How Will Aliens Find Us?

How Will Aliens Find Us?

Trying to keep a low profile, to prevent the aliens from invading? Bad news. Life has actually been broadcasting our existence to the Universe for hundreds of millions of years.

Have you heard these crazy plans to send signals out into deep space? What if evil aliens receive them, come steal our water, enslave, eat, and use us as guinea pigs for their exotic probulators. How we could stop these madmen from announcing our presence to the galaxy? A petition on whitehouse.gov? An all caps Facebook group? An all pusheen protest? Somebody call Reddit, they’ll know what to do.

If this is a worry for you and your friends, I’ve got bad news, or possibly good news depending on which side you come down on. We’ve already been broadcasting our existence for hundreds of millions of years. If aliens wanted to know we were here, all they needed to do was look through their telescopes.

We’re in a golden age of extrasolar planet discovery, recently crossing the thousand-planets-mark thanks to Kepler and other space telescopes. With all these amazing planetary candidates, our next challenge will be to study the atmospheres of these planets, searching for evidence of life. There are chemicals which are naturally occurring, like water and carbon dioxide, and there are substances that can only be present if some source is replenishing them. Methane, for example, would only last only few hundred years in the atmosphere if it wasn’t for farting cows and colonies of bacteria eating dead things.

If we see methane or oxygen in the atmosphere of an extrasolar planet, we’ll have a good idea there’s life there. And if we see the byproducts of an industrial civilization, like air pollution, we can pinpoint exactly where they are in their technical development. It will work for us, and that means it would work for aliens.

For the first few billion years, oxygen was toxic. But then cyanobacteria evolved photosynthesis and figured out how to work with oxygen more than 2.4 billion years ago. This is known as the Great Oxidation Event.

For the first billion years, all this biologically generated oxygen was absorbed by the oceans and the rocks. Once those oxygen sinks filled up, oxygen began accumulating in the atmosphere. By 500 million years ago, there was enough oxygen in the atmosphere to support the kind of breathing we do today. And this much oxygen would have been obvious to the aliens. They would have known that life had evolved here on Earth, and they could have sent out their berserker spaceships to steal our water and made us watch while they ate all our small rodents.

If the aliens waited, we would have given them more signs. The Industrial Revolution began in the mid 1700’s. And this time, it was humans that filled the atmosphere with the pollution of our industrial processes. Again, aliens watching the planet with their space telescopes would know the moment we became a technological civilization.

The innermost antennae along the north arm of the Very Large Array, superimposed upon a false-color representation of a radio (red) and optical (blue) image of the radio galaxy 3C31. Image courtesy of NRAO/AUI
The innermost antennae along the north arm of the Very Large Array, superimposed upon a false-color representation of a radio (red) and optical (blue) image of the radio galaxy 3C31. Image courtesy of NRAO/AUI

In the 20th century, we harnessed the power of radio transmissions, and began sending our messages out into space. For about a hundred years now, our transmissions have been expanding into a bubble of space. And so, any aliens listening within this expanding sphere of space might have a chance of hearing us. They know we’re here, and they know some of us really like Ke$ha.

And finally, for the last few decades, a few groups have tried broadcasting messages using our powerful radio telescopes directly at other stars. These messages haven’t gotten very far, but I honestly wouldn’t worry. Life itself gave away our position hundreds of millions of years ago. And life will help us find other civilizations, if they’re out there.

What do you think? Should we turn out the lights and pretend like we’re not home or keep on actively broadcasting our presence to the Universe? Tell us what you think we should do in the comments below.

NASA Offers $35,000 In Prizes For Citizen Scientists To Help Find Asteroids

Hypothetical astronaut mission to an asteroid. Credit: NASA Human Exploration Framework Team

Fancy yourself an asteroid hunter? There’s $35,000 available in prizes for NASA’s new Asteroid Data Hunter contest series, which will be awarded to citizen scientists who develop algorithms that could be used to search for asteroids.

