Showing posts with label News. Show all posts
Showing posts with label News. Show all posts

Tuesday, July 22, 2008

Aug. 1, 2008 Solar Eclipse

On August 1st, 2008, there will be a total solar eclipse for some portions of the world. The actual total solar eclipse will only be viewable from Northern Canada, Northern Russia (Siberia), Western Mongolia, and most of China. Most of North America, Europe, and Asia will experience a partial solar eclipse. The timeline for the August 1, 2008 solar eclipse is as follows:

08:04 UTC -- Partial eclipse begins.
09:11 UTC -- Total eclipse begins.
10:21 UTC -- Greatest eclipse.
11:21 UTC -- Total eclipse ends.
12:38 UTC -- Partial eclipse ends.

All times are UTC. To find your local time, add or subtract your local offset from UTC. For more info, see here: Time Zone Converter

One of the most interesting things about this eclipse is that in some of the far Northern reaches of the planet, there will be a "midnight eclipse". A midnight eclipse is an event where the eclipse occurs in a region that does not experience night during that time of year.

SAFETY FIRST!

Although you will want to look at this eclipse, DO NOT LOOK AT A SOLAR ECLIPSE without proper safety equipment. Doing so can cause permanent and irreversible eye damage and possibly blindness.


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Aug. 16, 2008 Partial Lunar Eclipse

On August 16, 2008, viewers in Europe, Africa, South America, and Australia will be treated to a partial Lunar eclipse. This is the second lunar eclispe of 2008. Viewers in Africa and Europe will be able to watch the whole show. Stargazers in South America will see the eclipse ending just after sunset, while Australian viewers will be able to see the eclipse just before sunrise. The timetable for the August 16th, 2008 partial lunar eclipse is as follows:

18:23 UTC -- Moon enters penumbra.
19:35 UTC -- Moon enters umbra.
21:40 UTC -- Maximum.
22:44 UTC -- Moon exits umbra.
23:57 UTC -- Moon exits penumbra.

penumbra -- the lighter section of the Earth's shadow.
umbra -- the darker section of the Earth's shadow.
maximum -- The darkest the moon will become during this eclipse.

All times are UTC. To find your local time, add or subtract your local offset from UTC. For more info, see here: Time Zone Converter

Unfortunately, I won't get to see this eclipse at all, nor will anyone living in North America.

Clear skies!


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Wednesday, July 2, 2008

Phoenix to Analyze Icy Sample

Recently, Phoenix scooped up a sample of soil that was intended to go into the on board ovens for analysis. This sample was suspected to contain water ice. However, unforeseen delays meant that the sample sat in the scoop for a few days, and has since dried out. Not wanting to waste the sample, NASA has decided to drop the dried out sample into the optical microscopy instrument, where it will be examined, much like one would with a conventional microscope. Any leftovers will then go to the wet chemistry instrument.


The delay arose when oven # 4 malfunctioned due to a vibration issue inside the spacecraft. Now NASA scientists must find a way to move the soil quickly from the ground to the instruments, to avoid losing any water ice or other items to sublimation. If all goes as planned, the icy sample should be ready to analyze some time next week.

Clear skies!


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Monday, June 23, 2008

Official 100th Post!!

This is officially the 100th post to this blog. It's been around for less than a year, and its come a long way! I'd like to thank my readers, both past, present, and future. To commemorate this 100th post, I've compiled a list of some of my favorite posts!


As always, Clear skies!


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Tuesday, June 17, 2008

Phoenix Begins "Baking"

NASA's Phoenix space probe has begun its task of sampling the Martian polar ice cap. The Phoenix lander has eight separate ovens inside it, that will allow it to "bake" samples of Martian soil and analyze their composition, in search of water. On June 3, NASA's Phoenix space probe found a white substance in nearby soil, which is believed to be possible water ice. On June 12, two trenches, which became known as "Dodo" and "Goldilocks", were dug by Phoenix's robotic arm to analyze this white material. The two trenches were again excavated and joined, forming the "Dodo-Goldilocks" trench, which is 8.7 inches wide, 13.8 inches long, and about 3 inches deep. The soil collected from these trenches was put into a sample oven and is currently being analyzed. The hope is that this white material is water ice.

