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

Approximately 75% of SkyMapper's observing time will be initially dedicated to the Southern Sky Survey, a comprehensive digital survey of the entire southern sky.

You will use new data from the Australian SKA Pathfinder survey, GASKAP-HI to help take the temperature of the Milky Way and Magellanic Clouds. PhD & Masters students on this project will have the opportunity to be among the first users of ASKAP.  

Student intake

Open for Bachelor, Honours, PhD students

People

The effective temperature is one of the most fundamental parameters of a star, and its precise determination is crucial for a number of purposes, e.g., from measuring chemical abundances and ages, to improving stellar and atmosphere models.

Student intake

Open for PhD students

People

M dwarfs are the most abundant stars in the universe, and prime targets for detecting Earth-like planets.

Student intake

Open for PhD students

People

We have a variety of projects that will use the new GASKAP-HI data to study the structure and temperature of hydrogen in the Magellanic System. 

Student intake

Open for Bachelor, Honours students

People

We are looking for ambitious students keen to join the project. They can be involved in different aspects, both observational and theoretical/computational

Student intake

Open for PhD students

People

News

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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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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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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