DIY ISS: Big Home Improvement Projects for Space Station

STS-126 Crew. Credit: NASA

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Astronauts on the crew of STS-126, scheduled to launch on space shuttle Endeavour on Friday, Nov. 14 will be doing some big home improvement projects on their visit to the International Space Station. This mission will allow the ISS to double its crew size, as well as making sure there will be enough power for everyone living on board the orbital outpost. “It’s the most jam-packed logistics module we have ever carried up there,” STS-126 Commander Chris Ferguson said. “We’re taking a three-bedroom, one-bathroom house and turning it into a five-bedroom, two-bathroom house with a gym.”

The major additions are extra sleeping compartments, another bathroom, specialized workout equipment, a state-of-the-art water recycling system, and a refrigerator. But spacewalking astronauts will also attempt to clean up a malfunctioning SARJ – the Solar Alpha Rotary Joint that allows the station’s solar arrays to constantly track the sun. The huge mechanism hasn’t worked right for more than a year, and astronauts will clean up metal shavings from grinding parts, replace the trundle bearing assemblies and add special lubrication. It’s a big job, and will take four spacewalks to complete, including adding lubrication the port side SARJ, which has been working fine. But NASA doesn’t want to take any chances.

So astronauts will be busy both outside and in at the station during the mission, which will bring 14,500 lbs of supplies and equipment to the ISS.

“We’re going to use up a lot of the new space that we’ve brought up on the past few missions, with Node 2 and Columbus and the Kibo module,” lead shuttle flight director Mike Sarafin said. “The six-person crew is an important step toward utilizing the space station to its full capability.”

STS-126 crew.  Credit: NASA
STS-126 crew. Credit: NASA

The crew includes: Christopher Ferguson, commander, Eric Boe, pilot, Sandra Magnus, Stephen Bowen, Donald Pettit, Robert (Shane) Kimbrough and Heidemarie Stefanyshyn-Piper.

But in addition to fully utilizing the space station, the equipment brought up will allow the space station to start depending less on the space shuttle. A new regenerative environmental control and life support system will give the station the ability to recycle urine and the condensation that the crew breathes into the air into pure water that can be used for drinking or to cool the station’s systems.

Endeavour’s commander, Christopher Ferguson, considers the water system the single most important piece of equipment that he’s delivering. It’s important for when the shuttle fleet is retired in 2010, and its water deliveries dry up. But Ferguson said the benefits go beyond the space station.

“This is really it, and it has no parallel. I would challenge you to find any other system on the Earth that recycles urine into drinkable water. It’s such a repulsive concept that nobody would even broach it. But that day will come on this planet, too, where we’re going to need to have these technologies in place, and this is just a great way to get started.”

“Up until this point, the majority of the station’s drinking water was coming up from the shuttle or the Russian’s Progress vehicle,” Sarafin said. “This sets us up for long-term sustainability of the station without the shuttle.”

Nobody will be drinking the water generated by the system just yet – an onboard purity monitor needs to be checked out and multiple water samples must be analyzed by scientists on the ground first. To get that water sample home as quickly as possible, Endeavour’s crew will take a shot at getting the system hooked up before they leave.

Here’s more info on the urine-to-water system.

The new additions to the space station will be a good way to mark the 10th birthday of the International Space Station on Nov. 20 – 10 years after the first station module was launched into space and construction began.

“We’ll be transitioning to true utilization and setting up for six-person crew at that 10-year bench mark,” Sarafin said. “It’s been a tremendous international effort to get to this point, and I can’t think of a better way to celebrate it.”

Source: NASA, Houston Chronicle

Impressive Craters on Earth

Vredefort Crater. Image: NASA

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Ever since our recent encounter with asteroid 2008 TC3 — the first asteroid that was correctly predicted to hit our planet — I’ve had impact craters on the brain. Earth has about 175 known impact craters, but surely our planet has endured more bashing than that in its history. All the other terrestrial planets and moons in our solar system are covered by impact craters. Just look at our Moon through a telescope or binoculars, or check out the recent images of Mercury sent back by the MESSENGER spacecraft, or pictures of Mars from the armada of spacecraft orbiting the Red Planet, and you’ll see that impact craters are the most common landforms in our solar system.

