Aliens
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Astronomy Picture of the Day
2007 April 14
Venus by the Lake
Credit & Copyright: Tunc Tezel
Explanation: Finding Venus in the night sky is not too hard these days. Now appearing as the evening star, Venus rules as the brightest celestial beacon in west just after sunset. And if you can find Venus tonight, you can also easily find the lovely Pleiades star cluster (aka M45) close by. In this serene skyview, recorded on Tuesday near Bolu, Turkey, Venus and the Pleiades are on the right, with brilliant Venus reflected in the calm waters of the small lake in the foreground. Left of Venus, the bright star Aldebaran anchors the V-shaped Hyades star cluster. Farther left are stars of the familiar constellation Orion with Rigel, at the foot of Orion, also reflected in the lake. Meanwhile, Sirius, in Canis Major, is the brightest star on the left side of the view. But the bright terrestrial light below Sirius is not a reflection, it's just a light near the lake shore.
2007 April 14
Venus by the Lake
Credit & Copyright: Tunc Tezel
Explanation: Finding Venus in the night sky is not too hard these days. Now appearing as the evening star, Venus rules as the brightest celestial beacon in west just after sunset. And if you can find Venus tonight, you can also easily find the lovely Pleiades star cluster (aka M45) close by. In this serene skyview, recorded on Tuesday near Bolu, Turkey, Venus and the Pleiades are on the right, with brilliant Venus reflected in the calm waters of the small lake in the foreground. Left of Venus, the bright star Aldebaran anchors the V-shaped Hyades star cluster. Farther left are stars of the familiar constellation Orion with Rigel, at the foot of Orion, also reflected in the lake. Meanwhile, Sirius, in Canis Major, is the brightest star on the left side of the view. But the bright terrestrial light below Sirius is not a reflection, it's just a light near the lake shore.
We're in the pipe , five by five.
- Tach Deneva
- Posts: 1546
- Joined: 18 Dec 2002, 18:51
- Location: KY
Astronomy Picture of the Day
Explanation: Why are parts of this asteroid's surface so smooth? No one is yet sure, but it may have to do with the dynamics of an asteroid that is a loose pile of rubble rather than a solid rock. The unusual asteroid has been visited recently by the Japanese spacecraft Hayabusa that has been documenting its unusual structure and mysterious lack of craters. Recent analyses of the border regions between smooth and rugged sections of Itokawa indicate that jostling of the asteroid might be creating segregation between large and small rocks near the surface, like the Brazil nut effect. In late 2005, Hayabusa actually touched down on one of the smooth patches, dubbed the MUSES Sea, and collected soil samples that are to be returned to Earth for analysis. Hayabusa will start its three-year long return trip to Earth this month. Computer simulations show that 500-meter asteroid Itokawa may impact the Earth within the next few million years.
-END-
What’s interesting about this is that Japan’s Hayabusa actually touched down on one of the smooth patches dubbed the MUSES Sea, and collected soil samples , Lifted off again and is returning to Earth for analysis. Nice… What I mean is that , it’s just part of the beginning of what is to come. Robots in space collecting asteroid soil samples for us? What’s next? Maybe someday will have robots like Huey , Duey and Luey working outside the International Space Station , like in the movie Silent Running.
Explanation: Why are parts of this asteroid's surface so smooth? No one is yet sure, but it may have to do with the dynamics of an asteroid that is a loose pile of rubble rather than a solid rock. The unusual asteroid has been visited recently by the Japanese spacecraft Hayabusa that has been documenting its unusual structure and mysterious lack of craters. Recent analyses of the border regions between smooth and rugged sections of Itokawa indicate that jostling of the asteroid might be creating segregation between large and small rocks near the surface, like the Brazil nut effect. In late 2005, Hayabusa actually touched down on one of the smooth patches, dubbed the MUSES Sea, and collected soil samples that are to be returned to Earth for analysis. Hayabusa will start its three-year long return trip to Earth this month. Computer simulations show that 500-meter asteroid Itokawa may impact the Earth within the next few million years.
-END-
What’s interesting about this is that Japan’s Hayabusa actually touched down on one of the smooth patches dubbed the MUSES Sea, and collected soil samples , Lifted off again and is returning to Earth for analysis. Nice… What I mean is that , it’s just part of the beginning of what is to come. Robots in space collecting asteroid soil samples for us? What’s next? Maybe someday will have robots like Huey , Duey and Luey working outside the International Space Station , like in the movie Silent Running.
We're in the pipe , five by five.
[glow=yellow]Now here’s an interesting read[/glow]
Out-of-This-World Hypothesis:
Cosmic Forces Control Life on Earth
By Ker Than
Staff Writer
posted: 23 April 2007
07:54 am ET
The rise and fall of species on Earth might be driven in part by the undulating motions of our solar system as it travels through the disk of the Milky Way, scientists say.
Two years ago, scientists at the University of California, Berkeley found the marine fossil record shows that biodiversity—the number of different species alive on the planet—increases and decreases on a 62-million-year cycle. At least two of the Earth’s great mass extinctions—the Permian extinction 250 million years ago and the Ordovician extinction about 450 million years ago—correspond with peaks of this cycle, which can’t be explained by evolutionary theory.
Now, a team of researchers at the University of Kansas (KU) have come up with an out-of-this-world explanation. Their idea hinges upon the fact that, appearances aside, stars are not fixed in space. They move around, sometimes rushing headlong through galaxies, or approaching close enough to one another for brief cosmic trysts.
In particular, our Sun moves toward and away from the Milky Way’s center, and also up and down through the galactic plane. One complete up-and-down cycle takes 64 million years— suspiciously similar to Earth’s biodiversity cycle.
