Wednesday, October 8, 2014

How to Take Great Photos of the Lunar Eclipse

How to Take Great Photos of the Lunar Eclipse:

On Wednesday morning October 8, Earth's shadow will nibble away at the moon for this year's second total lunar eclipse. Credit: Bob King


On Wednesday morning October 8, Earth’s shadow will nibble away at the moon during the wee hours eclipsing it for the second time this year. Credit: Bob King
Ready for Wednesday’s morning lunar eclipse Some people – and I envy them at times – treat an eclipse more casually. They enjoy the show with no desire to set up a telescope or take a photo. For those of us can’t part with our cameras, here’s a little guide to help you get better pictures.

From Philadelphia and other eastern U.S. cities the partial phases of the eclipse will take place with the moon well up in the western sky. By the start of totality, the moon will have dropped to within about 6º of the horizon as shown here. Source: Stellarium


From Philadelphia and other eastern U.S. cities the partial phases of the eclipse will take place with the moon well up in the western sky. By the start of totality, the moon will have dropped to within about 6º of the horizon as shown here. Source: Stellarium
If you’re also into photography and would like to grab a few shots, here are a few tips on what equipment you’ll need and camera settings. This eclipse offers unique opportunities especially for the eastern half of the country because the eclipsed moon will be low in the western sky near the start of and during morning twilight.

In the Midwest at the start of the hour-long totality, the red moon will be about 20º (two fists) above the western horizon. From the East Coast the moon slips into total eclipse only a half hour before sunrise 6-7º high. So if you live in the eastern half of the country, find a site with a good view to the west.

Seen from Denver, total eclipse begins with the moon 30º high (three fists). All of totality and all partial phases of the eclipse will be visible from western Midwest west to Hawaii and Alaska. Source: Stellarium


Seen from Denver, total eclipse begins with the moon 30º high (three fists). All of totality and all partial phases of the eclipse will be visible from western Midwest west to Hawaii and Alaska. Source: Stellarium
A low moon means easier framing with a pleasing foreground like a grove of fall trees, a church or distant line of mountain peaks. And the lower it drops, the longer the telephoto lens you can use to enlarge the moon relative to the foreground. When the moon is high in the sky it’s more difficult to find a suitable foreground.

Sometimes it's nice to have a foreground object to add character to your eclipse photos. Last April's totally eclipsed moon joins the old Central High School clock tower in downtown Duluth, Minn. Mars at upper right. Details: 80mm lens, f/5, 1.6-second exposure at ISO 400 on a tripod. Credit: Bob King


Sometimes it’s nice to have a foreground object to add character to your eclipse photos. Last April’s totally eclipsed moon joins the old Central High School clock tower in downtown Duluth, Minn. Mars at upper right. Details: 80mm lens, f/5, 1.6-second exposure at ISO 400 on a tripod. Credit: Bob King
As the scene brightens during twilight, balancing the light of the dim moon, your photos will get even more interesting. Textures and details in foreground objects will stand out instead of appearing as silhouettes.

Use the table below to plan when to watch depending on your time zone. The blanks mean the moon will have set by the time of the event.

Eclipse Events                                                EDT                 CDT                MDT                 PDT

Penumbra first visible 4:45 a.m. 3:45 a.m. 2:45 a.m. 1:45 a.m.
Partial eclipse begins 5:15 a.m. 4:15 a.m. 3:15 a.m. 2:15 a.m.
Total eclipse begins 6:25 a.m. 5:25 a.m. 4:25 a.m. 3:25 a.m.
Mid-eclipse 6:55 a.m. 5:55 a.m. 4:55 a.m. 3:55 a.m.
Total eclipse ends 7:24 a.m. 6:24 a.m. 5:24 a.m. 4:24 a.m.
Partial eclipse ends ——— 7:34 a.m. 6:34 a.m. 5:34 a.m.
Penumbra last visible ——— ——— 7:05 a.m. 6:05 a.m.


Exposures and lens settings

Partial phase during the April 14-15 eclipse this year. Details: Telescope (=1300mm telephoto lens) at f/11, 1/250 second at ISO 400. Credit: Bob King


Partial phase during the April 14-15 eclipse this year. Details: Telescope (=1300mm telephoto lens) at f/11, 1/250 second at ISO 400. Credit: Bob King
The full moon and even the partially eclipsed moon (up to about half) are so bright you can shoot a handheld photo without resorting to a tripod. Exposures at ISO 400 are in the neighborhood of f/8 at 1/250-1/500 second. Only thing is, all you’ll get is the moon surrounded by blackness. These exposures are so brief almost nothing will show in your foreground except for possibly moonlit clouds. That’s usually fine for the early partial phases.

Once the moon is more than half smothered by shadow, open up your lens to a wider setting – f/2.8 to f/4 – or increase the exposure. Let the back of the camera be your guide. If the images look too bright, dial back. If too dim, increase exposure or open the lens to a wider aperture.

To capture the encroaching shadow during partial phases you'll need to overexpose the sunlit part of the moon. Details: f/11, 2-second exposure at ISO 400. Credit: Bob King


To capture the encroaching shadow during partial phases you’ll need to overexpose the sunlit part of the moon. Details: f/11, 2-second exposure at ISO 400. Credit: Bob King
While you can continue to shoot the partially eclipsed moon at f/8 from 1/30-1/125 second, you’ll miss the best part – the portion filling up with Earth’s red shadow. To capture that, break out the tripod, open the lens all the way up – f/2.8-f/4 – and expose at ISO 400 between 1/4 and 1 second.

You can also shoot at ISO 800 and cut those times in half, important if you’re using a longish telephoto lens. Remember, Earth’s rotation means the moon’s on the move and will show trailing if you expose longer than a few seconds. On the other hand, this won’t be a problem if you’re shooting with a wide angle lens though they have their limits, too.

The moon completely immersed in Earth's umbra during totality. Details: f/11, 6-second exposure, ISO 400. Credit : Bob King


The moon completely immersed in Earth’s umbra during totality. Details: f/11, 6-second exposure, ISO 400. To prevent trailing I used a motorized mount to track the moon. Credit : Bob King
During totality, expose anywhere from 1/2 to 5 seconds at f/2.8-4.5 at ISO 400. Let’s say you want to include both scenic foreground and stars in the picture using a wide angle or standard lens. Dial up the ISO to 800, open your lens wide and expose between 6-10 seconds. On the 6-second end you’ll catch only the brightest stars, but the moon won’t show trailing; on the longer end you’ll get lots more stars with some overexposure of the eclipsed moon.

Of course, you can go to even higher ISOs and shorten exposure times considerably. But in all but the newest, high-end cameras that comes at the price of increased graininess and less color saturation.

