Hartley 2 Spawns Meteor Shower

Universe Image Gallery

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The comet of the year for 2010 seems to be Hartley 2. Although this comet is receding from Earth now (its closest approach was in the latter half of October) and growing fainter, it seems to have left us with one last hurrah: The spawning a brief meteor shower.


Although other comets, such as 2009 R1 (McNaught) and 2P/Encke have passed earlier this year, none has presented an especially tempting target for amateur astronomers (both McNaught and Encke were too close to the Sun during perihelion to be easily observed). Additionally, Hartley is the target of a flyby of the Deep Impact probe bringing it further attention.

Meanwhile, observationally, the comet has been somewhat difficult to observe. I went out on October 17th to hunt for it with a 4″ telescope, but despite my best efforts, couldn’t find it. Although the comet was predicted to reach 5th magnitude, the growing nucleus has apparently become so diffuse, reaching over 1° in the sky, that it’s hard to spot. Undeterred, I attempted again this past weekend with my 8″ SCT. Again, my attempts were frustrated. Even a 15 second exposure with my camera barely brought out more than a smudge.

Yet that night we observed several bright meteors radiating from near Cassiopeia which is where Hartley had been a few weeks prior. We checked to ensure there weren’t any other annual meteor showers from that region. Sure enough, there weren’t, and we wondered if there might be a connection between Hartley’s passing and the meteors we witnessed.

Sure enough, just such a shower was a predicted possibility. Whether or not the shower would occur would depend on just how much dust Hartley had given off in the past and how diffuse the cloud had grown (on this pass and others) since its closest approach to Earth was still 12 million km. Although the meteors my friends and I witnessed were notable (around 2nd to 3rd magnitude) they came from the wrong direction. Meteors spawning from Hartley should have a radiant in Cygnus, the swan. But while ours may not have caught these “Hartley-ids”, others have been witnessing a far grander show in the past few nights that seem to come from the right direction.

In Seascape California, Helga Cabral caught a bright fireball. “I saw a bright white ball and tail, arcing towards the ocean. It was quite beautiful and it looked like it was headed out to sea and so picture perfect it could have been a movie!” A similar fireball was reported the same night near Boston, Massachusetts by Teresa Witham. The predicted peak of this shower occurs tonight so if you have a chance and clear skies, go out and look. As with most showers, there may be some stragglers just before and after so you may be able to catch some for the next few nights if conditions tonight aren’t favorable.

Meteors from Hartley 2 will have a relatively low velocity upon entering our atmosphere since the comet is traveling roughly in the same direction. As such, the expected velocity as it hits our planet is a mere 7 miles a second. The result of this is that they will likely travel slowly across the sky, taking perhaps as much as a few seconds. In contrast, the Leonid showers coming later this month have a relative velocity of 45 miles per second, which causes the meteors to streak across the entire sky in less than a second. The lower velocity for the Hartley-ids will also mean they won’t undergo as much frictional heating and will likely glow fainter shades of reds and yellows.

Watch Live Coverage of EPOXI’s Hartley 2 Encounter on Nov. 4

Comet 103P/Hartley 2 Animation, created by images taken by Patrick Wiggins, NASA/JPL Solar System Ambassador to Utah. Used by permission.

Watch live coverage of the EPOXI mission’s close flyby of Comet Hartley 2. Live coverage begins on November 4, 2010 at 9:30 a.m. EDT (6:30 a.m. PDT) from mission control at the Jet Propulsion Laboratory. You can watch NASA TV’s Media Channel online at this link, (and make sure you click on the “Media Channel” tab on the right side of the “tv” screen). You can also watch on JPL’s UStream channel online. Coverage includes closest approach, an educational segment, and the return of close-approach images. Emily Lakdawalla of the Planetary Society Blog has posted a very detailed timeline of the encounter.
Continue reading “Watch Live Coverage of EPOXI’s Hartley 2 Encounter on Nov. 4”

Calculate the Effect of an Asteroid Impact on Earth

Impact Earth website

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A 20-km asteroid has just been predicted to hit Earth and you want to know if a. You should run for it, b. You should call Bruce Willis, or c. You can rest easy because your part of the world won’t be affected. All you have to do is input the parameters of the asteroid on the recently updated “Impact Earth” website, and you’ll find out everything about what an impactor will do to Earth, including an estimate of the size of the crater, how far away you’ll need to be in order to avoid being affected by the impact (and if that is possible), tsunami wave height, and other details of the subsequent disaster. The fun part is, you can simulate the destruction of Earth multiple times, without hurting anyone.

