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NASA TV to Air Announcement of Instruments for Europa Mission

Astronomy News - 22 May 2015 - 10:28am
NASA will announce on Tuesday, May 26, the selection of science instruments for a mission to Europa, to investigate whether Jupiter’s icy moon could harbor conditions suitable for life.

Vesta has no moons – is it unlucky or did it eat them?

Astronomy News - 22 May 2015 - 10:26am
The second-heaviest asteroid in the solar system has no orbiting companions, even though hundreds of smaller asteroids do. Where did they go?







The Dreadful Beauty of Medusa

Astronomy News - 21 May 2015 - 10:28am
Astronomers using ESO’s Very Large Telescope in Chile have captured the most detailed image ever taken of the Medusa Nebula. As the star at the heart of this nebula made its transition into retirement, it shed its outer layers into space, forming this colourful cloud. The image foreshadows the final fate of the Sun, which will eventually also become an object of this kind.

Supernova space bullets could have seeded Earth's iron core

Astronomy News - 21 May 2015 - 10:25am
Stellar explosions seed the universe with heavy elements, and they might have produced dense clouds of iron that went on to form other stars and planets







A strong ultraviolet pulse from a newborn type Ia supernova

Astronomy News - 21 May 2015 - 10:21am

A strong ultraviolet pulse from a newborn type Ia supernova

Nature 521, 7552 (2015). doi:10.1038/nature14440

Authors: Yi Cao, S. R. Kulkarni, D. Andrew Howell, Avishay Gal-Yam, Mansi M. Kasliwal, Stefano Valenti, J. Johansson, R. Amanullah, A. Goobar, J. Sollerman, F. Taddia, Assaf Horesh, Ilan Sagiv, S. Bradley Cenko, Peter E. Nugent, Iair Arcavi, Jason Surace, P. R. Woźniak, Daniela I. Moody, Umaa D. Rebbapragada, Brian D. Bue & Neil Gehrels

Type Ia supernovae are destructive explosions of carbon-oxygen white dwarfs. Although they are used empirically to measure cosmological distances, the nature of their progenitors remains mysterious. One of the leading progenitor models, called the single degenerate channel, hypothesizes that a white dwarf accretes matter from a companion star and the resulting increase in its central pressure and temperature ignites thermonuclear explosion. Here we report observations with the Swift Space Telescope of strong but declining ultraviolet emission from a type Ia supernova within four days of its explosion. This emission is consistent with theoretical expectations of collision between material ejected by the supernova and a companion star, and therefore provides evidence that some type Ia supernovae arise from the single degenerate channel.

No signature of ejecta interaction with a stellar companion in three type Ia supernovae

Astronomy News - 21 May 2015 - 10:21am

No signature of ejecta interaction with a stellar companion in three type Ia supernovae

Nature 521, 7552 (2015). doi:10.1038/nature14455

Authors: Rob P. Olling, Richard Mushotzky, Edward J. Shaya, Armin Rest, Peter M. Garnavich, Brad E. Tucker, Daniel Kasen, Steve Margheim & Alexei V. Filippenko

Type Ia supernovae are thought to be the result of a thermonuclear runaway in carbon/oxygen white dwarfs, but it is uncertain whether the explosion is triggered by accretion from a non-degenerate companion star or by a merger with another white dwarf. Observations of a supernova immediately following the explosion provide unique information on the distribution of ejected material and the progenitor system. Models predict that the interaction of supernova ejecta with a companion star or circumstellar debris lead to a sudden brightening lasting from hours to days. Here we present data for three supernovae that are likely to be type Ia observed during the Kepler mission with a time resolution of 30 minutes. We find no signatures of the supernova ejecta interacting with nearby companions. The lack of observable interaction signatures is consistent with the idea that these three supernovae resulted from the merger of binary white dwarfs or other compact stars such as helium stars.