Here’s where you can apply for the contest, which opens March 17 and runs through August. And we have a few more details about this joint venture with Planetary Resources Inc. below.

“The Asteroid Data Hunter contest series challenges participants to develop significantly improved algorithms to identify asteroids in images captured by ground-based telescopes,” NASA stated. “The winning solution must increase the detection sensitivity, minimize the number of false positives, ignore imperfections in the data, and run effectively on all computer systems.”

We got a sharp reminder of the danger of asteroids to Earth in February 2013 when a meteor slammed into the atmosphere above Chelyabinsk, Russia, causing damage and hundreds of injuries. Meanwhile, NASA is working on a project to redirect an asteroid closer to Earth for astronauts to explore, a concept that has funding allocated in their 2015 budget request to Congress.

In November, NASA announced that Planetary Resources (the company best known for the “selfie” space telescope) is going to work on “crowdsourced software solutions” with NASA-funded data to make it easier to find asteroids and other near-Earth objects.

Rise And Shine! Rosetta’s Comet Emerges From Behind Sun, Much Brighter Than Before

Artist's impression (not to scale) of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov–Gerasimenko. Credit: ESA–C. Carreau/ATG medialab.

After four months behind the sun from Earth’s perspective, comet 67P/Churyumov-Gerasimenko is back in view — and brighter than ever! New pictures of the comet reveal it is 50 percent brighter than the last images available from October 2013. You can see the result below the jump.

“The new image suggests that 67P is beginning to emit gas and dust at a relatively large distance from the Sun,” stated Colin Snodgrass, a post-doctoral researcher at the Max Planck Institute for Solar System Research in Germany. Snodgrass added that this confirms previous work he and his colleagues did showing that in March 2014, the comet’s activity could be seen from Earth.

Pictures were taken with the European Southern Observatory’s Very Large Telescope from 740 million kilometers (460 million miles) away. As you can see in the image below, several exposures were taken to obtain the fainter comet. And we know that scientists are eager to take a closer look with Rosetta.

Comet 67P/Churyumov-Gerasimenko on images obtained Feb. 28th, 2014 with the Very Large Telescope. Left: Several exposures were obtained of the faint comet, and superimposed upon each other, making stars appear as streaks. Right: The comet in an image processed to remove the stars. Credit: MPS/ESO
Comet 67P/Churyumov-Gerasimenko on images obtained Feb. 28th, 2014 with the Very Large Telescope. Left: Several exposures were obtained of the faint comet, and superimposed upon each other, making stars appear as streaks. Right: The comet in an image processed to remove the stars. Credit: MPS/ESO

In January, the Rosetta spacecraft woke up after 31 months of hibernation (a little later than expected, but still healthy as ever.) It’s en route to meet up with the comet in August and will stay alongside it at least until 2015’s end. The next major step is to wake up its lander, Philae, which will happen later this month.

Should all go to plan, Philae will make a daring landing on the comet in November to get an up-close view of the activity as the comet flies close to the sun. You can read more details in this past Universe Today story.

Source: Max Planck Institute for Solar System Research

Historic SpaceX Landing Leg Rocket and Dragon Bound for Station Check Fires Engines at T Minus 1 Week

A SpaceX Falcon 9 rocket with Dragon cargo capsule bound for the ISS launched from Space Launch Complex 40 at Cape Canaveral, FL. File photo. Credit: Ken Kremer/kenkremer.com

The historic blast off of the first SpaceX rocket equipped with ‘landing legs’ and also carrying a private Dragon cargo vessel bound for the Space Station is now slated for March 16 following a short and “successful” hot fire check test of the first stage engines on Saturday, March 8.

It’s T Minus 1 week to lift off !

The brief two second ignition of all nine upgraded Merlin 1D engines powering the first stage of SpaceX’s next generation, commercial Falcon 9 rocket at the end of a simulated countdown is a key test required to clear the way for next Sunday’s planned night time lift off at 4:41 a.m. EDT from Space Launch Complex 40 at Cape Canaveral Air Force Station in Florida.

