Showing posts with label planets. Show all posts
Showing posts with label planets. Show all posts

Tuesday, December 30, 2008

Ten Strangest Things About Our Universe - 2008


Artist's rendition of a hypervelocity star leaving a galaxy. Image Credit: Harvard-Smithsonian Center for Astrophysics

Ten Strangest Things About Our Universe - 2008

At the end of any year, one is confronted with many bottom up lists describing the important events, people, discoveries, and etc. over the course of the past year just lived.

This exercise always allows one to pause and reflect on what has been learned and to ponder what might be useful for the New Year ahead.

WE at Oblate Spheroid, marvel at how different life and the place the Earth has in the universe becomes the more we learn about the space we occupy.

The more we look among the stars and galaxies, the weirder things seem to get.

Even space itself is puzzling, for example; Recent studies suggest that the fabric of the universe stretches more than 150 billion light-years across -- in spite of the fact that the cosmos is 13.7 billion years old.

This excerpted and edited from The Discovery Channel –

Hypervelocity stars were first theorized to exist in 1988. The theory was that binary star systems at the galaxy's center would occasionally wander too close to the massive black hole looming there, which would disrupt their orbital dance. While one of the pair was captured by the black hole, the other would be sent rocketing off at an incredible speed. Caption: MSNBC - Image Credit: ESO

TOP 10 STRANGEST THINGS IN THE UNIVERSE

By Dave Mosher for The Discovery Channel - Article originally posted October 31, 2008.

10. Hypervelocity Stars

If you've ever gazed at the night sky, you've probably wished upon a shooting star (which are really meteors).

But shooting stars do exist, and they're as rare as one in 100 million.

In 2005, astronomers discovered the first "hypervelocity" star careening out of a galaxy at nearly 530 miles per second (10 times faster than ordinary star movement).

We have ideas about what flings these rare stars into deep space, but aren't certain; anything from off-kilter supernova explosions to supermassive black holes might be responsible.

9. Black Holes

Conception of a black hole pulling gas off of a nearby star. Image Credit: ESA/NASA

Speaking of black holes, what could be stranger?

Beyond a black hole's gravitational border -- or event horizon -- neither matter nor light can escape. Astrophysicists think dying stars about three to 20 times the mass of the sun can form these strange objects. At the center of galaxies, black holes about 10,000 to 18 billion times heavier than the sun are thought to exist, enlarged by gobbling up gas, dust, stars and small black holes.

What about mid-sized types? Perhaps surprisingly, evidence is both scarce and questionable for their existence.

8. Magnetars

Artist's rendition of a magnetar with magnetic fields shown. Image Credit: NASA

The sun spins about once every 25 days, gradually deforming its magnetic field.

Well, imagine a dying star heavier than the sun collapsing into a wad of matter just a dozen miles in diameter.

Like a spinning ballerina pulling his or her arms inward, this change in size spins the neutron star -- and its magnetic field -- out of control.

Calculations show these objects possess temporary magnetic fields about one million billion times stronger than the Earth's. That's powerful enough to destroy your credit card from hundreds of thousands of miles away, and deform atoms into ultra-thin cylinders.

7. Neutrinos

Construction of the NuMI neutrino source underway. Image Credit: BNL

Pull out a dime from your pocket and hold it up for a second... guess what? About 150 billion tiny, nearly massless particles called neutrinos just passed through it as though it didn't even exist.

Scientists have found that they originate in stars (living or exploding), nuclear material and from the Big Bang. The elementary particles come in three "flavors" and, stranger still, seem to disappear on a whim.

Because neutrinos occasionally do interact with "normal" matter such as water and mineral oil, scientists hope they can use them as a revolutionary telescope to see beyond parts of the universe obscured by dust and gas.

6. Dark Matter

False-color depiction of dark matter around a star cluster. Image Credit: J.-P. Kneib/ESA/NASA

If you put all of the energy and matter of the cosmos into a pie and divvy it up, the result is shocking.

All of the galaxies, stars, planets, comets, asteroids, dust, gas and particles account for just 4 percent of the known universe. Most of what we call "matter" -- about 23 percent of the universe -- is invisible to human eyes and instruments.

For now.

Scientists can see dark matter's gravitational tug on stars and galaxies, but are searching feverishly for ways to detect it first-hand. They think particles similar to neutrinos yet far more massive could be the mysterious, unseen stuff.

5. Dark Energy

Computer simulation of dark matter filaments. Image Credit: Science Magazine

What really has everyone on the planet confused -- including scientists -- is dark energy.
To continue with the pie analogy, dark energy is a Garfield-sized portion at 73 percent of the known universe. It seems to pervade all of space and push galaxies farther and farther away from one another at increasingly faster speeds.

Some cosmologists think this expansion will leave the Milky Way galaxy as an "island universe" in a few trillion years with no other galaxies visible.

Others think the rate of expansion will become so great that it will result in a "Big Rip." In this scenario, the force of dark energy overcomes gravity to disassemble stars and planets, the forces keeping particles sticking together, the molecules in those particles, and eventually the atoms and subatomic particles. Thankfully, humankind probably won't be around to witness to cataclysm.

4. Planets

Illustration of terrestrial, extrasolar planets. Image Credit: R. Hurt/NASA/JPL-Caltech

It might sound strange because we live on one, but planets are some of the more mysterious members of the universe.

So far, no theory can fully explain how disks of gas and dust around stars form planets -- particularly rocky ones.

Not making matters easier is the fact that most of a planet is concealed beneath its surface. Advanced gadgetry can offer clues of what lies beneath, but we have heavily explored only a few planets in the solar system.

Only in 1999 was the first planet outside of our celestial neighborhood detected, and in November 2008 the first bona fide exoplanet images taken.

