Milky Way is Twice as Thick as Previously Believed

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Imagine suddenly realizing that your house was twice as big as you originally thought. Okay, maybe that’s a little out there, but astronomers from Australia have calculated that the Milky Way is actually twice as thick as previously believed – doubling from the originally estimated 6,000 light-years to 12,000 light-years.

The calculation was made by a couple of astronomers from the University of Sydney. They were working with the accepted numbers for the dimensions of our home galaxy (6,000 light years thick, and 100,000 light-years wide) when they thought it might make sense to double check those basic assumptions.

They used an accepted technique for calculating distance; measuring the light from pulsars. When light from distant pulsars moves through the background material of the Milky Way (known as the Warm Ionised Medium), it slows down. The redder pulses of light actually slow down more than the bluer pulses.

By measuring the change in light from the pulsar, astronomers can determine how much material the light has traveled through.

When they used the old calculations for 40 different pulsars inside and above it, they got the old numbers. But when they just looked at 17 pulsars which are above and below the galactic disk they got a new, more accurate, estimate.

“Of the thousands of pulsars known in and around our Galaxy, only about 60 have really well known distances,” said Professor Bryan Gaensler. “But to measure the thickness of the Milky Way we need to focus only on those that are sitting above or below the main part of the Galaxy; it turns out that pulsars embedded in the main disk of the Milky Way don’t give us useful information.”

Their results were presented in January at the annual meeting of the American Astronomical Society in Austin, Texas. Some of Dr. Gaensler’s colleagues appreciated the revised calculations, while others… not so pleased at the implications for their own research.

Original Source: University of Sydney

Send in Your Eclipse Pictures, Tell Your Stories

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How was your view of this week’s lunar eclipse? The skies actually opened up here in Vancouver, and we were able to see good portions of the eclipse. The kids were really excited, and got to stay up late watching the eclipse – it was all they were talking about the next day.

So send me your eclipse pictures, and I’ll run a quick gallery. Email them to me at [email protected], and I’ll try to post them in the next few days.

And to tide you over, here’s an image captured by ESA astronomers from Spain.

Post your eclipse stories in the comments below.

Carnival of Space #42

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It’s time for another look around the space/astronomy community of websites. This week, the Carnival of Space is being hosted by celebrity blogger, Chris Lintott. Check this week’s collection of stories, including, the search for dark matter, the end of an important observatory, and a good long look at some of Saturn’s moons.

Click here to read the Carnival of Space #42

And if you’re interested in looking back, here’s an archive to all the past carnivals of space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, let me know if you can be a host, and I’ll schedule you into the calendar.

Finally, if you run a space-related blog, please post a link to the Carnival of Space. Help us get the word out.

Planet Hunter Prepped for Tests

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If you think the discoveries made by planet hunters is exciting already, just you wait. There are some missions in the works that are going multiply the number of planets discovered, and zoom in on the holy grail of finding habitable planets around other stars. The next planet hunter being readied for launch is NASA’s Kepler Mission. This week engineers conducted a series of tests on its image detectors – will it really be able to see planets?

Scheduled for launch in 2009, Kepler will detect planets using the transit method. This is where a planet passes in front of its parent star, briefly dimming the amount of light we see here on Earth. This has been done to detect Jupiter-scale planets, but nothing Earth-sized… yet.

Kepler will have sensitive enough instruments to be able to detect those slight variations in brightness, and determine just how many stars have planets in their habitable zones.

At the Ames Research Center, researchers have developed a Kepler Technology Demonstration test bed. This generates a field of stars that matches the part of the sky where mission scientists are planning to search for transits. The testing engineers can then modify the brightness of the artificial stars to mimic how transiting planets would look as they passed in front of stars.

“This is a major milestone for the Kepler mission,” said David Koch, deputy principal investigator for the Kepler Mission. “We will use hardware identical to what we will be flying on Kepler in the test bed at Ames. We will have the ability to create transits of a star so that we can see the change in the star’s brightness. By simulating transits, we will be able to demonstrate that the flight hardware will work,” Koch explained.

In the final mission, Kepler will be equipped with 42 CCD cameras attached to the spacecraft’s telescope. They make up a 30-cm square (1-foot) array; the largest that will have been flown in space to date. The spacecraft will be able to scan a region of the sky 30,000 times larger than Hubble is able to search.

This month’s test at AMES will have only a single CCD detector, measuring 2.5 cm by 5 cm (1-inch by 2-inches).

