Finally, Hubble’s View of Comet Holmes

2007-1115hubble.thumbnail.jpg

All right, here’s the picture we’ve all been waiting for. Step aside ground-based observatories, papa Hubble’s here with images of Comet Holmes, which is now larger than the Sun. But don’t get fooled. That beautiful image on the left was taken by amateur astronomer Alan Dyer from Alberta, Canada. Hubble’s version on the right. It’s not as pretty, but it’s got inner bigness.

You already know the story. Comet Holmes was a boring comet out near the orbit of Jupiter when it flared up on October 23rd. The coma of gas and dust expanded away from the comet, and now it extends to a volume larger than the Sun.

Of course, astronomers scrambled to turn the mighty Hubble Space Telescope to join in on the sky show. The space observatory’s Wide Field Planetary Camera 2 monitored the object for several days, capturing images on October 29, 31 and November 4.

The Hubble image on the right reveals the comet’s nucleus down to a resolution as small as 54 km (33 miles) across. The image was processed to reveal differences in dust distribution near the nucleus.

Astronomers found that there’s twice as much dust along the east-west direction as the north-south direction. This gives the comet a bowtie appearance. Even 12 days after the outburst, when this picture was captured, the nucleus is still surrounded by bright dust.

This isn’t the first time that Hubble has viewed Comet Holmes. Luckily, it actually captured an image back in June 15, 1999. Back then, there was no dust around the object, and Hubble couldn’t reveal the nucleus. By measuring its brightness, astronomers estimated that Holmes is approximately 3.4 km (2.1 miles) across.

Once Holmes settles down again, astronomers will use Hubble to make another accurate measurement of its brightness. By calculating the difference, astronomers will be able to figure out how much mass it lost during this outburst.

Original Source: Hubble News Release

Planets Found Forming in the Pleiades Star Cluster

2007-1114pleiades.thumbnail.jpg

As you gaze up at the familiar Pleiades star cluster, here’s something new you can think about. Planets recently collided around two of the stars in the cluster, kicking up vast clouds of dust. New worlds are being formed, and destroyed, right before our very eyes. At least, if you’ve got the help from some of the most powerful telescopes on Earth, and in space.

This announcement was made by a team of astronomers using the Gemini Observatory in Hawaii and the Spitzer Space Telescope. Their findings will be published in an upcoming issue of the Astrophysical Journal.

The Pleiades star cluster – located in the constellation Taurus – is one of the most famous objects in the night sky. Easily visible to the unaided eye, it’s even more spectacular in binoculars or a small telescope. Although it’s often referred to as the “seven sisters”, the cluster actually contains 1,400 stars, in various stages of formation.

One of the stars, known as HD 23514, has a little more mass than our Sun. The astronomers discovered that it’s surrounded by an enormous disk of hot dust particles. Astronomers think that this is the debris from a planetary collision.

It’s believed that these dust particles, the building blocks of planets, accumulate into comets and asteroid-size bodies and then clump together into larger and larger objects. This is a violent process, though. Some objects get bigger, and others collide, shattering into dust that astronomers can detect.

Astronomers think that this is a similar process that led to the formation of the Earth’s moon. At some point in the early Solar System, a Mars-sized object collided with the Earth. The debris from that collision became the Earth and the Moon.

Two stars in the Pleiades cluster, HD 23514 and BD +20 307, are thought to be in this stage of evolution. They’re between 100 and 400 million years old. Much younger stars can have this dust when they’re 10 million years old, but it’s usually dissipated by the time a star reaches 100 million years old. It takes enormous planetary collisions to get the dust spewing out again.

Original Source: UCLA News Release

Harmony Module Moved to its Final Home

2007-1114harmony.thumbnail.jpg

Astronauts on board the International Space Station used the station’s robotic arm to move the Italian-built Harmony module (aka Node 2) to its final location today. It’s now connected to the forward facing port of the US Destiny laboratory, making way for the upcoming European Columbus laboratory.