The original Impact Earth website was created in 2002 for use by NASA and homeland security. The new version, built in a collaboration between Purdue University and Imperial College London, is more user-friendly for the general public, as well as providing more visual details of an impact. Besides being rather fun to play around with, the website is highly educational about what a various sized impacts would do Earth, depending on if it hit ground or water.

Go play around with it.

It Could Be Our Only Hope for True 3D Holograms

This is great: Now anyone can send holographic appeals to Obi Wan Kenobi just like Princess Leia. A team from the University of Arizona’s College of Optical Sciences has developed a system that can produce truly three-dimensional images and the viewer is not required to wear special 3D glasses. The system allows the projection of a three-dimensional, moving image that refreshes every 2 seconds. So in many respects it would be very similar to R2D2’s projected holographic message in Star Wars.

“Holographic telepresence means we can record a three-dimensional image in one location and show it in another location, in real-time, anywhere in the world,” said Nasser Peyghambarian, who led the research team.
Continue reading “It Could Be Our Only Hope for True 3D Holograms”

Where In The Universe Challenge #124

It’s time once again for another Where In The Universe Challenge. Name where in the Universe this image was taken and give yourself extra points if you can name the telescope or spacecraft responsible for the image. Post your guesses in the comments section, and check back on later at this same post to find the answer. To make this challenge fun for everyone, please don’t include links or extensive explanations with your answer. Good luck!

And you can find the answer to last week’s WITU challenge here. (and no, it was not the view out the back window of the Enterprise as it Warps away from Kahn as he detonates the Genesis device — and neither is this one!)

UPDATE: The answer has now been posted (finally — sorry!)

This is one of the first images taken by the Very Large Telescope’s Infrared Spectrometer And Array Camera (ISAAC) instrument, way back in 1998. It is an infrared color composite of the quadruply lensed quasar system MG0414+0534. At the center is galaxy at redshift z = 0.96 which is responsible for the four (of which two are not completely resolved) gravitationally lensed images of a z = 2.64 quasar plus a faint arc.

See more about the image on the ESO website.

Carnival of Space #176

This week’s Carnival of Space is hosted by Wayne Hall over at Kentucky Space.

Click here to read the Carnival of Space #176.

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 Fraser know if you can be a host, and he’ll schedule you into the calendar.

Discovery’s Final Mission Delayed Again

Discovery on the launchpad. Credit: Alan Walters (awaltersphoto.com) for Universe Today

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UPDATE: Discovery has been cleared for a launch attempt on Nov. 4 at 3:29:43 p.m. EDT. After a review, NASA managers decided the electrical glitch that prompted a 24-hour delay was not a threat to flight safety. The only problem now is that the weather report calls for rain and clouds, and gave an 80% chance for conditions that would prohibit launch. We’ll keep you updated.

A power controller on space shuttle Discovery’s main engine number three failed to start during routine checks this morning causing shuttle managers to push the final launch of Discovery back at least 24 hours to Nov. 4. Engineers began troubleshooting the problem – when it appeared to correct itself. Circuit breakers have had problems like this before. However, NASA mission managers wanted to make sure they fully understood what was causing the problems.

“We make sure we truly understand the risk before we fly,” said Mike Moses, Mission Management Team Chair. “The problem is pretty simple and we wanted to make sure we’re not to aggressive on our response.”

Teams will work through the night and into Wednesday morning on this problem. To remove the affected circuit is a fairly invasive procedure and some of the circuits involved cannot be retested on the launch pad. If the launch does not occur Thursday NASA has until Sunday to launch before the launch window closes. Currently, Discovery is set to launch Thursday, Nov. 4 at 3:29 p.m. EDT.

From a crew perspective it made sense to take an additional 24 hours,” said Mike Leinbach, Shuttle Launch Director. “We’ll pick back up with our launch countdown on Thursday morning.”

Discovery is set to launch on her final, 11-day mission to the International Space Station on mission STS-133. The crew of Discovery consists of Commander Steve Lindsey, Pilot Eric Boe and Mission Specialists; Alvin Drew, Nicole Stott, Tim Kopra and Michael Barratt. The payload for this mission is the Leonardo Permanent Multipurpose Module which houses among other things the first humanoid robot to fly into space – Robonaut-2. Also onboard is the Express Logistics Carrier-4 and much-needed spare parts.