Galactic bow shock
The KU researchers independently confirmed the biodiversity cycle and have proposed a novel mechanism by which the Sun’s galactic travels is causing it.
Scientists know the Milky Way is being gravitationally pulled toward a massive cluster of galaxies, called the Virgo Cluster, located about 50 million light years away. Adrian Melott and his colleague Mikhail Medvedev, both KU researchers, speculate that as the Milky Way hurdles towards the Virgo Cluster, it generates a so-called bow shock in front of it that is similar to the shock wave created by a supersonic jet.
“Our solar system has a shock wave around it, and it produces a good quantity of the cosmic rays that hit the Earth. Why shouldn’t the galaxy have a shock wave, too?” Melott said.
The galactic bow shock is only present on the north side of the Milky Way’s galactic plane, because that is the side facing the Virgo Cluster as it moves through space, and it would cause superheated gas and cosmic rays to stream behind it, the researchers say. Normally, our galaxy’s magnetic field shields our solar system from this “galactic wind.” But every 64 million years, the solar system’s cyclical travels take it above the galactic plane.
“When we emerge out of the disk, we have less protection, so we become exposed to many more cosmic rays,” Melott told SPACE.com.
How cosmic rays affect life
The boost in cosmic–ray exposure could have both a direct and indirect effect on Earth’s organisms, said KU paleontologist Bruce Lieberman. The radiation could lead to higher rates of genetic mutations in organisms or interfere with their ability to repair DNA damage, potentially leading to diseases like cancer.
Cosmic rays are also associated with increased cloud cover, which could cool the planet by blocking out more of the Sun’s rays. They also interact with molecules in the atmosphere to create nitrogen oxide, a gas that eats away at our planet’s ozone layer, which protects us from the Sun’s harmful ultraviolet rays.
Richard Muller, one of the UC Berkeley physicists who co-discovered the cycle, said Melott and his colleagues have come up with a plausible galactic explanation for the biodiversity cycle. Muller and Robert Rohde also speculated that our solar system’s movement through the galactic plane was behind the cycle, but the pair could not conceive of any reason why conditions on the north and south side of the galactic plane should differ.
“That’s where they succeeded,” Muller said in a telephone interview. “They came up with something we didn’t think of, which puts an asymmetry in. I’m delighted they did that and I congratulate them.”
A first-step hypothesis
Richard Bambach, a paleontologist at the Smithsonian Museum of Natural History who was not involved in the study, said he is excited the biodiversity cycle has been independently confirmed, but cautions the galactic hypothesis is still in the early stages of formulation.
“It’s a first-step hypothesis,” Bambach said. “It’s an interesting idea, but we’re a long way from knowing if that is really why biodiversity changes.”
For one thing, scientists have yet to discover a bow shock around the Milky Way, though such shock waves have been found around other galaxies.
“I think it’s a very nice idea,” said Philip Appleton, a Caltech astronomer. “I think we’re only beginning to come to grips with these kinds of behaviors. We’re realizing that not only do galaxies interact with each other gravitationally, but also that the environment they’re traveling through—the ‘wind’ they create—can actually produce noticeable effects.”
Last year, Appleton and his team discovered a bow shock surrounding a galaxy in Stephan’s Quintet, a galactic cluster located 300 million light years away. The shock wave is traveling about 620 miles (1,000 km) per second relative to the cluster.
The Milky Way is hurtling toward the Virgo Cluster at about 125 miles (200 km) per second, so any bow shock it generates would consequently be weaker, Appleton said.
If future studies confirm the galaxy-biodiversity link, it would force scientists to broaden their ideas about what can influence life on Earth. “Maybe it’s not just the climate and the tectonic events on Earth,” Lieberman said. “Maybe we have to start thinking more about the extraterrestrial environment as well.”
Out-of-This-World Hypothesis:
Cosmic Forces Control Life on Earth
By Ker Than
Staff Writer
posted: 23 April 2007
07:54 am ET
The rise and fall of species on Earth might be driven in part by the undulating motions of our solar system as it travels through the disk of the Milky Way, scientists say.
Two years ago, scientists at the University of California, Berkeley found the marine fossil record shows that biodiversity—the number of different species alive on the planet—increases and decreases on a 62-million-year cycle. At least two of the Earth’s great mass extinctions—the Permian extinction 250 million years ago and the Ordovician extinction about 450 million years ago—correspond with peaks of this cycle, which can’t be explained by evolutionary theory.
Now, a team of researchers at the University of Kansas (KU) have come up with an out-of-this-world explanation. Their idea hinges upon the fact that, appearances aside, stars are not fixed in space. They move around, sometimes rushing headlong through galaxies, or approaching close enough to one another for brief cosmic trysts.
In particular, our Sun moves toward and away from the Milky Way’s center, and also up and down through the galactic plane. One complete up-and-down cycle takes 64 million years— suspiciously similar to Earth’s biodiversity cycle.
Galactic bow shock
The KU researchers independently confirmed the biodiversity cycle and have proposed a novel mechanism by which the Sun’s galactic travels is causing it.
Scientists know the Milky Way is being gravitationally pulled toward a massive cluster of galaxies, called the Virgo Cluster, located about 50 million light years away. Adrian Melott and his colleague Mikhail Medvedev, both KU researchers, speculate that as the Milky Way hurdles towards the Virgo Cluster, it generates a so-called bow shock in front of it that is similar to the shock wave created by a supersonic jet.
“Our solar system has a shock wave around it, and it produces a good quantity of the cosmic rays that hit the Earth. Why shouldn’t the galaxy have a shock wave, too?” Melott said.
