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The Opposing Tails of Comet Garradd

February 29th, 2012 Comments off

Why does
Comet Garradd have two tails?

Visible on the left,
Comet Garradd's
dust tail is composed of ice and dust bits that trial the comet in its orbit around the Sun.

Visible on the right, Comet Garradd's
ion tail,
is composed of
ionized gas blown directly out from the Sun by the solar wind.

Most comets
show two tails, although it is unusual for them to appear to point in nearly opposite directions.

Comet Garradd is currently showing
opposing tails because of the Earth's opportunistic intermediate viewing angle.

Subtle hues in the above image captured last week show the dust tail as slightly yellow as its large grains reflecting sunlight
achromatically, while the ion tail shines slightly blue as the carbon monoxide
ions reflect blue sunlight more efficiently.

In the center, surrounding the
comet's nucleus, is the green-tinted
coma,
so colored as it is a mix of dust and gasses that include
green-emitting cyanogen.

Although now drifting out from the Sun, Comet Garradd will make its closest approach to the Earth next week.

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Beside a Giant

February 29th, 2012 Comments off

Saturn's largest moon, Titan, looks small here, pictured to the right of the gas giant in this Cassini spacecraft view. Titan (3,200 miles, or 5,150 kilometers across) is in the upper right. Saturn's rings appear across the top of the image, and they cast a series of shadows onto the planet across the middle of the image. The moon Prometheus (53 miles, or 86 kilometers across) appears as a tiny white speck above the rings in the far upper right of the image. The shadow cast by Prometheus can be seen as a small black speck on the planet on the far left of the image, between the shadows cast by the main rings and the thin F ring. The shadow of the moon Pandora also can be seen on the planet south of the shadows of all the rings, below the center of the image towards the right side of the planet. Pandora is not shown here. This view looks toward the southern, unilluminated side of the rings from about 1 degree below the ringplane. The image was taken with the Cassini spacecraft wide-angle camera on Jan. 5, 2012 using a spectral filter sensitive to wavelengths of near-infrared light centered at 752 nanometers. The view was acquired at a distance of approximately 426,000 miles (685,000 kilometers) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 20 degrees. Image scale is 23 miles (37 kilometers) per pixel on Saturn. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. Image credit: NASA/JPL-Caltech/Space Science Institute

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Shocked by Supernova 1987A

February 27th, 2012 Comments off

Twenty five years ago, the
brightest supernova of modern times
was sighted.

Over time,
astronomers have watched and waited for
the expanding debris from this tremendous stellar
explosion to crash into
previously expelled material.

A clear result of such a collision is demonstrated in the above time lapse video of images
recorded by the Hubble Space Telescope between 1994
and 2009.

The movie depicts the collision of an outward
moving
blast wave
with the pre-existing, light-year wide ring.

The collision occurred at speeds near
60 million kilometers per hour and
shock-heats the
ring material causing it to glow.

Astronomers continue to study the collision as it
illuminates the interesting past of
SN 1987A, and provides clues to
the origin of the mysterious rings.

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The Mysterious Rings of Supernova 1987A

February 27th, 2012 Comments off

What's causing those odd rings in
supernova 1987A?

Twenty five years ago, in 1987, the brightest supernova
in recent history was seen in the
Large Magellanic Clouds.

At the center of the
above picture is an object central to the
remains of the violent stellar explosion.

Surrounding the center are
curious outer rings appearing as a flattened figure 8.

Although large telescopes including the
Hubble Space Telescope monitor the curious rings every few years, their origin remains a mystery.

Pictured above is a Hubble image of the SN1987A remnant taken last year.

Speculation into the cause of the rings includes beamed
jets emanating from an otherwise hidden
neutron star left over from the supernova, and the interaction of the
wind from the progenitor star with gas released before the explosion.

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Eastern Seaboard at Night

February 27th, 2012 Comments off

An Expedition 30 crew member aboard the International Space Station took this nighttime photograph of much of the Atlantic coast of the United States. Large metropolitan areas and other easily recognizable sites from the Virginia/Maryland/Washington, D.C. area are visible in the image that spans almost to Rhode Island. Boston is just out of frame at right. Long Island and the New York City area are visible in the lower right quadrant. Philadelphia and Pittsburgh are near the center. Parts of two Russian vehicles parked at the orbital outpost are seen in left foreground. This image was taken on Feb. 6, 2012. Image Credit: NASA

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Comment of the Day: Michio Kaku on Intelligent Extraterrestrial Life

February 26th, 2012 Comments off

 

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"As one commenter smartly points out: 'I see most commenters above are confusing predator with carnivore. Humans are omnivores, but we are still predators. Dr. Kaku is making a reasonable, but presently untestable assumption that intelligence arises from predatory behavior.'