But since two-thirds of Earth is covered by water, any asteroid impacts occurring in the oceans are difficult to find. And even though Earth’s atmosphere protects us from smaller asteroids, just like in the case of 2008 TC3, which broke up high in the atmosphere, weathering, erosion and the tectonic cycling of Earth’s crust have erased much of the evidence of Earth’s early bombardment by asteroids and comets. Most of Earth’s impact craters have been discovered since the dawn of the space age, from satellite imaging. In fact, a geologist recently discovered an impact crater using Google Earth!

Here’s my list of Earth’s Ten Most Impressive Impact Craters, starting with #1. the largest and oldest known impact crater, Vredefort Crater, shown above, located in South Africa. It is approximately 250 kilometers in diameter and is thought to to be about two billion years old. The Vredefort Dome can be seen in this satellite image as a roughly circular pattern. What an impact that must have been!

Manicouagan Reservoir.  Credit: NASA
Manicouagan Reservoir. Credit: NASA

2. Manicouagan Crater: fifth largest known impact crater. This crater is located in Quebec, Canada. It was created about 212 million years ago. Now, it is an ice-covered lake about 70 km across. This image, taken by space shuttle astronauts, shows an outer ring of rock. Close up, the rock reveals clear signs of having been melted and altered by a violent collision. The original rim of the crater, though now eroded away, is thought to have had a diameter of about 100 km.

Chicxulub Crater.
Chicxulub Crater.

3. Chicxulub Crater, third largest and possible dinosaur killer. The third largest impact crater lies mostly underwater and buried underneath the Yucatán Peninsula in Mexico. At 170km (105 miles) in diameter, the impact is believed to have occurred roughly 65 million years ago when a comet or asteroid the size of a small city crashed, unleashing the equivalent to 100 teratons of TNT. Likely, it caused destructive tsunamis, earthquakes and volcanic eruptions around the world, and is widely believed to have led to the extinction of dinosaurs, because the impact probably created a global firestorm and/or a widespread greenhouse effect that caused long-term environmental changes.

Aorounga Crater.  Credit: NASA
Aorounga Crater. Credit: NASA

4. Aorounga Crater: possible triple crater. The main Aorounga Crater in Chad, Africa, visible in this radar image from space, shows a concentric ring structure that is about 17 kilometers wide. But, this crater might have been formed as the result of a multiple impact event. A second crater, similar in size to the main crater, appears as a circular trough in the center of the image. And a third structure, also about the same size, is seen as a dark, partial circular trough on the right side of the image. The proposed crater “chain” could have formed when a 1 km to 2 km (0.5 mile to 1 mile) diameter object broke apart before impact. Ouch!
Clearwater craters. Credit: NASA
Clearwater craters. Credit: NASA

5. Clearwater Craters: two for the price of one. Twin, lake-filled impact craters in Quebec, Canada were probably formed simultaneously, about 290 million years ago, by two separate but probably related meteorite impacts. The larger crater, Clearwater Lake West has a diameter of 32 km, and Clearwater Lake East is 22 km wide.

Barringer Crater.
Barringer Crater.

6. Barringer Crater: well preserved. While this crater isn’t all that big, what’s most impressive about Barringer Crater in Arizona (USA) is how well preserved it is. Measuring 1.2 km across and 175 m deep, Barringer Crater was formed about 50,000 years ago by the impact of an iron meteorite, probably about 50 m across and weighing several hundred thousand tons. Most of the meteorite was vaporized or melted, leaving only numerous, mostly small fragments with in the crater and scattered up to 7 km from the impact site. Only about 30 tons, including a 693-kg sample, are known to have been recovered.
Wolfe Creek Crater
Wolfe Creek Crater

7. Wolfe Creek Crater, well preserved, too. Another relatively well-preserved meteorite crater is found in the desert plains of north-central Australia. Wolfe Creek crater is thought to be about 300,000 years old and is 880 meters across and and about 60 meters deep. It’s partially buried under the wind-blown sand of the region, and although the unusual landform was well-known to the locals, scientists didn’t find the crater until 1947.
Deep Bay Crater.  Credit: NASA
Deep Bay Crater. Credit: NASA

8. Deep Bay Crater: deep and cold. Deep Bay crater is located in Saskatchewan, Canada. The bay is a strikingly circular 13 km wide impact crater and is also very deep (220 m). It is part of an otherwise irregular and shallow lake. The age of the crater is estimated to be 99 million years old.

