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astronomy

ESPRESSO

ESPRESSO is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand ESPRESSO rather than just read about it. In short: ESPRESSO (Echelle Spectrograph for Rocky Exoplanet- and Stable Spectroscopic Observations) is a third-generation, fiber-fed, cross-dispersed, echelle spectrograph mounted on the European Southern Observatory's Very Large Telescope (VLT). The unit saw its first light with one VLT in December 2017 and first light with all four VLT units in February 2018.

ESPRESSO — main illustration
ESPRESSO — illustration

Key takeaways

  • ESPRESSO belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect ESPRESSO to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of ESPRESSO from memory before moving on to harder problems.

Reference excerpt

ESPRESSO (Echelle Spectrograph for Rocky Exoplanet- and Stable Spectroscopic Observations) is a third-generation, fiber-fed, cross-dispersed, echelle spectrograph mounted on the European Southern Observatory's Very Large Telescope (VLT). The unit saw its first light with one VLT in December 2017 and first light with all four VLT units in February 2018. ESPRESSO is the successor of a line of echelle spectrometers that include CORAVEL, Elodie, Coralie, and HARPS. It measures changes in the light spectrum with great sensitivity, and is being used to search for Earth-size rocky exoplanets via the radial velocity method. For example, Earth induces a radial-velocity variation of 9 cm/s on the Sun; this gravitational "wobble" causes minute variations in the color of sunlight, invisible to the human eye but detectable by the instrument. The telescope light is fed to the instrument, located in the VLT Combined-Coude Laboratory 70 meters away from the telescope, where the light from up to four unit telescopes of the VLT can be combined. In 2026, a solar telescope was installed to observe our own Sun. The Paranal Solar ESPRESSO Telescope (PoET) uses a 60 cm mirror to collect light from the Sun, sending it to ESPRESSO for analysis. The telescope is capable of focusing on small features such as sun spots, and allows ESPRESSO to be used during the day, while continuing its VLT observations after sunset.

Sensitivity

ESPRESSO builds on the foundations laid by the High Accuracy Radial Velocity Planet Searcher (HARPS) instrument at the 3.6-metre telescope at ESO's La Silla Observatory. ESPRESSO benefits 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 by laser frequency comb technology. The requirement is to reach 10 cm/s, but the aimed goal is to obtain a precision level of a few cm/s. This would mean a large step forward over current radial-velocity spectrographs such as ESO's HARPS. The HARPS instrument can attain a precision of 97 cm/s (3.5 km/h), with an effective precision of the order of 30 cm/s. The ESPRESSO would greatly exceed this capability making detection of Earth-size planets from ground-based instruments possible. Commissioning of ESPRESSO at the VLT started late 2017. The instrument is capable of operating in 1-UT mode (using one of the telescopes) 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 detects extremely faint objects. For example, for G2V type stars:

Rocky planets around stars as faint as V ≈ 9 (in 1-UT mode) Neptune-mass planets around stars as faint as V ≈ 12 (in 4-UT mode ) Earth-size rocky planets around stars as faint as V ≈ 9 (CODEX on the E-ELT) The best-suited candidate stars for ESPRESSO are non-active, non-rotating, quiet G dwarfs to red dwarfs. It operates at the peak of its efficiency for a spectral type up to M4-type stars.

Instrument

In the singleHR mode ESPRESSO can be fed by any of the four UTs.

… excerpt ends here. Continue reading the full article.

Illustrations

ESPRESSO: ESPRESSO spectrograph concept at the Preliminary Design Review
ESPRESSO spectrograph concept at the Preliminary Design Review
ESPRESSO: ESPRESSO spectrograph optical design at the Preliminary Design Review
ESPRESSO spectrograph optical design at the Preliminary Design Review
ESPRESSO: Data from ESPRESSO First Light[5]
Data from ESPRESSO First Light[5]
ESPRESSO: First light of the ESPRESSO instrument with all four unit telescopes[11]
First light of the ESPRESSO instrument with all four unit telescopes[11]
ESPRESSO: Engineering rendering of the ESPRESSO instrument[13]
Engineering rendering of the ESPRESSO instrument[13]

Worked examples

Example 1 — a first encounter with ESPRESSO

Start with the simplest possible case. Write down what ESPRESSO claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to ESPRESSO before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about ESPRESSO ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of ESPRESSO

In research
ESPRESSO appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses ESPRESSO in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
ESPRESSO is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical instruments, Exoplanet search projects, Spectrographs, so understanding it makes those chapters shorter.
In everyday life
Look for ESPRESSO outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study ESPRESSO in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what ESPRESSO means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain ESPRESSO out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is ESPRESSO in simple terms?

ESPRESSO (Echelle Spectrograph for Rocky Exoplanet- and Stable Spectroscopic Observations) is a third-generation, fiber-fed, cross-dispersed, echelle spectrograph mounted on the European Southern Observatory's Very Large Telescope (VLT). The unit saw its first light with one VLT in December 2017 an…

Why does ESPRESSO matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study ESPRESSO?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on ESPRESSO.

Tags

  • Astronomical instruments
  • Exoplanet search projects
  • Spectrographs
  • Telescope instruments

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