Wide scene from April's total eclipse with Spica below the moon and Mars to the right. Details: 24mm lens at f/2.8, 8-second exposure at ISO 800. The moon was deliberately overexposed to show it in a field of stars. You can vary the exposure to your taste but the shorter it is, the fewer stars. Longer exposures will show trailing. Credit: Bob King


Wide scene from April’s total eclipse with Spica below the moon and Mars to the right. Details: 24mm lens at f/2.8, 8-second exposure at ISO 800. The moon was deliberately overexposed to show it in a field of stars. You can vary the exposure to your taste but the shorter it is, the fewer stars. Longer exposures will show trailing. Credit: Bob King
Where parts of the eclipse happen in twilight, even mobile phones may suffice. There should be enough light to capture a pretty scene with the moon just emerging from total eclipse and during the ensuing partial phases.

The partial lunar eclipse of June 4, 2012, pre-dawn at moonset, from home in southern Alberta. This is a single exposure with the Canon 60Da and 18-200mm Sigma lens at 115mm and at f/5.6 for 0.4 sec at ISO 160. Copyright: Alan Dyer


The partial lunar eclipse of June 4, 2012, pre-dawn at moonset, from home in southern Alberta. This is a single exposure with the Canon 60Da and 18-200mm Sigma lens at 115mm and at f/5.6 for 0.4 sec at ISO 160. Copyright: Alan Dyer
If you’re clouded out or on the wrong side of the planet for the eclipse, you can catch live webcasts from the following sites:

* Gianluca Masi’s Virtual Telescope
* Griffith Observatory in Los Angeles
* SLOOH 

Clear skies!



About 

I'm a long-time amateur astronomer and member of the American Association of Variable Star Observers (AAVSO). My observing passions include everything from auroras to Z Cam stars. Every day the universe offers up something both beautiful and thought-provoking. I also write a daily astronomy blog called Astro Bob.
Tagged as: camera, eclipse, f-stop, lunar, Moon, shadow

Astrophoto: Old Faithful Geyser Erupts Under a Starry Sky

Astrophoto: Old Faithful Geyser Erupts Under a Starry Sky:

'Old Faithful' geyser in Yellowstone National Park in Wyoming under a beautiful night sky on September 28, 2014. Credit and copyright: astroval1 on Flickr.


‘Old Faithful’ geyser in Yellowstone National Park in Wyoming under a beautiful night sky on September 28, 2014. Credit and copyright: astroval1 on Flickr.
The Old Faithful geyser in Yellowstone National Park in the western US is one of the most predictable geographical features on Earth, as it erupts “faithfully” every 60 – 110 minutes. But you can never predict what the night sky will look like overhead. Astroval1 on Flickr captured this gorgeous shot of the stars over Old Faithful on September 28, 2014, with 30 seconds of exposure time.

Gorgeous!

Just another #MilkyWayMonday shot from Universe Today’s Flickr page! Enjoy browsing through all the great images from our readers and join our group to add your own astronomical imagery.

Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.

Tagged as: #milkywaymonday, Astrophotos, old faithful, Yellowstone national park

How to Turn Your Phone Into A Cosmic Ray Detector

How to Turn Your Phone Into A Cosmic Ray Detector:

Artist's impression of cosmic rays striking Earth (Simon Swordy/University of Chicago, NASA)

Artist’s impression of cosmic rays striking Earth (Simon Swordy/University of Chicago, NASA)
Quick, do you have an Android phone in your pocket? A few small changes and you could help physicists probe more of the curious nature of cosmic rays, high-energy particles that emanate from outside our solar system.

Just download an app, cover up your phone’s camera with duct tape, then place it somewhere (running idle) with the screen facing up. If a particle “event” happens, the information will be logged in a central database.

The project (called Distributed Electronic Cosmic-ray Observatory or DECO) aims to record secondary particles called muons that occur when cosmic rays hit the Earth’s atmosphere. Scientists believe cosmic rays are created in black holes and supernovas, but more studies are needed.

Screenshot of an Android app developed at the University of Wisconsin-Madison that aims to capture cosmic rays. Credit: Justin Vandenbroucke


Screenshot of an Android app developed at the University of Wisconsin-Madison that aims to capture cosmic rays. Credit: Justin Vandenbroucke
Researchers at the Wisconsin IceCube Particle Astrophysics Center (WIPAC), led by Justin Vandenbroucke, note that there are things about cosmic rays that confuse physicists. Their paths in space change as they go across magnetic fields, and it makes searching for other astronomy events difficult. That’s where they hope the phone study will be useful.

“Smartphone cameras use silicon chips that work through what is called the photoelectric effect, in which particles of light, or photons, hit a silicon surface and release an electric charge,” the University of Wisconsin-Madison wrote in a press release.

“The same is true for muons. When a muon strikes the semiconductor that underpins a smartphone camera, it liberates an electric charge and creates a signature in pixels that can be logged, stored and analyzed.”

For more details on how to run and use the app, consult this page (it’s the second item).

Source: University of Wisconsin-Madison



About 

Elizabeth Howell is the senior writer at Universe Today. She also works for Space.com, Space Exploration Network, the NASA Lunar Science Institute, NASA Astrobiology Magazine and LiveScience, among others. Career highlights include watching three shuttle launches, and going on a two-week simulated Mars expedition in rural Utah. You can follow her on Twitter @howellspace or contact her at her website.
Tagged as: cosmic rays

REAL Images of Eclipses Seen From Space

REAL Images of Eclipses Seen From Space:

JAXA


A screenshot of the ‘diamond ring effect’ as seen during a total solar eclipse captured by Kaguya from lunar orbit. Credit: JAXA/NHK.
That ‘amazing astro-shot that isn’t’ is making the rounds of ‘ye ole web again.

You know the one. “See an Amazing Image of an Eclipse… From SPACE!!!” screams the breathless headline, with the all-too-perfect image of totality over the limb of the Earth, with the Milky Way thrown in behind it for good measure.

As the old saying goes, if it looks too good to be true, it probably is. Sure, the pic is a fake, and it’s been debunked many, many times since it was first released into the wild a few years back. But never let reality get in the way of a good viral meme. As eclipse season 2 of 2 gets underway tonight with a total lunar eclipse followed by a partial solar eclipse on October 23rd both visible from North America, the image is once again making its rounds. But there’s a long history of authentic captures of eclipses from space that are just as compelling. We’ve compiled just such a roll call of real images of eclipses seen from space:

SDO


A partial solar eclipse as captured by SDO. Credit: NASA/SDO.
The Solar Dynamics Observatory:

Launched in 2010, The Solar Dynamics Observatory or SDO is NASA’s premier orbiting solar observatory. But unlike Sun-staring satellites based in low Earth orbit, SDO’s geosynchronous orbit assures that it tends to see a cycle of partial solar eclipses twice a year, roughly around the equinoxes. And like many satellites, SDO also passes into the Earth’s shadow as well, offering unique views of a solar eclipse by the limb of the Earth from its vantage point.

