Posts Tagged ‘Astronomy’

Rumor has it that the first dark matter particle has been found!

December 8th, 2009

Dark Matter

The physics blogs are abuzz with rumours that a particle of dark matter has finally been found.

If it is true, it is huge news. Dark matter is thought to make up 90 per cent of the universe’s mass and what evidence there is for it remains highly controversial. That’s why any news of a sighting is seized upon.
The Cryogenic Dark Matter Search experiment is one of several designed to look for the tell-tale signature of dark matter particles passing through. No one is sure what a dark matter particle will look like, though theory gives some pointers.
Most of the experiments have been designed to look for elusive massive particles called WIMPS that barely register as they pass through matter, because the only forces they experience are gravity and the weak nuclear force.
CDMS is located deep underground in the Soudan mine in Minnesota, to protect it from the hail of cosmic rays that would otherwise wash out any dark matter signal.
Earlier this year, the collaboration published a paper in Physical Review Letters (vol 102, p011301) based on two series of experiments between October 2006 and July 2007. They found nothing.
So researchers have been waiting eagerly for the next chapter of the story – maybe with more time, more experience running their detector and a sprinkling of luck, the team would spot a dark matter particle.
The gossip mill went into overdrive after a rumour leaked out that the CDMS collaboration has had a paper accepted by the journal Nature. Word is that the paper will appear in the 18 December issue.
Nature is an unusual place for particle physicists to publish their papers and this has prompted speculation that the news must be big.
A few physicists I know say that talks have hurriedly been scheduled for 18 December at SLAC National Laboratory, the University of California Santa Barbara and Fermilab – all prominent institutions within the CDMS collaboration.
We’ll have to wait and see if the rumours turn out to be true. Even if not, with NASA’s Fermi satellite looking for dark matter in space and the Large Hadron Collider up and running, 2010 could be the year we finally crack the dark matter mystery.

Via: New Scientist

Some black holes may actually be ‘quark stars’

December 7th, 2009

black hole, quark star

Think black holes are strange? Understandable, considering these powerhouses of the universe (many times heavier than our sun) are collapsed stars with gravity so strong that even light cannot escape their grasp.

But maybe they’re not “strange” enough, some astrophysicists suggest. “Stellar” black holes, ones only a few times heavier than the sun, may actually be something even weirder called a quark star, or “strange” star.

A physics team led by Zoltan Kovacs of the University of Hong Kong sizes up the issue in the current Monthly Notices of the Royal Astronomical Society. Quark stars are only theoretical right now, but “the observational identification of quarks stars would represent a major scientific achievement,” Kovacs says.

If quark stars exist, it could prove a theory that normal matter – the stuff of people, planets and stars – isn’t stable and could help explain the existence of the “dark matter” that fills much of the universe.

First suggested in 1970, a strange star is a collapsed star that doesn’t quite crumple enough to turn into a full-fledged black hole and yet is too heavy to become a so-called neutron star (at least 1.4 times heavier than the sun.) Neutron stars do exist, as astronomer Jocelyn Bell showed with the discovery of a pulsar, a spinning neutron star that streams particles from its poles.

In a quark star, gravity would be so strong that it squeezes the subatomic particles called quarks right out of the protons and neutron building blocks of the original star’s atoms. That would leave behind a solid mass of quark stuff called strange matter, hence the name “strange star.”

Earlier in the decade, astronomers suggested that a neutron star called RX J1856, about 400 light-years away (one light-year is about 5.9 trillion miles) was about one-third too small and might be a quark star. But a 2004 Nuclear Physics B journal report showed the star’s intense magnetic field explained its size, so it really was a neutron star.

So, if size alone won’t reveal a quark star, what will? In the new study, Kovacs and his colleagues, Cheng Kwong-sang and Tiberiu Harko, analyze the disks of dust and gas circling supposed black holes. Whipped to high speeds by the intense gravity of a black hole, these disks are thought to heat to high temperatures and emit powerful radiation. For a quark star, the radiation would be about 10% less than predicted around a black hole, they find. And a quark star would give off a dim light (called bremsstrahlung emission), unlike a black hole, emitted by a thin layer of electrons on its surface.

The complete article can be read at USAToday.com

Kepler Spacecraft Telescope Proves It Is Capable Of Finding Earthlike Planets

August 8th, 2009

Kepler NASA Spacecraft Telescope

Kepler, NASA’s Spacecraft Telescope is on a mission to find distant planets similar to our own Planet Earth, with the potential to be hospitable to life or contain water. Until now earth and space planet-hunting telescopes have only been capable to seek out planets both larger and hotter than planet earth. Kepler is different; it is designed to find planets the same size and temperature as our own planet. The data and images Kepler is cable of providing is revolutionary. “When the light curves from tens of thousands of stars were shown to the Kepler science team, everyone was awed; no one had ever seen such exquisitely detailed measurements of the light variations of so many different types of stars,” said William Borucki, the principal science investigator of the Kepler Team.  So far all data from Kepler is test data from its first 10 days in space and just a taste of things to come.  We will be following this story very closely.  Stay tuned.

Nasa Finds Massive Black Hole Sucking Up Stars At The Centre Of Galaxy

July 25th, 2009

NASA Black Hole

PASADENA, Calif. — NASA’s Spitzer Space Telescope has imaged a wild creature of the dark — a coiled galaxy with an eye-like object at its center.

The galaxy, called NGC 1097, is located 50 million light-years away. It is spiral-shaped like our Milky Way, with long, spindly arms of stars. The “eye” at the center of the galaxy is actually a monstrous black hole surrounded by a ring of stars. In this color-coded infrared view from Spitzer, the area around the invisible black hole is blue and the ring of stars, white.

