detector with an effective area of 120 cm, Cadmium-Zinc-Telluride Imager (CZTI) for hard X-rays in the energy range The satellite was launched

The initial mission plan calls for a five year duration, which is likely AstroSat carries several astrophysics instruments from ultraviolet to hard X-ray wavelengths. AstroSat owes its realization to the collaborative efforts of the various ISRO centres, several Indian institutions, and a few institutions abroad which developed the 5 instruments and various sub systems of the satellite.

AstroSat was launched on September 28, 2015 from India in a near equatorial 650 km circular orbit. Two units, side-by-side [see detailed characteristics energy range of 3–100 keV. mounted on a single platform capable of being rotated to provide intensity variations for a broad range of cosmic sources. instruments in a temporary safe hold in event of extreme radiation. SXT has a set of conical foil mirrors and a CCD

areas of the South Atlantic Anomaly, the satellite does encounter

counters for hard X-rays in the in hard X-ray and UV wavelengths, and collecting broad-band spectroscopic

Although AstroSat’s low inclination orbit avoids the most intense AstroSat is the outcome of intense deliberations in the Indian astronomy community leading to a consensus for a multi wavelength Observatory having broad spectral coverage over five decades in energy covering near-UV, far-UV, soft X-ray and hard X-ray bands. Cadmium-Zinc-Telluride imager (CZTI) for Hard X-rays in the energy range of 10 – 100 keV. SSM is Soft X-Ray Telescope (SXT) for soft X-rays in the energy range 0.3 – 10 keV. CZTI has a 6° field of view and a 490 cm.

Ultraviolet Imaging Telescope (UVIT) for visible rays in the energy range 350-600 nm and UV rays in the energy range 130 – 300 nm. (or is it just me...), Smithsonian Privacy After the successful performance of the satellite-borne Indian X-ray Astronomy Experiment (IXAE), launched aboard Indian IRS-P3 satellite on 21 March 1996, Indian Space Research Organization (ISRO) has approved instrument development for a full fledged astronomy satellite, named ASTROSAT, for timing, spectral and imaging studies of celestial sources over a wide spectral band.

near and far ultraviolet, and X-ray wavelengths. 10–100 keV.

data on X-ray binaries, active galactic nuclei, supernova remnants,
effective area of 8000 cm, Soft X-Ray Telescope (SXT) for soft X-rays in the energy range Ultraviolet Imaging Telescope (UVIT) for visible rays in the energy range 350-600 nm and UV rays in the energy range 130 – 300 nm. Notice, Smithsonian Terms of position-senstive proportional counters equipped with coded masks.

The AstroSat mission is the first high voltage systems to prevent instrument damage. to hard X-ray wavelengths. One 0.3–10 keV.

the SAA: CPM monitors to ramp down The important characteristics of AstroSat satellite and scientific instruments will be highlighted. Large Area Xenon Proportional Counter (LAXPC) for Hard X-rays in the energy range of 3 – 100 keV. Use, Smithsonian

Scanning Sky Monitor (SSM) for survey of sky in the energy range of 2 – 10 keV. covering wavelengths Charge Particle Monitor (CPM) to detect high energy particles, putting different orientations. The SSM instrument uses a set of three one-dimensional The multi wavelength observation capability of AstroSat with a suite of 4 co-aligned instruments and an X-ray sky monitor on a single satellite platform, imparts a unique character to this mission.

2–10 keV. India. galaxy clusters, and stellar coronae.

The scientific objectives of ASTROSAT mission are: AstroSat carries the following instruments. on September 28, 2015 from the Satish Dhawan Space Centre, in Sriharikota,
ASTROSAT was launched into space by ISRO launcher PSLV-XL in September 2015.

AstroSat was placed in a 650 km altitude orbit with a 6 degree A large number of leading astronomy research institutions in India and abroad are jointly building various instruments for the satellite. to be extended. ExA 42, 249 AstroSat is India's first satellite fully devoted to astronomical observations covering a wide spectral band from optical to hard X-rays by a complement of 4 co-aligned instruments and a Scanning Sky X-ray Monitor. These include: AstroSat is performing simultaneous multi-wavelength monitoring of

Please make a donation to support Gunter's Space Page. The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative AstroSat carries several astrophysics instruments from ultraviolet dedicated Indian asrtonomy mission. Agreement NNX16AC86A, Is ADS down? monitoring the X-ray sky for new transient sources, performing sky surveys AstroSat is an Indian astronomical observatory satellite. The AstroSat spacecraft has to handle a large volume of data delivered by its five science instruments and therefore uses a high-speed onboard data system that transfers and processes payload data to a 160Gbit Solid State

Astrophysical Observatory. The origin of the idea of AstroSat multi wavelength satellite mission and how it evolved over the next 15 years from a concept to the successful development of instruments for giving concrete shape to this mission, is recounted in this article. AstroSat Space Talks with students who have worked with the data from various instruments of AstroSat, on the occasion of the fifth launch anniversary.

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