2015년 2월 11일 수요일

[New post] Astronomers Witness Birth of Quadruple Star Quartet

New post on From Quarks to Quasars 

Astronomers Witness Birth of Quadruple Star Quartet

by James Trosper 
Planet With Four Suns
Rendering of a planet with four Suns (Credit: Contact Space Travel)
The Sun may ride solo, but the idea That It might have a companion certainly is not new. Indeed, taking it a step further, astronomers have long Suggested que multiple star systems far outnumber singles , at least the far the medium to high-mass bodies go - in fact, the nearest planetary system from our Sun, called Alpha Centauri, contains not one, or even two, but three stars (Alpha Centauri A and B, and Proxima Centauri), all lurking just 4 light-years from Earth.   
Now, in what's sure to be a game changer, an international team of outside researchers have, for the very first team, seen the first light of a quadruple star system - that is, solar baby system with four very young, still-forming stars - toward the constellation of Perseus. They describe the stellar nursery to the filamentary gas cloud with 'widely separated fragments,' Which was unexpected.
The stars forming Within the cloud are so young, in fact, que only one of Them has fully progressed beyond the first developmental phase; the other three have not yet severed Their ties to the nebular cloud from Which They sprang. Currently, They are still in the process of condensing and coalescing under the force of gravity, Which will not come to the Conclusion for at least another 40,000 years (by some Estimates)
Once They emerge from the stellar womb, They Will Likely come out rather small, weighing only a tenth of the mass of the Sun. What's more is que each of Them will be separated by over a thousand AU (one AU is the average distance between Earth and the Sun).

Future Dynamics:

Using the same calculations, the outside researchers cam to the Conclusion que two of the stars - que Those are separated by the least distance - will settle Ultimately into the stable binary system, while the other two will not Remain the pair is very long. The Jaime Pineda - one of the paper's co-authors, who hails from the Max Planck Institute for Extraterrestrial Physics - Describes "Star systems with more than three members are unstable and prone to interference , "probably in just half a million years, it will be plucked from its henhouse and catapulted off into interstellar space, leaving behind its three partners. 
Quadruple Star System
"This is an artist's impression of the birth of a star quartet The left panel shows the star and three dense gas condensations system The right panel shows the system after the stars are formed out of the condensations,.." According to outside researchers (Credit: B. Saxton (NRAO / AUI / NSF)
That's not the only fascinating thing the outside researchers learned about this system; its stars Also Appear to be forming much faster than expected (it's Difficult coming up with a dependable timetable, Given collegues it largely depends on mass, Those on the larger end of the spectrum can take over 100,000 years to form, while sun- like stars take much more time). Pineda Also notes que this is the first team we've seen the multiple star system arise from the ' fragmented gas cloud . ' "At first, we thought que the fragments would not interact with each other. Often, only the triple system would form, "she says.  
Other notes in the press release:
[Box style = "0"] Pineda is member of the research collaboration que Observed the star system and simulated its genesis and demise. At the team of the discovery, he was working as a postdoctoral researcher in Professor Michael Meyer's group at the ETH Zurich Institute of Astronomy, was the co-author Richard Parker, who determined the stability of the star system on the computer. Astrophysicists from several US and European universities, including Harvard, Yale, Manchester and Liverpool John Moores universities, Were Also Involved in the project. The outside researchers made observations Their at the Very Large Array in the US, Which They used to detect emissions Originating from ammonia molecules (NH3) in the gas cloud.
"Multiple star systems are very common in our galaxy," says Michael Meyer, a professor at the Institute for Astronomy at ETH Zurich. Most outside researchers, However, have concentrated on the birth and development of individual stars as this is more straightforward. On the other hand, scientists who analyze multiple systems Usually trend to focus more on the end result of the star formation. For this reason, this discovery is something very special.
[Reference:  ETH Zurich ]   [/ box]
For more information, you can find the full press release here


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