JAXA


The Moon ‘photobombs’ the view of Hinode. Credit: NASA/JAXA.
Hinode:

A joint mission between NASA and JAXA (the Japanese Aerospace Exploration Agency) launched in 2006, Hinode observes the Sun from low Earth orbit. As a consequence, it nearly has a similar vantage point as terrestrial viewers and frequently nabs passages of the Moon as solar eclipses occur. Such events, however, are fleeting; moving at about eight kilometres per second, such eclipses last only seconds in duration!

ESA


Catching the passage of the Moon during a brief partial eclipse. Credit: ESA.
Proba-2:

Like Hinode, Proba-2 is the European Space Agency’s flagship solar observing spacecraft based in low Earth orbit. It also catches sight of the occasional solar eclipse, and these fleeting passages of the Moon in front of the Earth happen in quick multiple cycles. Recent images from Proba-2 are available online.



Eclipses from the ISS:

The International Space Station isn’t equipped to observe the Sun per se, but astronauts and cosmonauts aboard have managed to catch views of solar eclipses in an unusual way, as the umbra of the Moon crosses the surface of the Earth. Such a view also takes the motion of the ISS in low Earth orbit into account. Cosmonauts aboard the late Mir space station also caught sight of the August 11th, 1999, total solar eclipse over Europe.

NASA GOES


NASA’ s GOES-WEST spies the umbra of the Moon. Credit: NASA-GOES.
NASA-GOES:

Weather satellites can, and do, occasionally catch sight of the inky black dot of the Moon’s penumbra crossing the disk of the Earth.  GOES-West snapped the above image of the November 13th, 2012, solar eclipse. The umbra of the Moon’s shadow races about 1700 kilometres per hour from west to east during an eclipse, and we can expect some interesting images in 2017 when the next total solar eclipse crosses the United States on August 21st, 2017.

NASA


An ‘Apollo eclipse!’ Credit: NASA.
Apollo-Soyuz Test Project:

The final mission of Apollo program, the 1975 Apollo-Soyuz Test Project, also yielded an unusual and little known effort to observe the Sun. The idea was to use the Apollo command module as a “coronagraph” and have cosmonauts image the Sun from the Soyuz as the Apollo spacecraft blocked it out after undocking. Unfortunately, the Apollo thrusters smeared the exposure, and it became a less than iconic— though unusual — view from the space age.

Gemini XII


A partial solar eclipse snapped by the crew of Gemini XII. Credit: NASA.
Gemini XII and the first eclipse seen from space:

On November 12th, 1966, a total solar eclipse graced South America. Astronauts James Lovell Jr. and Edwin “Buzz” Aldrin Jr. were also in orbit at the time, and managed to snap the first image of a solar eclipse from space. Gemini XII was the last flight of the program, and the astronauts initially thought they’d missed the eclipse after a short trajectory burn.

ISS


The 2012 transit of Venus as seen from the ISS. Credit: NASA/Don Pettit.
ISS Astronauts catch a transit of Venus:

We were fortunate that the International Space Station had its very own amateur astronomer in residence in 2012 to witness the historic transit of Venus from space. NASA astronaut Don Pettit knew that the transit would occur during his rotation, and packed a full-aperture white light solar filter for the occasion. Of course, a planetary transit meets the very loosest definition of a partial eclipse, but it’s a unique capture nonetheless.



Kaguya:

Japan’s SELENE-Kaguya spacecraft entered orbit around the Moon in 2007 and provided some outstanding imagery of our solitary natural neighbor. On February 10th, 2009, it also managed to catch a high definition view of the Earth eclipsing the Sun as seen from lunar orbit. A rare catch, such an event occurs during every lunar eclipse as seen from the Earth.

Mars eclipse


Curiosity captures a misshapen eclipse from the surface of Mars. Credit: NASA/JPL.
An unusual eclipse… seen from Mars:

We’re fortunate to live in an epoch in time and space where total solar eclipses can occur as seen from the Earth. But bizarre eclipses and transits can also be seen from Mars. The Spirit and Opportunity rovers have witnessed brief transits of the Martian moons Phobos and Deimos across the face of the Sun, and in 2010, the Curiosity rover recorded the passage of Phobos in front of the Sun in a bizarre-potato shaped “annular eclipse”. But beyond just the “coolness” factor, the event also helped researchers refine our understanding of orbital path of the Martian moon.

The future: It’s also interesting to think of what sort of astronomical wonders await travelers as we venture out across the solar system. For example, no human has yet to stand on the Moon and witness a solar eclipse. Or how about a ring plane passage through Saturn’s rings, thus far only witnessed via the robotic eyes of Cassini? Of course, for the best views of Saturn’s rings, we recommend a vacation stay on Iapetus, the only major Saturnian moon whose orbit is inclined to the ring plane. And stick around ‘til November 10th, 2084, and you can witness a transit of Earth, the Moon and Phobos as seen from the slopes of Elysium Mons on Mars:



Hopefully, they’ll have perfected that whole Futurama “head-in-a-jar” thing by then…

-Looking for eclipses in science fiction? Check out the author’s tales Exeligmos and Shadowfall.



About 

David Dickinson is an Earth science teacher, freelance science writer, retired USAF veteran & backyard astronomer. He currently writes and ponders the universe from Tampa Bay, Florida.
Tagged as: eclipse from space, eclipse from space fake, eclipses from other planets, real eclipse from space, total eclipse from space, Total Lunar Eclipse, total solar eclipse

Astrophoto: Nighttime at Horseshoe Bend

Astrophoto: Nighttime at Horseshoe Bend:

The night sky over Horseshoe Bend, near Page Arizona. Credit and copyright: Jack Fusco.


The night sky over Horseshoe Bend, near Page Arizona. Credit and copyright: Jack Fusco.
As the Milky Way now begins to set earlier in the evening here in the northern hemisphere, that doesn’t mean the photos of our night sky are any less stunning. This lovely shot for #TerrestrialTuesday by photographer Jack Fusco was taken this week at Horseshoe Bend in Arizona, a horseshoe-shaped meander of the Colorado River.

“During the day, the walk to Horseshoe Bend was full of tourists from all over the world,” Jack explained on Flickr. “At night, we sat alone and stared up at a brilliant star filled sky and only heard coyotes in the distance. It was an absolutely incredible location during the day and at night. This was shot with no Moon at the sky, so the area was at it’s absolute darkest. I was a little nervous setting up my gear for this shot as my tripod was just a few inches from a 1000ft drop down to the river. It was certainly an experience I’ll never forget.”