The Harmony module was delivered to the station during Discovery’s recent STS-120 mission. During the first spacewalk of the mission, the Harmony module was temporarily attached to the Unity module.

After Discovery returned to the Earth, the Expedition 16 crew relocated the space shuttle’s docking port, PMA2, from its current location on the Destiny module to the end of the Harmony module.

With all of that port shuffling out of the way, astronaut Daniel Tani used the station’s Canadarm2 robotic arm to move Harmony (and the attached docking port) to its final home, right at the front of ISS. This is where the shuttle will dock from here on out.

Harmony has been moved, but the astronauts still need to complete two more spacewalks on November 20th and 24th to fully outfit it.

The next launch of the space shuttle Atlantis, targeted for December 6th, will bring the European Columbus laboratory to the station. The astronaut crew of STS-122 will perform a series of spacewalks to connect the module to the starboard side of the Harmony module.

Original Source: ESA News Release

Rosetta Flyby Shows the Earth’s Night Side

2007-1114rosetta1.thumbnail.jpg

Right on schedule on November 13th, ESA’s Rosetta spacecraft made its 2nd earthly flyby; testing its scientific instruments, and receiving a much needed gravitational assist. About two hours before its flyby, the spacecraft captured this image of the Earth’s night side, including Asia, Africa and Europe.

When it captured this image, Rosetta was about 80,000 km (50,000 miles) away from the Earth, above the Indian Ocean. It imaged the planet using its OSIRIS instrument.

You can make out the continents Asia, Africa and Europe by the lighted areas of population centres. With less electricity, Africa has large darkened regions. Australia is down at the lower right-hand side of the image, partly lit by the Sun.

Rosetta’s closest approach occurred at 20:57 GMT (3:57 pm EST) at a height of 5,295 km (3,290 miles) above a region of the Pacific Ocean, just off the coast of Chile.

The spacecraft has now completed 3 billion km of its 7.1 billion km journey to reach comet 67/P Churyumov-Gerasimenko. This was the third planetary swing-by for Rosetta and its second swing-by of Earth.

Now on its way out, Rosetta will focus its instruments on the Moon, and the Earth/Moon system. You can expect more cool images, and maybe even one with both the Earth and the Moon in a single frame. Now that would put things into perspective.

Rosetta will be back. It’s expected to make its third and finally flyby in November 2009. But not before it makes a visit to the asteroid belt, to study asteroid Steins in September 2008.

Original Source: ESA News Release

Gigantic Delta 4-Heavy Blasts Off

2007-1113delta.thumbnail.jpg

On Saturday night, the largest US rocket blasted off, carrying a 2.3 tonne Defense Support Program satellite into orbit. This was the second time a Delta IV-Heavy rocket has ever lifted off. With three core boosters strapped together, it’s like three rockets launched at once.

The launch was made even more spectacular because it was held at night. Launched at 0150 GMT Sunday (20:50 EST on Saturday), the 70-metre tall (230 feet) rocket has three separate engines, each of which can generate more than 2,900 kiloNewtons (650,000 pounds) of force. They guzzle a tonne of propellant every second.

On board the rocket was the Defense Support Program 23 spacecraft; the last in a program of Earth observation satellites designed to spot enemy missile launches and nuclear explosions.

Although the Delta IV-Heavy can carry 13 tonnes into a geostationary transfer orbit, it’s not a commercial provider – just military and government satellites. Europe’s Ariane 5 ECA is the most powerful commercial provider, able to blast off with 10 tonnes.

The Delta IV-Heavy first flew back in 2004. Boeing had originally proposed it as the vehicle that could carry the next wave of space exploration vehicles into orbit. In the end, though, NASA decided to go with the new Ares vehicle for its post-shuttle program.

During that previous test flight, the Heavy encountered a problem with its fuel lines, which caused the engines to go out early, and left the rocket lower than its intended orbit.

Just to put the capabilities of the rocket in perspective, though, the Saturn 5 could put out three times the thrust.