Kara-Kul Crater.  Credit: NASA
Kara-Kul Crater. Credit: NASA

9. Kara-Kul Crater: high altitude crater. This crater was formed about 10 million years ago, and is located in Tajikistan, near the Afghan border. In total, the crater is about 45 km in diameter and is partially filled with a 25 km-wide lake. This might be the “highest” impact crater, almost 6,000 m above sea-level in the Pamir Mountain Range. It was found only recently from satellite images.

Bosumtwi Crater.
Bosumtwi Crater.

10. Bosumtwi Crater: built of bedrock. The last crater on our tour of impressive impact craters is this located in Ghana, Africa. It is about 10.5 km in diameter and about 1.3 million years old. The crater is filled almost entirely by water, creating Lake Bosumtwi. The lakebed is made of crystalline bedrocks.

Source:
Wikipedia: Impact Craters

The Horologium Constellation

Horologium chart (IAU chart). Credit: IAU

If you’ve got a clear view of the skies, and happen ti live in the southern hemisphere, there’s a relatively obscure constellation you should probably check out. It’s known as Horologium, a region of the sky that is named after an important historic personality, one who is largely responsible for how we measure time.

The constellation of Horologium was one of 14 created by Nicolas Louis de Lacaille to chart southern hemisphere skies. Originally named “Horologium Oscillitorium” to honor Christiaan Huygens – the inventor of the pendulum clock – it was later shortened to its present named when adopted as one of the 88 modern constellations by the IAU.

Horologium spans 249 square degrees of sky and consists of 6 mains stars in the asterism, with 10 Bayer/Flamsteed designated stars. It is bordered by the constellations of Eridanus, Hydrus, Reticulum, Dorado and Caelum. Horologium is visible to all observers at latitudes between +30° and ?90° and is best seen at culmination during the month of December.

Constellation Horologium
The constellation Horologium, as seen by the naked eye in the southern hemisphere. Credit: AlltheSky.com

Horologium was named to honor Christiaan Huygens, the Dutch mathematician, astronomer and physicist. While traveling in the southern hemisphere and charting the heavens, Nicholas de Lacaille (who loved all things science) found this dim constellation reminded him of Huygen’s newly invented pendulum clock.

Huygens clock incorporated the first harmonic oscillator – increasing the accuracy to within 15 seconds per day. His “horological innovation” so impressed Lacaille that he found the pattern for this invention in the stars.

Horologium is bordered by five different constellations: Eridanus (the Po River), Caelum (the chisel), Reticulum (the reticle), Dorado (the dolphinfish/swordfish), and Hydrus (the male water snake).

Spring driven pendulum clock, designed by Huygens, built by instrument maker Salomon Coster (1657),[96] and copy of the Horologium Oscillatorium,[97] Museum Boerhaave, Leiden
Spring driven pendulum clock, designed by Christiaan Huygens (1657) and copy of the Horologium Oscillatorium,  Museum Boerhaave, Leiden. Credit: Flickr/Rob Koopman

The official constellation boundaries are defined by a twenty-two sided polygon. Covering a total of 249 square degrees, Horologium ranks 58th in area out of the 88 modern constellations.

With almost no bright stars to claim, stargazing at Horologium can be a bit tricky. But with binoculars, a telescope, and a chart, there are plenty of opportunities for some picturesque views. Let’s start by taking a look in binoculars with Alpha Horologii – the “a” symbol on our map.

Located about 193 light years from Earth, this very normal K1 orange giant star – quietly fusing its core helium into carbon and oxygen. Nearby is Delta, the “8” symbol. It, too is rather ordinary. Delta is a spectroscopic binary star, located about 175 light years away.

So, with very little in the constellation in the way of stars, what is there to do with a telescope? First of all, there’s NGC 1261 (RA: 03:12:15.3; Dec: -55:13:01). This 8th magnitude globular cluster is very well condensed and is at home in a very picturesque field. Small wonder it made the Caldwell list at number 87. Look for a very bright core region and well resolved chains of stars at the edges of this pretty star cluster.