See more of Jack’s work on Flickr, Google+ and his website, www.jackfusco.com

Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.

Tagged as: #TerrestrialTuesday, arizona, Astrophotos, Horseshoe Bend, Jack Fusco, milky way

Stunning Photos of the Hunter’s Moon Lunar Eclipse

Stunning Photos of the Hunter’s Moon Lunar Eclipse:

Lunar eclipse timelapse into totality. Taken from Palmyra, New Jersey on the Delaware River near Philadelphia, Pennsylvania. Night began with stormy clouds and transitioned to clearer skies as the eclipse progressed. Sequence from approx 4AM EDT to 7AM sunrise. Credit and copyright: Frank Miller.


Lunar eclipse timelapse into totality. Taken from Palmyra, New Jersey on the Delaware River near Philadelphia, Pennsylvania. Night began with stormy clouds and transitioned to clearer skies as the eclipse progressed. Sequence from approx 4AM EDT to 7AM sunrise. Credit and copyright: Frank Miller.
Did you see it? On October 8, 2014, early risers in North and South America, east Asia, Australia and the Pacific saw unique and rare views of the Hunter’s Moon as was eclipsed by Earth’s shadow. We’ve got so many great pictures to share from our Flickr group and from social media! In some shots, the fully eclipsed Moon glows with a coppery red hue, and in others the partially eclipsed Moon appears to have a bite taken out of its bright surface. Some images pair the Moon with a faint planet Uranus.

This is the second and final total lunar eclipse of 2014, and the second of four in a quartet series of lunar eclipses known as a tetrad — a series of 4 consecutive total eclipses occurring at approximately six month intervals. The next total eclipse will be on April 4, 2015, with another occurring on Sept. 28, 2015.

Enjoy the images below!


Montage of the various views of the Moon during the lunar eclipse on October 8, 2014. Credit and copyright: Chuck Manges.


Montage of the various views of the Moon during the lunar eclipse on October 8, 2014. Credit and copyright: Chuck Manges.
Near-totality eclipsed Moon, in Pisces, with Uranus at left. Delta Psc is that brightest star at upper-right of Moon. Imaged near Calabash, North Carolina. Credit and copyright: Tavi Greiner.


Near-totality eclipsed Moon, in Pisces, with Uranus at left. Delta Psc is that brightest star at upper-right of Moon. Imaged near Calabash, North Carolina. Credit and copyright: Tavi Greiner.
The red 'blood Moon' of the October 8, 2014 lunar eclipse, as seen from the Mare Island Observatory. Credit and copyright: Clifton Reed.


The red ‘blood Moon’ of the October 8, 2014, lunar eclipse, as seen from the Mare Island Observatory. Credit and copyright: Clifton Reed.
The eclipsed Moon sets over the Andes (Mts. Lopez and Capilla, Bariloche). Credit and copyright: Guillermo Abramson.


The eclipsed Moon sets over the Andes (Mts. Lopez and Capilla, Bariloche). Credit and copyright: Guillermo Abramson.
Total Lunar Eclipse through the clouds as seen from Weatherly, PA on October 8, 2014. Credit and copyright: Tom Wildoner.


Total Lunar Eclipse through the clouds as seen from Weatherly, PA on October 8, 2014. Credit and copyright: Tom Wildoner.
'Eclipse on the edge,' shot from the front of the Mizpah Hotel in Tonopah, Nevada. Credit and copyright: David Dickinson.


‘Eclipse on the edge,’ shot from the front of the Mizpah Hotel in Tonopah, Nevada. Credit and copyright: David Dickinson.
Last moments of the eclipse as seen from Calama, Chile. Credit and copyright: srta Andrea on Flickr.


Last moments of the eclipse as seen from Calama, Chile. Credit and copyright: srta Andrea on Flickr.
The October 8th 2014 lunar eclipse from Houston, Texas, taken with a 500m lens featuring a statue of Sam Houston. Credit and copyright: Sergio Garcia Rill.


The October 8th, 2014, lunar eclipse from Houston, Texas, taken with a 500m lens featuring a statue of Sam Houston. Credit and copyright: Sergio Garcia Rill.
Image of the lunar eclipse taken just before the midpoint of totality. Taken with a modified Canon 450D + Celestron C6-N telescope. f/4 ISO400 4s exposure. Credit and copyright: Fred Locklear.


Image of the lunar eclipse taken just before the midpoint of totality. Taken with a modified Canon 450D + Celestron C6-N telescope. f/4 ISO400 4s exposure. Credit and copyright: Fred Locklear.
Lunar Eclipse on 10-08-2014 Huffman Dam, Dayton, Ohio Canon 6D, 80mm refractor,2x Barlow (1200mm) ISO 6400, 2 sec exposure. Credit and copyright: John Chumack/Galactic Images.


Lunar Eclipse on 10-08-2014
Huffman Dam, Dayton, Ohio
Canon 6D, 80mm refractor,2x Barlow (1200mm) ISO 6400,
2 sec exposure. Credit and copyright: John Chumack/Galactic Images.
@Nancy_A I managed to see it and got a pic after clouds and snow got out of the way in Jellicoe Ont. pic.twitter.com/TiHDLGxwCM

— Bill Magee (@88skywatcher88) October 8, 2014
@fcain @starstryder these photos were taken on my phone with a 11 inch dobsonian telescope at the Perth Observatory pic.twitter.com/xhqnNalpqM

— Matt Woods (@matty_woods) October 8, 2014
#BloodMoon at treetops 08OCT2014, 06:25:25 EST! @universetoday @CanonUSA @triadlivingmag @WFMY @WXII @weatherchannel pic.twitter.com/9Kz1yVCVGn

— J Farley Photography (@jfarleyphoto) October 8, 2014
Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.

Tagged as: Astrophotos, blood moon, eclipse, hunter's moon, lunar eclipse

Magical Images From Two Prolific Astronaut Tweeters Doing Their First Spacewalk

Magical Images From Two Prolific Astronaut Tweeters Doing Their First Spacewalk:

Photo of a spacewalker at work on the International Space Station on Oct. 7, 2014. "I don't have words to describe what we did today, but this photo gives a pretty good impression!" wrote European Space Agency astronaut (and spacewalk participant) Alexander Gerst on Twitter as a caption to this photo. Credit: Alexander Gerst / Twitter


Photo of a spacewalker at work on the International Space Station on Oct. 7, 2014. “I don’t have words to describe what we did today, but this photo gives a pretty good impression!” wrote European Space Agency astronaut (and spacewalk participant) Alexander Gerst on Twitter as a caption to this photo. Credit: Alexander Gerst / Twitter
What happens when you send two prolific social media astronauts out on a spacewalk? The best photos ever. Reid Wiseman (NASA) and Alexander Gerst (European Space Agency) both participated in their first extra-vehicular activity yesterday, and sent back amazing pictures of what the view looked like outside their visors.