I’ll give you an update once the tests are run. Those habitable planets can’t hide forever.

Original Source: NASA News Release

Meteor Blazed Above the Pacific Northwest Tuesday, February 19

Many lucky people in the Pacific Northwest United States got the treat of a lifetime on Tuesday morning. A bright fireball blazed across the sky at 5:31 am near Portland, Oregon. Apparently the meteor was so bright, people saw it in Washington, Idaho, and even as far away as British Columbia (hey, why didn’t I see it?).

Here’s a surveillance video captured by a camera in Boise, Idaho.

I often get emails from people who saw a bright fireball in the sky. When I’m done seething with jealousy, I suggest they contact their appropriate meteor society (for example, the American Meteor Society in the US) and report the details. Scientists working in this field will thank you.

So let me know, were you one of the lucky ones to see it? Post your story in the comments.

Valles Marineris, the Deepest Chasm in the Solar System

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The photographs coming back from the Martian orbiters sure help you appreciate the very different terrain on the Red Planet. And here’s an example of one of the extreme places on Mars: the Valles Marineris the deepest, longest valley in the Solar System. The image was captured by ESA’s Mars Express spacecraft and reveals a region of the valley called Candor Chasma.

Take a look at a photograph of Mars, and it’s easy to spot Valles Marineris. It’s a 3,000 km-long (1,800 mile) gash carved in the side of the Red Planet. Planetary geologists think it formed around the same time as the nearby Tharsis Bulge – the volcanic region that houses Olympus Mons, the largest mountain in the Solar System.

It’s likely a rift valley, similar to the East African Rift Valley here on Earth. As the giant volcanoes formed, the Valles Marineris opened up as a crack in the ground. Flowing carbon dioxide could have weathered it further, eroding it and forcing the walls to cave in.

As I mentioned above, this is just a tiny portion of the whole rift. The canyon walls tower 8,500 metres (28,000 feet) above the floor below.

And if there was one place in the whole Solar System that I could travel to and see with my own eyes, it would be right here. So come on NASA, hurry up with that mission to Mars already.

Original Source: ESA News Release

Bubble Experiment Fails to Find Dark Matter

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Astronomers have no idea what dark matter is, but they have a few guesses. Since they can’t see the stuff directly, they’re trying to chip away at what it can’t be, peeling away theory after theory. Eventually, there should be a few theories that have withstood the most experiments, and best model what astronomers see out in the Universe. Physicists at Fermilab have made one of those steps forward, constraining the characteristics of dark matter, and overturning a recent discovery… by not seeing anything unusual.

We can’t see dark matter, but we know it’s out there. Galaxies should spin themselves apart but they don’t thanks to being inside a halo of dark matter. Amazing images from the Hubble Space Telescope show dark matter’s gravitational distortion on the light from distant galaxies. Oh, it’s out there all right.

So what is it?

Astronomers have two theories. One is that their ideas about gravity are wrong. By modifying our understanding of how gravity works over large distances, you can remove the need for dark matter entirely.

The other possibility are “weakly interacting massive particles”. These are actual particles, made of “something”, but we can’t see them or detect them in any way except through their pull of gravity.

Particle physicists have been searching for dark matter particles using powerful atom smashers, just like they discovered all the sub-atomic particles they’ve found so far.

A new experiment at the US Department of Energy’s Fermi National Accelerator Laboratory announced this week that they’ve made some headway in this search. According to theories, when dark matter particles interact with regular matter, it’s different from the way regular matter interacts. The Fermilab experiment has ruled out one of the last possible ways that the theories have predicted this should happen.

Their experiment, called COUPP, uses a glass jar filled with a litre of iodotrifluoromethane (a fire-extinguishing liquid known as CF3I. As particles strike the CF3I, it causes tiny bubbles to form in the liquid. The scientists can detect these bubbles as they reach a millimetre in size. By watching the interactions, researchers should be able to know if they’re coming from regular matter or dark matter.

So far, their results contradict another search called the Dark Matter experiment (DAMA) in Italy, who claimed to see dark matter interactions. The results for the DAMA experiment predicted that COUPP should have found hundreds of dark matter interactions, but they didn’t see any.

This research appears in the February 15th issue of the journal Science.