The galactic bow shock is only present on the north side of the Milky Way’s galactic plane, because that is the side facing the Virgo Cluster as it moves through space, and it would cause superheated gas and cosmic rays to stream behind it, the researchers say. Normally, our galaxy’s magnetic field shields our solar system from this “galactic wind.” But every 64 million years, the solar system’s cyclical travels take it above the galactic plane.
“When we emerge out of the disk, we have less protection, so we become exposed to many more cosmic rays,” Melott told SPACE.com.
How cosmic rays affect life
The boost in cosmic–ray exposure could have both a direct and indirect effect on Earth’s organisms, said KU paleontologist Bruce Lieberman. The radiation could lead to higher rates of genetic mutations in organisms or interfere with their ability to repair DNA damage, potentially leading to diseases like cancer.
Cosmic rays are also associated with increased cloud cover, which could cool the planet by blocking out more of the Sun’s rays. They also interact with molecules in the atmosphere to create nitrogen oxide, a gas that eats away at our planet’s ozone layer, which protects us from the Sun’s harmful ultraviolet rays.
Richard Muller, one of the UC Berkeley physicists who co-discovered the cycle, said Melott and his colleagues have come up with a plausible galactic explanation for the biodiversity cycle. Muller and Robert Rohde also speculated that our solar system’s movement through the galactic plane was behind the cycle, but the pair could not conceive of any reason why conditions on the north and south side of the galactic plane should differ.
“That’s where they succeeded,” Muller said in a telephone interview. “They came up with something we didn’t think of, which puts an asymmetry in. I’m delighted they did that and I congratulate them.”
A first-step hypothesis
Richard Bambach, a paleontologist at the Smithsonian Museum of Natural History who was not involved in the study, said he is excited the biodiversity cycle has been independently confirmed, but cautions the galactic hypothesis is still in the early stages of formulation.
“It’s a first-step hypothesis,” Bambach said. “It’s an interesting idea, but we’re a long way from knowing if that is really why biodiversity changes.”
For one thing, scientists have yet to discover a bow shock around the Milky Way, though such shock waves have been found around other galaxies.
“I think it’s a very nice idea,” said Philip Appleton, a Caltech astronomer. “I think we’re only beginning to come to grips with these kinds of behaviors. We’re realizing that not only do galaxies interact with each other gravitationally, but also that the environment they’re traveling through—the ‘wind’ they create—can actually produce noticeable effects.”
Last year, Appleton and his team discovered a bow shock surrounding a galaxy in Stephan’s Quintet, a galactic cluster located 300 million light years away. The shock wave is traveling about 620 miles (1,000 km) per second relative to the cluster.
The Milky Way is hurtling toward the Virgo Cluster at about 125 miles (200 km) per second, so any bow shock it generates would consequently be weaker, Appleton said.
If future studies confirm the galaxy-biodiversity link, it would force scientists to broaden their ideas about what can influence life on Earth. “Maybe it’s not just the climate and the tectonic events on Earth,” Lieberman said. “Maybe we have to start thinking more about the extraterrestrial environment as well.”
We're in the pipe , five by five.
Astronomy Picture of the Day
I saw this the other day and I got to tell ya, it looked pretty cool.
Explanation: The two brightest objects in the night sky appeared to go right past each other last week. On the night of May 19, Earth's Moon and the planet Venus were visible in the same part of the sky, and at closest approach were less than one degree apart. The conjunction was captured in the above image taken from near Quebec City, Quebec, Canada. Venus appears on the lower left of the above photo. The spires that appear to emanate from Venus are diffraction spikes caused by the camera itself. The image is so clear that craters on the Moon are resolved. Of course, the real physical distance between the two heavenly bodies was not unusually small -- the apparent conjunction was really just an illusion of perspective. Although Earth's Moon passes Venus once each month, such a close passing visible in the evening sky is more rare.
I saw this the other day and I got to tell ya, it looked pretty cool.
Explanation: The two brightest objects in the night sky appeared to go right past each other last week. On the night of May 19, Earth's Moon and the planet Venus were visible in the same part of the sky, and at closest approach were less than one degree apart. The conjunction was captured in the above image taken from near Quebec City, Quebec, Canada. Venus appears on the lower left of the above photo. The spires that appear to emanate from Venus are diffraction spikes caused by the camera itself. The image is so clear that craters on the Moon are resolved. Of course, the real physical distance between the two heavenly bodies was not unusually small -- the apparent conjunction was really just an illusion of perspective. Although Earth's Moon passes Venus once each month, such a close passing visible in the evening sky is more rare.
We're in the pipe , five by five.
Astronomy Picture of the Day
Stars and the Solstice Sun
Composite Credit & Copyright: Jerry Lodriguss (Catching the Light)
Explanation:
If you could turn off the atmosphere's ability to scatter overwhelming sunlight, today's daytime sky might look something like this ... with the Sun surrounded by the stars of the constellations Taurus and Gemini. Of course, today is the Solstice. Traveling along the ecliptic plane, the Sun is at its northernmost position in planet Earth's sky, marking the astronomical beginning of summer in the north. Accurate for the exact time of today's Solstice, this composite image also shows the Sun at the proper scale (about the angular size of the Full Moon). Open star cluster M35 is to the Sun's left, and the other two bright stars in view are Mu and Eta Geminorum. Digitally superimposed on a night time image of the stars.
