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Results tagged “photos” from Breaking Orbit

Shortly after the Chandra X-ray Observatory opened its eye for the first time in 1999, the orbiting probe snapped its first picture of a supernova remnant about 190,000 light-years away that's lovingly called 1E 0102.2-7219—or E0102 for short.

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—Image courtesy NASA/CXC/SAO

Yesterday, ten years to the day after the probe's July 23 launch, the Chandra team released this updated version of the supernova's portrait:

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—X-ray (NASA/CXC/MIT/D.Dewey et al. & NASA/CXC/SAO/J.DePasquale); Optical (NASA/STScI)

In the immortal word of Keanu Reeves: Whoa.

The brilliant new picture (click here for a larger version) combines Chandra's x-ray data with a visible-light image from its orbiting partner the Hubble Space Telescope. Together the two orbiters show the supernova's hot outer blast wave as a blue halo around the cooler inner material, with bright stars glittering in the background.

The green blob in the lower right is a cloud of gas and dust being illuminated by one very massive star (not pictured), probably not unlike the one that went boom and created E0102.

While the x-ray data add some great visual details to the shot, Chandra also contributed to the scientific analysis of the remnant. The x-rays, for instance, have helped astronomers get a better picture of the geometry of the explosion.

That's because x-rays with different levels of energy shine differently for Chandra. Since energy levels are linked to direction, scientists can tell how the object's components are moving relative to each other.

To us, E0102 may look like a colorful cotton ball in space. But Chandra reveals that the supernova is actually shaped more like a cylinder, and we're simply seeing the rounded face. There's a nifty animation of this here, in case pictures speak loader than words...

Btw, in its ten years of data collection, it seems Chandra has done its share of capturing puffballs in outer space. Here's a "rogues gallery" of some of the more famous explosions:

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Tycho's Remnant

  • About 7,500 light-years away
  • Danish astronomer Tycho Brahe saw light from the initial explosion in 1572
  • Chandra snapped it in April 2003

—X-ray: NASA/CXC/SAO, Infrared: NASA/JPL-Caltech; Optical: MPIA, Calar Alto, O.Krause et al.







kepler.jpg

Kepler's Remnant

  • About 13,000 light-years away
  • Astronomer Johannes Kepler was among the first to see it as a new object in the sky in 1604
  • Chandra studied it from April to August 2006

—Image courtesy NASA/CXC/NCSU/S.Reynolds et al.






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Cassiopeia A

  • About 10,000 light-years away
  • Discovered in the constellation Cassiopeia via radio observations in 1947
  • Chandra snapped it in December 2007

—Image courtesy NASA/CXC/MIT/UMass Amherst/M.D.Stage et al.





sn1006c.jpg

SN1006

  • About 7,000 light-years away
  • The brightest supernova ever seen from Earth, witnessed in Asia, Europe, and the Middle East in A.D. 1006
  • Chandra snapped it in April 2003

—X-ray: NASA/CXC/Rutgers/G.Cassam-Chenai, J.Hughes et al.; Radio: NRAO/AUI/NSF/GBT/VLA/Dyer, Maddalena & Cornwell; Optical: Middlebury College/F.Winkler, NOAO/AURA/NSF/CTIO Schmidt & DSS

hubble-winner-274.png

You voted, and here's your new Hubble superstar: a pair of galaxies that seem to have locked arms in an interstellar dance.

Of the six choices in Hubble's contest, Arp 274 won by a landslide—67,021 votes, as compared to the next runner-up, the spiral galaxy NGC 5172, with 26,987 votes.

Now Hubble scientists are preparing to train the space telescope at their publicly elected target, with the goal of producing a spectacular new image by early April.

So stay tuned for more about this cosmic duo!

Space Candy: Helix Nebula's Gaping Maw

Posted on February 25, 2009 | 1 Comments

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—Image courtesy ESO

Going supernova is arguably the most popular way for a star to die. But stars like our sun actually end not with a bang, but a whimper [nods to T.S. Eliot].

These mid-size stars don't explode at the end of their lives, they swell, releasing shells of gas as they blossom into planetary nebulas, which for the record, don't have much to do with planets.

Such is the Helix, a widely imaged nebula that lies about 700 light-years away.

In a new picture taken by ESO's La Silla Observatory in Chile, astronomers can see distant galaxies through the nebula's thinly spread gases.

Is it just me, or does this version of the Helix look like a giant space fish about to swallow us whole?

Japan proposed, and Kaguya said yes.

The Japan Aerospace Exploration Agency (JAXA) yesterday released what's being touted as the first ever picture of a penumbral eclipse as seen from the moon.

