image credit: Indian Institute of Astrophysics
BENGALURU: The Indian Institute of Astrophysics (IIA) in Bengaluru has completed ten years of operations of the
UltraViolet Imaging Telescope (UVIT) on board AstroSat, India’s first dedicated space observatory. The telescope opened
its doors on Nov 30, 2015, two months after AstroSat’s launch on Sept 28, 2015, and remains India’s only ultraviolet
space instrument. It is also one of the few operating facilities worldwide that can observe in the far-UV, apart from
the Hubble Space Telescope. In ten years, the telescope has observed 1,451 targets and contributed to about 300 research
papers and 19 doctoral theses. Findings include hot compact companions to Be stars, blue stragglers in clusters,
extended UV discs in dwarf galaxies, novae in Andromeda, UV emission from distant galaxies at redshift 1.42 and links
between UV and X-ray emission from active galactic nuclei. Improved image products are being uploaded to Isro’s PRADAN
archive, while discussions at the workshop pointed to a proposed successor mission, the Indian Spectroscopic and Imaging
Space Telescope, aimed at expanding India’s ultraviolet astronomy capability. Built and delivered by the institute from
its Hosakote campus, the telescope was designed to capture ultraviolet light that cannot be studied from the ground.
“Since UV rays are absorbed by our atmosphere, they can only be observed using space telescopes,” IIA director and
calibration scientist for the mission, Annapurni Subramaniam, said. She added that the combination of a large field of
view and a spatial resolution finer than 1.5 arcseconds (a unit of angular measurement) has kept the instrument in
steady scientific use by astronomers in India and abroad. To mark the milestone and to look ahead at future UV missions,
IIA organised a one-day academic workshop in Bengaluru on Thursday. Former Isro chairman AS Kiran Kumar, speaking at the
event, recalled the role of the late K Kasturirangan in shaping AstroSat as a multi-institutional project. He said such
coordination remains vital as academic institutions and private groups gain more opportunities to build space-based
facilities. “Our ability to understand the Universe improves whenever we discover new ways of observing and measuring,”
he said. The telescope is built as a twin system. One unit studies the near-UV (200–300 nanometres) and visible bands,
while the other captures the far-UV (130–180 nanometres). This design allows astronomers to study hot stars, young
stellar populations, compact objects, and energetic processes with greater clarity. According to CS Stalin, who heads
the payload operations centre, the set-up gives the instrument an edge over earlier ultraviolet missions, including
Nasa’s GALEX, which offered coarser resolution. Its development involved a national consortium, including
Inter-University Centre for Astronomy and Astrophysics (IUCAA) in Pune, Tata Institute of Fundamental Research (TIFR) in
Mumbai and multiple Isro centres. The institute built clean rooms at its CREST campus to assemble and test the optics
without contamination. A collaboration with the Canadian Space Agency added experience from earlier UV projects. After
launch, the payload operations centre took charge of producing science-ready data, monitoring the telescope, evaluating
proposals and updating software.