Happy Summer Ya'll =]
June 21, 2007
Falker
Stars and the Solstice Sun
Composite Credit & Copyright: Jerry Lodriguss (Catching the Light)
Explanation:
If you could turn off the atmosphere's ability to scatter overwhelming sunlight, today's daytime sky might look something like this ... with the Sun surrounded by the stars of the constellations Taurus and Gemini. Of course, today is the Solstice. Traveling along the ecliptic plane, the Sun is at its northernmost position in planet Earth's sky, marking the astronomical beginning of summer in the north. Accurate for the exact time of today's Solstice, this composite image also shows the Sun at the proper scale (about the angular size of the Full Moon). Open star cluster M35 is to the Sun's left, and the other two bright stars in view are Mu and Eta Geminorum. Digitally superimposed on a night time image of the stars.
Happy Summer Ya'll =]
June 21, 2007
Falker
We're in the pipe , five by five.
Space Station to Get Japanese Take-Out
Hai, Japanese space food will soon be available on the International Space Station (ISS). The Japan Aerospace Exploration Agency (JAXA) has certified 29 Japanese food products for use in space. Astronauts and cosmonauts will soon enjoy such Japanese take-out standards as ramen, curry, onigiri (rice balls) and green tea (see photo). What took them so long?
The ISS has tough standards for food in space; it must be able to survive the changes in temperature and pressure on the ride up, and must be able to survive a year in storage at zero-g. Careful food service engineering is also required; for example, the ramen has a thick broth and the noodles are clumped together in bite-sized pieces. Food products are also packed in special containers, and can have preparation times no longer than an hour.
In 2008, Japanese astronaut Koichi Wakata will be joining the ISS staff; he will appreciate these JAXA-approved delicacies (made more tasty in zero-G by extra spices):
--Egg soup
--Rice with red azuki beans and wild greens
--Salmon onigiri (rice balls)
--Mackerel in miso sauce
--Kabayaki saury (broiled with sweet soy sauce)
And for dessert, a little bit of Kuroame (brown sugar candy); hopefully, the International Space Station also has stringent standards regarding brushing after meals.
Science fiction writers have been dreaming of elaborate space cuisine for generations. John W. Campbell anticipated the Star Trek food replicators in his 1934 story Twilight: The food was three hundred thousand years old, I suppose. I didn't know, and the machines that served it to me didn't care, for they made things synthetically, you see, and perfectly.
(Read more about Campbell's synthetic food dispenser).
Hai, Japanese space food will soon be available on the International Space Station (ISS). The Japan Aerospace Exploration Agency (JAXA) has certified 29 Japanese food products for use in space. Astronauts and cosmonauts will soon enjoy such Japanese take-out standards as ramen, curry, onigiri (rice balls) and green tea (see photo). What took them so long?
The ISS has tough standards for food in space; it must be able to survive the changes in temperature and pressure on the ride up, and must be able to survive a year in storage at zero-g. Careful food service engineering is also required; for example, the ramen has a thick broth and the noodles are clumped together in bite-sized pieces. Food products are also packed in special containers, and can have preparation times no longer than an hour.
In 2008, Japanese astronaut Koichi Wakata will be joining the ISS staff; he will appreciate these JAXA-approved delicacies (made more tasty in zero-G by extra spices):
--Egg soup
--Rice with red azuki beans and wild greens
--Salmon onigiri (rice balls)
--Mackerel in miso sauce
--Kabayaki saury (broiled with sweet soy sauce)
And for dessert, a little bit of Kuroame (brown sugar candy); hopefully, the International Space Station also has stringent standards regarding brushing after meals.
Science fiction writers have been dreaming of elaborate space cuisine for generations. John W. Campbell anticipated the Star Trek food replicators in his 1934 story Twilight: The food was three hundred thousand years old, I suppose. I didn't know, and the machines that served it to me didn't care, for they made things synthetically, you see, and perfectly.
(Read more about Campbell's synthetic food dispenser).
We're in the pipe , five by five.
Late September
Earth and Mars are converging, setting up a great skywatching opportunity for later this year. By the time you finish reading this sentence, you'll be about 25 miles closer to Mars, according to NASA calculations.
Here's what's going on: Earth has the inside track as the two worlds orbit the sun. Inner planets orbit more quickly than outer planets because of the laws of gravity. Earth requires 365 days to go around the sun once, where as a year on Mars is 687 Earth-day , and therefore every 26 months, Earth passes Mars on this orbital trek.
So by late September, Mars will be one of the brighter objects in the night sky. The closest approach will occur in December, when Mars will be brighter than every star in the sky. So break out the binoculars and telescopes folks. You might see some snow cap from another planet this year , (with your own eyes.) Exciting isn’t it?!
Next..
Geminids
December 13-14
What’s that? Well it’s a meteor shower… in December. In Fact , the most reliable meteor shower of the year, the Geminids are characterized by their multi-colored display--65% being white, 26% yellow, and the remaining 9% blue, red and green. So if you missed the last one like I did, go to higher ground this time. Even getting out of the city would be a big improvement for seeing a better night sky. Good Luck.
I suggest using WinStars Version 1 to find Mars. It’s easy to use .. I used this program several times and have found it relatively simple and painless to comprehend. I have not tried version 2 yet , I just took a quick look at it. . Today I'm actually using a different program to map the night sky called Planetarium, tho I need to update to Deepsky , or Starry Night someday.
WinStars Free:
http://www.winstars.net/version1/english/index2.html
Hears another list of free astronomy programs:
http://www.midnightkite.com/software.html
Buy new.. buying off of E-Bay may result in damaged or flawed mirrors , or even worn parts that are loose and wont calibrate well. For armatures , I suggest starting off with at least a 5 inch telescope. 130mm-diameter with 1.25” rack-and-pinion focuser. Make sure it has a good focal lenght ( depth = see deeper into space. ) like around 1000 to 1400 focal length or greater. Forget the finder scope with laser sight, it’s a waste of time. Buy optical finder scope one with Cross hairs. Way Better. Get them while there HOT! This year there’s going to be another back order and then a price hike soon after. It was like the that last time Mars came this close to Earth
We're in the pipe , five by five.