Image Courtesy of: NASA/JPL-Caltech/University of Arizona/Texas A&M University/NASA Ames Research Center


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Saturday, May 17, 2008

Phoenix Probe Nearing Mars

NASA's Phoenix spacecraft is nearing its destination at Mars, with a scheduled landing date of May 25, 2008. The Phoenix probe will land in Mars' far northern polar region, where it will conduct scientific experiments on the planet's polar ice cap. According to previous investigation, the landing site chosen for the Phoenix spacecraft possesses water ice near or at the surface. Phoenix is equipped to dig, if necessary, to reach such water deposits. After Phoenix has acquired the samples, it will analyze the samples using several on board instruments. By analyzing this data, scientists can learn a great deal about Mars' climatic history.

According to a NASA press release, Phoenix has three main goals to accomplish: to study the history of water on Mars, to determine if the Martian arctic soil could support life (including future human life), and to study Martian polar weather. Accomplishing these three goals will give scientists and astronomers a better understanding of the role water plays on both modern and historic Mars. It is possible, that on timescales of 50,000 years, that the climate of Mars changes, and water ice could become liquid water. Phoenix will provide useful insights into this process.

To help Phoenix accomplish these goals, it carries with it several important appendages and scientific instruments. The most important of these instruments is its aluminum and titanium robotic arm. Since Phoenix will be a stationary platform, it will not have the capability to rove around for samples. This stationary platform approach is also vulnerable to rocks on the surface, so the landing must go perfectly the first time. Phoenix will use its robotic arm to sample from its surrounding environment. This 7.7 foot long robotic arm will also have a camera attached to it, near its scoop. The camera will assist in collecting soil and ice samples, and provide close-up images of the Martian soil.

To analyze the samples retrieved by the robotic arm, Phoenix will use a full array of scientific equipment, including its surface stereo imager, several types of spectrometers, as well as microscopy, electrochemistry, and conductivity analysis equipment. The stereo imager is composed of two cameras, spaced similarly to a human pair of eyes. When the images are combined, a three-dimensional image is created. Think of it as 3-D glasses on Mars. The other instruments will determine the chemical and physical properties of the soil and ice.

We'll see in about a week how the landing went. Results should be in around 8 PM EST on May 25, 2008.

Clear skies!


Image courtesy of NASA/JPL.


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Tuesday, April 1, 2008

Water on Mars?

Scientists and astronomers may have found the secret to detecting water on Mars. The method involves a radar-based technique, and may be ready for future missions to Mars within a few years. By using this radar-like technique, scientists can probe deep into the Martian surface, without the need to actually do any digging. Detecting water on Mars would be a major milestone in the study of Mars' early geographical history, and could lend insights into our own planets past and future. The following is a demonstration of such a system.

Just kidding...



Happy April Fool's Day!!


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Tuesday, March 4, 2008

Spacecraft Experience Orbital Anomalies

As early as Pioneer 10 and Pioneer 11, NASA and other spaceflight agencies have noticed a small discrepancy in the expected and actual trajectories of space probes. The twin probes from the mid-70's flew by Jupiter and then Saturn. The spacecraft was then flung on its way out of the solar system using Saturn's gravity assist. The spacecraft, for the most part, has followed its expected path out of the solar system. There has been, however, a tiny discrepancy in the orbital trajectory of the spacecraft. This discrepancy has become known as the "Pioneer Anomaly". The Pioneer probes are not the only spacecraft to exhibit this strange effect, which has been observed numerous times more recently.

This effect has been observed by tracking the spacecraft's radio doppler shift. Using this data, scientists can obtain very accurate readings of its position and velocity. Standard gravitational models are used to predict its exact location and trajectory. These models, however, have been shown to be off by the most minute amount, and show a tiny acceleration towards the sun, not accounted for by gravity. What could this mean? There are many explanations, ranging from the mundane to the exotic. Some such explanations are given below, as partially quoted from this article on wikipedia:

