Category Astronomy/Space

Student astronomer discovers ‘Rosetta Stone’ for mysterious cosmic signals

Left: Accreting white dwarf illustration, created by Carl Knox (OzGrav, Swinburne University of Technology) and Joshua Preston Pritchard (CSIRO). Top right: Lead author Kovi Rose from the University of Sydney in front of illustration of the white dwarf binary. ©  Carl Knox Bottom Left: CSIRO ’s ASKAP radio telescope on Wajarri Yamaji Country. Credit: Alex Cherney.

An international team led by astronomers at the University of Sydney has uncovered the clearest evidence yet for the origin of an unusual class of cosmic signals. In doing so, they have identified a rare stellar system that is providing scientists with a natural laboratory to study extreme physics.

Using CSIRO’s ASKAP radio telescope, the team discovered a small, dense star, called a white dwarf, shredding material ...

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A natural chemistry laboratory in protostar shockwaves

A natural chemistry laboratory in protostar shock waves

Life exists because elements combine to form complex organic molecules. Astrochemistry studies this process, trying to understand how nature creates carbon-based molecules critical for life. One source for these types of molecules is the outflows emitted by protostars.

Protostars grow by accreting gas, and while they do so, they also emit energy. Protostars haven’t begun fusing hydrogen yet, so their energy comes from shocks on its surface generated by in-falling gas. They can also emit high speed streams of gas as astrophysical jets. These jets carry away excess angular momentum, allowing the protostars to keep growing. These jets also create illuminated shocks in the interstellar medium (ISM).

Shock fronts like these are where energy and matter are concentrated, and that’s whe...

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Is extracting oxygen from lunar soil the future of space exploration?

A new race to the moon is emerging between the United States and China. Unlike fifty years ago, the goal is no longer just about landing and leaving, but establishing a base that allows for a sustainable presence and extended stays on the surface of our natural satellite. The objective is now to use the moon as a testing ground for technologies that will enable us to travel further, particularly to Mars.

One of these key technologies is in-situ resource utilization (ISRU), which involves using available resources on-site to produce the consumables necessary for human activities: oxygen, water, rocket fuels, or construction materials...

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Peering into the Milky Way’s far side, Roman could unveil 100,000 worlds

Galactic Neighborhoods infographic
This infographic features artist’s concept views of our Milky Way galaxy: face-on at the left and edge-on at the right. It highlights different galactic environments that could influence the development of planets and potentially life. The center of the galaxy is rich in the elements that form planets (like silicon, oxygen, and magnesium), which are forged by multiple generations of stars and supernova explosions. Planets there may be more common or larger, but they would also be flooded with radiation from densely packed stars (including massive ones that emit enormous amounts of high-energy ultraviolet light and X-rays). In the outskirts of the galaxy, where stars are much more spread out, radiation is far milder but there are also smaller amounts of planet-building materials...
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