Original Source: United Launch Alliance

Oops, That Isn’t an Asteroid, it’s Rosetta

2007-1113rosetta.thumbnail.jpg

Remember when I mentioned that ESA’s Rosetta was inbound to make a flyby of the Earth on November 13th? Well, another group of astronomers were watching this “unknown” object, and thought that it was actually an asteroid that was going to be making a close flyby of our planet. The astronomers realized their mistake, but not after an alert was sent out to the astronomical community. Oops.

The alert was sent out by the Minor Planet Center, a clearinghouse of asteroid information organized by the Smithsonian Astrophysical Observatory for the International Astronomical Union.

Astronomers had been tracking the approaching object, designated 2007 VN84. After many observations from astronomers around the world, they calculated that it would pass us by at a distance of 1.89 radii (from the middle of the Earth).

It would have been huge news, but Denis Denisenko from Moscow’s Space Research Institute (IKI) realized that its flight path perfectly matched the upcoming Rosetta flyby.

Here’s a link to an animation, captured by astronomers in Germany, of Rosetta inbound to the Earth.

And so, just to set the record straight, ESA’s Rosetta spacecraft made its flyby on Tuesday, November 13th at 20:57 GMT, passing just 5,301 km above the Pacific Ocean. This has given it the gravitational boost it needs to meet up with Comet Churyumov-Gerasimenko in 2014.

Original Source: MPEC Alert

Astrosphere for November 13th, 2007

2007-1113m33.thumbnail.jpg

For the photo, enjoy this image of galaxy M33, captured by RickJ.

Now, I’d like to draw your attention to the 28th Carnival of Space, hosted this week by the Planetary Society’s Emily Lakdawalla.

We’re organizing the next episode of the Carnival of Space, so drop us an entry at [email protected]. And we’re always looking for new hosts to handle future carnivals.

I want to give you a last minute reminder to watch PBS Nova tonight for Judgment Day, Intelligent Design on Trial. You’ll need to check your local listings for time and channel; if you miss it tonight, I’m sure it’ll be on several times over the week. You can also watch the entire episode online at the PBS site.

Colony Worls reports on a new partnership between Russia and India for lunar research.

Selenian Boondocks has a great article about thrust augmented nozzles.

Astroprof reviews Sea Launch’s return to flight after their recent pad explosion.

The Stars my Destination reminds us that the Leonids are coming. The Leonids are coming!

Podcast: Uranus

2007-1113urans.thumbnail.jpg

This week, we’re on to the next planet in the solar system. Having only visited it up close once with Voyager 1, we don’t know much about this sideways-spinning ice giant. But today we’ll cover what we do know, including its faint rings, sideways axis of rotation and rocky core – a first in the gas planets we’ve encountered so far in our tour.
Click here to download the episode

Uranus – Show notes and transcript

Or subscribe to: astronomycast.com/podcast.xml with your podcatching software.

What’s Up this Week: November 12 – November 18, 2007

2007-1113agarum.thumbnail.jpg

Monday, November 12 – Can you spot the thin crescent of the Moon on the western horizon at sunset? Let Jupiter help you. Look for the slim appearance of Selene about 3 fingerwidths south.

Wouldn’t we all have loved to have been there in 1949 when the first scientific observations were made with the Palomar 5-meter (200-inch) telescope? Or to have seen what Voyager 1 saw as it made its closest approach to Saturn on this date in 1980? To watch Space Shuttle Columbia launch in 1981? Or even better, to have been around in 1833 – the night of the Great Leonid Meteor Shower! But this is here and now, so let’s make our own mark on the night sky as we view the Moon.

This evening have a look at the lunar surface and the southeast shoreline of Mare Crisium for Agarum Promontorium. To a small telescope it will look like a bright peninsula extending northward across the dark plain of Crisium’s interior, eventually disappearing beneath the ancient lava flow. Small crater Fahrenheit can be spotted at high power to the west of Agarum, and it is just southeast of there that Luna 24 landed. If you continue south of Agarum along the shoreline of Crisium you will encounter 15 kilometer high Mons Usov. To its west is a gentle rille known as Dorsum Termier – where the Luna 15 mission remains lie. Can you spot 23 kilometer wide Shapely further south?