The black hole is huge, about 100 million times the mass of our sun, and is feeding off gas and dust along with the occasional unlucky star. Our Milky Way’s central black hole is tame by comparison, with a mass of a few million suns.

“The fate of this black hole and others like it is an active area of research,” said George Helou, deputy director of NASA’s Spitzer Science Center at the California Institute of Technology in Pasadena. “Some theories hold that the black hole might quiet down and eventually enter a more dormant state like our Milky Way black hole.”

The ring around the black hole is bursting with new star formation. An inflow of material toward the central bar of the galaxy is causing the ring to light up with new stars.

“The ring itself is a fascinating object worthy of study because it is forming stars at a very high rate,” said Kartik Sheth, an astronomer at NASA’s Spitzer Science Center. Sheth and Helou are part of a team that made the observations.

In the Spitzer image, infrared light with shorter wavelengths is blue, while longer-wavelength light is red. The galaxy’s red spiral arms and the swirling spokes seen between the arms show dust heated by newborn stars. Older populations of stars scattered through the galaxy are blue. The fuzzy blue dot to the left, which appears to fit snuggly between the arms, is a companion galaxy.

“The companion galaxy that looks as if it’s playing peek-a-boo through the larger galaxy could have plunged through, poking a hole,” said Helou. “But we don’t know this for sure. It could also just happen to be aligned with a gap in the arms.”

Other dots in the picture are either nearby stars in our galaxy, or distant galaxies.

This image was taken during Spitzer’s “cold mission,” which lasted more than five-and-a-half years. The telescope ran out of coolant needed to chill its infrared instruments on May 15, 2009. Two of its infrared channels will still work perfectly during the new “warm mission,” which is expected to begin in a week or so, once the observatory has been recalibrated and warms to its new temperature of around 30 Kelvin (about minus 406 degrees Fahrenheit).

NASA’s Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope mission for NASA’s Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology, also in Pasadena. Caltech manages JPL for NASA. Spitzer’s infrared array camera, which made the observations, was built by NASA’s Goddard Space Flight Center, Greenbelt, Md. The instrument’s principal investigator is Giovanni Fazio of the Harvard-Smithsonian Center for Astrophysics.

Hubble Snaps Sharpest Image Yet of Jupiter Impact

July 25th, 2009

Hubble Telescope Image Of Jupiter

Source: Wired
Jupiter’s new scar has been photographed by the Hubble Space Telescope. The huge mark was left when a comet or asteroid plowed into the planet.

The image above is the sharpest yet of the Pacific Ocean–sized impact site, which was first observed by world’s luckiest amateur astronomer, Anthony Wesley. The new shot was taken by Hubble’s newest toy, the Wide Field Camera 3, which was installed during the most-recent servicing mission to the telescope in May.

The collision is believed to be the largest since Comet Shoemaker-Levy 9 busted into 21 pieces and slammed into the solar system’s largest planet 15 years ago.

If whatever hit Jupiter — and astronomers might never know what it was — had instead struck Earth, it would have caused catastrophic damage to human civilization.

It’s Confirmed – Jupiter Slamed By An Asteroid or Comet!

July 21st, 2009

Jupiter Asteroid Comet

ScienceMag.org is reporting the following:

A large object has slammed into Jupiter, leaving behind a giant black smudge that was first reported yesterday by an amateur astronomer. The find is only the second time in recorded history that scientists have glimpsed an impact scar in the atmosphere of a giant planet. “I never expected I’d get to see something like this,” says astronomer Leigh Fletcher, a postdoc at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California.

Just In: Jupiter hit by an asteroid ?

July 19th, 2009

Jupiter asteroid

Via: http://www.spaceweather.com/

IMPACT ON JUPITER?
“Jupiter has been hit by something similar to the Shoemaker-Levy 9 impacts in 1994,” reports astrophotographer Anthony Wesley. “There is a jet black circular impact mark near its south pole that I imaged tonight from my observatory in Murrumbateman, Australia.” South is up in this snapshot of the feature:

“I have imagery of that same location from 2 nights earlier without the impact mark so this is a very recent event,” he adds. “This image shows that the material has already begun to spread out in a fan shape on one side, and should be rapidly pulled apart by the fast jetstream winds.

I’m sure this will generate some interest around the astronomy community, as impacts like this are rare. I recorded a lot of footage, and will be generating more images and a rotation animation.”

I’ll try and post updates as more information becomes available.

Scientists Spot Gamma Ray: Oldest Ever Object In Universe!

April 29th, 2009

Gamma Ray Photo

Excerpt & Photo Via CNN. In addition, below the article clip, we have a great video with a very detailed description of the Gamma Ray.

A satellite detected a 10-second blast of energy known as a gamma ray burst coming from outer space. Telescopes around the world swiveled to focus on the explosion, soon picking up infrared radiation, which is produced after gamma rays in this kind of event. Berger was ready to view the visible light, which should have followed.

It never arrived.

“We were kind of blown away. We immediately knew what that meant,” Berger said.

What it meant was that he was looking at the oldest thing ever spotted — an enormous star exploding 13 billion years ago.

“At that point the age of the universe was only 600 million years,” he said. In other words, Berger said, he was looking “95 percent of the way back to the beginning of time.”

The star which exploded was 30 to 100 times larger than our own sun, and when it died, it gave off “about million times the amount of energy the sun will release in its entire lifetime,” Berger told CNN by phone from Harvard University, where he is an assistant professor of astronomy.