“Falcon 9 and Dragon conducted a successful static fire test in advance of next week’s CRS-3 launch to station!” SpaceX announced today.

The primary goal of the unmanned SpaceX CRS-3 mission is to deliver over 5000 pounds of science experiments, gear and supplies loaded inside Dragon to the six person crew living and working aboard the International Space Station (ISS) flying in low Earth orbit under NASA’s Commercial Resupply Services (CRS) contract.

“In this final major preflight test, Falcon 9’s 9 first-stage engines were ignited for 2 seconds while the vehicle was held down to the pad,” said SpaceX.

All four landing legs now mounted on Falcon 9 rocket being processed inside hanger at Cape Canaveral, FL for Mar 16 launch.  Credit: SpaceX/Elon Musk
All four landing legs now mounted on Falcon 9 rocket being processed inside hanger at Cape Canaveral, FL for Mar 16 launch. Credit: SpaceX/Elon Musk

The static hot firing is a full up assessment of the rocket, engines, propellant loading and countdown procedures leading to a launch. The engines typically fire for a barely a few seconds.

SpaceX engineers will evaluate the engine firing to ensure all systems are ready for launch.

This commercial Falcon 9 rocket is equipped for the first time with a quartet of landing legs, Elon Musk, the company’s founder and CEO, announced recently as outlined in my story – here.

The attachment of landing legs to the first stage of SpaceX’s next-generation Falcon 9 rocket counts as a major step towards the firm’s future goal of building a fully reusable rocket.

The eventual goal is to accomplish a successful first stage touchdown by the landing legs on solid ground back at Cape Canaveral, Florida.

For this Falcon 9 flight, the rocket will sprout legs for a controlled soft landing in the Atlantic Ocean guided by SpaceX engineers.

Extensive work and testing remains to develop and refine the technology before a land landing will be attempted by the company.

“F9 will continue to land in the ocean until we prove precision control from hypersonic thru subsonic regimes,” Musk says.

1st stage of SpaceX Falcon 9 rocket equipped with landing legs and now scheduled for launch to the International Space Station on March 16, 2014 from Cape Canaveral, FL. Credit: SpaceX/Elon Musk
1st stage of SpaceX Falcon 9 rocket equipped with landing legs and now scheduled for launch to the International Space Station on March 16, 2014 from Cape Canaveral, FL. Credit: SpaceX/Elon Musk

SpaceX hopes the incorporation of landing legs will one day lead to cheaper, reusable boosters that can be manufactured at vastly reduced cost.

The March 16 launch will be the fourth overall for the next generation Falcon 9 rocket, but the first one capped with a Dragon and heading to the massive orbital lab complex.

Falcon 9 and Dragon static fire test on March 8, 2014. Credit: SpaceX
Falcon 9 and Dragon static fire test on March 8, 2014. Credit: SpaceX

Three prior launches of the more powerful Falcon 9 lofting commercial telecom satellites in September and December 2013 and January 2014 were all successful and paved the way for SpaceX’s new mission to the ISS.

And this Dragon is loaded with the heaviest manifest yet.

The research cargo includes 100 protein crystal experiments that will allow scientists to observe the growth of crystals in zero-G.

In the absence of gravity, the crystals will hopefully grow to much larger sizes than here on Earth and afford scientists new insights into designing and developing new drugs and pesticides.

SpaceX is under contract to NASA to deliver 20,000 kg (44,000 pounds) of cargo to the ISS during a dozen Dragon cargo spacecraft flights over the next few years at a cost of about $1.6 Billion.