While skies are fairly dark be sure to keep watch for members of the Pegasid meteor shower – the radiant is roughly near the Great Square. This stream endures from mid-October until late November, and used to be quite spectacular. Watch for the peak on November 17.

Tuesday, November 13 – Today is the birthday of James Clerk Maxwell. Born in 1831, Maxwell was a leading English theoretician on electromagnetism and the nature of light.

Tonight when you’ve explored the lunar surface on your own, let’s take a journey of 150 light-years as we honor Maxwell’s theories of electricity and magnetism as we take a look at a star that is in nuclear decay – Alpha Ceti.

Its name is Menkar, and this second magnitude orange giant is slowly using up its nuclear fuel and gaining mass. According to Maxwell’s theories of the electromagnetic and weak nuclear forces, W bosons must exist in such circumstances – this was an extremely advanced line of thinking for the time. Without getting deep into the physics, simply enjoy reddish Alpha for the beauty that it is. Even small telescopes will reveal its 5th magnitude optical partner 93 Ceti to the north. It’s only another 350 light-years further away! You’ll be glad you took the time to look this one up, because the wide separation and color contrast of the pair make this tribute to Maxwell worth your time!

Wednesday, November 14 – Up before dawn this morning? Take the time to look on the eastern horizon and see if you can still spot Mercury!

This evening on the Moon we will be returning to familiar features Theophilus, Cyrillus and Catharina. Why not take the time to really power up on them and look closely? Curving away just to the southwest of Catharina on the terminator is another lunar challenge feature, Rupes Altai, or the Altai Scarp. Look for smaller craters beginning to emerge, such as Kant to the northwest, Ibn-Rushd just northwest of Cyrillus and Tacitus to the west.

On this day in 1971, Mariner 9 became the first space probe to orbit Mars. Why not wait until the Red Planet rises above the atmosphere’s influence and have a look at it as well? Right now (and until the end of the year) is one of the best times to view Mars at a reasonable hour. Enjoy!

Thursday, November 15 – Today marks a very special birthday in history. On this day in 1738, my personal hero William Herschel was born. Among this British astronomer and musician’s many accomplishments, Herschel was credited with the discovery of the planet Uranus in 1781, the motion of the Sun in the Milky Way in 1785, Castor’s binary companion in 1804; and he was the first to record infrared radiation. Herschel was well known as the discoverer of many clusters, nebulae, and galaxies. This came through his countless nights studying the sky and writing catalogs whose information we still use today. Just look at how many we’ve logged this year! Tonight let’s look towards Cassiopeia as we remember this great astronomer…

Almost everyone is familiar with the legend of Cassiopeia and how the Queen came to be bound in her chair, destined for an eternity to turn over and over in the sky, but did you know that Cassiopeia holds a wealth of double stars and galactic clusters? Seasoned sky watchers have long been familiar with this constellation’s many delights, but let’s remember that not everyone knows them all, and tonight let’s begin our exploration of this Cassiopeia with two of its primary stars.

Looking much like a flattened “W,” its southern-most bright star is Alpha. Also known as Schedar, this magnitude 2.2 spectral type K star was once suspected of being a variable, but no changes have been detected in modern times. Binoculars will reveal its orange/yellow coloring, but a telescope is needed to bring out its unique features. In 1781, Herschel discovered a 9th magnitude companion star and our modern optics easily separate the blue/white component’s distance of 63″. A second, even fainter companion at 38″ is mentioned in the list of double stars and even a third at 14th magnitude was spotted by S.W. Burnham in 1889. All three stars are optical companions only, but make 150 to 200 light-year distant Schedar a delight to view!