What Hanny’s Voorwerp Reveals About Quasar Deaths

The green "blob" is Hanny's Voorwerp. Credit: Dan Herbert, Peter Smith, Matt Jarvis, Galaxy Zoo Team, Isaac Newton Telescope

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Hanny’s Voorwerp is a popular topic of conversation due to its novel discovery by Hanny Van Arkel perusing images from the Galaxy Zoo project. The tale has become so well known, it was made into a comic book (view here as .pdf, 35MB). But another aspect of the story is how enigmatic the object is. Objects that are so green are rare and it lacked a direct power source to energize it. It was eventually realized a quasar in the neighboring galaxy, IC 2497 could supply the necessary energy. Yet images of the galaxy couldn’t confirm a sufficiently energetic quasar. A new paper discusses what may have happened to the source.


The evidence that a quasar must be involved comes from the green color of the voorwerp itself. Spectra of the object has shown that this coloration is due to a strong level of ionized oxygen, specifically the λ5007 line of O III. While other scenarios could account for this feature alone, the spectra also contained He II emission as well as Ne V and the lines were especially narrow. Should star formation or shockwaves energize the gas, the motions would cause Doppler broadening. An quasar powered Active Galactic Nucleus (AGN) was the best fit.

But when telescopes searched for this quasar in the galaxy, it proved elusive. Optical images from WIYN Observatory were unable to resolve the expected point source. Radio observations discovered an object emitting in this range, but far below the amount of energy necessary to power the luminous Voorwerp. Two solutions have been proposed:

“1) the quasar in IC 2497 features a novel geometry of obscuring material and is obscured at an unprecedented level only along our line of sight, while being virtually unobscured towards the Voorwerp; or 2) the quasar in IC 2497 has shut down within the last 70,000 years, while the Voorwerp remains lit up due to the light travel time from the nucleus.”

Recent observations from Suzaku have ruled out the first of these possibilities due to the lack of potassium absorption that would be expected if light from the galaxy were being absorbed in a significant amount. Thus, the conclusion is that the AGN has dropped in total output by at least two orders of magnitude, but more likely by four. In many ways, this is not entirely unexpected since quasars are plentiful in the distant universe where raw material on which to feed was more plentiful. In the present universe, quasars rarely have such material available and can’t maintain it indefinitely.

Analogs exist within our own galaxy. X-Ray Binaries (XRBs) are stellar mass black holes which form similar accretion disks and can shut down and excite on short timescales (~1 year). The authors of the new paper attempted to scale up a model XRB system to determine if the timescales would fit with the ~70,000 year upper limit imposed by the travel time. While they found a good agreement with the output from direct accretion itself (10,000–100,000 years) the team found a discrepancy in the disk. In XRBs, the material around the black hole is heated as well, and takes some time to cool down. In this case, the core of the galaxy should still retain a hot disc of material which isn’t present.

This oddity demonstrates that there is still a large amount of knowledge to be gained on the physics surrounding these objects. Fortunately, the relatively close proximity of IC 2497 allows for the potential for detailed followup studies.

Best of Earth from the ISS

Fire scars in Australia are featured in this image photographed by an Expedition 5 crewmember on the International Space Station (ISS). Bright orange fire scars show up the underlying dune sand in the Simpson Desert, Credit: NASA

The International Space Station has been orbiting the Earth every day for over 10 years, and the astronauts all say their favorite pastime is looking at the Earth. During the past 10 years, the crews have taken some great pictures of our planet, and these images provide a unique look at our world. These are just a few of the spectacular views of Earth from the space station.

Continue reading “Best of Earth from the ISS”

Ten Years Of the ISS in Pictures

Dextre, a large robotic manipulator to help with outside maintenence of the ISS was added in October of 2007. Credit: NASA

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Ten years ago, the first Expedition crew arrived at the International Space Station. Here’s a look back in time at how the station has changed and grown, and some of the people who were there to make it happen.

And if you’re really feeling the love for the ISS today, check out our 2008 article, “I Heart the ISS; Ten Reasons to Love the International Space Station.”