Globular Cluster NGC 1261: SOFI infrared multimode instrument on the ESO 3.58-m New Technology Telescope at La Silla, Chile. Credit: ESO
Globular Cluster NGC 1261 as observed from the New Technology Telescope at La Silla, Chile. Credit: ESO

For larger telescopes, try NGC 1512 (RA 4:03.9 Dec -43:21). At slightly brighter than magnitude 11, this barred spiral galaxy belongs to the Dorado group and is located about 30 million light years away. While you won’t find much details here, NASA’s Galaxy Evolution Explorer show spiral galaxy NGC 1512 sitting slightly northwest of elliptical galaxy NGC 1510.

The two galaxies are currently separated by a mere 68,000 light-years, leading many astronomers to suspect that a close encounter is currently in progress. The overlapping of two tightly wound spiral arm segments makes up the light blue inner ring of NGC 1512. Meanwhile, the galaxy’s outer spiral arm is being distorted by strong gravitational interactions with NGC 1510.

Another challenge? Then try NGC 1433 (RA 3:42.0 Dec -47:13). This magnitude 10 galaxy is an example of a ringed barred spiral. While physically you may only notice a bright nucleus and the soft bar, the stars orbiting the disk of this galaxy shows its internal motions photographically. A small elliptical ring can develop near the nucleus – blue proof of star formation. Always keep a watch, because this galaxy had a supernova event in 1985.

Source: Wikipedia
Chart Courtesy of Your Sky.

Phoenix Lander At Mission’s End

Capturing the world's attention: Phoenix (NASA/UA)

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The Phoenix Mars Lander has not communicated since Nov. 2, and engineers from the mission assume the vehicle is now completely out of power. Therefore, at a news conference today, mission managers announced the Phoenix the mission is now officially over. “At this time we’re pretty convinced the vehicle is no longer available for us to use, and we’re declaring the end of the mission,” said Barry Goldstein, Phoenix project manager. “We’ve been surprised by this vehicle before, and we’re still listening. We’ll try to hail Phoenix, but no one has the expectation we’ll hear from it again. We’re completely proud of what we’ve accomplished. We’ve achieved all of the science goals and then some.”

But there’s still more to come from Phoenix, as scientists can now focus fully on analyzing the science data returned by the lander. Could Phoenix have found possible organic substances on Mars?

Peter Smith, Principal Investigator for Phoenix, didn’t rule out the possibility. “We haven’t analyzed the data at that level yet,” he said. “These are subtle signatures. We have the data sets that could reveal that. But until we actually do the work, we can’t say we didn’t find it…I’m still holding out hope here. Its’ really a question of what is the truth on Mars, and we’re trying to make sure we get the right answer here and not come rushing out with a quick analysis. This is very tricky stuff and the data sets are quite complex in regards to organics.”

Tests done by Phoenix didn’t reveal the acid soils Smith and his team were expecting to find, but alkaline salts and perchlorates, which are possible energy sources and nutrients for microbes. Smith doesn’t think there’s anything alive on Mars now, its just too cold. “It’s possible that in a warmer and wetter period on it Mars, it could have been habitable,” he said.

As anticipated, the seasonal decline in sunshine at the arctic landing site is not providing enough sunlight for the solar arrays to collect the power necessary to charge batteries that operate the lander’s instruments. And a dust storm at the landing site made the sunlight decrease even further, ending the mission a little sooner than the team had hoped.

As for any possibility of re-contacting the lander next year when spring returns to Mars’ northern arctic, Goldstein didn’t rule it out, but said its not very likely. “By the mid October (2009) time frame, there would be enough sunlight hitting the solar arrays to create power,” he said. “But its highly unlikely the vehicle will come back. It will be encased in CO2 ice, in temperatures under -150 C. The solar arrays will likely crack and fall off the vehicle,… the electronics will become brittle and break, so the wiring boards won’t work. But this vehicle has behaved so superlatively, we’ll look again in October.”

Look for an official epitaph for Phoenix from Universe Today soon.

Carnival of Space #78

This week the Carnival of Space moves to Simostronomy. We’ve got news about magnetic field interactions, the Large Hadron Collider, and riding balloons to the edge of space.

Click here to read the Carnival of Space #78

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

Finally, if you run a space-related blog, please post a link to the Carnival of Space. Help us get the word out.

