| 词条 | Small Astronomy Satellite 2 |
| 释义 |
| name = Small Astronomy Satellite 2 | image = SAS 2.gif | image_caption = Artist's impression of SAS-2 | mission_type = Earth science | operator = NASA | COSPAR_ID = 1972-091A | SATCAT = 6282 | mission_duration = 1 year | spacecraft_bus = | manufacturer = | dry_mass = | launch_mass = {{convert|166.0|kg|lb}} | power = | launch_date = {{start-date|19 November 1972 22:13:46|timezone=yes}} UTC | launch_rocket = Scout D-1 | launch_site = San Marco | last_contact = {{end-date|June 8, 1973}} | decay_date = | orbit_epoch = 1972{{vague|date=September 2013}} | orbit_reference = Geocentric | orbit_regime = Low Earth | orbit_periapsis = {{convert|443|km|mi|sp=us}} | orbit_apoapsis = {{convert|632|km|mi|sp=us}} | orbit_inclination = 1.9 degrees | orbit_semimajor = | orbit_eccentricity = 0.01366 | orbit_period = 95.40 minutes | apsis = gee | programme = Explorers | previous_mission = Explorer 47 | next_mission = Explorer 49 }} The Small Astronomy Satellite 2, also known also as SAS-2, SAS B or Explorer 48, was a NASA gamma ray telescope. It was launched on 15 November 1972 into the low Earth orbit with a periapsis of 443 km and an apoapsis of 632 km. It completed its observations on 8 June 1973.[1][2] SAS 2 was the second in the series of small spacecraft designed to extend the astronomical studies in the X-ray, gamma-ray, ultraviolet, visible, and infrared regions. The primary objective of the SAS-B was to measure the spatial and energy distribution of primary galactic and extragalactic gamma radiation which energies between 20 and 300 MeV. The instrumentation consisted principally of a guard scintillation detector, an upper and a lower spark chamber, and a charged particle telescope. SAS-2 was launched from the San Marco platform off the coast of Malindi, Kenya, into a nearly equatorial orbit. The orbiting spacecraft was in the shape of a cylinder approximately 59 cm in diameter and 135 cm in length. Four solar paddles were used to recharge the 6 amp-h nickel-cadmium battery and provide power to the spacecraft and telescope experiment. The spacecraft was spin stabilized, and a magnetically torqued commandable control system was used to point the spin axis of the spacecraft to any position in space within approximately 1 degree. The experiment axis lay along this axis allowing the telescope to look at any selected region of the sky with its plus or minus 30 degree acceptance aperture. The nominal spin rate was 1/12 rpm. Data were taken at 1000 bit/s and could be recorded on an onboard tape recorder and simultaneously transmitted in real time. The recorded data were transmitted once per orbit. This required approximately 5 minutes. The telescope experiment was initially turned on Nov 20 1972, and by Nov 27 1972, the spacecraft became fully operational. The low-voltage power supply for the experiment failed on Jun 8 1973. No useful scientific data were obtained after that date. With the exception of a slightly degraded star sensor, the spacecraft control section performed in an excellent manner. SAS-2 first detected Geminga, a pulsar believed to be the remnant of a supernova that exploded 300,000 years ago.[3] See also
Notes1. ^{{cite web | url=http://nssdc.gsfc.nasa.gov/nmc/spacecraftOrbit.do?id=1972-091A | title=NASA - NSSD - Spacecraft - Trajectory Details (SAS-B) | publisher=NASA | accessdate=2008-02-27}} 2. ^{{cite web | url=http://nssdc.gsfc.nasa.gov/nmc/spacecraftDisplay.do?id=1972-091A | title=NASA - NSSDC - Spacecraft - Details (SAS-B) | publisher=NASA | accessdate=2008-02-27}} 3. ^Geminga, The Internet Encyclopedia of Science References{{commonscat|Small Astronomy Satellite 2}}
5 : 1972 in spaceflight|Artificial satellites formerly orbiting Earth|Explorers program (NASA)|Gamma-ray telescopes|Space observatories |
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