Barely a year has passed since its first interplanetary mission, MANGALYAAN, entered the orbit of MARS, and ISRO has crossed yet another important milestone. The ASTROSAT, is India's first attempt at setting up an observatory in space, a place from where it can study cosmological phenomena. ISRO also Launches SIX different satellite of foreign countries.
ASTROSAT, carrying five payloads, including an Ultraviolet Image Telescope, is being described as India's version of Hubble Telescope. All the payloads and instrument on ASTROSAT are meant for observation of celestial processes, and the mission is aimed at obtaining data that will help in a better understanding of the universe.
In some ways, ASTROSAT is very different mission for ISRO and will add a new dimension to its capabilities. Chandrayaan and Mangalyaan, the moon and Mars missions respectively, were essentially technology demonstration projects. But with ASTROSAT, ISRO has attempted to fulfill the core mandate of space agency- study of astronomical phenomena.
ASTROSAT has life of 5 years and has a lift-off mass of 1513kg. It has been lunched into a 650km orbit orbit inclined at an angle of 6deg to the equator by the launching vehicle PSLV-C30. After the injection into orbit, the two solar panels of ASTROSAT are automatically deployed in quick succession. The spacecraft control centre at Mission Operation Complex(MOX) of the ISRO Telemetry, Tracking and Command Network(ISTRAC) at Bangalore will manage the satellite during its mission life.
The Scientific objectives of ASTROSAT mission are :
- To understand high energy processes in binary star system containing neutron stars and black holes.
- Estimate magnetic fields of neutron stars.
- Study star birth regions and high energy process in star system lying beyond our galaxy.
- Detect new briefly bright X-Ray sources in the Sky.
- Perform a limited deep field survey of the Universe in the ultraviolet region.
Payloads of ASTROSAT :
Five payloads of ASTROSAT are chosen to facilitate a deeper insight into the various astrophysical objects constituting our universe. These payloads rely on the visible, Ultaviolet and X-rays coming from distant celestial sources.
- The Ultraviolet Image Telescope(UVIT), capable of observing the sky in the visible,Near Ultraviolet and Far Ultraviolet regions of electromagnetic spectrum.
- Large Area X-Ray Proportional Counter(LAXPC) is designed for study the variations in the emission of X-ray from source like X-ray binaries, Active Galactic Nuclei and other cosmic sources.
- Soft X-ray telescope(SXT) is designed for studying how the X-ray spectrum of 0.3-8keV range coming from distant celestial bodies varies with time.
- Cadmium Zinc Telluride Imager (CZTI) functioning in the X-ray region, extends the capability of the satellite to sense X-ray of high energy in the 10-100keV range.
- Scanning Sky Monitor(SSM) is intended to scan the sky for long term monitoring of bright X-ray sources in binary stars, and for the detection and location of sources that become bright in X-rays for a short duration.