  • Observational error - The problem with this explanation is that 7 separate and independent analyses have confirmed the Pioneer Anomaly.
  • An unaccounted for deceleration - This is a distinct possibility. It could be that gas or fuel leaks are actually changing the orbits of the spacecraft. This is unlikely, also, because of the numerous spacecraft that have reported very similar problems.
  • Electromagnetic repulsion or attraction, due to charges accumulated on spacecraft.
  • Friction with the interplanetary media - An unlikely explanation, as the interplanetary media is much too sparse to adversely affect an orbit.
  • Statistical variation in the measurement of the spacecraft's orbits - Again, many satellites and probes have reported similar measurements.
  • The effects of dark matter and dark energy on our current understanding of astrophysics.
  • The effects of distribution of matter in the Milky Way.
Several modern spacecraft are also reporting Pioneer anomalies. Six recent flybys of the Earth were considered: two by Galileo, the NEAR mission to Eros, Rosetta, Cassini, and the recent Messenger. In five of these six flybys, the anomaly was detected. The anomaly measured in these craft are very much real. The NEAR mission's anomaly was measured to be off by 13 mm/s with an accuracy of 0.1 mm/s. The spacecraft's velocity error was less than 0.0000001 %, which may seem tiny, but it is very much real, and previously unaccounted for. If this seems tiny, think about it on astronomical scales. Data shows that Pioneer 10 and Pioneer 11 are both about 240,000 miles (400,000 kilometers) closer to the sun than they should be. Now that's cause for concern. The question is, how will we account for this anomaly? What could really be causing it?

Recent theories propose that Pioneer's anomalous acceleration towards the sun [(8.74 ± 1.33) x 10−10 m/s2] is actually quite close to the product of the Hubble constant, which pertains to galaxies' redshifts [70.4+1.5−1.6 (km/s)/Mpc] and the speed of light [c = 2.99 x 108]. This is an interesting proposal. We will have to wait, however, to see what its implications are, and whether it is correct. Scientists will be closely watching the trajectory of Rosetta's second flyby and New Horizon's trajectory as it speeds towards Pluto. We'll see if these two craft exhibit similar anomalies. If they do, it could mean a rethinking of our current physical models.

Clear skies!


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Monday, March 3, 2008

Avalanche!

NASA's Mars Reconnaissance Orbiter has caught Mars in the act of geological change! Recent images recieved from the orbiting camera station show a large avalanche on February 19, 2008. The dust cloud seen in the image below is about 590 feet (180 meters) across and 625 feet (190 meters) long.


This is actually one of four such landslide seen in one larger photo, available here. The 2,300 foot (700 meters) cliff seen in this image is part of the raised section that comprises Mars' northern polar region. The ice on the west side of the image is part of Mars' polar ice cap, a frozen deposit of carbon dioxide and water ice. Many of the images obtained by the Mars Reconnaissance Orbiter show seasonal and small-scale changes, such as dust devils. This, however, is the first image of large-scale change in progress, a rare sight indeed.

While the mechanism responsible for the collapse are as of yet unknown, several causes have been proposed. It could have been a "Mars-quake", or a small meteorite impact. It also appears that sections of the upper cliff face have been cracked and eroded by the timely expansion and contraction of the polar ice cap. These weakened sections of the cliff face could be dislodged by gravity or Martian winds. Information gathered from these images could help planetary geologists piece together one more aspect of Mars' mysterious geological history.

Clear skies!

Image courtesy of: NASA / JPL-Caltech / University of Arizona


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Thursday, February 28, 2008

NASA To Slam Moon with Impactor

NASA is planning a mission to the moon, but there will be no humans or rovers to speak of. Their mission is to slam an impactor probe into the moon's south polar region. Although this seems like a rather destructive and barbaric mission, it actually has good scientific merit. The mission will be known as the Lunar Crater and Observation Sensing Satellite, or LCROSS. The premise for LCROSS stems from a discovery by NASA's Lunar Prospector that showed abnormally high concentrations of hydrogen in the Lunar south polar region. Scientists have speculated that the hydrogen could be associated with water ice locked deep under the Lunar surface. By impacting the surface at a very high velocity, the impactor can throw Lunar debris into space, where it can be analyzed further by the host spacecraft.

