The project is supported by the federal government's Australian Space Research Program (ASRP) and will use small-satellite technology provide a new communications infrastructure.

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

The Australian Plasma Thruster (APT) will help deep-space probes travel for longer and further into space and be used to de-orbit satellites at the end of their lifetimes. The engine of the thruster will be based on ANU Professor Christine Charles's Helicon Double Layer Thruster (HDLT), which is the first of its kind in the world.

Data archives

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

In this project you will develop use and further develop the Chronostar tool to identify thousands of previously unknown young stars near the sun - ideal targets for future exoplanet detection campaigns.

In this project you will develop use and further develop the Chronostar tool to identify thousands of previously unknown young stars near the sun - ideal targets for future exoplanet detection campaigns.

Even from our telescopes on the tops of high mountains, the Earth’s atmosphere blurs observations reducing their clarity.

The Gemini South Adaptive Optics Imager - known as GSAOI - is a $6.3 million, wide-field, infrared camera that was designed and manufactured by RSAA engineers and technicians for the Gemini South telescope in Chile.

GMTIFS is a near-infrared imager and integral-field spectrograph.

We are building a powerful new instrument to work with the Giant Magellan Telescope to record images and spectra ten times sharper than possible with the Hubble Space Telescope.

The Australian company ViPAC Engineers & Scientists Pty. Ltd. is leading a project to develop a space-based monitoring system to improve the measurement of greenhouse gases, funded by under the government's Australian Space Research Program (ASRP).

Using both the Wide-Field Spectrograph (WiFeS) on the ANU 2.3m telescope and the 1.4 GHz radio band on the Australia Telescope Compact Array (ATCA), the student will address how the radio jets from the supermassive black hole interact with the Seyfert host galaxy to affect the evolution of the galaxy.

The Giant Magellan Telescope (GMT) is being designed and built by an international consortium of institutions and will be the largest optical telescope in the world when it is completed around 2020.

Using ANU's SkyMapper Telescope we follow up on gravitational-wave events from LIGO/Virgo to characterise the ejecta from neutron-star collisions.