- Tach Deneva
- Posts: 1546
- Joined: 18 Dec 2002, 18:51
- Location: KY
Win Stars 2.0
Well I finally had the time to check out Win Stars 2.0 astronomy program the other day. This program is stellar. In planetarium mode the options are easy enough to figure out , and you can zoom in on the sky with a new powerful 3D feature that rocks. Very nice…You can zoom in on Nebulas , Galaxies or pretty much anything out there within the Win Stars data base. ( I use my mouse wheel ) Then go far-away... out into orbit and take in a view of the Earth and it’s surrounding solar system.
Pros:
Global Positions: Yes.. The global time in your time zone is allot more accurate with this program. Say if you where living in Ohio , you could point it out on the Win Stars map , and the program calculates what the night sky will look like in your area. It also synchronies your Telescope ( via PC ) and uploads your star map findings to the telescopes computer data base. After that all you’ll need to do is punch in the Win Stars object number. Your telescope will move right to the objects location in the night sky. Sounds good huh.
Cons:
There’s not allot of information on the objects in the sky. You’ll need to know what your looking for before you look for it on Win Stars 2.0 Also…It will show you where it is.. then just give a brief description of it.
Cons:
I have a motor for my telescope but , not a computerized location finder.
Overview:
Still not a bad program that’s become more accurate …. For Free!
Well I finally had the time to check out Win Stars 2.0 astronomy program the other day. This program is stellar. In planetarium mode the options are easy enough to figure out , and you can zoom in on the sky with a new powerful 3D feature that rocks. Very nice…You can zoom in on Nebulas , Galaxies or pretty much anything out there within the Win Stars data base. ( I use my mouse wheel ) Then go far-away... out into orbit and take in a view of the Earth and it’s surrounding solar system.
Pros:
Global Positions: Yes.. The global time in your time zone is allot more accurate with this program. Say if you where living in Ohio , you could point it out on the Win Stars map , and the program calculates what the night sky will look like in your area. It also synchronies your Telescope ( via PC ) and uploads your star map findings to the telescopes computer data base. After that all you’ll need to do is punch in the Win Stars object number. Your telescope will move right to the objects location in the night sky. Sounds good huh.
Cons:
There’s not allot of information on the objects in the sky. You’ll need to know what your looking for before you look for it on Win Stars 2.0 Also…It will show you where it is.. then just give a brief description of it.
Cons:
I have a motor for my telescope but , not a computerized location finder.
Overview:
Still not a bad program that’s become more accurate …. For Free!
We're in the pipe , five by five.
Mars Magic: Red Planet Shines Bright
posted: 18 December 2007
Mars is closer to Earth now than any time until the year 2016, offering skywatchers a great look.
The Hubble Space Telescope took advantage of the opportunity, too, photographing the red planet earlier this month. The images were pasted together into a video showing Mars' full rotation.
The red planet is now the brightest "star" in the evening sky, easily visible by mid-evening until dawn. It comes closest to the Earth today at 6:46 p.m. EST, when it will be 54,783,381 miles (88,165,305 kilometers) from us.
Mars looks like an orange star to the naked eye, but it's revealed as a disk with many features in modest telescopes. It will put on a good show all month.
Although 2003 offered astronomers a view of Mars 20 million miles (32 million kilometers) closer than this year's approach, Hubble's most recent detailed look at the red planet shows it's free of dust storms. However, ice crystal clouds in the northern and southern polar caps can be seen.
Two dark patches lie just south of the equator in Hubble's view: The large triangular shape to the right is Syrtis Major while the horizontal lane to the left is Sinus Meridiani. NASA's Mars Exploration Rover named Opportunity landed in the western part of this region in January 2004.
As the Martian winter closes in, Opportunity's dust-laden companion called Spirit is scouting out a place to survive the poorly lit winter for about six months.
We're in the pipe , five by five.
Defunct Spy Satellite Falling From Orbit
By Eileen Sullivan
Associated Press
posted: 26 January 2008
WASHINGTON - A large U.S. spy satellite has lost power and propulsion and could hit the Earth in late February or March, government officials said Saturday.
The satellite, which no longer can be controlled, could contain hazardous materials, and it is unknown where on the planet it might come down, they said. The officials spoke on condition of anonymity because the information is classified as secret.
"Appropriate government agencies are monitoring the situation," said Gordon Johndroe, a spokesman for the National Security Council. "Numerous satellites over the years have come out of orbit and fallen harmlessly. We are looking at potential options to mitigate any possible damage this satellite may cause."
He would not comment on whether it is possible for the satellite to be perhaps shot down by a missile. He said it would be inappropriate to discuss any specifics at this time.
A senior government official said that lawmakers and other nations are being kept apprised of the situation.
The largest uncontrolled re-entry by a NASA spacecraft was Skylab, the 78-ton abandoned space station that fell from orbit in 1979. Its debris dropped harmlessly into the Indian Ocean and across a remote section of western Australia.
In 2000, NASA engineers successfully directed a safe de-orbit of the 17-ton Compton Gamma Ray Observatory, using rockets aboard the satellite to bring it down in a remote part of the Pacific Ocean.
In 2002, officials believe debris from a 7,000-pound science satellite smacked into the Earth's atmosphere and rained down over the Persian Gulf, a few thousand miles from where they first predicted it would plummet.
