Photo Source: S. Brunier; Design & Illustration: P. Vosteen (CC BY-ND)
A team of astronomers has discovered what appears to be a grand exodus of more than 100 hydrogen clouds streaming away from the center of the Milky Way and heading into intergalactic space. This observation, made with the National Science Foundation’s Green Bank Telescope (GBT), may give astronomers a clearer picture of the so-called Fermi Bubbles, giant balloons of superheated gas billowing out above and below the disk of our galaxy.
The results are presented today at the 231st meeting of the American Astronomical Society in Washington, D.C.
“The center of the Milky Way is a special place,” notes Jay Lockman, an astronomer at the Green Bank Observatory in West Virginia. “At its heart is a black hole several million times more massive than the Sun and there are regions of intense star birth and explosive star destruction.”
These energetic processes, perhaps individually or together, have generated a powerful cosmic “wind” that has blown two enormous bubbles above and below the disk of the Milky Way that are filled with gas at tens-of-millions of degrees. This superheated gas, however, shines feebly at radio, X-ray and gamma-ray wavelengths.
The bubbles appear prominently in observations made by NASA’s Fermi Gamma-ray Space Telescope, which is why astronomers refer to them as the Fermi Bubbles.
“One problem that hinders study of this hot cosmic wind is that the gas has such low density that its emission is very faint, so there is no practical way to track its motion,” notes Lockman. “This is where the hydrogen clouds come in.”
Just like a handful of dust thrown into the air can show the motion of wind on Earth, the hydrogen clouds can act as test particles revealing the flow of the hotter, invisible wind from the center of the Milky Way.
Neutral hydrogen gas, the principal component of these clouds, shines brightly at the radio wavelength of 21 centimeters. These hydrogen clouds were first discovered by a team led by Naomi McClure-Griffiths of the Australian National University using a radio telescope array in Australia. However, that survey was confined to a region just a few degrees around the galactic center, so it gave only limited information on the number and extent of these clouds.
New research with the 100-meter GBT greatly extends these observations.
A group led by Lockman, McClure-Griffiths, and Enrico DiTeodoro, who is also with the Australian National University, mapped a much larger area around the galactic center in search of additional hydrogen clouds that might be entrained in the nuclear wind. They found a gigantic swarm of more than 100 high-velocity gas clouds. The properties of these clouds allow the scientists to learn about the shape of the wind-blown region and the enormous energies that are involved.
“The signature of these clouds being blown out of the Milky Way is that their velocities are crazy,” said Lockman. “Gas motions in the Milky Way are usually quite regular and are dominated by the orderly rotation of the Galaxy. In the Fermi Bubbles we see clouds right next to each other on the sky that have velocities differing by as much as 400 kilometers per second.”
According to the researchers, the most likely explanation for these wildly differing velocities is that they’re traveling within a cone of material that is expanding upward and away from the galactic center, so the front portion is coming toward us and the back part is flying away.
By modeling the distribution and velocities of the clouds, the astronomers found that they would fill a cone stretching above and below the galaxy to a distance of at least 5,000 light-years from the center. The clouds have an average speed of about 330 kilometers per second.
Di Teodoro notes: “What is especially puzzling is that we have not yet found the edge of the swarm of clouds. Somewhere above the galactic center, the hydrogen clouds have to dissipate or become ionized. But we have not found that edge yet, so there’s still a lot to learn.”
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Artist concept of fast radio burst. Image Credit: Design: Danielle Futselaar; photo usage: shutterstock.com
Green Bank, January 10, 2018 – Using two of the world’s largest radio telescopes, an international team of astronomers have gained new insight into the extreme home of a mysterious source of cosmic radio bursts. The discovery suggests that the source of the radio emission lies near a massive black hole or within an extremely powerful nebula, and may help shed light on what is causing these strange bursts.
The team presented their findings at the American Astronomical Society’s winter meeting (#AAS231) in Washington, D.C. The results are presented in the journal Nature.
Image above is similar to what West Virginians will see if they observe the eclipse this August! (Image source: RedOrbit.com)
Have you heard?! This summer, you have the chance to experience a spectacular stellar event! On August 21, the star that brings us spring flowers, warm days by the pool, and the northern lights, a.k.a. our Sun, will be eclipsed by the Moon. Want to see it? You’re invited!
The Green Bank Observatory in Green Bank, WV is hosting a Great American Eclipse viewing party. Don’t miss out on this rare event. It’s been 26 years since a partial solar eclipse was visible from West Virginia!
A solar eclipse occurs when the Moon’s orbit puts the moon directly between the Sun and Earth, casting a shadow on the Earth’s surface. This only happens during the new moon phase, but we don’t see an eclipse every month because the Moon’s orbital path around the Earth is tilted relative to the Earth’s path around the sun. A perfect alignment between Sun, Moon and Earth is needed for an eclipse.
The relative positions of the Earth and Moon matter a lot when determining whether the eclipse will be a total or partial eclipse. This eclipse is called the Great American Eclipse because across an entire narrow swath of the country from west to east, the eclipse will be total. West Virginians will be able to see a 90% partial eclipse this August. This means only 10% of the Sun’s light will be visible from behind the Moon!
So join us from 11:00 AM until 4:00 PM for a day of food, fun, and education!
- Hands-on Activities from 11 AM- 12 PM
- Lunch and Exhibits from 12 PM – 4 PM
- SAFE Eclipse Viewing through telescopes and projections. Plus live streaming video of the eclipse provided by NASA from 1 PM – 4 PM
Our Great American Eclipse lunch will be “All American” too! For $5.00 you will be able to purchase:
- Two slices of pizza and a soda
- Two hotdogs, chips, and a drink*
- A hamburger, chips, and a drink*
*Cash Only Options. Additional bags of chips and drinks may be purchased for $0.50 and $1.00 respectively while supplies last.
Showing up for the event is free so tell your neighbors, pack up the family, and head to 155 Observatory Rd. Green Bank, WV 24944.
Important Note: To safely view the eclipse with your eyes you need to use special eclipse glasses. These are super dark – much darker than sunglasses! So whether you join our eclipse party or plan to be somewhere else on August 21, you can purchase a pair of eclipse glasses for just $2.00 each at our Gift Shop. Eclipse glasses are on sale now, call (304) 456-2150 for details!
Learn more about eclipses and specifically about the Great American Eclipse:
- The Great American Eclipse
- Path of Totality from Mr. Eclipse
- Historical information and eclipse countdown
- Make Your Own Eclipse Demonstrator Template and Instructional Video
We would love to know if you’re joining us! Visit our Great American Eclipse event page on Facebook and let us know you’re attending today!
A team of astronomers has unveiled a striking new image of the Orion Molecular Cloud (OMC) – a bustling stellar nursery teeming with bright, young stars and dazzling regions of hot, glowing gas.
The researchers used the National Science Foundation’s (NSF) Green Bank Telescope (GBT) in West Virginia to study a 50 light-year long filament of star-forming gas that is wending its way through the northern portion of the OMC known as Orion A.
The GBT rendered this image by detecting the faint radio signals naturally emitted by molecules of ammonia that suffuse interstellar clouds. Scientists study these molecules to trace the motion and temperature of vast swaths of star-forming gas.
These observations are part of the first data release from a large campaign known as the Green Bank Ammonia Survey. Its purpose is to map all the star-forming ammonia and other key tracer molecules in a massive structure known as the Gould Belt.
The Gould Belt is an extended ribbon of bright, massive stars stretching about 3,000 light-years in an arc across the sky. This first release covers four distinct Gould Belt clouds, one located in Taurus, one in Perseus, one in Ophiuchus, and Orion A North in Orion.