DVD Review: The Universe – Season Two

The Universe - Season 2

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The 5 DVD package of the complete Season Two of The Universe by the History Channel provides over 14 hours of captivating science. Bright lights and driving sound push information to the viewer as if a mad scientist had been let loose in a vault containing an infinite supply of paint and sound effects. And with the universe being as big as things get, there’s no end of great subjects on the discs.

Though having a broad mandate, the producers stay focused upon the wonders of space. The included 18 episodes have exotic titles and serious subjects. For instance, wild weather looks at storms on far away planets with wind speeds of many hundreds of kilometres per hour. Or, the cosmic web, a structure of super-galaxies and black matter, is the largest thing envisionable. Each come up with great fanfare and usually a broad dash of fun, thus keeping the viewer interested for the duration.

However, not all is song and dance. Documentary interviews with current investigators get interspaced amongst the visuals. And, accurate models, footage of real hardware and imagery from ongoing science programs serve to reinforce the factual nature. These continually remind the viewer that the subjects are very real and that many people are dedicating their lives to adding to our knowledge.

Most of us won’t be able to wander the surface of Europa or bounce in and out of black holes. Therefore, productions like these episodes are perhaps the best way of experiencing the wonders that surround us. Vibrant and lively, they lift us off the couch and into another realm that’s part fact and part imagination. As a teaching aid or self-learning tool, the 5 DVDs of The Universe – Season Two will resonate with a flurry of science amid a furor of colour and sound.

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

Podcast: Ice in Space, Expansion of the Universe, and Death from the Skies

Saturn's moon Iapetus. Image credit: NASA/JPL/SSI

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Another week, another batch of questions. If ice disappears in your freezer, how can it last in space? How can the Universe be expanding faster than the speed of light? And what is the risk from a coronal mass ejection in an airplane? All this and even more questions. If you’ve got a question for the Astronomy Cast team, please email it in to [email protected] and we’ll try to tackle it for a future show. Please include your location and a way to pronounce your name.

Click here to download the episode.

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

Ice in Space, Expansion of the Universe, and Death from the Skies – Transcript and show notes.

Podcast: The Moon, Part 1

Chandrayaan-1's first picture of the moon. Credit: ISRO

Hey, here’s a topic we haven’t really gotten around to yet… the Moon. Today we look at our closest astronomical companion: the Moon. What impact does the Moon have on our lives, where did it come from, who walked on it, and are we ever going to walk on it again? We’re going to learn about the phases, the tides, and even a little bit about NASA’s plans to send humans back to the Moon.

Click here to download the episode.

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

The Moon, Part 1 – Transcript and show notes.

Hercules

Hercules

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The constellation of Hercules belongs to one of the 48 originals plotted by Ptolemy and has survived time to become one of the 88 modern constellations adopted by the International Astronomical Union. Spanning an impressing 1225 square degrees of sky and containing 22 stars in the asterism, it has 106 Bayer/Flamsteed designated stellar designations. Hercules is bordered by the constellations of Draco, Bootes, Corona Borealis, Serpens Caput, Ophiuchus, Aquila, Sagitta, Vulpecula and Lyra. It is visible to all observers at latitudes between +90° and ?50° and is best seen at culmination during the month of July. There is one annual meteor shower associated with Hercules, the Tau Herculids, which peak on or near June 3. The radiant, or point of origin, is near the Hercules/Corona Borealis border and the meteor shower itself last about a month beginning around two weeks before and lasting about two weeks after the peak date. Most of these meteors are quite faint and at maximum, expect to see no more than 15 per hour average.

The mythology surrounding Hercules is a long and very colorful one. He was considered the greatest of all heroes – both Greek and Roman. The legendary strong man was supposed to be the son of Zeus; immortal, yet forever challenged by Hera by his circumstance of birth. His tasks were many: killing a lion with a hide that could not be punctured, destroying the many headed Hydra, cleaning out nasty stables, fighting birds with knife-like feathers, capturing a bull that breathed fire, taming horses that ate flesh, stealing cattle from monsters, stealing golden apples, fighting dragons, snatching a three-headed dog, loosing the love of his life, accidentally killing his teacher and so much more… It is no wonder that Hercules is so often depicted as kneeling in the sky! Even an immortal would be tired from so much… But at last, Hercules earned his place in the stars and he remains there to this day… The fifth largest constellation in the night sky.

