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
's Very Large Telescope
. Its main feature is the spectroscopic stability and the radial velocity
precision. With incredible spectroscopic precision, it will be able to detect Earth-like planet
s. For example, our Earth induces a radial-velocity variation of 9 cm/s
on our Sun.
The requirement is to reach 10 cm/s
, but the aimed goal is to obtain a precision level of a few cm/s
. 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.
Ref:
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 (CODEXCodexA 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... |
|
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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 spectrographCORALIE spectrographThe 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 spectrographSOPHIE échelle spectrographThe 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 spectrographELODIE spectrographELODIE 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