galaxy

Galactic archaeology

Employs galactic archaeology to explore the Milky Way's history and structure by analysing the properties of stars, gas, and other celestial bodies, aided significantly by the SkyMapper Southern Sky Survey.

About

Like traditional archaeologists, who study human history by investigating the remnants that can be excavated and observed today, galactic archaeologists trace the history and formation of the Milky Way galaxy from detailed observations of the stars, gas and other structures that can be observed from Earth.  

Researchers at RSAA work on a wide range of areas and problems within this theme, including:

  • understanding the chemical and dynamical properties of different stellar populations in the Galaxy
  • searching for extremely metal-poor stars, which include the oldest stars that formed early in the history of the Galaxy
  • investigating the nature and origins of globular clusters
  • searching for satellite galaxies of the Milky Way 
  • mapping the structure of the galaxy, including stellar streams and substructure formed during the accretion of neighbouring galaxies
  • studying the properties of the Large and Small Magellanic Clouds, dwarf galaxies that are relatively nearby neighbours to our Galaxy.

The Southern Sky Survey that is being carried out by the SkyMapper telescope will be instrumental to scientists studying the properties of the Milky Way, since it will provide a census of over 5 billion stars in the Galaxy. The instrument and survey design will allow astronomers to derive measurements of metallicity, gravity, temperature, and variability for many of these stars, and to continue to map the structure of the Milky Way and the Magellanic Clouds in increasing detail.

Projects

Ambitious students will investigate optimal ways to measure the stellar properties (eg Teff, age, mass) and chemical composition of this immense amount of data.

In this project you will use existing and new data to understand the nature of filamentary structure in galaxies and how they relate to magnetic fields.

Student intake

Open for Bachelor, Honours, PhD students

People

In the spectra of distant stars, we can often find a series of absorption features, such as Diffuse Interstellar Bands (DIBs) or those of neutral atomic potassium, K I. Although the exact carriers of DIBs are still a matter of debate, various candidates have been proposed over the years.

Student intake

Open for Bachelor students

People

Dust in the Milky Way affects astronomical observations. Here we try too improve our knowledge of its distribution.

Magnetic fields are present throughout the universe on all scales: from planets and stars, star-forming clusters and spiral arms, entire galaxies, to galaxy clusters and cosmic filaments.

Student intake

Open for Bachelor, Honours students

People

News

This is a really exciting opportunity not only to study a red dwarf at close quarters, but to study one around which young planets will most likely be forming.

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The researchers discovered proof of a vast filament of material that connects our Milky Way galaxy to nearby clusters of galaxies, which are similarly interconnected to the rest of the Universe.

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Nobel winner Professor Brian Schmidt's press conference at Parliament House

The ANU Channel on YouTube features ANU Professor Brian Schmidt giving a press conference at Parliament House in Canberra, to discuss receiving the Nobel Prize for Physics.

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Whilst observing with the ANU 2.3m telescope at Siding Spring, Dr Jerjen recently made a very surprising discovery.

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