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ESO Awards Contracts for Cameras for New Planet Finder

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Posted August 8, 2013

ESO has signed contracts with Winlight Systems (France) for the construction of two cameras for the powerful new exoplanet-finding instrument, ESPRESSO.

ESPRESSO (Echelle SPectrograph for Rocky Exoplanet and Stable Spectroscopic Observations) is an ultra-stable spectrograph that will be installed at ESO’s Paranal Observatory in Chile in 2016. It will be capable of combining light from all four Unit Telescopes of the Very Large Telescope (VLT) to create a virtual 16-metre aperture telescope [1]. E

This picture shows an engineering rendering of the main mechanical components of the ESPRESSO instrument on ESO’s Very Large Telescope at the Paranal Observatory in northern Chile. ESPRESSO will be an ultra-precise spectrograph that is capable of combining light from all four VLT Unit Telescopes to create a virtual 16-metre aperture telescope. The instrument is mounted inside a vacuum vessel that is in turn inside two thermal isolation enclosures to shield it from external disturbances. The extensions from the top of the instrument are parts of the instrument’s two cameras, one each for the red and blue parts of the spectrum.

This picture shows an engineering rendering of the main mechanical components of the ESPRESSO instrument on ESO’s Very Large Telescope at the Paranal Observatory in northern Chile. ESPRESSO will be an ultra-precise spectrograph that is capable of combining light from all four VLT Unit Telescopes to create a virtual 16-metre aperture telescope. The instrument is mounted inside a vacuum vessel that is in turn inside two thermal isolation enclosures to shield it from external disturbances. The extensions from the top of the instrument are parts of the instrument’s two cameras, one each for the red and blue parts of the spectrum.

SPRESSO is being developed by a consortium consisting of ESO and seven further scientific institutes:

  • Centro de Astrofísica da Universidade do Porto (Portugal)
  • Faculdade de Ciências da Universidade de Lisboa, CAAUL & LOLS (Portugal)
  • INAF–Osservatorio Astronomico di Trieste (Italy)
  • INAF–Osservatorio Astronomico di Brera (Italy)
  • Instituto de Astrofísica de Canarias (Spain)
  • Physikalisches Institut der Universität Bern (Switzerland)
  • Université de Genève (Switzerland).
This engineering rendering shows the front-end part of the ESPRESSO instrument on ESO’s Very Large Telescope at the Paranal Observatory in northern Chile. ESPRESSO will be an ultra-precise spectrograph that is capable of combining light from all four VLT Unit Telescopes to create a virtual 16-metre aperture telescope. This picture shows how the beams coming in from the four different telescopes enter the instrument before being fed to the main spectrograph.

This engineering rendering shows the front-end part of the ESPRESSO instrument on ESO’s Very Large Telescope at the Paranal Observatory in northern Chile. ESPRESSO will be an ultra-precise spectrograph that is capable of combining light from all four VLT Unit Telescopes to create a virtual 16-metre aperture telescope. This picture shows how the beams coming in from the four different telescopes enter the instrument before being fed to the main spectrograph.

ESPRESSO will build on the foundations laid by the hugely successful High Accuracy Radial velocity Planet Searcher (HARPS) instrument at the 3.6-metre telescope at ESO’s La Silla Observatory. ESPRESSO will benefit not only from the much larger combined light-collecting capacity of the four 8.2-metre VLT Unit Telescopes, but also from improvements in the stability and calibration accuracy that are now possible (for example, laser frequency comb technology).

ESPRESSO is expected to allow astronomers to detect Earth-like planets around nearby stars using the radial velocity method [2]. It will also have many other science applications, including the search for possible variations of the constants of nature at different times and in different directions through the study of the light from very distant quasars.

This picture shows an engineering sample of one of the CCD detectors to be used in the cameras of the ESPRESSO instrument. These very large CCD samples were provided by the company e2v and have more than 80 million pixels over an area 92 x 92 millimetres.

This picture shows an engineering sample of one of the CCD detectors to be used in the cameras of the ESPRESSO instrument. These very large CCD samples were provided by the company e2v and have more than 80 million pixels over an area 92 x 92 millimetres.

The new contract is for the provision of the two refractive cameras, one for the red and one for the blue parts of the spectrum. These are vital components of the instrument. Utilising highly non-spherical surfaces and novel design principles, they achieve excellent image quality over a large field with only three optical elements.

Notes

[1] ESPRESSO will be the first instrument that combines light from all four Unit Telescopes at an incoherent focus. The PIONIER instrument has already achieved the combination of four beams for the purposes of interferometry, where the beams are combined coherently (ann11021).

[2] A planet in orbit around a star introduces a small and regular variation in the velocity component as measured along the line of sight (known as the radial velocity) by a distant observer on Earth. This variation can be observed as a “wobble” in the spectrum of the star as the lines shift to and fro about their central position as a result of the Doppler effect. As the planet moves away from the observer the radial velocity change induces a shift of the star’s spectrum towards longer wavelengths (a redshift) and shorter wavelengths as it moves closer (a blueshift). These tiny shifts in the star’s spectrum (corresponding to velocities as low as 10 cm/s; about the speed of a tortoise) can be measured with a high-precision spectrograph such as ESPRESSO, and can be used to infer the presence of planets.

Source: ESO

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