Due to the spread of COVID19 virus across the world and as per the direction given by the government on preventive measures, the visitor program at VBO is suspended until further notice
The Observatory is currently functioning and observations are being carried out in service mode. We are making best efforts to keep the Observatory functioning. We will reevaluate the situation periodically to ensure that the health of the observing staff is not affected and, if the situation warrants, may close the Observatory.
- Telescopes at VBO |
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- VBO Instruments |
- Location Of VBO |
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- Observing Conditions |
- Reaching VBO
The Vainu Bappu Observatory
The Vainu Bappu Observatory (VBO) is located in the picturesque neighbourhood of the village of Kavalur in the Javadi Hills, in the state of Tamil Nadu. Established in the 1970s, VBO hosts the 1m Carl Zeiss Telescope, the 1.3m J.C. Bhattacharya Telescope (JCBT) and the 2.3m Vainu Bappu Telescope (VBT)
Telescopes at VBO
Vainu Bappu Telescope (VBT)
The 2.34-m Vainu Bappu Telescope (VBT) is situated in the Javadi hills of Tamilnadu, at an elevation of about 750 m above the mean sea level. It is operated as a National Facility for optical astronomy. It has two foci, an f/3.5 prime focus (with an image scale of 27 arcsec/mm) and an f/13 Cassegrain focus (with a scale of 6.7 arcsec/mm). At the prime focus, CCD cameras are used for imaging with various filters. A high resolution Echelle spectrometer is in operation where the light is fed through an optical fibre from the prime focus directly to the spectrograph slit. A spectral resolution of 70000 has been achieved with the spectrograph in the visible range. By narrowing the slit, it is possible to obtain a spectral resolution better than 100,000. At the Cassegrain focus, an OMR spectrograph is used for low-to medium resolution spectroscopy. A Boller and Chivens CCD spectrograph earlier used for spectroscopy has been converted to a spectro-polarimeter.
J.C. Bhattacharya Telescope (JCBT)
1.3m Telescope was installed in the Vainu Bappu Observatory and it was named after the ex-Director of IIA, Prof J.C. Bhattacharya in April 2014. The telescope has Ritchey-Chretien F/8 optical configuration, with a primary mirror of 1.3m diameter. The field of view of the telescope is 30 minutes of arc and the plate scale is 20 arc sec/mm. It has three instrument ports. We have a 2k x 4k CCD system for direct imaging at the main port
The 1m telescope at VBO was installed in 1972. The telescope has a Ritchey-Chretien F/13 optical configuration, with a primary mirror of 1.02m diameter and with a plate scale of 15.5 arcsec/mm. The telescope is attached with a stellar optical polarimeter and a medium resolution UAGS spectrograph.
Proposals are invited for telescope time on the 2.3m VBT (National) and the 1m Zeiss telescope (IIA only). On the 1.3m JCBT, 20% time is available for non-IIA proposals. The observing cycles are for a 4-month period, and proposals are invited three times a year. The three cycle periods and their corresponding deadlines are given below.
1.3 m JCBT Online Proposal Submission
Proposal forms for 1.0m telescope (download the tex file)
Detector details for 1.3 m JCBT (download the pdf file)
Proposals to be submitted to firstname.lastname@example.org
Guidelines for VBT time allocation and Data Policy
The Vainu Bappu Observatory is located about 175 km south-east of Bangalore, and about 200 km south-west of Chennai (formerly Madras).
Latitude : 12° 34'
Longitude : +78° 50'
Altitude : ~750m
Local Time : Indian Standard Time (IST) : IST = GMT + 05 30hrs
Vainu Bappu Observatory
Indian Institute of Astrophysics
Kavalur Alangayam 635701
Vellore District Tamil Nadu
Tel : +91 4174 203119, 203118, 203117
E-Mail : anbu[At]iiap.res.in
Peninsular India is usually hit by two monsoons in a year - the southwest monsoon starting around the beginning of June, and the northeast monsoon which settles in around the end of October. The peak observing season is January - April or May.
The telescope seeing at the Zeiss 1m telescope is very close to the site seeing and is in the range of ~0".8-2" (FWHM), 1.5" being typical. The dome + mirror seeing at the Vainu Bappu Telescope (VBT) is somewhat worse; the range is ~1"-3" (FWHM), with ~2".5 being the typical value.
The nearest airport to VBO is Bangalore, which besides being an international airport, is connected by direct flights to Chennai (formerly Madras), Mumbai (formerly Bombay), New Delhi and Kolkata.
The nearest train stations are Vaniyambadi (29km from VBO) and Jolarpettai (46km from VBO), which have connections from Bangalore, Chennai , Mumbai and New Delhi.
The VBO, located near the village of Kavalur, may be reached by road from Bangalore, via Hosur-Krishnagiri-Vaniyambadi-Alangayam-Kavalur.
Information for the Public
The night sky can be seen through the 15cm telescope on every Saturday from 7 PM to 10 PM, if the sky is clear.
Vainu Bappu Observatory is 11 Kms from Alangayam, which is 18 Kms from Vaniyambadi. Vaniyambadi is on the Vellore-Bangalore highway.
The visitor program at VBO is suspended until further notice.