Their comments are also fun: “reasonably INSANE” and “learning to fly” are among the phrases they put on Twitter, which you can see in the photo gallery below. The spacewalkers accomplished the major task of yesterday’s spacewalk, placing a failed International Space Station pump module in a permanent location, and doing a couple of minor maintenance tasks.

The view was reasonably INSANE during the #spacewalk pic.twitter.com/V8PbaPo2Rg

— Reid Wiseman (@astro_reid) October 7, 2014
Learning to fly. #EVA27 #selfie pic.twitter.com/LmoYKLaIJt — Alexander Gerst (@Astro_Alex) October 8, 2014
What an experience and an honor to share it with @Astro_Alex pic.twitter.com/3WACwhCPOQ

— Reid Wiseman (@astro_reid) October 7, 2014
Safe to say, this was the most amazing thing I have done in my life. #spacewalk #EVA27 pic.twitter.com/HiX6ZrN0U7 — Alexander Gerst (@Astro_Alex) October 8, 2014

Guilty pleasure to turn the camera upon thyself during a #spacealk pic.twitter.com/ivCZ4rxNyF

— Reid Wiseman (@astro_reid) October 7, 2014
My friend @astro_reid doing what he’s good at. #EVA27 #spacewalk https://t.co/iYXV91FvXi pic.twitter.com/8SzrIJUwRm — Alexander Gerst (@Astro_Alex) October 8, 2014
And here’s a bonus for those who scrolled to the end of this post — the first Vine video posted real-time during a spacewalk! This comes courtesy of NASA’s account. Click on the video to access the audio, which is Reid Wiseman exclaiming on the view over southern South America.


Tagged as: alexander gerst, Expedition 42, reid wiseman

Comet Siding Spring: Close Call for Mars, Wake Up Call for Earth?

Comet Siding Spring: Close Call for Mars, Wake Up Call for Earth?:

Five orbiters from India, the European Union and the United States will nestle behind the Mars as comet Siding Springs passes at a speed of 200,000 km/hr (125,000 mph). At right, Comet Shoemaker-Levy 9 impacts on Jupiter, the Chelyabinsk Asteroid over Russia. (Credits: NASA,ESA, ISRO)


Five orbiters from India, the European Union and the United States will nestle behind Mars as comet Siding Springs passes at a speed of 200,000 km/hr (125,000 mph). At right, Shoemaker-Levy 9 impacts on Jupiter, the Chelyabinsk Asteroid over Russia. (Credits: NASA,ESA, ISRO)
It was 20 years ago this past July when images of Jupiter being pummeled by a comet caught the world’s attention. Comet Shoemaker-Levy 9 had flown too close to Jupiter. It was captured by the giant planet’s gravity and torn into a string of beads. One by one the comet fragments impacted Jupiter — leaving blemishes on its atmosphere, each several times larger than Earth in size.

Until that event, no one had seen a comet impact a planet. Now, Mars will see a very close passage of the comet Siding Spring on October 19th. When the comet was first discovered, astronomers quickly realized that it was heading straight at Mars. In fact, it appeared it was going to be a bulls-eye hit — except for the margin of error in calculating a comet’s trajectory from 1 billion kilometers (620 million miles, 7 AU) away.

It took several months of analysis for a cataclysmic impact on Mars to be ruled out. So now today, Mars faces a just a cosmic close shave. But this comet packs enough energy that an impact would have globally altered Mars surface and atmosphere.

So what should us Earthlings gather from this and other events like it? Are we next? Why or why not should we be prepared for impacts from these mile wide objects?

For one, ask any dinosaur and you will have your answer.

Adding Siding Spring to the Comet 67P atop Los Angeles provides a rough comparison of sizes. This images was expanded upon U.T.'s Bob King - "What Comets, Parking Lots and Charcoal Have in Common". (Credit: ESA, anosmicovni)


An illustration of the Siding Spring comet in comparison to the Comet 67P atop Los Angeles. The original image was the focus of Bob King’s article – “What Comets, Parking Lots and Charcoal Have in Common“. (Credit: ESA, anosmicovni)
One can say that Mars was spared and also the five orbiting spacecraft from India (Mars Orbiter Mission), the European Union (Mars Express) and the United States (MOD,MRO,MAVEN). We have Scottish-Australian astronomer Robert McNaught to thank for discovering the comet on January 3, 2013 using the half meter (20 inch) Uppsala Southern Schmidt Telescope at Siding Spring, Australia.

Initially the margin of error in the trajectory was large, but a series of observations gradually reduced the error. By late summer 2014, Mars was in the clear and astronomers could confidently say the comet would pass close but not impact. Furthermore, as observations accumulated — including estimates of the outpouring of gases and dust — comet Siding Spring shrunk in size, i.e. the estimates of potentially tens of kilometers were down to now 700 meters (4/10th of a mile) in diameter. Estimates of the gas and dust production are low and the size of the tail and coma — the spherical gas cloud surrounding the solid body — are small and only the outer edge of both will interact with Mars’ atmosphere.

The mass, velocity and kinetic energy of celestial bodies can be deceiving. It is useful to compare the Siding Spring comet to common or man-made objects.


The mass, velocity and kinetic energy of celestial bodies can be deceiving. It is useful to compare the Siding Spring comet to common or man-made objects.
Yet, this is a close call for Mars. We could not rule out a collision for over six months. While this comet is small, it is moving relative to Mars at a speed of 200,000 kilometers/hour (125,000 mph, 56 km/sec). This small body packs a wallop. From high school science or intro college Physics, many of us know that the kinetic energy of an object increases by the square of the velocity. Double the velocity and the energy of the object goes up by 4, increase by 3 – energy increases by 9.

So the close shave for Mars is yet another wake up call for the “intelligent” space faring beings of the planet Earth. A wake up call because the close passage of a comet could have just as easily involved Earth. Astronomers would have warned the world of a comet heading straight for us, one that could wipe out 70% of all life as happened 65 million years ago to the dinosaurs. Replace dinosaur with humans and you have the full picture.

Time would have been of the essence. The space faring nations of the world — those of the ESA, and Russia, the USA, Japan and others — would have gathered and attempted to conceive some spacecrafts with likely nuclear weapons that could be built and launched within a few months. Probably several vehicles with weapons would be launched at once, leaving Earth as soon as possible. Intercepting a comet or asteroid further out would give the impulse from the explosions more time to push the incoming body away from the Earth.