Next Generation SpaceX Falcon 9 rocket blasts off with SES-8 communications satellite on Dec. 3, 2013 from Pad 40 at Cape Canaveral, FL. Credit: Ken Kremer/kenkremer.com
Next Generation SpaceX Falcon 9 rocket blasts off with SES-8 communications satellite on Dec. 3, 2013 from Pad 40 at Cape Canaveral, FL. Credit: Ken Kremer/kenkremer.com

To date SpaceX has completed two operational cargo resupply missions. The last flight dubbed CRS-2 blasted off a year ago on March 1, 2013 atop the initial version of the Falcon 9 rocket.

If the launch takes place as planned on March 16, Dragon will rendezvous and dock at the Earth facing port on the station’s Harmony module, after a two day orbital chase, on March 18.

The Harmony port was recently vacated by the Orbital Sciences built Cygnus cargo spacecraft to make way for Dragon.

Both the Dragon and Cygnus resupply spacecraft were privately developed with seed money from NASA in a public-private partnership in order to restore the cargo up mass capability the US completely lost following the retirement of NASA’s space shuttle orbiters in 2011.

The Dragon docking will take place a few days after Monday’s (March 10) scheduled departure of three crew members aboard a Russian Soyuz capsule.

Watch the Soyuz leave live on NASA TV.

The departure of Russian cosmonauts Oleg Kotov and Sergey Ryazanskiy along with NASA astronauts Mike Hopkins marks the end of Expedition 38 and the beginning of Expedition 39.

It also leaves only a three person crew on board to greet the Dragon.

The Soyuz return to Earth comes amidst the ongoing Crimean crisis as tensions continue to flare between Russian, Ukraine and the West.

American and station partner astronauts are 100% dependent on Russia’s three seat Soyuz capsule and rocket for rides to the ISS and back.

Expedition 38 crew members proudly sport their national flags in this March 2014 picture from the International Space Station. Pictured (clockwise from top center) are Russian cosmonaut Oleg Kotov, commander; Japan Aerospace Exploration Agency astronaut Koichi Wakata, Russian cosmonaut Sergey Ryazanskiy, NASA astronauts Rick Mastracchio and Mike Hopkins, and Russian cosmonaut Mikhail Tyurin, all flight engineers. Credit: NASA
Expedition 38 crew members proudly sport their national flags in this March 2014 picture from the International Space Station. Pictured (clockwise from top center) are Russian cosmonaut Oleg Kotov, commander; Japan Aerospace Exploration Agency astronaut Koichi Wakata, Russian cosmonaut Sergey Ryazanskiy, NASA astronauts Rick Mastracchio and Mike Hopkins, and Russian cosmonaut Mikhail Tyurin, all flight engineers. Credit: NASA

Command of the station was passed today from Oleg Kotov to the Japan Aerospace Exploration Agency astronaut Koichi Wakata.

With the start of Expedition 39, Wakata thus becomes the first Japanese astronaut to command the ISS.

Wakata and NASA astronaut Rick Mastracchio with use the stations Canadarm 2 to grapple and berth Dragon to its docking port.

SpaceX Falcon 9/Dragon  CRS-3 mission patch. Credit: SpaceX
SpaceX Falcon 9/Dragon CRS-3 mission patch. Credit: SpaceX

Dragon is due to stay at station for about three weeks until April 17.

Then it will undock and set course for a parachute assisted splash down in the Pacific Ocean off the coast of Baja California.

For the return to Earth, Dragon will be packed with more than 3,500 pounds of highly valuable experiment samples accumulated from the crews onboard research as well as assorted equipment and no longer need items.

Stay tuned here for Ken’s continuing SpaceX, Orbital Sciences, commercial space, Orion, Chang’e-3, LADEE, Mars rover, MAVEN, MOM and more planetary and human spaceflight news. Learn more at Ken’s upcoming presentations at the NEAF astro/space convention on April 12/13.

And watch for Ken’s upcoming SpaceX launch coverage at Cape Canaveral & the Kennedy Space Center press site.