Because the constellation of Hercules has no particularly bright stars, it is sometimes difficult to navigate through with binoculars until you learn a few “key” ingredients. There is a large asterism which is fairly easy to recognize that forms a lopsided box, referred to as the “keystone”. The northeast corner is Pi. The northwest corner is Eta. The southeast corner is Epsilon. The southwest corner is Zeta. Always remember when you look at a star chart that north and south are up and down… But east is to the left and west is to the right! To find the “keystone”, let bright Vega guide you…. just start by looking southwest.

Have you found Pi Herculis, yet? If you’re seeing two stars in your binoculars and you’re not sure which one, Pi is the slightly redder and slightly brighter of the pair. Situated about 370 light years from Earth, Pi Herculis is a cool, red supergiant star that was born about 140 million years ago. Although you can’t see it, Pi also has an orbiting substellar companion about 27 times larger than Jupiter there, too! Now, drop south for Epsilon – another binary star. Chances are good this pair of twin stars are almost identical to each other – about twice the size and mass of our Sun – and orbit each other so closely they nearly touch.

Don’t stop moving south. Our next stop is Gamma Herculis, the “8” shape on our map. Gamma is also a very cool star – one with a dead helium core that’s waiting to become a red giant. In maybe 8 million or so years, it will begin to fuse helium into carbon and become much brighter than it is tonight. If you see a faint companion star, it is only an optical one in binoculars – but Gamma is also a genuine binary star.

Next stop? Further south for Alpha – the “a” shape on our map. Now here is a great star! Named Rasalgethi and located about 380 light years away, here we have one of the finest double stars in the night sky. The primary star is a magnificent red class M supergiant that’s over 475 more luminous than our Sun and whose size would fill up our solar system clear out to the orbit of the asteroid belt. But that’s not all… Aim a telescope at Rasalgethi and you’ll see it has a fifth magnitude companion five seconds of arc away. It is also a binary star – an F2 giant with a close orbiting dwarf star companion. Surrounding this whole system is an envelope of gas expelled from the primary star’s incredible solar winds… Enjoy the unusual red and green hues of this colorful double star! And keep watching… Because Rasalgethi is also an irregular variable star – whose brightness changes from magnitude 2.7 to 4.0 within a period of about three months.

Next up? Return to the “keystone” and the northwest corner for Eta – the “n” shape on our map. Shining away about 50 times brighter than our own Sun at a distance of 112 light years, there is nothing particularly impressive about Eta, except where it leads. Begin moving your optics slowly south towards Zeta and you will encounter the “Great Hercules Cluster” – M13! Easily seen in binoculars, sometimes visible to the unaided eye in a dark sky location and absolutely magnificent in any telescope, Messier 13 is perhaps the most famous of all northern globular clusters. Located about 25,000 light years away and home to more than half a million stars, this 12 billion year old system spans no more than 100 light years across. Also known as NGC 6205, this impressive ball of stars was first discovered by Edmund Halley in 1714 and catalogued by Charles Messier on June 1, 1764. If you aren’t impressed, then take the words of Kurt Vonnegut to heart: “”Every passing hour brings the Solar System forty-three thousand miles closer to Globular Cluster M13 in Hercules — and still there are some misfits who insist that there is no such thing as progress.”

Ready for more? Then take another look at Eta and Pi and form an imaginary triangle on the sky using these two stars as the base. The apex is very near where you will find another amazing globular cluster for binoculars or small telescopes – Messier 92. First discovered by Johann Elert Bode in 1777 and independently rediscovered by Charles Messier on March 18, 1781, M92 is a 16 billion year old beauty – formed back at the Milky Way Galaxy’s beginnings. Hiding in there are 16 variable stars and one rare eclipsing binary. What a treat to have two such bright objects so near to one another!