There is no way that humanity could sit on their collective hands and wait for astronomers to observe and measure for months until they could claim that it would just be a close call for Earth. We could imagine the panic it would cause. Recall the scenes from Carl Sagan’s movie Contact with people of every persuasion expressing at 120 decibels their hopes and fears. Even a small comet or asteroid, only a half kilometer – a third of a mile in diameter would be a cataclysmic event for Mars or Earth.

But yet, in the time that has since transpired from discovery of the comet Siding Spring (1/3/2013), the Chelyabinsk asteroid (~20 m/65 ft) exploded in an air burst that injured 1500 people in Russia. The telescope that discovered Comet Siding Spring was decommissioned in late 2013 and the Southern Near-Earth Object Survey was shutdown. This has left the southern skies without a dedicated telescope for finding near-Earth asteroids. And proposals such as the Sentinel project by the B612 Foundation remain underfunded.

We know of the dangers from small celestial bodies such as comets or asteroids. Government organizations in the United States and groups at the United Nations are discussing plans. There is plenty of time to find and protect the Earth but not necessarily time to waste.

Previous U.T. Siding Spring stories:
What Comets, Parking Lots and Charcoal Have in Common“, Bob King, Sept 5, 2014
MAVEN Mars Orbiter Ideally Poised to Uniquely Map Comet Siding Spring Composition
– Exclusive Interview with Principal Investigator Bruce Jakosky”, Ken Kremer“, Sept 5, 2014
NASA Preps for Nail-biting Comet Flyby of Mars“, BoB King, July 26,2014


Tagged as: asteroid, comet, esa, Impacts, ISRO, Mars, Mars Express, MAVEN, MOM, MRO, NASA, Siding Spring

Suspected Black Hole Unmasked as Ultraluminous Pulsar

Suspected Black Hole Unmasked as Ultraluminous Pulsar:

M82

An Ultraluminous X-ray Source (ULX) that astronomers had thought was a black hole is really the brightest pulsar ever recorded. ULXs are objects that produce more X-rays than most "normal" X-ray binary systems, in which a star is orbiting a neutron star or a stellar-mass black hole. Black holes in these X-ray binary systems generally weigh about five to thirty times the mass of the sun.

Astronomers used NASA's NuSTAR (Nuclear Spectroscopic Telescope Array) and Chandra X-ray Observatory to study two ULXs in the center of M82, a galaxy located just over 11 million light years from Earth. This composite image shows X-rays from NuSTAR (purple) and Chandra (blue) that have been combined with optical data from the NRAO 2.1 meter telescope (gold). The extended X-ray emission is unrelated to the two ULXs.

Until now, astronomers have thought that matter falling onto black holes powered the bright X-ray emission in all ULXs. Most of the black holes in ULXs are thought to weigh at least 10 to 50 times the mass of the Sun, but some of the brightest ULXs are thought to weigh 100 times the Sun's mass, or more.

The new X-ray data provide a critical clue to the nature of one of the ULXs in M82. Using NuSTAR, scientists have discovered regular variations, or "pulsations," in the object known as M82X-2. This object pulses once on average every 1.37 seconds, and pulsations change in a regular pattern with a period of 2.5 days.

These types of pulsations are not seen with black holes. Rather, they are the signatures of so-called pulsars, rapidly rotating neutron stars. The apparent shifts in the pulsation period are due to the motion of the star in its orbit. Assuming that the pulsar weighs 1.4 times the mass of the Sun (the common size of a pulsar or neutron star), the data imply that the companion star's mass is at least 5.2 times the mass of the Sun.

More information at http://chandra.harvard.edu/photo/2014/m82nu/index.html

-Megan Watzke, CXC

A 'Comet' Lands in Pasadena

A 'Comet' Lands in Pasadena:

The interactive comet sculpture
Add caption
The interactive comet sculpture "Metamorphosis" is on display during the AxS Festival, an arts and sciences celebration in Pasadena, California. Image credit: NASA/JPL-Caltech

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AxS (pronounced axis) is a citywide festival produced by the Pasadena Arts Council that celebrates the California town as the "City of Art and Science." It runs through Oct. 5.

JPL space science-related highlights of the festival include:

"Metamorphosis"
Nine-feet-high and lit from within, this steel sculpture emits a fine water mist and was inspired by the comet which the Rosetta spacecraft is currently orbiting. The sculpture will also be on display at the JPL Open House, Oct. 11 and 12.

"REALSPACE"
Data and imagery from NASA's Curiosity Mars rover, the Dawn mission's exploration of giant asteroid Vesta, and the optical science of light and space are the subjects of various works in this exhibition.

For specific dates, times, locations and other information on all AxS events, visit:
http://axsfestival.org/2014/

For details regarding the free 2014 JPL Open House, see:
http://www.jpl.nasa.gov/news/news.php?release=2014-330

Media Contact

Stephanie L. Smith

Jet Propulsion Laboratory, Pasadena, Calif.

slsmith@jpl.nasa.gov

818-393-5464

2014-337

NASA Holds Teleconference on NuSTAR Discovery

NASA Holds Teleconference on NuSTAR Discovery:

Artist's concept of NuSTAR on orbit. Artist's concept of NuSTAR on orbit. NuSTAR has a 10-m (30') mast that deploys after launch to separate the optics modules (right) from the detectors in the focal plane (left). Image credit: NASA/JPL-Caltech

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NASA will host a news teleconference at 10 a.m. PDT (1 p.m. EDT) Wednesday, Oct. 8, to announce new findings from its Nuclear Spectroscopic Telescope Array (NuSTAR) mission. The results describe an unusual source of X-rays that will leave theorists scratching their heads, but also will help astronomers learn more about how black holes and galaxies are formed.

Details of the findings are under embargo by the journal Nature until 10 a.m. PDT (1 p.m. EDT), Oct. 8.

Participants in the teleconference are:

-- Paul Hertz, director of astrophysics division, NASA Headquarters, Washington

-- Fiona Harrison, NuSTAR principal investigator, California Institute of Technology, Pasadena

-- Matteo Bachetti, astronomer, University of Toulouse, France

-- Jeanette Gladstone, astronomer, University of Alberta, Canada

Audio of the teleconference will be streamed live at:

http://www.nasa.gov/newsaudio

Visuals will be posted at the start of the event at:

http://www.nasa.gov/jpl/nustar/telecon

Audio and supporting visuals will be streamed live at:

http://www.ustream.tv/NASAJPL2

For more information on NuSTAR, visit:

http://www.nasa.gov/nustar

Media Contact

Whitney Clavin Jet Propulsion Laboratory, Pasadena, Calif.