Ken Kremer

Watch a Bright Star Disappear Behind the Moon Monday Night

Lambda Geminorum at 10:43 p.m. March 11 just two minutes before disappearing behind the moon as seen from Minneapolis, Minn. US. Stellarium

Ever dabbled in the occult? You’ll have your chance Monday night March 10 when the waxing gibbous moon glides in front of the star Lambda Geminorum for much of North America, occulting it from view for an hour or more. Occultations of stars by the moon happens regularly but most go unnoticed by casual skywatchers. Lambda is an exception because it’s one of the brighter stars that happens to lie along the moon’s path. Shining at magnitude +3.6, any small telescope and even a pair of 10×50 or larger binoculars will show it disappear along the dark edge of the moon. 

Map showing where the occulation of Lambda Gem will be visible. Credit: International Occultation Timing Assn. (IOTA)
Map showing where the disappearance (right half of tube-like figure) and reappearance of Lambda Gem will be visible. Credit: International Occultation Timing Assn. (IOTA)

With a telescope you can comfortably watch the star creep up to the moon’s edge and better anticipate the moment of its disappearance. The fun starts a few minutes before the impending black out when the moon, speeding along its orbit at some 2,280 mph (3,700 km/hr),  draws very close to the star. During the final minute, Lambda may seem to hover forever at the moon’s invisible dark limb, and then – PFFFT – it’s gone! Whether you’re looking through telescope or binoculars, the star will blink out with surprising suddenness because the moon lacks an atmosphere.

Disappearance and reappearance seen from Minneapolis, Minn. Monday night. I've lightened the moon so you can see the dark limb. You'll likely not see this edge in a telescope because of glare. Stellarium
Disappearance and reappearance seen from Minneapolis, Minn. Monday night. I’ve lightened the moon so you can see the dark limb. You’ll likely not see this edge in a telescope because of glare. Stellarium

If there was air up there, Lambda would gradually dim and disappear. Even without special instruments, early astronomers could be certain the moon had little if anything to protect it from the vacuum of space by observing occultations.

As the moon moves approximately its own diameter in an hour, you can watch Lambda re-emerge along the bright limb roughly an hour later, though its return will lack the drama and contrast of a dark limb disappearance. While occultations allow us to see how swiftly the moon moves in real time as well as provide information on its atmosphere or lack thereof, real science can be done, too.


Planets also are occasionally occulted by the moon. Time lapse of Venus’ disappearance on May 16, 2010

Observers along the occultation boundary in the southern U.S. can watch the star pop in and out of view as it’s alternately covered and uncovered by lunar peaks jutting from the moon’s limb. Before spacecraft thoroughly mapped the moon, careful timings made during these “grazing occultations” helped astronomers refine the profile of the moon’s limb as well as determine elevations of peaks and crater walls in polar regions. They can still be useful for refining a star’s position and motion in the sky.

The moon’s limb can also be used much like a doctor’s scalpel  to split unsuspected  double stars that otherwise can’t be resolved by direct observations. Take Lambda Gem for instance. We’ve known for a long time that it totes around a magnitude +10.7 companion star 10 arc seconds to its north-northeast,  but previous occultations of the star have revealed an additional companion only a few hundredths of an arc second away orbiting the bright Lambda primary. The star plays a game of hide-and-seek, visible during some occultations but not others. Estimated by some as one magnitude fainter than Lambda, keep an eye out for it Monday night in the instant after Lambda goes into hiding.


Lunar occultation and reappearance of Antares Oct. 21, 2009

I watched just such a  “two-step” disappearance of Antares and it fainter companion some years back. With brilliant Antares briefly out of view behind the moon’s limb, I easily spotted its magnitude +5.4 companion just 2.5 arc seconds away – an otherwise very difficult feat at my northern latitude.

Want to know more about things that disappear (and reappear) in the night? Make a visit to the International Occultation Timing Association’s website where you’ll find lists of upcoming events, software and how to contribute your observations. If you’re game for Monday night’s occultation, click HERE for a list of cities and times. Remember that the time show is Universal or Greenwich Time. Subtract 4 hours for Eastern Daylight, 5 for Central, 6 for Mountain and 7 for Pacific.  Wishing you clear skies as always!