By Eileen Sullivan
Associated Press
posted: 26 January 2008
WASHINGTON - A large U.S. spy satellite has lost power and propulsion and could hit the Earth in late February or March, government officials said Saturday.
The satellite, which no longer can be controlled, could contain hazardous materials, and it is unknown where on the planet it might come down, they said. The officials spoke on condition of anonymity because the information is classified as secret.
"Appropriate government agencies are monitoring the situation," said Gordon Johndroe, a spokesman for the National Security Council. "Numerous satellites over the years have come out of orbit and fallen harmlessly. We are looking at potential options to mitigate any possible damage this satellite may cause."
He would not comment on whether it is possible for the satellite to be perhaps shot down by a missile. He said it would be inappropriate to discuss any specifics at this time.
A senior government official said that lawmakers and other nations are being kept apprised of the situation.
The largest uncontrolled re-entry by a NASA spacecraft was Skylab, the 78-ton abandoned space station that fell from orbit in 1979. Its debris dropped harmlessly into the Indian Ocean and across a remote section of western Australia.
In 2000, NASA engineers successfully directed a safe de-orbit of the 17-ton Compton Gamma Ray Observatory, using rockets aboard the satellite to bring it down in a remote part of the Pacific Ocean.
In 2002, officials believe debris from a 7,000-pound science satellite smacked into the Earth's atmosphere and rained down over the Persian Gulf, a few thousand miles from where they first predicted it would plummet.
We're in the pipe , five by five.
Space Freighter Finishes Docking Dress Rehearsals
Posted: 31 March 2008
02:08 pm ET
Europe's massive "Jules Verne" space freighter wrapped up its final dress rehearsal high above the Earth, priming the ship for a Thursday docking at the International Space Station (ISS).Looking something like an overweight X-wing fighter from the movie "Star Wars," the 21-ton automated cargo ship crept within a bus length of the space station Monday, then performed an escape maneuver below the orbital laboratory.
A joint international team of mission controllers led the "demo day" operations and are now discussing whether or not to proceed with an April 3rd docking attempt at the space station. Today's activities, however, appeared to occur without issue.Led by commander Peggy Whitson, the Expedition 16 space station crew will unload vital supplies from the spacecraft after docking, if all goes according to plan this week. Also known as an automated transport vehicle (ATV), the craft departed Earth on March 8 and has been trailing the space station ever since.
Three control centers — one each in France, Russia and the U.S — led the ship through its second of two testing days with some on-orbit help from Whitson and space station flight engineer Yuri Malenchenko. Saturday's dress rehearsal was completed without any problems, setting the ship up for today's events.The space freighter began its dress rehearsal today some 2 miles (3.2 km) behind the space station, closing the gap to the ISS by using advanced laser- and video-ranging systems.
During the more than two-hour operation, mission controllers commanded the Jules Verne into several built-in retreats to see if the craft could safely pull away from the space station, in the end resuming positioning it at a holding point about 36 feet (11 m) behind the Russian-built Zvezda service module.After the solar-panel feathered ship parked behind the space station, Malenchenko instructed it to back off around 12:52 p.m. EDT (1652 GMT) and swing below the space station to a safe point — an escape maneuver astronauts can use in the event of an emergency during docking.
The disposable 1.3 billion euro ($1.9 billion) spacecraft is the first of up to seven planned by the ESA. It is designed to deliver three times the fuel, oxygen, water, hardware and other supplies to the ISS than Russian Progress cargo ships are able to.
We're in the pipe , five by five.
DARPA Works to Perfect Self-Forging, High-Velocity 'Spears'
posted: 29 April 2008
06:43 am ET
In his 1955 novel Earthlight, science fiction author Arthur C. Clarke thought of an incredible superweapon that used giant electromagnets to shoot a stream of molten metal at lightning speed. Now, the Defense Advanced Research Projects Agency (DARPA) wants one for America's military.
They are calling it MAHEM, which stands for Magneto Hydrodynamic Explosive Munition. The intent is to create a device that creates a powerful enough electromagnetic field to propel streams of molten metal at enemy armor. If it works, the device will be a big improvement on a technology that got its start in World War II — the self-forging penetrator. Self-forging penetrators, as they are currently used, result from a conventional chemical explosion directed against a specially-shaped metal liner. When the device is set off, the blast causes the metal liner to achieve a new shape, suitable for penetrating deep into even moderately armored vehicles, and driven forward at a high velocity. The technology dates back to WWII.
This kind of weapon can be highly effective (it is currently being used against troops in Iraq). The drawbacks of this kind of weapon from the standpoint of US military planners is that they are one-time-use weapons, and cannot efficiently form multiple SFPs from a single charge. If it is possible to use a powerful electromagnet to accelerate a molten jet of metal, it could overcome the drawbacks mentioned above, and even achieve higher velocities and better targeting. DARPA hopes that it could provide the following capabilities:
"This could provide the warfighter with a means to address stressing missions such as: lightweight active self-protection for vehicles (potential defeat mechanism for a kinetic energy round), counter armor (passive, reactive, and active), mine countermeasures, and anti-ship cruise missile final layer of defense." Science fiction readers wonder what took DARPA planners so long; we've known about this idea for more than a half-century. In Earthlight, Arthur C. Clarke makes use of exactly this idea in a battle between a stationary facility on the Moon and several attacking space ships, including the aptly named Lethe.
Quotes:
Listen to the incomparable Clarke describe the battle for you, which takes place in the Sea of Rains.
"In utter silence, the battle was rising to its climax. Millions of years ago the molten rock had frozen to form the Sea of Rains, and now the weapons of the ships were turning it once more to lava. Out by the fortress, clouds of incandescent vapor were being blasted into the sky ...