818-354-4673

whitney.clavin@jpl.nasa.gov

Felicia Chou
NASA Headquarters,
Washington
202-358-0257
felicia.chou@nasa.gov

2014-339

NASA Holds Briefing to Discuss Comet Flyby of Mars Observations

NASA Holds Briefing to Discuss Comet Flyby of Mars Observations:

Artist's concept of comet Siding Spring (C/2013 A1) heading toward Mars. Artist's concept of comet Siding Spring (C/2013 A1) heading toward Mars. Image Credit: NASA

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NASA will host a briefing at 11 a.m. PDT (2 p.m. EDT) Thursday, Oct. 9, to outline the space and Earth-based assets that will have extraordinary opportunities to image and study a comet from relatively close range to Mars on Sunday, Oct. 19.

The briefing will be held at NASA Headquarters' and broadcast live on NASA Television and the agency's website.

Comet C/2013 A1 Siding Spring will miss Mars by only about 88,000 miles (139,500 kilometers). That is less than half the distance between Earth and its moon and less than one-tenth the distance of any known comet flyby of Earth. The comet's nucleus will come closest to Mars at about 11:27 a.m. PDT (2:27 p.m. EDT), hurtling at about 126,000 mph (56 kilometers per second), relative to Mars.

The concerted campaign of observations by multiple spacecraft at Mars and by numerous NASA assets is directed at the comet and its effect on the Martian atmosphere. The observations of the comet may yield fresh clues to our solar system's earliest days more than four billion years ago.

Panelists include:

- Jim Green, director, Planetary Science Division (PSD), NASA Headquarters, Washington

- Kelly Fast, program scientist, PSD

- Carey Lisse, senior astrophysicist, Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland

- Padma Yanamandra-Fisher, senior research scientist, Space Science Institute, Rancho Cucamonga Branch, California

The public may ask questions on social media using the hashtag #askNASA.

The news conference will be available live and archived on:

http://www.ustream.tv/nasajpl

For more about the comet, visit:

http://mars.nasa.gov/comets/sidingspring

For NASA Television downlink information, scheduling information and streaming video, visit: http://www.nasa.gov/nasatv

Media Contact

D.C. Agle/Guy Webster

Jet Propulsion Laboratory, Pasadena, Calif.

818-393-9011/818-354-6278

agle@jpl.nasa.gov/guy.webster@jpl.nasa.gov

Dwayne Brown

NASA Headquarters, Washington

202-358-1726

dwayne.c.brown@nasa.gov

2014-340

Sunday, October 5, 2014

Glorious Global 3-D Mars from ISRO’s MOM and ESA’s Rosetta

Glorious Global 3-D Mars from ISRO’s MOM and ESA’s Rosetta:

3-D image of Mars generated from multiple pictures acquired by Mars Color Camera on-board Mars Orbiter Spacecraft on Sept 28, 2014. Credit: ISRO


3-D image of Mars generated from multiple pictures acquired by Mars Color Camera on-board Mars Orbiter Spacecraft on Sept 28, 2014. 3-D red/blue glasses required. Credit: ISRO
Here’s another breathtakingly glorious view from India’s Mars Orbiter Mission (MOM) – her first global 3-D portrait of her new home careening around the Red Planet.

MOM is India’s first deep space voyager to explore beyond the confines of her home planet’s influence and just successfully arrived at the Red Planet after the “history creating” orbital insertion maneuver on Sept. 23/24 following a ten month journey.

This newly released 3-D view from MOM expands upon the initial 2-D global color view of Mars released by the Indian Space Research Organization (ISRO), India’s space agency. See below and detailed in my earlier story – here.

The 3-D image was generated from multiple pictures acquired by MOM’s on-board Mars Color Camera on Sept 28, 2014, from the very high altitude of approximately 74,500 kilometers as the spacecraft orbits Mars.

ISRO's Mars Orbiter Mission captures spectacular portrait of the Red Planet and swirling dust storms with the on-board Mars Color Camera from an altitude of 74500 km on Sept. 28, 2014. Credit: ISRO


ISRO’s Mars Orbiter Mission captures spectacular portrait of the Red Planet and swirling dust storms with the on-board Mars Color Camera from an altitude of 74,500 km on Sept. 28, 2014. Credit: ISRO
The images were taken by the tri-color camera as MOM swooped around the Red Planet in a highly elliptical orbit whose nearest point to Mars (periapsis) is at 421.7 km and farthest point (apoapsis) at 76,993.6 km, according to ISRO.

Therefore, the 3-D Red Planet portrait was captured nearly at apoapsis. And being three dimensional, it gives a stereo sense of the huge dust storm swirling over a large swath of the planet’s Northern Hemisphere set against the blackness of space.

Below right is the southern polar ice cap. To see the 3-D effect, whip out your handy pair of left-eye red, right-eye blue color anaglyph glasses.

And while we’re on the subject of spacely 3-D, it’s worth noting that another of humanity’s ground breaking probes currently making news – ESA’s comet hunting Rosetta probe – likewise snapped a glorious 3-D view of Mars way back in 2007, during the brief, but critical, gravity assist slingshot maneuver that flung Rosetta along her vast 10 year path through interplanetary space.

So by way of comparison let’s take a trip down memory lane and be sure to look back at Rosetta’s global 3-D Martian views (below) taken by the high resolution OSIRIS camera on 24 February 2007 at 19:28 CET from a distance of about 240,000 kilometers.

Mars 3-D anaglyph (black & white) taken by ESA’s Rosetta spacecraft during Mars flyby on 24 February 2007 from a distance of about 240 000 km. Image resolution is about 5 km. Credit: MPS for OSIRIS Team MPS/UPD/LAM/ IAA/ RSSD/ INTA/ UPM/ DASP/ IDA


Mars 3-D anaglyph (black & white) taken by ESA’s Rosetta spacecraft during Mars flyby on 24 February 2007 from a distance of about 240,000 km. Image resolution is about 5 km. Credit: MPS for OSIRIS Team MPS/UPD/LAM/ IAA/ RSSD/ INTA/ UPM/ DASP/ IDA
The Rosetta team created both color and black & white 3-D views of Mars.

Mars 3-D anaglyph (color) taken by ESA’s Rosetta spacecraft during Mars flyby on 24 February 2007 from a distance of about 240 000 km. Image resolution is about 5 km. Credit: MPS for OSIRIS Team MPS/UPD/LAM/ IAA/ RSSD/ INTA/ UPM/ DASP/ IDA


Mars 3-D anaglyph (color) taken by ESA’s Rosetta spacecraft during Mars flyby on 24 February 2007 from a distance of about 240,000 km. Image resolution is about 5 km. Credit: MPS for OSIRIS Team MPS/UPD/LAM/ IAA/ RSSD/ INTA/ UPM/ DASP/ IDA
And be sure to check out Rosetta’s 2-D true color view showing a different swatch of the Red Planet compared to MOM, along with a more expansive view of the southern polar ice cap.

