IRAM 30-metre telescope

Alternative names	Pico Veleta observatory
Part of	Event Horizon Telescope
Location(s)	Veleta, Sierra Nevada, Dílar, Monachil, Spain
Coordinates	37°03′58″N 3°23′34″W / 37.066161°N 3.392719°W / 37.066161; -3.392719
Organization	Institut de radioastronomie millimétrique
Altitude	2,850 m (9,350 ft)
Wavelength	0.8 mm (370 GHz)–3 mm (100 GHz)
Telescope style	radio telescope
Diameter	30 m (98 ft 5 in)
Website	iram-institute.org/observatories/30-meter-telescope/
Location of IRAM 30-metre telescope
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IRAM 30m telescope is a radio telescope, located in the Sierra Nevada mountain range, Spain. It is operated by the Institute for Radio Astronomy in the Millimetre Range (IRAM) for observing astronomical objects in the millimetre range of the electromagnetic spectrum. With its large surface and wide-angle camera, the telescope is capable of exploring large cosmic objects. It is one of the largest and most sensitive millimetre wavelength telescopes in the world, serving over 200 astronomers annually. The telescope is primarily used to study interstellar clouds, star birthplaces, galaxies, and black hole jets.

Together with IRAM's second facility, the NOEMA observatory, the telescope is part of the global Event Horizon Telescope array. It was the only station in Europe to participate in the 2017 EHT observing campaign that produced the first image of a black hole.^[1]

Operation

Built from 1980 to 1984,^[2][3] the telescope operates at 2850 meters above sea level. Due to its large surface in the shape of a parabola and 420 panels adjusted to a precision of 55 micrometres, the IRAM is one of the most sensitive single dish radio telescopes in the world.^[1] The telescope can be pointed towards a celestial source, allowing astronomers to build up radio images of complete galaxies or regions of star formations.

The telescope is equipped with a suit of heterodyne receivers and continuum cameras operating at wavelengths of around 0.8, 1.0, 2.0, and 3.0 millimetres. The telescope can observe these wavelengths simultaneously, allowing it to produce multiple images of the same region in different wavelengths at once.

IRAM also offers guided tours through the observatory and public talks during the summer months. A virtual tour is provided on IRAM's website.^[4]

Science

Unlike optical astronomy telescopes, which are suitable for observing hot objects which emit visible radiation, radio telescopes that operate in the millimetre wavebands can view much colder objects that emit lower frequency radiation. For instance, supermassive black holes are very cold, with some larger black holes on the order of 10^-14 K, and as such the Event Horizon Telescope is composed of radio telescopes. Cold cosmic objects include planets, distant galaxies, and large gas clouds.^[3]

As part of the Event Horizon Telescope array, the IRAM 30-meter telescope obtained the first-ever image of a black hole. The IRAM 30-meter telescope also produced the first high-resolution radio observations of the heart of the Milky Way galaxy and its black hole named Sagittarius A* in 1995 along with the NOEMA array (formerly the Plateau de Bure Interferometer). Together with NOEMA, it discovered one-third of the interstellar molecules known to date.^[5]

Gallery

• 
  The IRAM 30-meter telescope scanning the night sky.
• 
  The IRAM 30-meter telescope.
• 
  The NOEMA observatory, IRAM's second facility.

References