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

Stellar spectra capture the light of a star across multiple wavelengths and include absorption features of numerous atoms and molecules from a star’s photosphere. The abundance data many stars then allow us to study the chemical evolution across large scales in our Galaxy and decipher Galactic trends.

Student intake

Open for Bachelor, Honours students

People

In this project you will use a new cosmic ray propagation code, CRIPTIC, to model the injection, transport, and final annihilation of positrons in the interstellar medium of the inner Galaxy.

Student intake

Open for Honours, PhD students

People

In this project you will use some combination of theoretical population synthesis calculations and/or analysis of public data from the Fermi telescope to examine the question: what is the real origin of the Galactic Centre Gamma-Ray Excess?

Student intake

Open for Honours, 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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