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Lopsided Galaxy NGC 2276 – HubbleSite

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Summary
The myriad spiral galaxies in our universe almost all look like fried eggs. A central bulge of aging stars is like the egg yolk, surrounded by a disk of stars that are the egg white. The galaxy in this Hubble photo looks like it is sliding off the frying pan. The central bulge is off in one corner relative to the surrounding disk of bright young blue stars. In reality, the stars on the right side of the galaxy are being pulled like taffy by the gravitational tug of a neighboring galaxy, not seen in this close-up view. Galaxies are not solid objects but tenuous agglomerations of tens of billions of stars. When two galaxies come close to each other they feel each other’s gravity and are distorted, like pulling on cotton candy. It’s the universe’s equivalent of the 19th century children’s poem about two stuffed animals – the gingham dog and calico cat — who got into a spat and ate each other. It’s not so dramatic in this case. The galaxies are only getting a little chewed up because of their close proximity.
NGC 2276
The magnificent spiral galaxy NGC 2276 looks a bit lopsided in this Hubble Space Telescope snapshot. A bright hub of older yellowish stars normally lies directly in the center of most spiral galaxies. But the bulge in NGC 2276 looks offset to the upper left. 
In reality, a neighboring galaxy to the right of NGC 2276 (NGC 2300, not seen here) is gravitationally tugging on its disk of blue stars, pulling the stars on one side of the galaxy outward to distort the galaxy’s normal fried-egg appearance.
This sort of “tug of war” between galaxies that pass close enough to feel each other’s gravitational pull is not uncommon in the universe. But, like snowflakes, no two close encounters look exactly alike.
In addition, newborn and short-lived massive stars form a bright, blue arm along the upper left edge of NGC 2276. They trace out a lane of intense star formation. This may have been triggered by a prior collision with a dwarf galaxy. It could also be due to NGC 2276 plowing into the superheated gas that lies among galaxies in galaxy clusters. This would compress the gas to precipitate into stars, and trigger a firestorm of starbirth.
The spiral galaxy lies 120 million light-years away, in the northern constellation Cepheus.
This image was taken as part of the Hubble observation program #15615 (PI: P. Sell), a collaboration between the University of Florida (USA), the University of Crete/FORTH (Greece), INAF-Brera (Italy), and the Center for Astrophysics | Harvard & Smithsonian (USA).
The Hubble Space Telescope is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy in Washington, D.C.

MEDIA CONTACT:
Ray Villard
Space Telescope Science Institute, Baltimore, Maryland

RELEASE: NASA, ESA, Paul Sell (University of Florida)

ACKNOWLEDGMENT: Leo Shatz

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Galaxies Interacting Galaxies Spiral Galaxies



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NGC 2276
NGC 2276 Wide-Field
NGC 2276 Compass
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The NASA Hubble Space Telescope is a project of international cooperation between NASA and ESA. AURA’s Space Telescope Science Institute in Baltimore, Maryland, conducts Hubble science operations.

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Sanjeev Ramachandran has found ultimate joy all through his 23-year-long journalism career by writing for national and international newspapers, websites and blogs. From technology to politics to sports to entertainment, he has been able to express ideas and pen opinion pieces on whatever triggers his interest. Currently at the helm of his own content and public relations company, called Siyahi – The Content & PR People, he makes sure that he doesn’t always let administrative tasks take over his writing space.