"Wheeler saw it strike upward, a solid bar of light stabbing at the stars... He did not have time to reflect on the staggering violation of the laws of optics which this phenomenon implied, for he was staring at the ruined ship above his head. The beam had gone through Lethe as if she did not exist; the fortress had speared her as an entomologist pierces a butterfly with a pin."
The "beam" was a molten jet of metal hurled into space by enormous electromagnets.
This is not the only example of science-fictional weaponry sought by US government agencies:
Ghostbuster Approach To Neutralizing WMD.
You knew that someday it would come to this; Homeland Security calls upon Ghostbuster tech.
Navy EMRG Hypervelocity Projectiles
This weapon can even strike targets on the other side of mountains. Via MAgneto Hydrodynamic Explosive Munition (MAHEM)
Note:
I read a few Sci-Fi books dealing with space battles on this concept and it sounds promising. I hope they work out the kinks and get this up and running. I also think that someday this kind of technology can be used to launch a spacecraft into orbit. Wouldn’t that be something.
We're in the pipe , five by five.
Scientists Revisit Mars Sample Return Plans
Space News Correspondent
posted: 9 May 2008
ET
ALBUQUERQUE, N.M. — International planning is under way to reinvigorate plans for a Mars sample return mission, with researchers assessing science priorities and strategies to maximize the scientific output from such an undertaking.
Over the last several years, an armada of orbital and surface missions has revealed Mars to be surprisingly more complex than once thought, imbued with a variety of distinct environments — each of value in terms of possible scientific payback given a sample return effort. Mars samples returned to state-of-the-art Earth laboratories are considered by many to be the only way to unravel a host of unresolved questions about the red planet. A sample return mission also is viewed by many as a key tool to help space agencies prepare for future human expeditions to Mars.
Mars scientists, space engineers and program planners met here April 21-23 to take part in "Ground Truth from Mars: Science Payoff from a Sample Return Mission." Discussions focused on what scientific data can be extracted from the return of Mars samples to Earth. Another major topic was the packaging, care and handling of martian materials that would be needed to ensure that the specimens offer great payoff for their potential to reveal past and present conditions on the red planet. The meeting was initiated by the Curation and Analysis Planning Team for Extraterrestrial Materials, a standing committee of scientists who advise NASA.
Surprises on Mars
While no nation or group of nations has committed to fund what is likely to be a multibillion-dollar Mars sample return program, scientists feel that groundwork is being laid now, albeit in piecemeal fashion. The work of Mars rovers Spirit and Opportunity, for example, has been scientifically stellar, said Doug Ming, a space scientist within the Astromaterials Research and Exploration Science Office at NASA's Johnson Space Center in Houston. "We were surprised when we got on the ground to see an enormous diversity of materials. It took us all by surprise," Ming said. The two robot geologists independently have been exploring Gusev Crater and Meridiani Planum for more than four years, yielding "an enormous wealth of information that can be fed forward into a Mars sample return mission," he said. Ming and other scientists at the meeting suggested that a Mars sample return involving either of the rover sites could be viewed as the first leg of a two-part mission to bring samples back to Earth.
Cache and carry
NASA's Mars Science Laboratory, which is scheduled to launch in 2009, carries a container for caching bits and pieces of select martian samples. The cache could be saved until it could be transported back to Earth as part of a future Mars sample return mission, said John Karcz of the SETI Institute and NASA's Ames Research Center in Mountain View, Calif. The large nuclear-powered Mars Science Laboratory rover is being designed to wheel across Mars for a full martian year, equal to nearly two Earth years. The cache device would be set up to contain from five to 10 or more samples, Karcz said, "if we have the time, resources and inclination during the traverse."
The samples would be held in a container designed to allow photo-documentation of the samples over the course of the Mars Science Laboratory mission. The hockey puck-sized cache container is designed for easy removal by a future Mars sample return rover, Karcz said, for subsequent transport back to Earth. Meanwhile, the powerful eyes of several spacecraft already in orbit around Mars — NASA's Mars Odyssey and the Mars Reconnaissance Orbiter, joined by Europe's Mars Express — are examining areas that show promise in the search for extinct or extant martian biology and studies of the planet's evolution.
NASA's Phoenix Mars lander, which is set to land May 25, was designed to study the history of water and the potential uses of the martian arctic's ice-rich soil to provide life support and other needs of future human crews that will explore the planet. In many ways, Mars researchers find themselves in a candy store of scientific sweet spots — several candidate sites that seem ideal for a Mars return sample mission.
For example, the high-powered zoom lens of the Mars Reconnaissance Orbiter was used to identify two possible ancient hydrothermal springs that might have been a cozy niche providing warm, liquid water to harbor martian life forms as the climate on the red planet became colder and drier, said Carlton Allen, the astromaterials curator and manager of the Astromaterials Acquisition and Curation Office at NASA's Johnson Space Center (JSC).Allen and Dorothy Oehler, a JSC research colleague, view these possible springs as an area of potentially great importance to astrobiology. "This may well be the type of site that would have high priority for sample return," Allen said. "If this is what we claim ... it may well be one of the most significant, best astrobiological sites on the planet."
Pricey and risky
There is no question that a Mars sample return mission will be a pricey and risky initiative and opinions at the meeting varied widely when it came time to discuss the best way to get the greatest scientific returns for the least money.
"We don't want to engineer the [heck] out of this and make it a $10 billion return mission. We'll never get samples back. Let's be realistic," said Clive Neal, a professor of civil engineering and geological sciences at the University of Notre Dame in Indiana."A Mars sample return will be much more costly than other Mars missions. That's not actually a thesis ... I think that's a given," said David Mittlefehldt of the Astromaterials Research Office. "Orbital study is getting increasingly sophisticated. Nevertheless, it doesn't reliably provide an accurate description of the geology of the surface. And that's really what you need in order to plan a Mars sample return mission," he said. "Therefore, I think we should go some place where wheels-on-the-ground provide that geologic context."
