Cosmos

Structure and evolution of the Cosmos

Explores the vast complexities of the cosmos, focusing on the formation and interaction of galaxies, the early universe, dark matter, and cosmic expansion, contributing to groundbreaking discoveries like the accelerating expansion of the universe, a phenomenon pivotal to our understanding of cosmic evolution.

About

On the largest and most distant scales, astrophysicists and cosmologists at RSAA study many types of distant galaxies, investigate the nature of the early universe, and measure the expansion of space itself. Areas of study in these fields include:

  • understanding how galaxies form and interact with each other and their environments
  • observing how interactions between galaxies affect their development
  • the effects of internal processes, such as star formation and central supermassive black holes, on the growth of a galaxy
  • the role and nature of dark matter in the formation of structure in the universe
  • measuring the rate of acceleration of the expansion of the universe and understanding the implications for cosmological models
  • modelling and observing enigmatic phenomena such as gamma ray bursts, supernovae and other transients to understand the physical processes that cause them.

Research led by cosmologists at ANU led to the discovery that the Universe is expanding at an ever-increasing rate; work for which the 2011 Nobel Prize in Physics was awarded. RSAA astronomers continue to investigate what this means for theoretical models of the Universe, to understand the role of dark energy or the cosmological constant that drives this accelearation. They are also improving measurements of distance to the exploding stars, or supernovae, that are used as beacons in mapping the expansion rate to refine the results that constrain these models. One of the major goals for the SkyMapper Telescope's Southern Sky Survey is to discover tens of thousands of new supernova occurring in distant galaxies. This will significantly increase the sample of observed events and enable astronomers to make detailed follow-up observations to help improve understanding of the physical processes that occur during these stellar explosions.

Projects

We aim to build an innovative framework to leverage future 21-cm experiments to observe cosmic dawn, and to forecast the optimal constraints on dark matter.

Student intake

Open for Honours, PhD students

People

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

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

This research project employed the Wide-Field Spectrograph (WiFeS)  to study the extended filaments surrounding a sample of brightest cluster galaxies (BCGs) in massive clusters. Integral-field spectroscopy provides the opportunity to measure the distribution, emission properties, and velocities of the emitting gas across the extent of the galaxies.

Student intake

Open for PhD students

The ISM of spiral galaxies is a dynamic environment consisting of thermal gas, relativistic particles, magnetic fields, and dust. The project aims to decipher the origin of filamentary structures in the ISM using numerical simulations as well as observational data.

Student intake

Open for Bachelor, Honours, PhD students

People

This project will simulate observations of the rotation measure (RM) at high Galactic latitude that traces the magnetic structures of the Milky Way. The goal is to pinpoint the cause of the recently discovered asymmetry in the RM patterns between the two Galactic hemispheres.

Student intake

Open for Bachelor, Honours students

People

Members

Academic

Christoph Federrath

Associate Director HDR
Former ARC Future and Stromlo Fellow
Research School of Astronomy and Astrophysics

Faculty

Christoph Federrath

Associate Director HDR
Former ARC Future and Stromlo Fellow
Research School of Astronomy and Astrophysics

News

SkyMapper will be the first survey telescope to create a detailed digital map of the southern skies

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A team of Australian astronomers is looking for the trigger of a cosmic explosion discovered by Dutch astronomer Tycho Brahe in 1572. It is still unclear why events like this, which are refered to as supernovae, occur. 

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

Professor Brian Schmidt from the Research School of Astronomy and Astrophysics has won the 2011 Nobel Prize for Physics.

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Events

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Tuesday, 15 Jul 2025, 11am

Resolving the subgrid physics of galactic winds.

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Tuesday, 29 Jul 2025, 11am

In pursuit of realistic star formation histories from SED fitting.

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