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Galaxy And Mass Assembly survey

Galaxy And Mass Assembly survey 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 Galaxy And Mass Assembly survey rather than just read about it. In short: The Galaxy And Mass Assembly (GAMA) survey is a project that plans to exploit the latest generation of ground-based wide-field survey facilities to study cosmology and galaxy formation and evolution. GAMA plans to bring together data from a number of world class instruments: The Anglo-Australian Telescope (AAT), The VLT Survey Telescope (VST) The Visible and Infrared Survey Telescope for Astronomy (VISTA) The Austra…

Galaxy And Mass Assembly survey — main illustration
Galaxy And Mass Assembly survey — illustration

Key takeaways

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

Reference excerpt

The Galaxy And Mass Assembly (GAMA) survey is a project that plans to exploit the latest generation of ground-based wide-field survey facilities to study cosmology and galaxy formation and evolution. GAMA plans to bring together data from a number of world class instruments:

The Anglo-Australian Telescope (AAT), The VLT Survey Telescope (VST) The Visible and Infrared Survey Telescope for Astronomy (VISTA) The Australian Square Kilometre Array Pathfinder (ASKAP) The Herschel Space Observatory The Galaxy Evolution Explorer (GALEX) Data from these instruments will be used to construct a state-of-the-art multi-wavelength database of ~375,000 galaxies in the local Universe over a 360 deg2 region of sky, based on a spectroscopic redshift survey on the AAT's AAOmega spectrograph. The main objective of GAMA is to study structure on scales of 1 kpc to 1 Mpc. This includes galaxy clusters, groups, mergers and coarse measurements of galaxy structure (i.e., bulges and discs). It is on these scales where baryons play a critical role in the galaxy formation and subsequent evolutionary processes and where our understanding of structure in the Universe breaks down. GAMA's primary goal is to test the CDM paradigm of structure formation. In particular, the key scientific objectives are:

A measurement of the dark matter halo mass function of groups and clusters using group velocity dispersion measurements. A comprehensive determination of the galaxy stellar mass function to Magellanic Cloud masses to constrain baryonic feedback processes. A direct measurement of the recent galaxy merger rates as a function of mass, mass ratio, local environment and galaxy type. In August 2012 GAMA received worldwide attention for its announcement of a galaxy system very similar to our own Milky-Way Magellanic Cloud system, centred on GAMA202627.

See also Lambda-CDM model (ΛCDM) Halo mass function

References

Illustrations

Galaxy And Mass Assembly survey illustration

Worked examples

Example 1 — a first encounter with Galaxy And Mass Assembly survey

Start with the simplest possible case. Write down what Galaxy And Mass Assembly survey 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 Galaxy And Mass Assembly survey 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 Galaxy And Mass Assembly survey 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 Galaxy And Mass Assembly survey

In research
Galaxy And Mass Assembly survey 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 Galaxy And Mass Assembly survey 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
Galaxy And Mass Assembly survey is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical surveys, so understanding it makes those chapters shorter.
In everyday life
Look for Galaxy And Mass Assembly survey 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 Galaxy And Mass Assembly survey in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Galaxy And Mass Assembly survey 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 Galaxy And Mass Assembly survey out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Galaxy And Mass Assembly survey in simple terms?

The Galaxy And Mass Assembly (GAMA) survey is a project that plans to exploit the latest generation of ground-based wide-field survey facilities to study cosmology and galaxy formation and evolution. GAMA plans to bring together data from a number of world class instruments: The Anglo-Australian Te…

Why does Galaxy And Mass Assembly survey 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 Galaxy And Mass Assembly survey?

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 Galaxy And Mass Assembly survey.

Tags

  • Astronomical surveys

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