]].<ref name="nasascimis"/><ref name="Tanaka">{{cite journal |title=The X-ray astronomy satellite ASCA |journal=Publications of the Astronomical Society of Japan |first1=Yasuo |last1=Tanaka |first2=Hajime |last2=Inoue |first3=Stephen S. |last3=Holt |volume=46 |issue=3 |pages=L37–L41 |date=June 1994 |bibcode=1994PASJ...46L..37T}}</ref>

==X-ray astronomy mission==
ASCA was the first [[History of X-ray astronomy|X-ray astronomy mission]] to combine imaging capability with a broad [[passband]], good [[spectral resolution]], and a large effective area. The mission also was the first satellite to use [[Charge-coupled device|CCDs]] for [[X-ray astronomy]]. With these properties, the primary scientific purpose of ASCA was the [[X-ray spectroscopy]] of astrophysical plasmas, especially the analysis of discrete features such as [[emission lines]] and [[absorption spectrum|absorption edges]].

ASCA carried four large-area [[X-ray telescope]]s. At the focus of two of the telescopes is a [[gas imaging spectrometer]] (GIS), while a [[solid-state imaging spectrometer]] (SIS) is at the focus of the other two.<ref name=nasascimis/><ref name=Tanaka/> The GIS is a gas-imaging scintillation proportional counter and is based on the GSPC that flew on the second Japanese X-ray astronomy mission, [[Tenma]]. The two identical [[charge-coupled device]] (CCD) cameras were provided for the two SISs by a hardware team from MIT, Osaka University and ISAS.

==Significant contributions==
The ASCA was launched by ISAS (Institute of Space and Astronautical Sciences), Japan.

The sensitivity of ASCA's instruments allowed for the first detailed, broad-band spectra of distant quasars to be derived. In addition, ASCA's suite of instruments provided the best opportunity at the time for identifying the sources whose combined emission makes up the cosmic X-ray background.<ref name="nasascimis">{{cite web|url=https://science.nasa.gov/missions/asca |title=ASCA |work=NASA Science Missions |publisher=NASA |archive-url=https://web.archive.org/web/20111007123952/https://science.nasa.gov/missions/asca |archive-date=7 October 2011 |url-status=dead }}</ref><ref name="Tsusaka">{{cite journal |title=Characterization of the Advanced Satellite for Cosmology and Astrophysics X-ray telescope: Preflight calibration and ray tracing |journal=Applied Optics |first1=Yoshiyuki |last1=Tsusaka |first2=Hisanori |last2=Suzuki |first3=Koujun |last3=Yamashita |first4=Hideyo |last4=Kunieda |first5=Yuzuru |last5=Tawara |first6=Yasushi|last6=Ogasaka|first7=Yasuhiro|last7=Uchibori|first8=Hirohiko|last8=Honda|first9=Masayuki|last9=Itoh|first10=Hisamitsu|last10=Awaki|first11=Hiroshi|last11=Tsunemi|first12=Kiyoshi|last12=Hayashida|first13=Susumu|last13=Nomoto|first14=Mikio|last14=Wada|first15=Emi|last15=Miyata|first16=Peter J.|last16=Serlemitsos|first17=Lalit|last17=Jalota|first18=Yang|last18=Soong|display-authors=5 |volume=34 |issue=22 |pages=4848–4856 |date=August 1995 |doi=10.1364/AO.34.004848 |bibcode=1995ApOpt..34.4848T |pmid=21052325}}</ref>

It performed over 3000 observations, and produced over 1000 publications in refereed journals so far. The ASCA archive contains significant amounts of data for future analyses. Furthermore, the mission is termed highly successful when reflecting on what scientists in many counties have accomplished using ASCA data up to this time.

The U.S. contributed significantly to ASCA's scientific payloads. In return, 40% of ASCA observing time was made available to U.S. scientists. (ISAS also opened up 10% of the time to ESA scientists as a good-will gesture.) In addition, all ASCA data enter the public domain after a suitable period (1 year for U.S. data, 18 months for Japanese data) and become available to scientists worldwide. The design of ASCA was optimized for X-ray spectroscopy; thus it complemented [[ROSAT]] (optimized for X-ray imaging) and [[RXTE]] (optimized for timing studies). Finally, ASCA results cover almost the entire range of objects, from nearby stars to the most distant objects in the universe.<ref>{{cite web |url=http://heasarc.gsfc.nasa.gov/docs/asca/outreach/asca_asca.html |title=ASCA's Significant Contributions to Astrophysics |work=ASCA Guest Observer Facility |publisher=NASA |access-date=18 November 2016}}</ref>

==Mission end==
The mission operated successfully for over 7 years until attitude control was lost on 14 July 2000 during a [[geomagnetic storm]], after which no scientific observations were performed. ASCA reentered the atmosphere on 2 March 2001 after more than 8 years in orbit.

The primary responsibility of the U.S. ASCA GOF was to enable U.S. astronomers to make the best use of the ASCA mission, in close collaboration with the Japanese ASCA team.<ref name="misend">{{cite web |url=http://heasarc.gsfc.nasa.gov/docs/asca/ascagof.html |title=The ASCA Mission: (1993-2000) |publisher=NASA |date=20 May 2011 |access-date=15 September 2011}}</ref>

==References==
{{Include-NASA}}
{{Reflist}}

==External links==
*[https://web.archive.org/web/20131030112716/http://www.isas.jaxa.jp/e/enterp/missions/asca/index.shtml ASCA website] by JAXA
*[http://heasarc.gsfc.nasa.gov/docs/asca/ ASCA website] by NASA

{{Space observatories}}
{{Japanese space program}}

{{DEFAULTSORT:Advanced Satellite For Cosmology And Astrophysics}}
[[Category:1993 in spaceflight]]
[[Category:Satellites of Japan]]
[[Category:Space program of Japan]]
[[Category:Space telescopes]]
[[Category:X-ray telescopes]]
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