The Lunar probe will be comprised of two main segments. These include the Shepherding Spacecraft, and the Centaur impactor. The Centaur impactor will weigh about 4,400 pounds (2,000 kgs). Once in orbit about the Moon, the Centaur impactor will separate from its host spacecraft and begin its descent towards the surface. The impactor will slam into the surface at a velocity of approximately 1.6 miles per second (2.5 km/s), and is expected to eject over 1,100 tons of Lunar dust. The Shepherding Spacecraft will then fly through this cloud of dust, and sample it using onboard sensors. LCROSS will be launched along with the Lunar Reconnaissance Orbiter on October 28, 2008. Impact is scheduled for February of 2009. I'll keep the site updated with any news of whether this event will be visible to amateur astronomers. I would imagine that one should be able to see it in moderate sized telescopes.

This won't be the first time a space agency has punched a heavenly body, however. NASA's Deep Impact mission slammed into Comet Tempel 1 in 2005, and the ESA made a recent Lunar impact with Smart-1 in 2006. This recent trend toward violent impactors has some astronomers and scientists concerned, however. While good scientific data is obtained from such events, some believe that these missions are too destructive to their targets. Surely, a few more craters on the moon won't hurt, right?

Clear skies!

Image courtesy of NASA/AMES.


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Thursday, February 21, 2008

Satellite USA-193 Destroyed

Satellite USA-193 has been successfully struck with a Standard Missile 3 on Wednesday night at about 10:30 PM EST over Hawaii. USA-193 was a spy satellite that had lost power some time ago. To prevent the satellite from reentering the atmosphere and releasing its hydrazine fuel, US officials shot the satellite out of the sky. China conducted a similar exercise last year. The event was not visible from my midwestern location, but the debris cloud from the event may make several passes over the US. This video shows the expected path of the debris cloud after the satellite's destruction.



Watch for debris reentering the atmosphere over the next few days. It will appear somewhat like a meteor. If you see anything, please leave a comment. I'd be interested to hear about sightings!

Clear skies!


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Meteor Strike on Tape!

Breaking News!

An Idaho Air National Guard security camera at Gowen Field in Boise, Idaho, captured this meteor like object as it ripped through the atmosphere and appears to have impacted the surface at 5:30 AM PST. Not many details are currently available, but I'll fill you in as I get them.




Anyone else see this?

Clear skies!


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Wednesday, February 20, 2008

STS-122 Makes Safe Landing

Space Shuttle Atlantis landed safely at NASA's Kennedy Space Center today, after a two week stay in space. Atlantis' STS-122 mission was to put the ESA's Columbus space station module into orbit and dock it with the International Space Station. According to NASA, the mission went "very well". Among the astronauts of STS-122 were Commander Steve Frick, Pilot Alan Poindexter, Mission Specialists Leland Melvin, Rex Walheim, Stanley Love, Dan Tani and ESA astronaut Hans Schlegel.


Space Shuttle Atlantis after touchdown.
Image courtesy of NASA/Bill Ingalls.

Commander Frick was quoted,
"The station missions now are so busy ... It's been a tremendous experience. We were very excited and pleased to bring Columbus to the International Space Station."

Here is a video of STS-122's final approach and landing at NASA's Kennedy Space Center, viewed both from the ground and from Atlantis.



Video courtesy of NASA.

Hot on the trail of Atlantis is Space Shuttle Endeavor, which is scheduled for launch March 11th. Atlantis will return to its hangar to get ready for its August mission to the Hubble Space Telescope.


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Tuesday, February 19, 2008

US-193 Scheduled for Destruction

The US-193 satellite has been officially scheduled for destruction on February 21st, 2008 at 03:30 UTC. The satellite will be shot down near Hawaii, in restricted airspace over the Pacific Ocean to avoid debris reaching land. US-193 had lost power and communications a while ago, and its orbit has been decaying since. So if you're on the West coast, keep an eye out at this time. More information on US-193's destruction is available here. Here on the East coast, we probably won't be able to see the event, but we might get to see the debris field. Also notice that the destruction of this satellite falls in line with the upcoming lunar eclipse. Probably a pure coincidence, though.


Ground track during US-193's destruction.

Clear skies!


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Sunday, February 17, 2008

Are Rocky Exo-Planets Common?

