ESPRESSO
Encyclopedia
ESPRESSO is a new-generation, high-resolution, fiber-fed and cross-dispersed echelle spectrograph (R = 140,000) for the visible wavelength range (350 nm – 720 nm), for the European Southern Observatory
European Southern Observatory
The European Southern Observatory is an intergovernmental research organisation for astronomy, supported by fifteen countries...

's Very Large Telescope
Very Large Telescope
The Very Large Telescope is a telescope operated by the European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT consists of four individual telescopes, each with a primary mirror 8.2m across, which are generally used separately but can be used together to...

. Its main feature is the spectroscopic stability and the radial velocity
Radial velocity
Radial velocity is the velocity of an object in the direction of the line of sight . In astronomy, radial velocity most commonly refers to the spectroscopic radial velocity...

 precision. With incredible spectroscopic precision, it will be able to detect Earth-like planet
Earth-like planet
Earth-like planet is used as a synonym for either of the following:* Earth analog, denoting planets of a higher degree of similarity to Earth than terrestrial planets...

s. For example, our Earth induces a radial-velocity variation of 9 cm/s
Second
The second is a unit of measurement of time, and is the International System of Units base unit of time. It may be measured using a clock....

 on our Sun.

The requirement is to reach 10 cm/s
Second
The second is a unit of measurement of time, and is the International System of Units base unit of time. It may be measured using a clock....

, but the aimed goal is to obtain a precision level of a few cm/s
Second
The second is a unit of measurement of time, and is the International System of Units base unit of time. It may be measured using a clock....

. Installation and commissioning of ESPRESSO at the VLT is foreseen in 2016.

The instrument is capable of operating in 1-UT mode and in 4-UT mode. In 4-UT mode, in which all the four 8-m telescopes are connected incoherently to form a 16-m equivalent telescope the spectrograph will reach extremely faint objects.

Sensitivity

For example (for G2V type stars):
  • Rocky Planets around stars as faint as V ~ 9 in (in 1 UT mode)
  • Neptune mass planets around stars as faint as V ~ 12 (in 4 UT mode )
  • Earth-like planets around stars as faint as V ~ 9 (CODEX
    Codex
    A codex is a book in the format used for modern books, with multiple quires or gatherings typically bound together and given a cover.Developed by the Romans from wooden writing tablets, its gradual replacement...

     on the E-ELT ) (2025)

Comparison between ESPRESSO and CODEX

ESPRESSO CODEX
Codex
A codex is a book in the format used for modern books, with multiple quires or gatherings typically bound together and given a cover.Developed by the Romans from wooden writing tablets, its gradual replacement...

Telescope
Telescope
A telescope is an instrument that aids in the observation of remote objects by collecting electromagnetic radiation . The first known practical telescopes were invented in the Netherlands at the beginning of the 1600s , using glass lenses...

VLT
VLT
VLT may stand for:* Very Large Telescope, a system of four large optical telescopes organized in an array formation, located in northern Chile...

 (8m)
E-ELT (42m)
Scope Rocky Planets Earth-Like
Sky Aperture
Aperture
In optics, an aperture is a hole or an opening through which light travels. More specifically, the aperture of an optical system is the opening that determines the cone angle of a bundle of rays that come to a focus in the image plane. The aperture determines how collimated the admitted rays are,...

1 arcsec 0.80 arcsec
R 150000 150000
λ
Lambda
Lambda is the 11th letter of the Greek alphabet. In the system of Greek numerals lambda has a value of 30. Lambda is related to the Phoenician letter Lamed . Letters in other alphabets that stemmed from lambda include the Roman L and the Cyrillic letter El...

 Coverage
350-730 nm 380-680 nm
λ
Lambda
Lambda is the 11th letter of the Greek alphabet. In the system of Greek numerals lambda has a value of 30. Lambda is related to the Phoenician letter Lamed . Letters in other alphabets that stemmed from lambda include the Roman L and the Cyrillic letter El...

 Precision
5 m/sec
Second
The second is a unit of measurement of time, and is the International System of Units base unit of time. It may be measured using a clock....

1 m/sec
Second
The second is a unit of measurement of time, and is the International System of Units base unit of time. It may be measured using a clock....

RV
Radial velocity
Radial velocity is the velocity of an object in the direction of the line of sight . In astronomy, radial velocity most commonly refers to the spectroscopic radial velocity...

 Stability
< 10 cm/s
Second
The second is a unit of measurement of time, and is the International System of Units base unit of time. It may be measured using a clock....

< 2 cm/s
Second
The second is a unit of measurement of time, and is the International System of Units base unit of time. It may be measured using a clock....

4-VLT mode
(D=16m)
with RV=1m/sec
Second
The second is a unit of measurement of time, and is the International System of Units base unit of time. It may be measured using a clock....


Ref:

See also

  • HARPS
  • HIRES
  • CORALIE spectrograph
    CORALIE spectrograph
    The CORALIE spectrograph is an echelle type spectrograph used for astronomy. This instrument used with a telescope to measure star spectra for the Doppler effect to detect the presence of extrasolar planets by the radial velocity method...

  • SOPHIE échelle spectrograph
    SOPHIE échelle spectrograph
    The SOPHIE échelle spectrograph is a high-resolution echelle spectrograph installed on the 1.93m reflector telescope at the Haute-Provence Observatory located in south-eastern France...

  • ELODIE spectrograph
    ELODIE spectrograph
    ELODIE was an echelle type spectrograph installed at the Observatoire de Haute-Provence 1.93m reflector in south-eastern France for the . Its optical instrumentation was developed by André Baranne from the Marseille Observatory. The purpose of this instrument was extrasolar planet detection by the...

  • List of extrasolar planets
The source of this article is wikipedia, the free encyclopedia.  The text of this article is licensed under the GFDL.
 
x
OK