Intelligent decisions
An ambitious mission like Mars sample return needs a lot of push, a lot of energy, and it needs a lot of people explaining why it is important to do, said Carl Agee, a co-convener of the meeting and director of the Institute of Meteoritics at the University of New Mexico in Albuquerque. Agee told Space News that the time to get started on Mars sample return is now so we can "make intelligent decisions about where to go, rather than just landing blindly." A synergistic Mars program — one that does not pit sample return versus orbital mission versus on-site study — will "show how all of this fits together to plan the strategy for exploration," he said."I think that we're in danger of trying to over-achieve with our first sample collection and thereby shoot ourselves in the foot," said Derek Sears, director of the Arkansas Center for Space and Planetary Sciences and head of the Cosmochemistry Group at the University of Arkansas in Fayetteville.
The goal should be to get to Mars and obtain the simplest and most obvious rocks from a sensible place and get them back, Sears advised. "Don't worry if we upset the rocks a little bit on the way back. Just get them back. Get them in the lab and we'll figure it all out. Don't over-worry the problem because it'll kill you," he told Space News. A Mars sample return mission that gets under way as early as 2020 is of great interest to both NASA and the European Space Agency, said David Beaty, chief scientist of the Mars Exploration Directorate at the Jet Propulsion Laboratory in Pasadena, Calif., and also a co-convener of the meeting. There is a growing desire to create an international version of a Mars sample return mission, not only in the United States and Europe, but also in Japan and Canada, Beaty told Space News.
Beaty said there already is a task force, the International Mars Architecture for Return of Samples (IMARS), with representatives from more than a half-dozen countries, along with NASA, the European Space Agency, the Canadian Space Agency and the Japan Aerospace Exploration Agency."They are trying to develop a potential plan for Mars sample return that can be separately presented to the different countries to generate budget," Beaty said. "Ultimately, we need to have the same plan being presented in multiple places."
Note:
This reminds me of Sandkings:
From the series The Outer Limits.
The scientist Dr. Simon Kress (Beau Bridges) has been researching the development of a species using eggs found in a sample of Martian soil. When one bug escapes from the laboratory breaking the security of the facility, the project is shut-down by the government due to its hazard. Dr. Simon expected to win the Nobel Prize and steals 275 g of the sample ground, bringing it to the barn of his property and developing new species. He hides the truth from his wife Cathy (Helen Shaver) and shares the secret with his smart son Josh (Dylan Bridges). Along the days, Simon realizes how intelligent the creatures are and feels like a god since they seem to worship him. However, when Simon is bitten by a subject, he changes his irresponsible behavior to insanity, jeopardizing his family, his friend and mankind.
We're in the pipe , five by five.
Astronomy Picture of the Day
2008 May 14
Explanation:
Looking out a window of the International Space Station brings breathtaking views. Visible vistas include a vast and colorful Earth, a deep dark sky, and an occasional spaceship sent to visit the station. Visible early last month was a Soyuz TMA-12 spacecraft carrying not only supplies but also three newcomers. The three new astronauts were Expedition 17 commander Sergei Volkov, flight engineer Oleg Kononenko, and spaceflight participant So-yeon Yi. Yi returned to Earth a few days later, while Volkov and Konenenko are scheduled to return in a few months. The docking module pictured above involved the Pirs Docking Compartment. The Expedition 17 crew, including NASA flight engineer Gregory Chamitoff, will carry out repairs on the ISS, explore new methods of living in space, and conduct research in space including the effects of space radiation on vitamin molecules.
We're in the pipe , five by five.
[fade]Astronomy Picture of the Day [/fade]
Explanation: What will become of these galaxies? Spiral galaxies NGC 5426 and NGC 5427 are passing dangerously close to each other, but each is likely to survive this collision. Most frequently when galaxies collide, a large galaxy eats a much smaller galaxy. In this case, however, the two galaxies are quite similar, each being a sprawling spiral with expansive arms and a compact core. As the galaxies advance over the next tens of millions of years, their component stars are unlikely to collide, although new stars will form in the bunching of gas caused by gravitational tides. Close inspection of the above image taken by the 8-meter Gemini-South Telescope in Chile shows a bridge of material momentarily connecting the two giants. Known collectively as Arp 271, the interacting pair spans about 130,000 light years and lies about 90 million light-years away toward the constellation of Virgo. Quite possibly, our Milky Way Galaxy will undergo a similar collision with the neighboring Andromeda Galaxy in about five billion years.
Explanation: What will become of these galaxies? Spiral galaxies NGC 5426 and NGC 5427 are passing dangerously close to each other, but each is likely to survive this collision. Most frequently when galaxies collide, a large galaxy eats a much smaller galaxy. In this case, however, the two galaxies are quite similar, each being a sprawling spiral with expansive arms and a compact core. As the galaxies advance over the next tens of millions of years, their component stars are unlikely to collide, although new stars will form in the bunching of gas caused by gravitational tides. Close inspection of the above image taken by the 8-meter Gemini-South Telescope in Chile shows a bridge of material momentarily connecting the two giants. Known collectively as Arp 271, the interacting pair spans about 130,000 light years and lies about 90 million light-years away toward the constellation of Virgo. Quite possibly, our Milky Way Galaxy will undergo a similar collision with the neighboring Andromeda Galaxy in about five billion years.
We're in the pipe , five by five.