Astronomy: Quasar quartet in galactic nursery

Astronomy News - 21 May 2015 - 10:17am

Astronomy: Quasar quartet in galactic nursery

Nature 521, 7552 (2015). doi:10.1038/521263a

Astronomers have discovered a massive cluster of four quasars — a rare find of galaxies just being born.Quasars are young, bright galaxies powered by supermassive black holes and are hard to find because this youthful period is brief. Using the W. M. Keck Observatory

Astronomy: Spots spotted on Vega star

Astronomy News - 21 May 2015 - 10:16am

Astronomy: Spots spotted on Vega star

Nature 521, 7552 (2015). doi:10.1038/521262b

One of the brightest stars in the night sky seems to have surface structures called starspots — a surprising finding for this particular star.Torsten Böhm at the University of Toulouse in France and his colleagues used a telescope at France's Haute-Provence Observatory to look

Ancient stories record natural world

Astronomy News - 19 May 2015 - 10:15am

How Aboriginal legend is informing science

The First Martian Marathon

Astronomy News - 18 May 2015 - 10:31am
On Earth, a fast runner takes a few hours to complete a marathon. On Mars, it's taken 11 years. NASA's Opportunity rover crossed that finish line in 2015.

Retirement in the suburbs - Hubble traces the migration of white dwarfs in cluster 47 Tucanae [heic1510]

Astronomy News - 15 May 2015 - 10:24am

Astronomers using the NASA/ESA Hubble Space Telescope have, for the first time, collected a census of young white dwarf stars beginning their migration from the crowded centre of an ancient star cluster to its less populated outskirts. The new results challenge our ideas about how and when a star loses its mass near the end of its life.

Hubble Catches a Stellar Exodus in Action

Astronomy News - 15 May 2015 - 10:23am

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Globular star clusters are isolated star cities, home to hundreds of thousands of stars. And like the fast pace of cities, there's plenty of action in these stellar metropolises. The stars are in constant motion, orbiting around the cluster's center. Past observations have shown that the heavyweight stars live in the crowded downtown, or core, and lightweight stars reside in the less populated suburbs.

Galaxies die by slow 'strangulation'

Astronomy News - 15 May 2015 - 10:06am

A study suggests that when most galaxies stop forming stars, this death is a slow process that gradually chokes them of the necessary cool gases.

The Dark Side of Star Clusters

Astronomy News - 14 May 2015 - 10:17am
Observations with ESO’s Very Large Telescope in Chile have discovered a new class of “dark” globular star clusters around the giant galaxy Centaurus A. These mysterious objects look similar to normal clusters, but contain much more mass and may either harbour unexpected amounts of dark matter, or contain massive black holes — neither of which was expected nor is understood.

Corkscrew planets spiral back and forth between two stars

Astronomy News - 14 May 2015 - 10:16am
In some rare cases, a planet in a binary system may spiral around the axis that connects its two stars – although how such planets come to be is unclear







Found: giant spirals in space that could explain our existence

Astronomy News - 14 May 2015 - 10:16am

Why there is any matter at all is one of physics' biggest mysteries. Hints of a spiralled intergalactic magnetic field could solve it







Strangulation as the primary mechanism for shutting down star formation in galaxies

Astronomy News - 14 May 2015 - 10:15am

Strangulation as the primary mechanism for shutting down star formation in galaxies

Nature 521, 7551 (2015). doi:10.1038/nature14439

Authors: Y. Peng, R. Maiolino & R. Cochrane

Local galaxies are broadly divided into two main classes, star-forming (gas-rich) and quiescent (passive and gas-poor). The primary mechanism responsible for quenching star formation in galaxies and transforming them into quiescent and passive systems is still unclear. Sudden removal of gas through outflows or stripping is one of the mechanisms often proposed. An alternative mechanism is so-called “strangulation”, in which the supply of cold gas to the galaxy is halted. Here we report an analysis of the stellar metallicity (the fraction of elements heavier than helium in stellar atmospheres) in local galaxies, from 26,000 spectra, that clearly reveals that strangulation is the primary mechanism responsible for quenching star formation, with a typical timescale of four billion years, at least for local galaxies with a stellar mass less than 1011 solar masses. This result is further supported independently by the stellar age difference between quiescent and star-forming galaxies, which indicates that quiescent galaxies of less than 1011 solar masses are on average observed four billion years after quenching due to strangulation.

Cause of galactic death: strangulation

Astronomy News - 14 May 2015 - 10:13am

As murder mysteries go, it’s a big one: how do galaxies die and what kills them? A new study, published today in the journal Nature, has found that the primary cause of galactic death is strangulation, which occurs after galaxies are cut off from the raw materials needed to make new stars.

