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Related papers: Liquid Mirror Telescopes: A Review

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We review the present status of liquid mirror telescopes. Interferometric tests of liquid mirrors (the largest one having a diameter of 2.5 meters ) show excellent optical qualities. The basic technology is now sufficiently reliable that it…

The surface of a spinning liquid takes the shape of a paraboloid that can be used as a reflecting mirror. This very old and nearly forgotten concept has recently been revived and I review its present status. Extensive interferometric tests…

Astrophysics · Physics 2007-05-23 Ermanno F. Borra

I argue that there is a crisis in optical Astronomy due to a paucity of telescopes and thus the need for a paradigm shift in telescope technology. Large increases in collecting areas and observing time/astronomer are only possible if we…

Astrophysics · Physics 2007-05-23 E. F. Borra

We present preliminary results of observations made, during the spring of 1996, with the 3-m liquid mirror telescope of the NASA Orbital Debris Observatory. A 20-arcmin-wide strip of sky was observed at latitude of 32deg56 N using 10…

Astrophysics · Physics 2007-05-23 Remi A. Cabanac

Liquid mirror telescopes are of interest to Astronomy because of their very low capital and operating costs. Low cost has a potentially revolutionary impact since it allows one to dedicate a large telescope to a narrowly focused project…

Astrophysics · Physics 2007-05-23 Ermanno F. Borra

Interferometric tests of a f/1.2 2.5-m diameter liquid mirror show RMS surface deviations about wave/20 and Strehl ratios of order 0.6, showing that it is diffraction limited. The mirror is certainly better than implied by the data because…

Astrophysics · Physics 2009-10-30 Luc Girard , Ermanno F. Borra

I discuss the modalities of zenith observing with LMTs, their limitations and advantages. The main limitation comes from the relatively small regions of the sky that LMTs can access. The main advantage comes from low cost, for inexpensive…

Astrophysics · Physics 2007-05-23 E. F. Borra

Deformable mirrors are increasingly used in astronomy. However, they still are limited in stroke for active correction of high amplitude optical aberrations. Magnetic Liquid deformable mirrors (MLDMs) are a new technology that has…

Instrumentation and Methods for Astrophysics · Physics 2015-06-05 E. F. Borra

The results of a search for peculiar astronomical objects using very low resolution spectra obtained with the NASA Orbital Debris Observatory (NODO) 3 meter diameter liquid mirror telescope (LMT) are compared with results of spectra…

Instrumentation and Methods for Astrophysics · Physics 2015-05-27 E. F. Borra

The International Liquid Mirror Telescope (ILMT) project was motivated by the need for an inexpensive 4 metre diameter optical telescope that could be devoted entirely to astronomical surveys. Its scientific programmes include the detection…

The present article is based upon an invited talk delivered at the occasion of the inauguration of the 4m International Liquid Mirror Telescope (ILMT) which took place in Devasthal (ARIES, Uttarakhand, India) on 21st of March 2023. We…

The International Liquid Mirror Telescope (ILMT) project is a scientific collaboration in observational astrophysics between the Li{\`e}ge Institute of Astrophysics and Geophysics (Li{\`e}ge University, Belgium), the Aryabatta Research…

A 4-m International Liquid Mirror Telescope (ILMT) is being built in the north of Chile by an international consortium and will become operational in two years from now. We present here a short description of the telescope as well as…

Astrophysics · Physics 2007-05-23 C. Jean , J. -F. Claeskens , J. Surdej

We report the successful development and operation of a large astronomical liquid-mirror telescope. Employing a rotating 2.7-meter diameter mirror with a surface of liquid mercury, the telescope images a half-degree diameter field centered…

Astrophysics · Physics 2019-08-17 P. Hickson , E. F. Borra , R. Cabanac , R. Content , B. K. Gibson , G. A. H. Walker

The 4m International Liquid Mirror Telescope (ILMT) installation activities have recently been completed at the Devasthal observatory (Uttarakhand, India). The ILMT will perform continuous observation of a narrow strip of the sky…

Instrumentation and Methods for Astrophysics · Physics 2022-03-02 Brajesh Kumar , Vibhore Negi , Bhavya Ailawadhi , Sapna Mishra , Bikram Pradhan , Kuntal Misra , Paul Hickson , Jean Surdej

Mirrors are a subset of optical components essential for the success of current and future space missions. Most of the telescopes for space programs ranging from Earth Observation to Astrophysics and covering all the electromagnetic…

Instrumentation and Methods for Astrophysics · Physics 2020-10-02 D. Garoli , L. V. Rodriguez De Marcos , J. I. Larruquert , A. J. Corso , R. Proietti Zaccaria , M. G. Pelizzo

We have studied the feasibility and scientific potential of zenith observing liquid mirror telescopes having 20 to 100 m diameters located on the moon. They would carry out deep infrared surveys to study the distant universe and follow up…

The upcoming 4-m International Liquid Mirror Telescope (ILMT) facility will perform deep imaging (in single scan $g'$ $\sim$22 mag.) of a narrow strip of sky each clear night in the Time Delayed Integration mode. A cadence of one day…

Instrumentation and Methods for Astrophysics · Physics 2018-02-02 Brajesh Kumar , S. B. Pandey , Kanhaiya L. Pandey , G. C. Anupama , J. Surdej

The need for both high quality images and lightweight structures is one of the main drivers in space telescope design. An efficient wavefront control system will become mandatory in future large observatories, retaining performance while…

Instrumentation and Methods for Astrophysics · Physics 2013-05-03 Marie Laslandes , Emmanuel Hugot , Marc Ferrari , Claire Hourtoule , Christian Singer , Christophe Devilliers , Celine Lopez , Frederic Chazallet

To meet the scientific goals of the Thirty Meter Telescope Project, full diffraction-limited performance is required from the outset and hence the entire observatory is being designed, as a system, to achieve this. The preliminary design…

Astrophysics · Physics 2009-11-13 David Crampton , Luc Simard , David Silva
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