That is about the density of a galaxy that was recently discovered by an international team of astronomers led by a Michigan State University faculty member.
Astronomers have discovered what may be the densest galaxy in the nearby universe. The team that discovered the rare ultra-compact dwarf galaxy was led by MSU’s Jay Strader. The larger image was captured by NASA’s Chandra X-ray Observatory. The inset photo of the galaxy was taken by the Hubble Space Telescope.
“This galaxy is more massive than any ultra-compact drawfs of comparable size,” said Jay Strader, MSU assistant professor of physics and astronomy, “and is arguably the densest galaxy known in the local universe.”
As detailed in the recent edition of the publication Astrophysical Journal Letters, the ultra-compact dwarf galaxy was found in what’s known as the Virgo cluster of galaxies, a collection of galaxies located about 54 million light years from our own Milky Way.
What makes this galaxy, dubbed M60-UCD1, so remarkable is that about half of its mass is found within a radius of only about 80 light years. This would make the density of stars about 15,000 times greater than found in Earth’s neighborhood in the Milky Way.
“Traveling from one star to another would be a lot easier in M60-UCD1 than it is in our galaxy,” Strader said. “Since the stars are so much closer in this galaxy, it would take just a fraction of the time.”
The discovery of ultra-compact galaxies is relatively new – only within the past 10 years or so. Until then, astronomers could see these “things” way off in the distance but assumed they were either single stars or very-distant galaxies.
Another intriguing aspect of this galaxy is the presence of a bright X-ray source in its center. One explanation for this is a giant black hole weighing in at some 10 million times the mass of our sun.
Astronomers are trying to determine if M60-UCD1 and other ultra-compact dwarf galaxies are either born as really jam-packed star clusters or if they are galaxies that get smaller because they have stars ripped away from them. The possible massive black hole, combined with the high galaxy mass and sun-like levels of elements found in the stars, favor the latter idea.
A giant black hole at the center of M60-UCD1 helps tip the scales against the scenario where this galaxy was once a star cluster, since such large black holes are not found in these types of objects.
The galaxy was discovered using NASA’s Hubble Space Telescope. Follow-up observations were done with NASA’s Chandra X-ray Observatory and ground-based optical telescopes, including the Keck 10-meter telescope in Hawaii.
“Twenty years ago we couldn’t have done this,” Strader said. “We didn’t have Hubble or Chandra. This is one of those projects where you bring together the full force of NASA’s great observatories, plus ground-based resources.”
Tom Oswald | EurekAlert!
FAST detects neutral hydrogen emission from extragalactic galaxies for the first time
02.07.2020 | Chinese Academy of Sciences Headquarters
First exposed planetary core discovered
01.07.2020 | Universität Bern
A promising operating mode for the plasma of a future power plant has been developed at the ASDEX Upgrade fusion device at Max Planck Institute for Plasma...
Live event – July 1, 2020 - 11:00 to 11:45 (CET)
"Automation in Aerospace Industry @ Fraunhofer IFAM"
The Fraunhofer Institute for Manufacturing Technology and Advanced Materials IFAM l Stade is presenting its forward-looking R&D portfolio for the first time at...
With an X-ray experiment at the European Synchrotron ESRF in Grenoble (France), Empa researchers were able to demonstrate how well their real-time acoustic monitoring of laser weld seams works. With almost 90 percent reliability, they detected the formation of unwanted pores that impair the quality of weld seams. Thanks to a special evaluation method based on artificial intelligence (AI), the detection process is completed in just 70 milliseconds.
Laser welding is a process suitable for joining metals and thermoplastics. It has become particularly well established in highly automated production, for...
A research team from the Max Planck Institute for the Structure of Dynamics (MPSD) and the University of Oxford has managed to drive a prototypical antiferromagnet into a new magnetic state using terahertz frequency light. Their groundbreaking method produced an effect orders of magnitude larger than previously achieved, and on ultrafast time scales. The team’s work has just been published in Nature Physics.
Magnetic materials have been a mainstay in computing technology due to their ability to permanently store information in their magnetic state. Current...
The Venus flytrap (Dionaea muscipula) takes only 100 milliseconds to trap its prey. Once their leaves, which have been transformed into snap traps, have...
02.07.2020 | Event News
19.05.2020 | Event News
07.04.2020 | Event News
02.07.2020 | Event News
02.07.2020 | Life Sciences
02.07.2020 | Life Sciences