NASA Lunar Orbiter snaps Spectacular Images of Yutu Moon Rover driving around Chang’e-3 Lander

Yutu rover drives around Chang’e-3 lander – from Above And Below. Composite view shows China’s Yutu rover and tracks driving in clockwise direction around Chang’e-3 lander from Above And Below (orbit and surface). The Chang’e-3 timelapse lander color panorama (bottom) and orbital view (top) from NASA’s LRO orbiter shows Yutu rover after it drove down the ramp to the moon’s surface and began driving around the landers right side, passing by craters and heading south on Lunar Day 1. It then moved northwest during Lunar Day 2. Arrows show Yutu’s positions over time. Credit: CNSA/NASA/Ken Kremer/Marco Di Lorenzo/Mark Robinson

Yutu rover drives around Chang’e-3 lander – from Above And Below
Composite view shows China’s Yutu rover and tracks driving in clockwise direction around Chang’e-3 lander from Above And Below (orbit and surface). The Chang’e-3 timelapse lander color panorama (bottom) and orbital view (top) from NASA’s LRO orbiter shows Yutu rover after it drove down the ramp to the moon’s surface and began driving around the landers right side, passing by craters and heading south on Lunar Day 1. It then moved northwest during Lunar Day 2. Arrows show Yutu’s positions over time.
Credit: CNSA/NASA/Ken Kremer/Marco Di Lorenzo/Mark Robinson
See below more mosaics and LRO imagery
Story updated[/caption]

The powerful telescopic camera aboard NASA’s Lunar Reconnaissance Orbiter (LRO) has captured spectacular new images detailing the traverse of China’s Yutu moon rover around the landing site during its first two months exploring the Moon’s pockmarked grey terrain.

The newly released high resolution LRO images even show Yutu’s tracks cutting into the lunar surface as the world famous Chinese robot drove in a clockwise direction around the Chang’e-3 lander that delivered it to the ground in mid-December 2013.

You can precisely follow Yutu’s movements over time – from ‘above and below’ – in our new composite view (shown above) combining the latest LRO image with our timelapse mosaic showing the rover’s history making path from the touchdown point last December to today’s location.

Yutu is China’s first ever Moon rover and successfully accomplished a soft landing on the Moon on Dec. 14, 2013, piggybacked atop the Chang’e-3 mothership lander.

Barely seven hours after touchdown, the six wheeled moon buggy drove down a pair of ramps onto the desolate gray plains of the lunar surface at Mare Imbrium (Sea of Rains) covered by volcanic material.

LROC February 2014 image of Chang'e 3 site. Blue arrow indicates Chang'e 3 lander; yellow arrow points to Yutu (rover); and white arrow marks the December location of Yutu. Yutu's tracks can be followed clockwise around the lander to its current location. Image width 200 meters (about 656 feet).  Credit:  NASA/Goddard/Arizona State University
LROC February 2014 image of Chang’e 3 site. Blue arrow indicates Chang’e 3 lander; yellow arrow points to Yutu (rover); and white arrow marks the December location of Yutu. Yutu’s tracks can be followed clockwise around the lander to its current location. Image width 200 meters (about 656 feet). Credit: NASA/Goddard/Arizona State University

Altogether three images of the rover and lander have been taken to date by the Lunar Reconnaissance Orbiter Camera (LROC) aboard LRO – specifically the hi res narrow angle camera (NAC).

The LROC NAC images were captured on Dec. 25, 2013, Jan. 21, 2014 and Feb. 17, 2014 as LRO soared overhead.

The four image LRO composite below includes a pre-landing image taken on June 30, 2013.

