Telescopio Nazionale Galileo
Coordinates: 28°45′14.4″N 17°53′20.6″W / 28.754000°N 17.889056°W
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The dome of the Telescopio Nazionale Galileo near time of sunset. | |
| Organization | Italian National Institute of Astrophysics (INAF) |
|---|---|
| Location | Roque de los Muchachos Observatory, La Palma (Canary Islands) |
| Wavelength | optical, near-infrared |
| Built | 1998 (first light) |
| Telescope style | Ritchey-Chretien |
| Diameter | 3.58 m |
| Collecting area | ~12 m2 |
| Mounting | altazimuthal |
| Website | http://www.tng.iac.es/ |
The Telescopio Nazionale Galileo, or TNG, is a 3.58m Italian telescope located on the island of San Miguel de La Palma (or, more simply, La Palma), in the Canary Islands archipelago. It is one of the largest telescopes hosted by the Roque de los Muchachos Observatory, a very important observing site in the northern hemisphere. It is now operated by the "Fundación Galileo Galilei, Fundación Canaria", a no-profit institution which manages the telescope on behalf of INAF, the Italian National Institute of Astrophysics. The telescope saw its first light in 1998.
Observations at the TNG can be proposed through the Italian Time Allocation Committee (TAC) which assigns, based on the scientific merit of the proposals, 75% of the available time. The rest of the time is at disposal of the Spanish and international astronomical communities. The TNG is open to new proposals two times a year, typically in March–April and September–October.
Technical characteristics
The TNG is an altazimuthal reflecting telescope with a Ritchey-Chretien optical configuration and a flat tertiary mirror feeding two opposite Nasmyth foci. It has a design derived from the New Technology Telescope (NTT), an ESO 4-meters class telescope located in La Silla (Chile). Therefore, the optical quality of the telescope is ensured by an active optics system performing real-time corrections of the optical components and compensating, in particular, for the deformations of the primary mirror, which is too thin to be completely rigid.
The interface between the telescope fork and the instruments at both Nasmyth foci is provided by two rotator/adapters. Their main function is to compensate for the field rotation by a mechanical counter rotation. The best quality of the TNG is that all the available instruments are permanently mounted at the telescope. This guarantees flexibility during an observing session, since it is possible to change instrument during the night with a loss of time limited to a few minutes.
The science based on observational data from the TNG is varied. Proposed observing programs go from the study of the planets and minor bodies of the solar system up to researches of cosmological interest (e.g. large-scale structure of the Universe and systems of galaxies).
Scientific instruments
The TNG is equipped with four instruments:
- HARPS-N ("High Accuracy Radial velocity Planet Searcher"), echelle spectrograph dedicated to the discovery of extrasolar planets;
- DOLoRes ("Device Optimized for the Low Resolution"), CCD camera and low-resolution spectrograph for observations in the visible band;
- NICS ("Near Infrared Camera and Spectrometer"), camera and spectrograph for observations in the near-infrared;
- GIANO, high-resolution echelle spectrograph for observations in the near-infrared.
Decommissioned instruments:
- SARG ("Spettrografo ad Alta Risoluzione del Galileo"), high-resolution spectrograph for observations in the visible band;
- OIG ("Optical Imager Galileo"), CCD camera dedicated to optical images at high resolution;
- Speckle camera, dedicated to observations in the visible band at the diffraction limit of the telescope;
- AdOpt@TNG, adaptive optics system working in the near-infrared.