3. Gravity

Artist depiction of gravity waves around merging black holes. Image Credit: NASA

The force that helps stars ignite, planets stay together and objects orbit is one of the most pervasive yet weakest in the cosmos

Scientists have fine-tuned just about every equation and model to describe and predict gravity, yet its source within matter remains a complete and utter mystery.

Some think infinitesimal particles called gravitons exude the force in all matter, but whether or not they could ever be detected is questionable.

Still, a massive hunt is on for major shake-ups in the universe called gravitational waves. If detected (perhaps from a merger of black holes), Albert Einstein's concept that the universe has a "fabric" of spacetime would be on solid ground.

2. Life

E. coli bacteria. Image Credit: NIH

Matter and energy abound in the universe, but only in a few places is the roll of the cosmic dice perfect enough to result in life.

The basic ingredients and conditions necessary for this strange phenomenon are better understood than ever before, thanks to abundant access to life here on Earth.

But the exact recipe -- or recipes -- to go from the basic elements of carbon, hydrogen, nitrogen, oxygen, phosphorus and sulfur to an organism is a prevailing mystery.

Scientists seek out new areas in the solar system where life could have thrived (or still may, such as below the surface of watery moons), in hopes of arriving at a compelling theory for life's origins.

1. The Universe

Illustration showing the creation and expansion of the universe. Image Credit: NASA

The source of energy, matter and the universe itself is the ultimate mystery of, well, the universe.

Based on a widespread afterglow called the cosmic microwave background (and other evidence), scientists think that the cosmos formed from a "Big Bang" -- an incomprehensible expansion of energy from an ultra-hot, ultra-dense state.

Describing time before the event, however, may be impossible.

Still, atom smasher searches for particles that formed shortly after the Big Bang could shed new light on the universe's mysterious existence -- and make it a bit less strange than it is today.
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Saturday, March 22, 2008

Hubble Discovers Life Basics On Distant Sphere

A NASA developed rendering of HD 189733b, an extrasolar planet, is located more than 60 light years from Earth, which has the organic molecule methane in its atmosphere. Image Credit: NASA, ESA, and G. Bacon (STScI)

Hubble Discovers Life Basics On Distant Sphere

The upgraded Hubble telescope, with its perch circling above the Oblate Spheroid out in space, has discovered what is considered the basic evidence of the “signature” that life (as we understand it) could exist on another planet. The distant sphere is located 63 million light years away and is known as HD 189733b.

The process of the creation of life requires the existence of carbon based gasses and other chemicals on which bacteria and other life forms are composed. It is believed that without these signature compounds, life could and would not develop.

Stellar spectrography by a flame-cutting grid - Capella's Spectrum, order 1 spectral image taken by a Philips vesta webcam. Image Credit: lightfrominfinity.org

So the discovery of such signature evidence through spectrography with instruments on platforms like the Hubble Telescope, on spheres that exist in other solar systems, makes for a better understanding and pushes the envelop of current scientific techniques.

This excerpted from WIRED -

Molecular Basis of Life Discovered on Extrasolar Planet
By Alexis Madrigal, Wired - 03.19.08 6:15 PM

Scientists using the Hubble Space Telescope have for the first time found the telltale signature of methane, an organic molecule, in the atmosphere of a planet outside our solar system.

Methane is one of the chemicals of life, an organic compound in the class of molecules containing carbon. However, no life is likely to exist on the large, gaseous planet known as HD 189733b. Its daily temperatures can reach 1,340 degrees Fahrenheit.

"These measurements are a dress rehearsal for future searches for life," said
Mark Swain, a scientist at NASA's Jet Propulsion Laboratory and the lead author of a new study that appears in Nature tomorrow. "If we were able to detect [methane] on a more hospitable planet in the future, it would really be something exciting."
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Since the discovery of the first so-called exoplanet 13 years ago, scientists have been able to glean little about the 270-plus known extrasolar planets. Even rough sizes and masses have been calculated for a mere 30 of those planets. It is only in the last year that scientists have begun to characterize the conditions on these planets, like their surface temperatures, and as in this case, the chemical composition of their atmosphere. Such findings not only shed light on other solar systems, but also on our own.
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HD 189733b, a so-called "hot Jupiter," located 63 light years away, has proven a boon for scientists studying exoplanets. Its large size and proximity to its star mean that it dims the star's light more than any other known exoplanet. Combine that with its home star's high brightness, and scientists find that the system creates the best viewing conditions of any known extrasolar system.
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At different wavelengths, every atom and molecule has its own telltale footprint, so scientists can convert what are known as absorption spectra into the chemical composition of the object they're looking at.

The technique, known as spectrography, will remain the main scientific technique for learning about exoplanets into the future with planets that could support life.
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"Twenty years from now, we'll be able to do this for superearths," said
Jonathan Fortney, an astronomy professor at the University of California, Santa Cruz. "We'll be able to see methane in the atmosphere of an Earth-like planet."

To do so, however, astronomers will need new tools. Swain's team used Hubble's Near Infrared Camera and Multi-Object Spectrometer to capture rough spectrographic data. They were forced to use the low-resolution tool because the dedicated instrument for spectrography -- the Space Telescope Imaging Spectrograph -- broke in 2003, Redfield said.

"The STIS spectrograph would get resolutions several orders of magnitude higher than the tool they used," said
Seth Redfield, a Hubble postdoctoral fellow at the University of Texas at Austin, who previously identified sodium in HD 189733b's atmosphere.

He said NASA was planning to try to fix the tool in late summer of this year, and that access to the tool could lead to new discoveries. In the meantime, scientists will keep plugging away, revealing the properties of planets dozens of light years away, molecule by molecule.

"We know so little observationally about these planetary atmospheres that any sort of measurement is tremendously exciting," Redfield said.

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