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Weekend Feature: "Coming of Age in the Young Universe" –Harvard-Smithsonian Center for Astrophysics (VIDEO)

February 26th, 2012 Comments off

 

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This gorgeous island universe  just begs the question: "are we alone?" With an estimated 200 billion galaxies in the known Universe, we think not. Well, perhaps in the Milky Way. NGC 7331, 50 million light-years distant in the northern constellation Pegasus, is often touted as a twin spiral analog to our Milky Way. 

Arthur C Clarke once wrote that a trillion years from now an advnaced civilization will look back at us with envy and say "They knew the Universe when it was young."


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Weekend Debate: What Do You Think?

February 26th, 2012 Comments off

 

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"Chances are, when we meet intelligent life forms in outer space, they're going to be descended from predators."  

- Michio Kaku


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Stephan’s Quintet

February 26th, 2012 Comments off

The first identified compact galaxy group,
Stephan's Quintet
is featured in
this eye-catching image constructed with data drawn from
the extensive Hubble Legacy Archive.

About 300 million light-years away, only four of these five galaxies
are actually
locked
in a cosmic dance

of repeated close encounters.

The odd man out is easy to spot, though.

The interacting galaxies,
NGC 7319, 7318A, 7318B, and 7317
have an overall yellowish cast.

They also tend to have distorted
loops and tails, grown under the
influence of disruptive gravitational tides.

But the predominantly bluish galaxy, NGC 7320,
is closer, just 40 million light-years distant,
and isn't part of the interacting group.

Stephan's Quintet
lies within the boundaries of the high flying
constellation
Pegasus
.

At the estimated distance of the quartet of interacting galaxies,
this field of view spans about 500,000 light-years.

However, moving just beyond this field, above and to the left,
astronomers can identify another galaxy,
NGC 7320C, that is also 300 million
light-years distant.

Of course, including it would bring the
interacting quartet back up to quintet status.

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"Rogue Planets May Help Seed Microbial Life in the Universe" –Stanford University Researchers

February 24th, 2012 Comments off




"If any of these nomad planets are big enough to have a thick atmosphere, they could have trapped enough heat for bacterial life to exist," said Louis Strigari, leader of the team that reported the result in a paper submitted to the Monthly Notices of the Royal Astronomical Society. Although nomad planets don't bask in the warmth of a star, they may generate heat through internal radioactive decay and tectonic activity.

Searches over the past two decades have identified more than 500 planets outside our solar system, almost all of which orbit stars. Last year, researchers detected about a dozen nomad planets, using a technique called gravitational microlensing, which looks for stars whose light is momentarily refocused by the gravity of passing planets.

The research produced evidence that roughly two nomads exist for every typical, so-called main-sequence star in our galaxy. The new study estimates that nomads may be up to 50,000 times more common than that.To arrive at what Strigari himself called "an astronomical number," the KIPAC team took into account the known gravitational pull of the Milky Way galaxy, the amount of matter available to make such objects and how that matter might divide itself up into objects ranging from the size of Pluto to larger than Jupiter.

Not an easy task, considering no one is quite sure how these bodies form. According to Strigari, some were probably ejected from solar systems, but research indicates that not all of them could have formed in that fashion.

t"To paraphrase Dorothy from The Wizard of Oz, if correct, this extrapolation implies that we are not in Kansas anymore, and in fact we never were in Kansas," said Alan Boss of the Carnegie Institution for Science, author of The Crowded Universe: The Search for Living Planets, who was not involved in the research. "The universe is riddled with unseen planetary-mass objects that we are just now able to detect."

A good count, especially of the smaller objects, will have to wait for the next generation of big survey telescopes, especially the space-based Wide-Field Infrared Survey Telescope and the ground-based Large Synoptic Survey Telescope, both set to begin operation in the early 2020s.A confirmation of the estimate could lend credence to another possibility mentioned in the paper – that as nomad planets roam their starry pastures, collisions could scatter their microbial flocks to seed life elsewhere.

"Few areas of science have excited as much popular and professional interest in recent times as the prevalence of life in the universe," said co-author and KIPAC Director Roger Blandford. "What is wonderful is that we can now start to address this question quantitatively by seeking more of these erstwhile planets and asteroids wandering through interstellar space, and then speculate about hitchhiking bugs."

If any of these nomad planets are big enough to have a thick atmosphere, they could have trapped enough heat for bacterial life to exist,” said Louis Strigari, leader of the team that reported the result in a paper submitted to theMonthly Notices of the Royal Astronomical Society.

Last year, researchers detected about a dozen nomad planets, using a technique called gravitational microlensing. A confirmation of the estimate could lend credence to another possibility mentioned in the paper — that as nomad planets roam their starry pastures, collisions could scatter their microbial flocks to seed life elsewhere.

The image above is an artistic rendition of a nomad object wandering the interstellar medium (intentionally blurry to represent uncertainty about whether it has an atmosphere). 

KIPAC is a joint institute of Stanford University and the SLAC National Accelerator Laboratory.

The Daily Galaxy via Stanford University

Image credit: . Greg Stewart/SLAC National Accelerator Laboratory

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