The configuration of the ISS when the first expedition crew arrived on Nov. 2, 2000. Credit: NASA

Expedition Two crewmembers Yury Usachev (left), mission commander, Jim Voss, flight engineer, and Susan Helms, flight engineer, share a dessert in the Zvezda Service Module. Credit: NASA
This image was taken on April 21, 2001 during Expedition 2; the first large solar arrays were added during the STS-100 space shuttle mission. Credit: NASA
The Expedition Five crewmembers in the Destiny laboratory on the ISS. From the left are cosmonaut Valery Korzun, mission commander; astronaut Peggy A. Whitson, who became the ISS’s first science officer, and cosmonaut Sergei Treschev. Credit: NASA
The Microgravity Science Glovebox was added to the Destiny lab on the ISS during Expedition 5. Credit: NASA
The Expedition Six crew pose for a crew photo in the Zarya module on the ISS; Don Pettit (front), science officer; cosmonaut Nikolai Budarin (left back), flight engineer; and astronaut Ken Bowersox, mission commander. Credit: NASA
During Expedition 6, the space shuttle Columbia accident occurred, and the shuttle program was on hold. ISS astronauts Don Pettit (left) and Ken Bowersox had to do a variety of maintenance tasks outside the ISS that normally visiting shuttle crews would have taken care. Credit: NASA.
It was rather lonely times for awhile on the ISS -- with no space shuttles flying, only two crewmembers were able to be on board the ISS. Here are Expedition 7's Yuri Malenchenko and Ed Lu. Credit: NASA
The Russian Soyuz vehicle serves as transportation and rescue vehicle for the ISS. Credit: NASA
New Crew member? No, this is the European Matroshka-R Phantom experiment, which operated during Expedition 12 in the Zvezda Service Module of the International Space Station. Matroshka, the name for the traditional Russian set of nestling dolls, is an antroph-amorphous model of a human torso designed for radiation studies. Credit: NASA
Stuff happens it space. During a spacewalk, Expedition 16 commander Fyodor Yurchikhin noticed damage to a multi-layer insulation (MLI) protective blanket on the Zarya module. The damage, he noted, was apparently from a micrometeoroid impact. The date the damage occurred is unknown but has had no impact to vehicle operations. Credit: NASA
Shuttles returned to flight in July of 2005, and this is how the ISS looked when space shuttle Discovery visited, the first shuttle visit in over 2 years. Credit: NASA
The ISS as it looked in June of 2007, during the STS-117 mission. Credit: NASA
The backbone of the ISS is the huge truss, brought up to the ISS in smaller segments, which are still huge by themselves. Dave Williams, STS-118 mission specialist from Canada works outside the ISS, helping to attach the Starboard 5 (S5) segment, and works on the forward heat-rejecting radiator from the station's Port 6 (P6) truss. Credit: NASA
A look inside the Harmony node that was brought to the ISS in on the STS-120 mission in 2007. Credit: NAS
Sunita Williams, Expedition 15 flight engineer, works on a science experiment in April of 2007. Credit: NASA
Backdropped by the thin line of Earth's atmosphere and the blackness of space, a portion of the International Space Station is featured in this image photographed by an Expedition 20 crew member aboard the station. in May 2009. Credit: NASA
A torn solar array panel in the ISS, which was installed during the STS-120 mission. See below for the repair job. Credit: NASA
The repaired solar array, fixed by STS-120 astronauts. Credit: NASA
European Space Agency (ESA) astronaut Hans Schlegel, STS-122 mission specialist, works on the new Columbus laboratory that was installed in February 2008. Credit: NASA
Astronauts work on adding the Japanese logistics module-pressurized section in March of 2008 during the STS-123 mission. Credit: NASA
Dextre, a large robotic manipulator to help with outside maintenence of the ISS was added in October of 2007. Credit: NASA
A motley-looking crew of the Expedition 17 and 18 crewmembers in the Harmony node in Oct. 2008. Credit: NASA
Here's how the ISS looked durng the STS-128 mission in September of 2009. Credit: NASA
During the STS-130 mission in Feb. 2010, the Cupola and Tranquility Node were added. The Cupola provides unprecidented views of Earth and space from the ISS. Credit: NASA
How the ISS looked during the STS-130 mission in February 2010. Credit: NASA
The Russian Mini Research Module was added in May of 2010 on STS-132. Credit: NASA
NASA astronauts Shannon Walker (left), Expedition 24/25 flight engineer; Tracy Caldwell Dyson, Expedition 23/24 flight engineer; and Doug Wheelock, Expedition 24 flight engineer and Expedition 25 commander, pose for photo in the Poisk Mini-Research Module 2 (MRM2) of the International Space Station.
How the ISS looks today (as of this writing), and as it looked following the STS-132 mission in May of 2010. Credit: NASA

For a complete list of pictures of each of the ISS Expedition crews, see NASA’s gallery which shows all those who have served on the space station over the past 10 years.