Four LROC NAC views of the Chang'e 3 landing site. A) before landing, June 30, 2013 B) after landing, Dec. 25, 2013 C) Jan. 21, 2014 D) Feb. 17, 2014 Width of each image is 200 meters (about 656 feet). Follow Yutu's path clockwise around the lander in "D."  Credit: NASA/Goddard/Arizona State University
Four LROC NAC views of the Chang’e 3 landing site. A) before landing, June 30, 2013 B) after landing, Dec. 25, 2013 C) Jan. 21, 2014 D) Feb. 17, 2014 Width of each image is 200 meters (about 656 feet). Follow Yutu’s path clockwise around the lander in “D.” Credit: NASA/Goddard/Arizona State University

Since the solar incidence angles were different, the local topography and reflectance changes between images showing different levels of details.

“In the case of the Chang’e 3 site, with the sun higher in the sky one can now see the rover Yutu’s tracks (in the February image),” wrote Mark Robinson, Principal Investigator for the LROC camera in an LRO update.

The solar powered rover and lander can only operate during periods of lunar daylight, which last 14 days each.

During each lunar night, they both must power down and enter hibernate mode since there is no sunlight available to generate power and no communications are possible with Earth.

Here is a gif animation from the NASA LRO team combining all four LROC images.

Four views of the Chang'e 3 landing site from before the landing until Feb. 2014. Credit: NASA/GSFC/Arizona State University
Four views of the Chang’e 3 landing site from before the landing until Feb. 2014. Credit: NASA/GSFC/Arizona State University

During Lunar Day 1, Yutu drove down the landers ramps and moved around the right side in a clockwise direction.

By the end of the first lunar day, Yutu had driven to a position about 30 meters (100 feet) south of the Chang’e-3 lander, based on the imagery.

See our complete 360 degree timelapse color panorama from Lunar Day 1 herein and at NASA APOD on Feb. 3, 2014 – assembled by Marco Di Lorenzo and Ken Kremer.

360-degree time-lapse color panorama from China’s Chang’e-3 lander. This new 360-degree time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at five different positions, including passing by crater and heading south and away from the Chang’e-3 lunar landing site forever during its trek over the Moon’s surface at its landing site from Dec. 15-22, 2013 during the 1st Lunar Day. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com.  See our Yutu timelapse pano at NASA APOD Feb. 3, 2014: http://apod.nasa.gov/apod/ap140203.htm
360-degree time-lapse color panorama from China’s Chang’e-3 lander. This new 360-degree time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at five different positions, including passing by crater and heading south and away from the Chang’e-3 lunar landing site forever during its trek over the Moon’s surface at its landing site from Dec. 15-22, 2013 during the 1st Lunar Day. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com. See our Yutu timelapse pano at NASA APOD Feb. 3, 2014: http://apod.nasa.gov/apod/ap140203.htm

After awakening for Lunar Day 2, Yutu then moved northwest and parked about 17 meters (56 feet) southwest of the lander, according to Robinson.

By comparing the Janaury and February images “it is apparent that Yutu did not move appreciably from the January location,” said Robinson.

At this moment Yutu and the companion Chang’e-3 lander are sleeping through their 3rd Lunar Night.

They entered hibernation mode on Feb. 22 and Feb. 23, 2014 respectively.

Hopefully both probes will awaken from their slumber sometime in the next week when the Moon again basks in daylight glow to begin a 4th day of lunar surface science operations.

“We all wish it would be able to wake up again,” said Ye Peijian, chief scientist of the Chang’e-3 program, according to CCTV, China’s state run broadcaster.

However, the hugely popular ‘Yutu’ rover is still suffering from an inability to maneuver its life giving solar panels. It is also unable to move – as I reported here.

The 140 kg rover is now nearing its planned 3 month long life expectancy on a moon roving expedition to investigate the moon’s surface composition and natural resources.