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—Image copyright JAXA/NHK

The moon-orbiting probe Kaguya (named for a lunar princess in Japanese folklore) snapped the high-definition footage on February 10 as Earth moved between the moon and the sun.

From our planet's surface, the lunar eclipse was barely noticeable, as the moon was moving through the outer parts of Earth's shadow—the penumbra—where only some sunlight gets blocked.

But from the moon, the disk of the Earth almost fully covered the sun. During the progression of this unusual eclipse, Kaguya caught sight of the so-called diamond ring effect.

Diamond rings are normally seen from Earth during solar eclipses. As the moon moves between the sun and Earth, slight bumps and grooves on the lunar surface cause sunlight shining from behind to "bead" around the edges.

When the moon is slightly offset from the sun, a single bead can shine brightest, creating the appearance of a gem perched on of a ring of light.

This time, though, Earth played the part of the moon, blotting out the sun from Kaguya's perspective.

It seems fitting that in a year being celebrated worldwide as the 400th anniversary of telescopic astronomy, NASA and ESA have chosen one of Galileo's first loves, Jupiter, as their next top planet.

Cut-away images show the insides of Io, Ganymede, ...

moons1.jpg

In January of 1610 the famed Italian Galileo Galilei pointed a homemade 'scope at the heavens and witnessed something shocking: four "stars" moving in fixed paths around Jupiter.

What he saw were actually the gas giant's four biggest moons, which became known as the Galilean satellites—Io, Europa, Ganymede, and Callisto.

... Europa, and Callisto

moons2.jpg

—Images courtesy NASA/JPL

The tiniest of these, Europa, is only slightly smaller than Earth's moon. In fact, if it weren't for big, fat Jupiter's light drowning them out, people on Earth would be able to see all four of the satellites without the aid of a telescope.

Today NASA and ESA announced that Jupiter and its four famous moons will get priority as science targets for the next flagship mission, following in the footsteps of Cassini (Saturn) and New Horizons (Pluto).

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Hubble Rocks the Vote

Posted on January 29, 2009 | 0 Comments

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Planetary nebula NGC 2818. Bask in its glory.
—Image courtesy NASA, ESA, Hubble Heritage Team (STScI / AURA)

Have you ever looked at the latest bit of space glam from the Hubble Space Telescope and thought to yourself: Yeah, that's nice, but I *so* wish they'd snap a few shots of Planetary Nebula NGC 6072, that'd kick it hardcore.

Well, now's your chance to tell NASA what to do.

As part of the ongoing International Year of Astronomy, the folks at Hubble are giving you the opportunity to aim that ginormous telescope at an object of your choice.

The idea is that we'd get new images of something Hubble has never looked at before. The result would be not only purty pictures but some pretty neat science, hopefully.

Of course, the best we have to go on right now are blurry, grainy, and in some cases overexposed pictures of objects that we don't know a lot about. That's the point, but it also makes it hard to know what the best target would be, scientifically speaking.

They've narrowed the options down to six candidates based on the brightest things the 'scope would be able to see in the given observation window.

Over at Hubblesite, you can check out low-res sky survey images of your choices—a star-forming nebula, two planetary nebulae, and three different takes on galaxies.

For some help deciding, the site also has a brief video of Dr. Frank Summers, Hubble astronomer, walking you through the candidates' qualifications.

Nominations are due by March 1, and the Hubble shot of the winning object will be released in April. So get out there and vote, kiddies!

Imagine trying to spot a moth flying around the rim of a searchlight. If the light is a few feet from you, there's a chance you would catch the occasional flicker of motion, but the moth would be largely hidden by the glare.

star-boat.jpg

Now imagine the spotlight shines as bright as the sun and is several light-years away. Chances are all signs of that moth are obliterated.

Such is the challenge placed at the feet of those searching for habitable Earthlike worlds orbiting sunlike stars.

Prowling the poster hall here at the winter meeting of the American Astronomical Society in Long Beach, I came across a group of people who hope to overcome the obstacles by sending a giant gold daisy into space.

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It's IYA, Baby!

Posted on January 4, 2009 | 1 Comments

After shaking off the daze induced by family, bubbly, and the vast amounts of tamales that accompany my winter holidays, I have washed up on the shores of Long Beach, California, where almost 2,500 astronomers are gathered for the 213th meeting of the American Astronomical Society.

The biggest astro-nerd fest of the year is even bigger for 2009, because the meeting is playing host to the U.S. kick-off of the International Year of Astronomy, tied to the 400th anniversary of Galileo's telescope. Woot!

Having peeked at the press conference sked and session lists, I can tell there's some fun things in the works, including the imminent arrival of Galileo's *actual* original telescope to the U.S. But that comes later.