Just north of Alpha is the next destination for tonight…Eta Cassiopeiae. Discovered by Herschel in August of 1779, Eta is quite possibly one of the most well-known of binary stars. The 3.5 magnitude primary star is a spectral type G, meaning it has a yellowish color much like our own Sun. It is about 10% larger than Sol and about 25% brighter. The 7.5 magnitude secondary (or B star) is very definitely a K-type: metal poor, and distinctively red. In comparison, it is half the mass of our Sun, crammed into about a quarter of its volume and is around 25 times dimmer. In the eyepiece, the B star will angle off to the northwest, providing a wonderful and colorful look at one of the season’s finest!

Friday, November 16 – Today in 1974, there was a party at Arecibo, Puerto Rico, as the new surface of the giant 1000-foot radio telescope was dedicated. At this time, a quick radio message was released in the direction of the globular cluster M13.

To give you a rough idea of how large craters really are on the Moon, take a look at Sacrobosco tonight – just west of the Theophilus, Cyrillus and Catharina trio. When you’ve located it, power up. As huge as the Arecibo dish looks, it would take 91 of them lined side by side to reach from edge to edge of Sacrobosco’s largest interior crater. Can you imagine the possibilities if we could use a lunar crater to house an even larger radio telescope?!

Now wait for the Moon to set, because the annual Leonid meteor shower is underway. For those of you seeking a definitive date and time, it isn’t always possible. The meteor shower itself belongs to the debris shed by comet 55/P Tempel-Tuttle as it passes our Sun in its 33.2 year orbital period. Although it was once assumed that we would merely add around 33 years to each observed “shower,” we later came to realize that the debris formed a cloud that lagged behind the comet and dispersed irregularly. With each successive pass of Tempel-Tuttle, new filaments of debris were left in space along with the old ones, creating different “streams” that the orbiting Earth passes through at varying times, which makes blanket predictions unreliable at best.

Saturday, November 17 – If you didn’t stay up late, then get up early this morning to catch the Leonids. Each year during November, we pass through the filaments of debris – both old and new – and the chances of impacting a particular stream from any one particular year of Tempel-Tuttle’s orbit becomes a matter of mathematical estimates. We know when it passed… We know where it passed… But will we encounter it and to what degree?

Traditional dates for the peak of the Leonid meteor shower occur as early as the morning of November 17 and as late as November 19, but what about this year? On November 8, 2005 the Earth passed through an ancient stream shed in 1001. Predictions ran high for viewers in Asia, but the actual event resulted in a dud. There is no doubt that we crossed through that stream, but its probability of dissipation is impossible to calculate. Debris trails left by the comet in 1333 and 1733 look the most promising for this year, but we simply don’t know.

We may never know precisely where and when the Leonids might strike, but we do know that a good time to look for this activity is well before dawn on November 17, 18 and 19th. With the Moon mostly out of the way, wait until the radiant constellation of Leo rises and the chances are good of spotting one of the offspring of periodic comet Tempel-Tuttle. Your chances increase significantly by traveling a dark sky location, but remember to dress warmly and provide for your viewing comfort.

On this day in 1970, the long running Soviet mission Luna 17 successfully landed on the Moon. Its Lunokhod 1 rover became the first wheeled vehicle on the Moon. Lunokhod was designed to function three lunar days but actually operated for eleven. The machinations of Lunokhod officially stopped on October 4, 1971, the anniversary of Sputnik 1. Lunokhod had traversed 10,540 meters, transmitted more than 20,000 television pictures, over 200 television panoramas and performed more than 500 lunar soil tests. We’ll take a look at its landing site in the days ahead. Spaseba!

Sunday, November 18 – If you got clouded out of the Leonids yesterday morning, there is no harm in trying again before dawn! The meteor stream varies, and your chances are still quite good of catching one of these bright meteors.

Tonight let’s head toward the lunar surface as we have a look at a series of lunar club challenges you may not have logged yet. Just slight below central towards lunar south, look for a series of rings which grow smaller as they progress. Once again, these are Ptolemaeus, Alphonsus and Arzachel. But, focus your attention on the largest of these, and in particular the small crater caught on its northern edge.