Could rocky, Earth-like exo-planets exist? If so, how common are they? This question had plagued astronomers for years, until recently. Early discoveries of exo-planets were mostly of the so-called "hot Jupiter" planets. These types of planets were monstrous planets, some larger than Jupiter, and orbiting very close to their star. This at first looked discouraging to astronomers hoping to find an Earth-like exo-planet. It turns out, however, that the reason astronomers are finding so many hot Jupiters is that the current method of detecting planets is only sensitive enough to detect very massive planets by measuring the wobble imparted on its parent star. However, new data from the Spitzer space telescope point towards rocky, terrestrial exo-planets being more common than we had thought.

Astronomers started their hunt by choosing six sets of stars similar in mass to our own, but differing in age. Then, by utilizing Spitzer's infrared capabilities, astronomers can estimate the temperature of the star's surrounding dust cloud. Dust near the center of each stellar system would be warmer than the more distant dust. Astronomers can look at the distribution and temperature of this dust, and get useful data about the star's evolutionary progress. Michael Meyer, of the University of Arizona, Tucson, has found that after 300 million years of evolution, most of the dust which corresponds to planet formation is gone.

This, of course, does not imply that these stars have rocky exo-planets. It does, however, imply that stars between the ages of three million and 300 million years are undergoing similar planet-forming stages as our own solar system. Using this data, astronomers have estimated that up to 62% or stars may either have or are creating rocky, terrestrial exo-planets. This may be an optimistic estimate, but it points to a universe where planets like our own are not a freak accident.

More information


Clear skies!


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Thursday, February 14, 2008

US to Blow Failed Satellite Out of Sky

Lately, there has been much ado in the media about satellite US-193. This satellite is a National Reconnaissance Office satellite. In other words, it's a spy satellite, on a classified mission. There's not much one can hide from amateur astronomers, however, as the satellite can often be seen in the afternoon. Click here for information on when you can see it. It has been known for some time now that it had lost power and communications and would be re-entering the atmosphere at some point. Now, the government is concerned about this re-entry and is actually planning to blow the satellite out of the sky, before it reaches the surface.

US-193 weighs about 5,000 pounds. While a good portion of this mass would burn up in the atmosphere, about 2,500 pounds could impact the surface. This could cause major damage in a populated area. Another concern is that the satellite's hydrazine fuel, a hazardous substance could be dissipated upon impact. This would mean nearly 1,000 pounds of toxic fumes being thrown into a possibly populated area. If the US were to destroy the satellite in space, it could disperse the hydrazine harmlessly. The trouble is, there's only a short window in which it could be effectively destroyed. If the missile were fired too late, it would not only defeat the purpose, but would be extremely difficult. This is because as the satellite re-enters the atmosphere, its motion will become mostly erratic.



Current position of US-193, courtesy of Heavens-Above.com

Another reason that the government wants to shoot down this satellite is its very purpose itself. The satellite is a spy satellite, so the US government would not like it to fall into the wrong hands, if any parts survived. This exercise is also a good excuse to test out new "Star Wars" style weapons defense systems. Last year, China destroyed one of its own satellites using a ground based missile. This could be an attempt to show, "We can do that too." What better excuse to destroy a satellite? Could this be the next Cold War in space? Most likely not. We'll probably see the conspiracy theorists come out of the woodwork on this one.

Hopefully, this satellite will be destroyed when on the night side of the Earth, visible to amateur astronomers. If details come up about the time and location of its destruction, I'll keep you posted.

Clear skies!


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Wednesday, February 13, 2008

Columbus Lab Open for Business

The International Space Station's new Columbus laboratory is now open for business. The 23-foot long, 10-ton research laboratory was opened for the first time Tuesday, Feb. 12, 2008. The Columbus module will be used mainly for microgravity research both internally and externally to the module.


NASA officials have commented that the opening went reasonably well, all things considered. Theres was a small cooling system glitch in the beginning, but nothing that will hamper the overall functioning of the laboratory. Astronauts wore protective gear upon first entering the module, just in case of any debris that had shown up during launch and transport.

Getting the Columbus lab setup, however, is going to be a chore. Astronauts from STS-122 are going to be extending the mission by one day in order to get the Columbus lab fully assembled and ready to go. Atlantis is now scheduled to return on Feb. 19.

Clear skies!

Image courtesy of NASA TV.


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Monday, February 11, 2008

Name a Satellite!

