Institute of Astronomy

Astronomy News

First Signs of Self-interacting Dark Matter?

15 April 2015 - 9:39am
For the first time dark matter may have been observed interacting with other dark matter in a way other than through the force of gravity. Observations of colliding galaxies made with ESO’s Very Large Telescope and the NASA/ESA Hubble Space Telescope have picked up the first intriguing hints about the nature of this mysterious component of the Universe.

Rosetta and Philae find comet not magnetised

15 April 2015 - 9:38am
Measurements made by Rosetta and Philae during the probe's multiple landings on Comet 67P/Churyumov-Gerasimenko show that the comet's nucleus is not magnetised.

Philae's sensors show comet 67P has almost no magnetic field

15 April 2015 - 9:37am
Comet 67P/Churyumov–Gerasimenko surprisingly has a negligible magnetic field, which has implications for how planets formed







Comet lander tells magnetic story

15 April 2015 - 9:25am

The comet being trailed through space by Europe's Rosetta probe has no magnetic field of its own - an important observation in the understanding of how the icy dirt-ball formed billions of years ago.

Coloured Pluto comes into view

15 April 2015 - 9:25am

The New Horizons probe, which is bearing down on Pluto, has captured its first colour image of the distant dwarf planet.

Dark matter becomes less 'ghostly'

15 April 2015 - 9:24am

Scientists have uncovered a vital new insight into the nature of dark matter.

Solar Orbiter launch moved to 2018

14 April 2015 - 9:46am

The launch of Solar Orbiter, an ESA mission to explore the Sun in unprecedented detail, is now planned to take place in October 2018. The launch was previously targeted for July 2017.

Final chance to present a talk or poster at the 2015 National Astronomy Meeting!...

14 April 2015 - 9:46am
Final chance to present a talk or poster at the 2015 National Astronomy Meeting!

The extended abstract deadline is tomorrow, Tues 14 April

http://nam2015.org/


National Astronomy Meeting 2015
nam2015.org
National Astronomy Meeting 2015

Two mysterious bright spots on dwarf planet Ceres are not alike

14 April 2015 - 9:45am
The bright spots on the dwarf planet Ceres continue to baffle scientists as infrared images reveal they have different thermal properties







Dwarf Ceres captured in colour

14 April 2015 - 9:16am

The US space agency's Dawn mission to Ceres has released its first colour map of the dwarf planet.

Evidence of liquid water on Mars

14 April 2015 - 9:16am

Nasa's Curiosity rover has found that water can exist as a liquid near the Martian surface.

Dark matter map yields first results

14 April 2015 - 9:05am

A huge effort to make a map of dark matter, the invisible stuff holding galaxies in place across the cosmos, releases its first batch of results.

Native Hawaiians halt construction of giant telescope

13 April 2015 - 8:51am

The Thirty Meter Telescope being built atop Mauna Kea flouts environmental rules and desecrates sacred ground, say native Hawaiian activists







Looking into the voids could help explain dark energy

13 April 2015 - 8:51am

The influence of dark energy on big empty patches in space could aid us in understanding the expansion of the universe – and predicting its ultimate fate







Heart of the black auroras revealed by Cluster

10 April 2015 - 9:37am

Most people have heard of auroras - more commonly known as the Northern and Southern Lights - but, except on rare occasions, such as the recent widespread apparition on 17 March, they are not usually visible outside the polar regions. Less familiar are phenomena known as black auroras, dark patches which often subdivide the glowing curtains of red and green light.

Our Sun Came Late to the Milky Way's Star-Birth Party

10 April 2015 - 9:36am

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Our Sun missed the stellar "baby boom" that erupted in our young Milky Way galaxy 10 billion years ago. During that time the Milky Way was churning out stars 30 times faster than it does today. Our galaxy was ablaze with a firestorm of star birth as its rich reservoir of hydrogen gas compressed under gravity, creating myriad stars. But our Sun was not one of them. It was a late "boomer," arising 5 billion years later, when star birth had plunged to a trickle.

Citizen Scientists Discover Yellow "Space Balls"

10 April 2015 - 9:35am
Citizen scientists scanning images from a NASA observatory have found "yellow balls" in space that may hold important clues to the mysteries of starbirth.

Complex Organic Molecules Discovered in Infant Star System

9 April 2015 - 9:42am
For the first time, astronomers have detected the presence of complex organic molecules, the building blocks of life, in a protoplanetary disc surrounding a young star. The discovery, made with the Atacama Large Millimeter/submillimeter Array (ALMA), reaffirms that the conditions that spawned the Earth and Sun are not unique in the Universe. The results are published in the 9 April 2015 issue of the journal Nature.

A primordial origin for the compositional similarity between the Earth and the Moon

9 April 2015 - 9:40am

A primordial origin for the compositional similarity between the Earth and the Moon

Nature 520, 7546 (2015). doi:10.1038/nature14333

Authors: Alessandra Mastrobuono-Battisti, Hagai B. Perets & Sean N. Raymond

Most of the properties of the Earth–Moon system can be explained by a collision between a planetary embryo (giant impactor) and the growing Earth late in the accretion process. Simulations show that most of the material that eventually aggregates to form the Moon originates from the impactor. However, analysis of the terrestrial and lunar isotopic compositions show them to be highly similar. In contrast, the compositions of other Solar System bodies are significantly different from those of the Earth and Moon, suggesting that different Solar System bodies have distinct compositions. This challenges the giant impact scenario, because the Moon-forming impactor must then also be thought to have a composition different from that of the proto-Earth. Here we track the feeding zones of growing planets in a suite of simulations of planetary accretion, to measure the composition of Moon-forming impactors. We find that different planets formed in the same simulation have distinct compositions, but the compositions of giant impactors are statistically more similar to the planets they impact. A large fraction of planet–impactor pairs have almost identical compositions. Thus, the similarity in composition between the Earth and Moon could be a natural consequence of a late giant impact.

Saturn’s fast spin determined from its gravitational field and oblateness

9 April 2015 - 9:39am

Saturn’s fast spin determined from its gravitational field and oblateness

Nature 520, 7546 (2015). doi:10.1038/nature14278

Authors: Ravit Helled, Eli Galanti & Yohai Kaspi

The alignment of Saturn’s magnetic pole with its rotation axis precludes the use of magnetic field measurements to determine its rotation period. The period was previously determined from radio measurements by the Voyager spacecraft to be 10 h 39 min 22.4 s (ref. 2). When the Cassini spacecraft measured a period of 10 h 47 min 6 s, which was additionally found to change between sequential measurements, it became clear that the radio period could not be used to determine the bulk planetary rotation period. Estimates based upon Saturn’s measured wind fields have increased the uncertainty even more, giving numbers smaller than the Voyager rotation period, and at present Saturn’s rotation period is thought to be between 10 h 32 min and 10 h 47 min, which is unsatisfactory for such a fundamental property. Here we report a period of 10 h 32 min 45 s ± 46 s, based upon an optimization approach using Saturn’s measured gravitational field and limits on the observed shape and possible internal density profiles. Moreover, even when solely using the constraints from its gravitational field, the rotation period can be inferred with a precision of several minutes. To validate our method, we applied the same procedure to Jupiter and correctly recovered its well-known rotation period.