In a neat little cosmic alignment, the start of the meeting also coincides with the five-year anniversary of the twin Mars rovers Spirit and Opportunity, those plucky little workhorses that have been roaming the Martian landscape since 2004.

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Opportunity snaps dunes in Endurance Crater tinted blue in false color due to the presence of hematite-rich spherules known as blueberries
—Image courtesy NASA/JPL

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Biggest Full Moon Photos

Posted on December 12, 2008 | 1 Comments

As luck would have it, the weather just did not feel like playing nice with me today.

I was super excited to see the rain clear up over Washington, D.C., this morning, and I got a couple nice peeks of tonight's biggest full moon of the year as I was walking home.

By the time I got out on my balcony with a camera, however, an almost impenetrable blanket of clouds had swept over the Arlington skies, and that glorious moon played hide-and-seek with me for a good hour.

This was the best I could do before my frozen body insisted I go back inside and eat a hot meal.

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8:43 p.m. EST
—Photo by Victoria Jaggard

Kinda spooky, I guess, but not very detailed, so I just had to try again.

By around 11 p.m. the clouds had cleared, and I braved the crisp winter air to snap a few more rounds.

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A Crater By Any Other Name

Posted on October 22, 2008 | 1 Comments

It's been just over two weeks since the MESSENGER spacecraft swooped past Mercury during its second flyby of the innermost planet.

Since the initial fervor, the MESSENGER team has been faithfully releasing images collected during the close encounter, some of which are providing data-hungry scientists with fodder for speculation about Mercury's geologic processes.

Today's offering highlights what I think must be one of the more frustrating aspects of being a planetary explorer: naming stuff.

Where in the universe—other than your local Barnes & Noble—can you find Arabic, Swiss, Ukrainian, and ancient Roman poets sitting next to a Baroque-era French composer being cut in half by one of Captain Cook's ships?

That'd be Mercury's southern side, which is just packed with craters first seen during the original Mariner 10 flybys in 1974 and '75.

mercury-craters.jpg

—Image courtesy NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Now, gone are the days when being the first person to see something and, whenever possible, stick a flag in it grants you the automatic right to bestow upon it a name. In astronomy they's got rules, and the rules for naming things can get pretty specific.

[Thank goodness for this, by the way, or the list of gas giant planets in our solar system might have been Jupiter, Saturn, Neptune, and George.]

For Mercury, the International Astronomical Union states that all craters must be named for famous dead artists, musicians, or writers. Rupes, or cliffs, are named after famous explorers' ships.

Given these constraints, creating the list of approved crater names on heavily pockmarked Mercury must have really stumped even the most ardent trivia fans.

Consider too that most of these monikers were decided before we'd even gotten to see more than 45 percent of the planet's surface.

In April the IAU added six crater names to Mercury's approved list, and more are sure to come as the onslaught of MESSENGER images gets scrutinized.

Hubble Repairs Hit the Brakes

Posted on October 17, 2008 | 0 Comments

Oops, Hubble did it again.

As the media touting Hubble's revival late last night, NASA engineers ran smack into Murphy's Law: A pair of seemingly unrelated glitches snarled efforts to fix the science data formatter, the bit on the space telescope that sends its collected information back to Earth.

The primary formatter had failed on September 27, so engineers had sent Hubble into safe mode to remotely switch to an onboard backup system.

It was smooth sailing until yesterday afternoon, when something snagged during calibration of two of the science instruments that feed data into the formatter.

"We experienced an issue late yesterday on Hubble that we're still troubleshooting," Goddard spokesperson Ed Campion told National Geographic News this morning.

"We've stopped trying to activate science."

NatGeo News reporter Anne Minard was right on top of the action—you can read her breaking report on the events posted this morning, as well as a more detailed followup based on an afternoon press conference.

No doubt the flurry of drama will revive concerns about the cost and effort of maintaining Hubble. It's an 18-year-old piece of equipment, after all, and it relies on human intervention via the also aging and highly controversial shuttle program to keep everything operational.

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One of Hubble's most famous images, the "pillars of creation" in the Eagle nebula
—Photograph courtesy NASA, ESA, STScI, J. Hester and P. Scowen (Arizona State University)

But Hubble's successor, the James Webb Space Telescope, isn't due for launch until 2013, leaving quite a gap in data collection if we let the old boy go.

With the U.S. in the grip of an escalating financial crisis, will the public balk at the millions of dollars it will take to get Hubble once again up to its fullest potential? Or will the telescope's reputation for eye-popping visuals keep it afloat no matter the cost?

America, how much is Hubble worth to you?

Mission to Mercury: Just the Facts

Posted on October 7, 2008 | 0 Comments

messenger-new.jpg

—Image courtesy NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

NASA's MESSENGER space probe sent some postcards home this morning from its second jaunt past Mercury, that tiny planet nearest to the sun.