Researchers from the University of Cambridge and the Royal Observatory Edinburgh have found that levels of metals contained in dead galaxies provide key ‘fingerprints’, making it possible to determine the cause of death.

There are two types of galaxies in the Universe: roughly half are ‘alive’ galaxies which produce stars, and the other half are ‘dead’ ones which don’t. Alive galaxies such as our own Milky Way are rich in the cold gas – mostly hydrogen – needed to produce new stars, while dead galaxies have very low supplies. What had been unknown is what’s responsible for killing the dead ones.

Astronomers have come up with two main hypotheses for galactic death: either the cold gas needed to produce new stars is suddenly ‘sucked’ out of the galaxies by internal or external forces, or the supply of incoming cold gas is somehow stopped, slowly strangling the galaxy to death over a prolonged period of time.

In order to get to the bottom of this mystery, the team used data from the Sloan Digital Sky Survey to analyse metal levels in more than 26,000 average-sized galaxies located in our corner of the universe.

“Metals are a powerful tracer of the history of star formation: the more stars that are formed by a galaxy, the more metal content you’ll see,” said Dr Yingjie Peng of Cambridge’s Cavendish Laboratory and Kavli Institute of Cosmology, and the paper’s lead author. “So looking at levels of metals in dead galaxies should be able to tell us how they died.”

If galaxies are killed by outflows suddenly pulling the cold gas out of the galaxies, then the metal content of a dead galaxy should be the same as just before it died, as star formation would abruptly stop.

In the case of death by strangulation however, the metal content of the galaxy would keep rising and eventually stop, as star formation could continue until the existing cold gas gets completely used up.

While it is not possible to analyse individual galaxies due to the massive timescales involved, by statistically investigating the difference of metal content of alive and dead galaxies, the researchers were able to determine the cause of death for most galaxies of average size.

“We found that for a given stellar mass, the metal content of a dead galaxy is significantly higher than a star-forming galaxy of similar mass,” said Professor Roberto Maiolino, co-author of the new study. “This isn’t what we’d expect to see in the case of sudden gas removal, but it is consistent with the strangulation scenario.”

The researchers were then able to independently test their results by looking at the stellar age difference between star-forming and dead galaxies, independent of metal levels, and found an average age difference of four billion years – this is in agreement with the time it would take for a star-forming galaxy to be strangled to death, as inferred from the metallicity analysis.

“This is the first conclusive evidence that galaxies are being strangled to death,” said Peng. “What’s next though, is figuring out what’s causing it. In essence, we know the cause of death, but we don’t yet know who the murderer is, although there are a few suspects.” 

Astronomers have partially solved an epic whodunit: what kills galaxies so that they can no longer produce new stars?

This is the first conclusive evidence that galaxies are being strangled to deathYingjie Pengre-activeArtist’s impression of one of the possible galaxy strangulation mechanisms: star-forming galaxies (fed by gas inflows) are accreted into a massive hot halo, which ‘strangles’ them and leads to their death.


The text in this work is licensed under a Creative Commons Attribution 4.0 International License. For image use please see separate credits above.

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Watch this animation introducing significant moments in our understanding of lig...

Astronomy News - 14 May 2015 - 10:12am
Watch this animation introducing significant moments in our understanding of light!

Produced by The Open University with funding from the RAS and SEPnet, to celebrate the International Year of Light 2015

http://www.ras.org.uk/education-and-careers/for-everyone/2636-international-year-of-light-2015


International Year of Light

Learn more about the International Year of Light from The Open University http://www.open.edu/openlearn/whats-on/events/international-year-light-2015 --- DES...

Astrophysics: The slow death of red galaxies

Astronomy News - 14 May 2015 - 10:10am

Astrophysics: The slow death of red galaxies

Nature 521, 7551 (2015). doi:10.1038/521164a

Authors: Andrea Cattaneo

For most galaxies, the shutdown of star formation was a slow process that took 4 billion years. An analysis of some 27,000 galaxies suggests that 'strangulation' by their environment was the most likely cause. See Letter p.192