Cosmic giants and dwarfs do battle in space

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Optical collision between galaxies NGC 2207 and IC 2163. Optical collision between galaxies NGC 2207 and IC 2163. Image: Stuart Rankin
  • Galaxy collison favours bigger guy
  • Larger galaxy forms stars at expense of smaller galaxy
  • Milkyway and Andromeda to collide in four billion years
WHO IS the winner when two galaxies hurtling towards each other on a collision course through space smash together?
The collision of cosmic proportions was considered by researchers at the International Centre for Radio Astronomy Research (ICRAR) who determined that the bigger guy always comes out on top.
Previously, astronomers thought that when two galaxies smash into each other their gas clouds get churned up and seed the birth of stars much faster than if they remained separate.
However, research headed by astrophysicist Dr Luke Davies, from the UWA node of ICRAR, suggests the outcome depends on the size of each galaxy.
“When two ‘giants’ collide, they both increase their stellar birth rate, but when one galaxy significantly outweighs the other, the ‘giant’ begins rapidly forming new stars, whereas the ‘dwarf’ suddenly struggles to make any at all,” he says.
Dr Davies says the different outcome is likely due to how long the collisions take to happen.
He says when two ‘giants’ get close they smash into each other very quickly and form a single galaxy before they use up all of their gas.
An animation of galaxies colliding. Credit: ICRAR

But when a ‘giant’ and ‘dwarf’ meet they take a very long time to actually reach each other, and the longer collision timescale means they have time to use up all of their star-forming gas and stop making new stars.
“I like to think of this as the dwarf staying out of arms reach of the giant for a long time, but running around so much that they eventually run out of steam—while the two giants just smash straight into each other in a flurry,” he says.
Dr Davies has studied more than 20,000 merging galaxies as part of the Galaxy and Mass Assembly (GAMA) survey.
“GAMA accurately measures the positions in space of hundreds of thousands of galaxies, so we can work out which ones are very close and more likely to collide in the near future,” Dr Davies says.
“The light emitted from these galaxies is measured at lots of different wavelengths, and from that we can work out their characteristics, such as how many stars they have and how fast they are forming new stars.”
Dr Davies says the Milky Way and our nearest neighbour, Andromeda, are like ‘cosmic tanks’ on a collision course, and in about four billion years they will merge to become a new galaxy Milkdromeda.
Notes
ICRAR is a joint venture between Curtin University and the University of Western Australia with support and funding from the State Government of Western Australia.

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global warming pause

Ocean 'weather balloons' detect cause of global warming pause

Sea temperature data, some collected by a fleet of drifting and diving probes, shows that a decade-long slowdown in global surface warming masked a coincident rise in ocean temperature below 300 feet, according to NASA JPL researchers.
That finding, which was published recently in the journal Science, is the latest paper to take on the controversial topic of the global warming pause, or hiatus. Last month, researchers at the National Oceanographic and Atmospheric Administration argued that the slowdown never occurred.
In the JPL study, climate scientists Veronica Nieves, Josh Willis and William Patzert pored over sea temperature data dating back two decades.
A large portion of this information was collected by the Argo array -- a network of more than 3,000 automated sea probes that can dive deeper than a mile, take temperature and salinity readings, then return to the surface where they transmit the information to orbiting satellites.
"They're the oceans' weather balloons," Willis said of the devices.
What researchers discovered was that during the period of the hiatus -- from roughly 2003 to 2013 -- sea surface temperatures in the Pacific and Indian oceans rose more slowly than they had in previous years.
However, heat was actually accumulating in a layer of water just below the surface, in an area between 300 and 1,000 feet deep.
This layer of warming showed that even though the rise in global average surface temperature had slowed, the ocean continued to absorb heat generated by greenhouse gasses, authors said.
"Basically what happened is the heat missing from the surface went to a subsurface layer in the Pacific and Indian oceans," said Nieves, the lead study author.
The precise mechanism by which the oceans trapped heat in this middle layer of water remains unclear, but researchers say it occurs on a decadal timescale.
Patzert said that this subsurface heating gradually "piled up" in the western Pacific Ocean,  then "leaked" into the Indian Ocean.
The idea that the Pacific Ocean absorbed heat that would have otherwise led to a rise in global average surface temperature is not new.
However, the JPL study is the first to use only direct observations to describe the phenomenon and specify a precise area of warming.
Lead author Nieves said that previous studies have relied on model-based data, or a combination of models and observations, to frame their conclusions.
"This can lead to completely different results," Nieves said.