Ready for an alternative binocular tour of Hercules? Then let’s use what you’ve learned. Start by locating magnificent M13 and move 3 degrees northwest – about a binocular field. What you will find is a splendid loose open cluster of stars known as Dolidze/Dzimselejsvili (DoDz) 5 – and it looks much like a miniature of the constellation Hercules. Just slightly more than 4 degrees to its east and just about a degree south of Eta Herculis is DoDz 6, which contains a perfect diamond pattern and an asterism of brighter stars resembling the constellation of Sagitta. Now we’re going to move across the constellation of Hercules towards Lyra. East of the “keystone” is a tight configuration of three stars – Omicron, Nu, and Xi. About the same distance separating these stars northeast you will find DoDz 9. You’ll see a pretty open cluster of around two dozen mixed magnitude stars. Now look again at the “keystone” and identify Lambda and Delta to the south. About midway between them and slightly southeast you will discover the stellar field of DoDz 8. This last is easy – all you need to do is return to Alpha. Move about 1 degree northwest (Rasalgethi will stay in the field) to discover the star-studded open cluster DoDz 7. These great open clusters are very much off the beaten path and will add a new dimension to binocular and fast-telescope observing!

Would you like a challenge? Then go back to M13 with a large telescope and take a look about 40 arc minutes to the northeast for NGC 6207 (RA 16:43.1 Dec +36:50). At near magnitude 12, this small spiral galaxy isn’t for everyone, but it’s always a smile a bonus when you’re in the area, despite the lack of details. Try NGC 6210 (RA 16:44.5 Dec +23:49), too. This bright planetary nebula is suited for all telescopes and takes magnification very well. Look for a blue/green color in larger telescopes, and adding a nebula filter can sometimes reveal some subtle details of a shell around this one. But be sure to take the filter out if you want to catch the central star!

Sources: Chandra Observatory, SEDS
Chart Courtesy of My Sky.

Forgotten Apollo Data Could Solve Moon Dust Problem

An IMB 726, a precursor of the 729 data recorder. Credit: IBM

Old, forgotten data from three Apollo moon missions could help overcome one of the biggest environmental hurdles facing future lunar colonists. Pervasive moon dust can clog equipment, scratch helmet visors –or worse, get inside astronaut lungs and cause serious health problems. But 173 data tapes hold information that could be essential in overcoming the problems the dust causes. The only trouble is that the tapes are archived on “ancient” 1960’s technology and no one could find the right equipment to playback the tapes. However, the Australian Computer Museum has an old IBM729 Mark 5 tape drive that should do the trick, IF the machine can be restored to operable condition again…

The IBM729 Mark 5 tape recorder is about as big as a household refrigerator. It recorded data from Apollo 11, 12 and 14 missions that carried “dust detectors.” Information from the detectors was beamed back to earth and recorded onto tapes. Copies of the tapes were supposedly sent to NASA, but the tapes were lost or misplaced before they could be archived in NASA’s holdings. But the original data tapes have sat in Perth, Australia for almost 40 years.

Physicist Brian O’Brien invented the detectors. He wrote a couple of papers on the information in the 1970’s, but no one was very interested in moon dust back then. However now, scientists realize this information could help make future missions to the moon more feasible.

Apollo astronaut Gene Cernan covered with moon dust.  Credit: NASA
Apollo astronaut Gene Cernan covered with moon dust. Credit: NASA

“These were the only active measurements of moon dust made during the Apollo missions, and no one thought it was important,” said O’Brien. “But it’s now realised that dust, to quote Harrison Schmitt, who was the last astronaut to leave the moon, is the number one environmental problem on the moon.”

O’Brien quit his work on lunar dust when he left the University of Sydney. Two years ago, someone at NASA remembered the data had been taken, but couldn’t find the duplicate tapes.

O’Brien says there is no indication as to when exactly the tapes were lost, but he guesses that it was “way, way back.” When O’Brien learned of the tape loss, he was contacted by Guy Holmes from a data recovery company who offered to try and extract the information on the old, original tapes. But Holmes realized he needed some old equipment to do the job, and came across the right IBM tape drive at the Australian Computer Museum.

The archaic-looking recorder is in need of refurbishing, however. Holmes jokes that a 1970s Toyota Corolla fan belt could be used to get the recorder up and running.

“The drives are extremely rare, we don’t know of any others that are still operating,” he said.

“It’s going to have to be a custom job to get it working again. It’s certainly not simple, there’s a lot of circuitry in there, it’s old, it’s not as clean as it should be and there’s a lot of work to do.”

Holmes is hopeful of getting the tape recorder working again in January, and then he says it should only take a week to extract information that has been locked away since the early 1970s.

Source: Australia’s ABC News