These words, which open Shelley’s poem "When the Lamp is Shattered," employ visions of nature to symbolize life in decay and rebirth. It's as if he had somehow foreseen the creation of this new Gemini Legacy image, and penned a caption for it. What Gemini has captured is nothing short of poetry in motion: the colorful and dramatic tale of a life-and-death struggle between two galaxies interacting. All the action appears in a single frame, with the stunning polar-ring galaxy NGC 660 as the focus of attention.
This image of the ring galaxy NGC 660, captured with the Gemini Multi-Object Spectrograph on the Fredrick C. Gillett Gemini North telescope on Mauna Kea in Hawai‘i, was obtained in August of 2012. The optical image, made using g, r, I, and hydrogen alpha filters, were assigned the colors of blue, green, orange and red respectively. The field of view is 9.3x5.6 arcminutes and is oriented 8 degrees clockwise from north at right and east up. The total exposure (integration) time was 1,620 seconds cumulative for all filters.
Color composite produced by Travis Rector, University of Alaska Anchorage.
Credit: Gemini Observatory/AURA
Polar-ring galaxies are peculiar objects. Astronomers have found only a handful of them, so not much is known about their origins. Most have an early-type spiral system, called a lenticular galaxy, as the central showpiece. But NGC 660, which lies about 40 million light-years distant toward the direction of Pisces the Fishes, is the only polar-ring galaxy known with what is called a late-type lenticular galaxy as its host. All, however, display a ring of stars, dust, and gas that extends tens of thousands of light-years across space along an orbit nearly perpendicular to the main disk.
Models of how polar-ring galaxies form offer two general formation scenarios: 1) a piercing merger between two galaxies aligned roughly at right angles, or 2) when the host galaxy tidally strips material from a passing gas-rich spiral and strews it into a ring.
What you see in this new Gemini Legacy image, then, is not a single dynamic body but either the “bloody” aftermath of one galaxy piercing the heart of another or the remains of a furious tidal struggle between two galaxies that shattered one galaxy’s "lamp," scattered its dust and gas, and formed a colorful, 40,000-light-year-long ring of visual glory.Born of Violence
NGC 660’s polar ring resolves into hundreds of objects, a considerable part of which are blue and red supergiant stars. The youngest detected stars in the ring formed only about 7 million years ago, indicating a long, ongoing process.
"Gemini's incredible definition of the active star forming regions strewn through the polar ring in NGC 660, juxtaposed against the exquisite crossing dust lanes, is simply beautiful. It really is the most incredible picture I've seen of the galaxy," Svoboda exclaims. "None of the other images I've seen, including those from the Hubble Space Telescope, show the star forming regions with such clarity."Weighing the Evidence
"A tidal accretion event will place gas in the polar ring without strongly interacting with the original gas rich host," Svoboda explains. "Tidal interaction is consistent with an influx of gas into the nuclear region creating the starburst that we observe now." Further evidence, he says, is NGC 660's lack of a double nucleus (i.e. two super-massive black holes), which one would expect from a merger.
Astronomers have not detected any "tails" extending from NGC 660, a key signature of many tidal interactions. Usually, when galaxy passes close to another, tidal forces eject stars, gas, and dust into a graceful tail of extragalactic debris and stretched them far into space. But both polar-ring models have produced systems without tidal tails while creating active star formation in the polar ring.
While it can’t be proven with a great deal of confidence, in the case of NGC 660, Svoboda says, "I think that there is good evidence to suggest that the origin of the polar ring lies in the tidal accretion event scenario." Particularly he notes that the ring may be about 1 billion years old, so the stripped galaxy could have moved out of the field by the time of our observations now.Life from Death?
Galaxies usually have a majority of old red stars at their cores, but one of the violent scenarios that created NGC 660 has triggered a furious burst of star formation at the galaxy’s core. Either way, the gravitational interaction between the two galaxies created shock waves that plowed into giant clouds of gas, causing them to collapse into behemoth blue stars, many likely containing more than 100 times the mass of our Sun. These monstrous, short-lived, stars exploded shortly thereafter as supernovae, which generated more shock waves, creating a domino effect that has ever since perpetuated the creation of youthful stars at NGC 660’s core. NGC 660, then, is not only a polar-ring galaxy but also a starburst galaxy. These systems are among the most dense and intense star-forming environments known.Probing Dark Matter
Astronomers believe dark matter influences the dynamics of all galaxies. Yet understanding dark matter remains one of the astronomy’s greatest challenges. Further observations of the enigmatic environment of NGC 660 may shed more light on this … well … dark matter.Peter Michaud
Peter Michaud | EurekAlert!
Gamma-ray flashes from plasma filaments
18.04.2018 | Max-Planck-Institut für Kernphysik
How does a molecule vibrate when you “touch” it?
17.04.2018 | Universität Regensburg
Novel highly efficient and brilliant gamma-ray source: Based on model calculations, physicists of the Max PIanck Institute for Nuclear Physics in Heidelberg propose a novel method for an efficient high-brilliance gamma-ray source. A giant collimated gamma-ray pulse is generated from the interaction of a dense ultra-relativistic electron beam with a thin solid conductor. Energetic gamma-rays are copiously produced as the electron beam splits into filaments while propagating across the conductor. The resulting gamma-ray energy and flux enable novel experiments in nuclear and fundamental physics.
The typical wavelength of light interacting with an object of the microcosm scales with the size of this object. For atoms, this ranges from visible light to...
Stable joint cartilage can be produced from adult stem cells originating from bone marrow. This is made possible by inducing specific molecular processes occurring during embryonic cartilage formation, as researchers from the University and University Hospital of Basel report in the scientific journal PNAS.
Certain mesenchymal stem/stromal cells from the bone marrow of adults are considered extremely promising for skeletal tissue regeneration. These adult stem...
In the fight against cancer, scientists are developing new drugs to hit tumor cells at so far unused weak points. Such a “sore spot” is the protein complex...
In an article that appears in the journal “Review of Modern Physics”, researchers at the Laboratory for Attosecond Physics (LAP) assess the current state of the field of ultrafast physics and consider its implications for future technologies.
Physicists can now control light in both time and space with hitherto unimagined precision. This is particularly true for the ability to generate ultrashort...
The Atlantic overturning – one of Earth’s most important heat transport systems, pumping warm water northwards and cold water southwards – is weaker today than any time before in more than 1000 years. Sea surface temperature data analysis provides new evidence that this major ocean circulation has slowed down by roughly 15 percent since the middle of the 20th century, according to a study published in the highly renowned journal Nature by an international team of scientists. Human-made climate change is a prime suspect for these worrying observations.
“We detected a specific pattern of ocean cooling south of Greenland and unusual warming off the US coast – which is highly characteristic for a slowdown of the...
13.04.2018 | Event News
12.04.2018 | Event News
09.04.2018 | Event News
19.04.2018 | Power and Electrical Engineering
19.04.2018 | Life Sciences
18.04.2018 | Materials Sciences