Original Source: Fermilab News Release

Hubble Finds Dozens of Gravitationally Lensed Galaxies

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One of the breakthroughs in modern astronomy is the use of gravitational lenses, where a closer galaxy or star focuses the light from a more distant object. The more astronomers look, the more they find these helpful objects, allowing them to peer at objects much further away. The number of known gravitationally-lensed galaxies jumped up today, when astronomers announced another 67 new lenses.

These 67 lenses were part of the COSMOS project; a detailed survey of small region of the sky about the same as 9 times the area of the Moon. Both Earth and space-based telescopes are working together to provide a survey of the sky which is very deep. And one of the key instruments in the project is the Hubble Space Telescope.

One of the big surprises of this survey is just how many lenses turned up in such a small area of the sky. Based on this discovery rate, researchers think that there could be 500,000 similar gravitationally-lenses galaxies out there.

At least 4 of the lenses are Einstein rings. This is a situation where the foreground and background galaxy are lined up so perfectly, the distorted distant galaxy forms a ring around the closer one.

In order to find the lenses, astronomers had to sift through a collection of 2 million candidate galaxies. Then the researchers had to look through each COSMOS image by eye and identify any potentially strong gravitational lenses. Finally, they checked both the foreground and background galaxy to make sure that they’re really two separate objects separated by billions of light years, and not just a strangely shaped galaxy.

Now that the researchers have so many gravitational lenses, they can do some really interesting things. For example, they’ll be able to study the dark matter distribution around the galactic lenses. And they’ll also be able to start accumulating a census of galaxy masses to see if they match predictions.

Original Source: Hubble News Release

Cassini Uncovers Invisible Rings at Saturn

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Even in the smallest telescopes, Saturn’s bright rings pop into view. But those might be just the tip of the iceberg. During a recent flyby of the planet, NASA’s Cassini spacecraft noticed empty patches where the constant rain of high-energy electrons slowed down. Perhaps there are partial rings there, invisible to the spacecraft’s cameras. And where are these rings coming from?

When NASA’s Cassini spacecraft nears Saturn, its bombarded by a flurry of high energy electrons. But researchers from the Max Planck Institute for Solar System Research noticed that during the spacecraft’s journey, there were two times when it wasn’t being hit with so many particles. In their research article, published in the latest issue of the journal Icarus, they propose that there are invisible rings, generated by two of Saturn’s smallest moons: Methone and Anthe.

The gap in the rain of electrons occurred just as Cassini was passing through the orbits of Methone and Anthe. The drop in intensity lasted while the spacecraft covered a swath as wide as 1,000 to 3,000 km (600 to 1,900 miles) across. This is too wide for the tiny moons themselves, but arcs of ejected material could explain it.

“These observations tell us that even Saturn’s smallest moons could be a source of dust in the Saturnian system,” said Elias Roussos, the paper’s lead author from the Max Planck Institute for Solar System Research in Katlenburg-Lindau, Germany.

So, even the smallest moons around Saturn are feeding dust into the ring system. This released material may develop into partial ring arcs because of the gravitational “tug of war” between the planet’s larger moons, like Mimas. A situation like this has been found with Saturn’s G-ring.

Where’s all this material coming from? The researchers think that the constant rain of micrometeoroids on the surface of the tiny moons dislodges the icy material. Since they’re so small and have very little gravity, it doesn’t take much for the material to escape into space.

Strangely, these theorized rings are invisible. Meteoroids are thought to be generating the faint rings at Janus, Epimetheus and Pallene; but they’re visible to Cassini. The spacecraft can’t see these newly discovered rings with its cameras. Perhaps the two different classes of moons are releasing differently-sized grains of dust.

Original Source: NASA/JPL/SSI News Release

Astrosphere for February 19, 2008

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It might not look like it, but this photograph is mind-bendingly cool. The bright streak is the path of the International Space Station, and the dimmer one is the US military satellite that’s going to crash back to Earth – both seen passing through the heart of Orion. Good job Autoclub!

Centauri Dreams talks about using the Sun’s gravity as a natural telescope lens. Problem is, you have to get out to 550 AU to make it work.

The Space Review has a great article about people preparing for space tourism. So far, 93% have passed the physical tests.

In the future, solar power will rule!

APOD has a great picture of a recent spacewalk outside Columbus.

NY Times is reporting that NASA thinks it can fix a serious flaw in its Ares rocket design.

Astropixie wants to be Stephen Colbert’s astrophysicist.

And finally, one of the best posts of read in a long time. Phil perfectly explains why science isn’t faith.