Named for Sir William himself, crater Herschel spans 41 kilometers wide and drops to a depth of 3770 kilometers below the surface. While you’re journeying, look for small Ammonius caught in Ptolemaeus’ interior. Further south, see if you can catch Alphonsus’ bright central peak. Ranger 9’s remains lay just northeast of there!

The Voice of Dr. Wernher von Braun

2007-1113braun.thumbnail.jpg

A bit of inspiration and a pound of sweat. Sounds like a perfect recipe for advancement, but sometimes more is needed. Space pioneers had inspiration and certainly worked wonders in the lab and at the desk. But, they also had to be spokespeople for the completely new field. This need is readily apparent in the book crafted by Irene Powell-Willhite entitled The voice of Dr. Wernher von Braun – An Anthology. Through careful selection and editing, she provides copies of 47 speeches given or written by Dr. von Braun. From them, it’s clear that after the 9 to 5 work hours, still much effort was necessary to keep the space program alive.

Dr. von Braun is the German engineer who is credited with being the driving force for the development of the V2 military rocket of World War II. At the end of the war, he and many of his colleagues purposefully surrendered to the Americans with the hope and desire of continuing rocket development. However, for many years they languished at back woods military research centres. His skills weren’t in demand until the U.S. public got a fright from the U.S.S.R’s Sputnik satellite. Even then, von Braun realized that broad public support was necessary to continually advance the U.S. military and subsequent civilian rocket programs. In particular, only with the nation’s support would humans land on Mars.

This need for continual advocacy is readily apparent from the collection presented by Powell-Willhite. Von Braun’s audiences included rotary clubs, NATO groups, SHAPE, press clubs and even dental associations. From them, the reader will readily recognize von Braun’s skill in effectively joining the interests of the audience with his own. Usually he did so by referring to the audience’s hopes and fears. Rarely did he introduce technical or quantitative elements, unless the audience expected such. Interestingly enough, one of the early speeches identified the alien menace as a purpose. However, he usually focused upon hard immediate gains, such as satellites for television transponders, satellites for weather forecasting, methods for program management, and construction of specialized material. Through his speeches, the reader sees that von Braun consistently demonstrated that humans in space were leading to a betterment in the lives of everyone in the nation.

Such a support of the space program is expected when coming from one of the prime racketeers. And, this anthology has other aspects. As the speeches appear in a chronological fashion, the reader can see how the progress of the space program added substance. Early speeches talked about future gains, while later speeches talked about the advancements already made. On a more sombre note is the diminishing hope shown for the program’s future. Early speeches championed flights to Mars, while toward the end, von Braun talked about a strong anti-science mood that was permeating society, especially within institutes for early education. Yet, the speeches never showed anger or regret, only desire and advocacy. From this, the reader can see change, from von Braun the dreamer to von Braun the practical manager.

Powell-Willhite’s anthology can serve a number of other purposes in addition to being an interesting reflection of von Braun’s attitude to the space program. For example, advocates and speech writers from any field can see how to write a speech on one topic so as to interest an audience that has only cursory interest. It’s also interesting to see how Braun massaged technical data to suit the expected level of the audience. Hence, from a public relations perspective, this anthology may offer many interesting perspectives.

Where this anthology fails is the lack of perspective from Powell-Willhite herself. There’s no basis for the selection of the 47 speeches, even though von Braun is purported to have given nearly 500. There is no perspective or overview or suggestion on what the reader should look for. Each speech lies in its own chapter and, aside from the title of the speech (if one exists) and the speech itself, there is usually naught else. This is great if the reader just wants to read the speeches. However, if the reader is looking for a little more on the why and wherefore, it’s not here.

There’s good reason for Dr. von Braun being given credit for boosting the U.S’s space program. His engineering and management skills and his advocacy did wonders. Evidence of this springs forth in the book by Irene Powell-Willhite entitled The Voice of Dr. Wernher von Braun – An Anthology. Its collection of speeches show a man dedicated to helping humankind take another step into the future.

Read more reviews or purchase a copy online from Amazon.com.