The flyby is part of some maneuvering MESSENGER has to do to ease itself from orbiting the sun to orbiting Mercury.

Using the gravity of other planets helps the orbiter reach Mercury while saving on fuel, a bit of technique that was not even feasible until the 1980s.

MESSENGER's entire trajectory, looking down on Earth's orbit plane

messenger-orbit.jpg
—Image courtesy NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

NatGeo News reporter Anne Minard has the skinny on what scientists are saying about the new images, including the implication that geologic processes on Mercury might be an awful lot like those on the moon.

Minard also collected a great set of facts and figures about Mercury and its exploration that didn't make the cut for the news story, but that I think deserve a bit of airtime:

  • Mercury has a metal-rich core 60 percent denser than Earth's.
  • The planet's thin atmosphere is contains sodium, calcium, potassium, and, surprisingly, water vapor.
  • Mercury's daytime surface temperatures can reach over 800 degrees Fahrenheit (426 degrees Celsius), but it looks like the planet still manages to have ice in some of its craters.
  • Mariner 10 flew by Mercury three times in 1974 and 1975, capturing images of about 45 percent of the planet's cratered surface.
  • MESSENGER launched on August 3, 2004. It carried about 1,323 pounds (600 kilograms) of liquid chemical propellant at launch, nearly 55 percent of its total launch weight.

messenger-launch.jpg

  • The spacecraft conducted an Earth flyby in 2005 and two Venus flybys in 2006 and 2007 on its way to Mercury.
  • MESSENGER first flew by Mercury in January of this year, imaging a further 20 percent of the surface.
  • On its second flyby, MESSENGER flew 124 miles (200 kilometers) above Mercury's surface during its closest approach on October 6, 2008.
  • The craft imaged 30 percent of the surface not seen during previous space-based missions.
  • As of today [October 7, 2008] MESSENGER is about 61million miles (99 million kilometers) from Earth.
  • The craft is halfway through a 4.9-billion-mile (7.9-billion-kilometer) journey into Mercury's orbit that includes more than 15 trips around the sun.

—Image courtesy NASA

Sometimes it must seem like the Hubble Space Telescope is a time traveler.

Within hours of Hubble making headlines because it shut itself down due to a serious mechanical failure, mission scientists released a survey of galactic diversity based on new Hubble images.

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NGC 253, Sculptor Group galaxy, 13 million light-years away
—Image courtesy NASA, ESA, J. Dalcanton and B. Williams (University of Washington)

Using two of its powerful cameras, Hubble captured high-resolution views of 69 galaxies that lie 6.5 million to 13 million light-years away. This sounds pretty distant, but it's actually right in our cosmic backyard.

The project—delightfully named the ACS Nearby Galaxy Survey Treasury, or ANGST, program—aims to use the new, detailed views of old stars in nearby galaxies like a fossil record.

More distant galaxies are younger galaxies to Earth-based observers, because the light had to travel for millions of years to reach us, so what we see now is how a galaxy looked in it's early days.

The young/far galaxies are loaded with active star formation and are good models in general for figuring out how galaxies grow up.

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NGC 300, Sculptor Group galaxy, 7 million light-years away

—Image courtesy NASA, ESA, J. Dalcanton and B. Williams (University of Washington)


By comparing the closer, geriatric galaxies to their younger cousins, scientists hope to trace how various types of galaxies might have evolved, as well as possibly getting a clearer picture of stellar life cycles. [Yes, I know I'm supposed to be talking about planets here, but you gotta have stars for planets to form, right?]

But, you might ask, NASA says Hubble is broken, so how is it still releasing new images?

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Stormy Saturn and Some Space Trivia

Posted on September 30, 2008 | 0 Comments

Move over, Mars, you're not the only act in town that can show folks some extreme weather.

The orbiting Cassini spacecraft took this image, released today by NASA, of Saturn's northern latitudes, including an edge of the planet's famed atmospheric hexagon that swirls around its north pole.

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—Image courtesy NASA/JPL/Space Science Institute

The tight, high-resolution shot was captured on August 25 using a wide-angle camera with a spectral filter (no, ghost hunters, it's not what you think) that lets in infrared light.

Taken from about 336,000 miles (541,000 kilometers) above the planet, the shot encompasses 18 miles (29 kilometers) per pixel, which should give viewers some idea of the scale of those swirling storms.

As a gas giant, Saturn is almost all atmosphere, and it's raging winds really book it—hustling the clouds around at up to 1,100 miles (1,770 kilometers) an hour.

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About This Blog

The moon
From dwarf planets to hot Jupiters, join NatGeo News space and tech editor Victoria Jaggard in a global discussion about all things extraterrestrial.


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