The first true-colour image of Mars from ESA’s Rosetta generated using the OSIRIS orange (red), green and blue colour filters. The image was acquired on 24 February 2007 at 19:28 CET from a distance of about 240 000 km; image resolution is about 5 km/pixel. Credit: MPS for OSIRIS Team MPS/UPD/LAM/ IAA/ RSSD/ INTA/ UPM/ DASP/ IDA


The first true-color image of Mars from ESA’s Rosetta generated using the OSIRIS orange (red), green and blue color filters. The image was acquired on 24 February 2007 at 19:28 CET from a distance of about 240,000 km; image resolution is about 5 km/pixel. Credit: MPS for OSIRIS Team MPS/UPD/LAM/ IAA/ RSSD/ INTA/ UPM/ DASP/ IDA
The $73 million MOM mission is expected to last at least six months.

MOM’s success follows closely on the heels of NASA’s MAVEN orbiter which also successfully achieved orbit barely two days earlier on Sept. 21 and could last 10 years or more.



Tagged as: Comet 67P, Comet 67P/Churyumov–Gerasimenko, esa, european space agency, indian space program, Indian Space Research Organization, ISRO, Mars, Mars 3 D, Mars Orbiter Mission, MOM, OSIRIS Camera, red planet, rosetta

Friday, October 3, 2014

ISRO and NASA Ink Deal to Collaborate on Red Planet and Home Planet Science Missions

ISRO and NASA Ink Deal to Collaborate on Red Planet and Home Planet Science Missions:

The NASA-ISRO Synthetic Aperture Radar (NISAR) mission, targeted to launch in 2020, will make global measurements of the causes and consequences of a variety of land surface changes on Earth. Image Credit: NASA


The NASA-ISRO Synthetic Aperture Radar (NISAR) mission, targeted to launch in 2020, will make global measurements of the causes and consequences of a variety of land surface changes on Earth. Image Credit: NASA
ISRO and NASA have inked a deal to collaborate on future missions to jointly explore the Red Planet and our Home Planet hot on the heels of ISRO’s wildly successful Mars Orbiter Mission (MOM), India’s first ever interplanetary voyager to explore Mars.

NASA Administrator Charles Bolden and K. Radhakrishnan, chairman of the Indian Space Research Organisation (ISRO), signed an agreement to collaborate on future science missions to explore Mars as well as to build and launch a joint NASA-ISRO mission to observe Earth.

The leaders of NASA and ISRO met in Toronto, Canada on Tuesday, Sept. 30 and “signed two documents to launch a NASA-ISRO satellite mission to observe Earth and establish a pathway for future joint missions to explore Mars,” according to a NASA statement.

Bolden and Rao met at the International Astronautical Congress underway in Toronto.

ISRO's Mars Orbiter Mission captures the limb of Mars with the Mars Color Camera from an altitude of 8449 km soon after achieving orbit on Sept. 23/24, 2014. . Credit: ISRO


ISRO’s Mars Orbiter Mission captures the limb of Mars with the Mars Color Camera from an altitude of 8449 km soon after achieving orbit on Sept. 23/24, 2014. . Credit: ISRO
They signed one agreement defining each agency’s responsibilities for the joint NASA-ISRO Synthetic Aperture Radar (NISAR) mission, targeted to launch in 2020. NISAR will make global measurements of the causes and consequences of land surface changes.

The second agreement “establishes a NASA-ISRO Mars Working Group to investigate enhanced cooperation between the two countries in Mars exploration.”

“The signing of these two documents reflects the strong commitment NASA and ISRO have to advancing science and improving life on Earth,” said NASA Administrator Charles Bolden, in a NASA statement.

“This partnership will yield tangible benefits to both our countries and the world.”

NISAR will be the first Earth observing mission to be equipped two different synthetic aperture radar (SAR) frequencies (L-band and S-band) – one each from NASA and ISRO.

NASA will also provide “the high-rate communication subsystem for science data, GPS receivers, a solid state recorder, and a payload data subsystem.”

ISRO will provide the spacecraft bus and launch vehicle.

The radars will be able to measure subtle changes in Earth’s surface of less than a centimeter across stemming from the flow of glaciers and ice sheets as well as earthquakes and volcanoes.

Regarding Mars, the first subject the joint working group will tackle will be to coordinate observations from each nation’s recently arrived Mars orbiters – ISRO’s MOM and NASA’s MAVEN. They will also examine areas of future collaboration on surface rovers and orbiters.

“NASA and Indian scientists have a long history of collaboration in space science,” said John Grunsfeld, NASA Associate Administrator for Science.

“These new agreements between NASA and ISRO in Earth science and Mars exploration will significantly strengthen our ties and the science that we will be able to produce as a result.”

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

MAVEN is NASA’s next Mars orbiter and launched on Nov. 18, 2014 from Cape Canaveral, Florida. It will study the evolution of the Red Planet’s atmosphere and climate. Universe Today visited MAVEN inside the clean room at the Kennedy Space Center. With solar panels unfurled, this is exactly how MAVEN looks when flying through space and circling Mars and observing Comet Siding Spring. Credit: Ken Kremer/kenkremer.com


MAVEN is NASA’s next Mars orbiter and launched on Nov. 18, 2014, from Cape Canaveral, Florida. It will study the evolution of the Red Planet’s atmosphere and climate. Universe Today visited MAVEN inside the clean room at the Kennedy Space Center. With solar panels unfurled, this is exactly how MAVEN looks when flying through space and circling Mars and observing Comet Siding Spring. Credit: Ken Kremer/kenkremer.com


About 

Dr. Ken Kremer is a speaker, scientist, freelance science journalist (Princeton, NJ) and photographer whose articles, space exploration images and Mars mosaics have appeared in magazines, books, websites and calanders including Astronomy Picture of the Day, NBC, BBC, SPACE.com, Spaceflight Now and the covers of Aviation Week & Space Technology, Spaceflight and the Explorers Club magazines. Ken has presented at numerous educational institutions, civic & religious organizations, museums and astronomy clubs. Ken has reported first hand from the Kennedy Space Center, Cape Canaveral and NASA Wallops on over 40 launches including 8 shuttle launches. He lectures on both Human and Robotic spaceflight - www.kenkremer.com. Follow Ken on Facebook and Twitter
Tagged as: Climate Change, Earth science, indian space program, Indian Space Research Organization, ISRO, Mars, Mars MAVEN, Mars Orbiter Mission, MAVEN, MOM, NASA, NISAR, red planet