NASA and Sonoma State University's GLAST (Gamma-ray Large Area Space Telescope) satellite will be the first space-based observatory to monitor powerful phenomenon such as black holes, gamma ray bursts, and dark matter. The GLAST name, however, isn't very catchy, so NASA is hosting a "name that satellite contest", much like they did for the Spirit/Opportunity rovers.


The satellite launches in mid-2008, and names for the mission should be submitted by March 31, 2008. According to their website,

  • The deadline for submissions is March 31, 2008.
  • The name should capture the excitement of GLAST’s mission, bringing attention to gamma rays and high-energy astronomy.
  • The name should be catchy, something that people will talk about.
  • Make it simple and easy to say. Nothing says complex and inaccessible like a mouthful of acronyms.
  • In keeping with NASA tradition, the satellite will not be named after a person who is still living.
  • Finally, the name must be original and not associated with any past, present or future astronomical observatory or space mission (domestic or international) or any NASA program. Sorry, Voyager fans!
The form also requires a 25 word or less summary of why you think they should choose your suggestion. Give it a try, they might just choose yours!

Clear skies!

Image courtesy of NASA E/PO, Sonoma State University, Aurore Simonnet.


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Sunday, February 10, 2008

Interactive STS-122 Flight Plan

NASA has put a new interactive flight plan for STS-122 on their website. The interactive Flash application allows users to view the shuttle's schedule and relevant pictures. Simply roll the mouse over each day to see the astronaut's agenda for that day.


STS-125 has become known unofficially as the "Voyage of Columbus", due to its cargo, the Columbus laboratory. The Columbus laboratory is a European Space Agency contribution to the International Space Station. The Columbus laboratory's main purpose during its 10-year mission is to further study the effects of microgravity on biological and other specimens.


The Columbus module in Atlantis' cargo bay.

Some events for the STS-122 mission include docking the Columbus module on day 4 and several spacewalks for maintenance of the ISS.

Images courtesy of NASA/JPL.

Clear skies!


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Thursday, February 7, 2008

Full Lunar Eclipse - Feb. 20, 2008

On the night of February 20/21, 2008, viewers on the night side of the Earth will observe a total lunar eclipse, which occurs when the moon passes directly behind the Earth, and enters its shadow. Observers in the Americas, Europe, and Africa will be posed for the best views.


The following table represents the predicted timetable for the lunar eclipse, as provided by Curt Renz, whose helpful astronomy website can be found at www.curtrenz.com/astronomical.html.

00:37 UT – Moon enters penumbra (gray fringe shadow)
01:43 UT – Moon enters umbra (dark inner shadow)
02:18 UT – 50% of Moon’s diameter covered by umbra
03:01 UT – Totality begins (magnitude 1.000)
03:26 UT – Maximum eclipse (magnitude 1.105)
03:51 UT – Totality ends (magnitude 1.000)
04:34 UT – 50% of Moon’s diameter covered by umbra (magnitude 0.500)
05:09 UT – Moon exits umbra (dark inner shadow)
06:16 UT – Moon exits penumbra (gray fringe shadow)

The times given in this table are Universal Time (UT), also known as Greenwich Mean Time (GMT), for the night of the 20/21. Therefore, these times are mostly in the very early morning of the 21st, just after midnight UT. To find your corresponding local time, subtract your time zone's offset from this number. So for example, Eastern time is GMT-5, so I would subtract 5 hours from each of the times listed here, so 00:37 UT becomes 7:37 PM EST. Central time is GMT-6, Mountain time is GMT-7, and Pacific time is GMT-8. Other time zone offsets are available here.

The moon will actually appear to turn a blood red color during maximum eclipse. This is an optical effect due to the refraction of sunlight by the Earth's atmosphere. Red light is bent most readily and is projected upon the face of the moon. Also notice Saturn's close proximity to the moon during the eclipse. I'll be setting up a composite shot of the eclipse with Youngstown's skyline, assuming skies are clear. This, however, is a slim chance in Northeast Ohio...

This is the last total lunar eclipse until two total eclipses on December 21, 2010, and June 15, 2011, so don't miss it!

Clear skies! (hopefully)...

EDIT: A composite image of the eclipse that I made from Youngstown, Ohio is available here.

Eclipse timetable courtesy of Curt Renz.


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