Chang’e-3/Yutu Timelapse Color Panorama  This newly expanded timelapse composite view shows China’s Yutu moon rover at two positions passing by crater and heading south and away from the Chang’e-3 lunar landing site forever about a week after the Dec. 14, 2013 touchdown at Mare Imbrium. This cropped view was taken from the 360-degree timelapse panorama. See complete 360 degree landing site timelapse panorama herein and APOD Feb. 3, 2014. Chang’e-3 landers extreme ultraviolet (EUV) camera is at right, antenna at left. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com.   See our complete Yutu timelapse pano at NASA APOD Feb. 3, 2014:  http://apod.nasa.gov/apod/ap140203.htm
Chang’e-3/Yutu Timelapse Color Panorama
This newly expanded timelapse composite view shows China’s Yutu moon rover at two positions passing by crater and heading south and away from the Chang’e-3 lunar landing site forever about a week after the Dec. 14, 2013 touchdown at Mare Imbrium. This cropped view was taken from the 360-degree timelapse panorama. See complete 360 degree landing site timelapse panorama herein and APOD Feb. 3, 2014. Chang’e-3 landers extreme ultraviolet (EUV) camera is at right, antenna at left. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com. See our complete Yutu timelapse pano at NASA APOD Feb. 3, 2014: http://apod.nasa.gov/apod/ap140203.htm

China is only the 3rd country in the world to successfully soft land a spacecraft on Earth’s nearest neighbor after the United States and the Soviet Union.

Stay tuned here for Ken’s continuing Chang’e-3, Orion, Orbital Sciences, SpaceX, commercial space, LADEE, Mars and more planetary and human spaceflight news. Learn more at Ken’s upcoming presentations at the NEAF astro/space convention on April 12/13.

Ken Kremer

Chang’e-3 lander and Yutu rover – from Above And Below  Composite view shows China’s Chang’e-3 lander and Yutu rover from Above And Below (orbit and surface) – lander color panorama (top) and orbital view from NASA’s LRO orbiter (bottom). Chang’e-3 lander color panorama shows Yutu rover after it drove down the ramp to the moon’s surface and began driving around the landers right side to the south. Yellow lines connect craters seen in the lander panorama and the LROC image from LRO (taken at a later date after the rover had moved), red lines indicate approximate field of view of the lander panorama. Credit: CNSA/NASA/Ken Kremer/Marco Di Lorenzo/Mark Robinson
Chang’e-3 lander and Yutu rover – from Above And Below Composite view shows China’s Chang’e-3 lander and Yutu rover from Above And Below (orbit and surface) – lander color panorama (top) and orbital view from NASA’s LRO orbiter (bottom). Chang’e-3 lander color panorama shows Yutu rover after it drove down the ramp to the moon’s surface and began driving around the landers right side to the south. Yellow lines connect craters seen in the lander panorama and the LROC image from LRO (taken at a later date after the rover had moved), red lines indicate approximate field of view of the lander panorama. Credit: CNSA/NASA/Ken Kremer/Marco Di Lorenzo/Mark Robinson
LRO slewed 54 degrees to the east on Feb. 16, 2014, to allow the LROC instrument to snap a dramatic oblique view of the Chang'e 3 site (arrow). Crater in front of lander is 450 meters (about 1,476 feet) in diameter. Image width is 2,900 meters (about 9,500 feet) at the center. Credit: NASA/Goddard/Arizona State University
LRO slewed 54 degrees to the east on Feb. 16, 2014, to allow the LROC instrument to snap a dramatic oblique view of the Chang’e 3 site (arrow). Crater in front of lander is 450 meters (about 1,476 feet) in diameter. Image width is 2,900 meters (about 9,500 feet) at the center. Credit: NASA/Goddard/Arizona State University

Weekly Space Hangout – March 7, 2014: Cosmos Premiere & NASA Budget

Host: Fraser Cain
Astrojournalists: David Dickinson, Matthew Francis, Casey Dreier, Jason Major, Brian Koberlein, Alan Boyle

This week’s stories:

Alan Boyle (@b0yle, cosmiclog.com ):
Cosmos premiere!

David Andrew Dickinson (@astroguyz):
Watch the Close Pass of NEO 2014 DX110
Daylight Saving time: A Spring Forward or a Step Back?
A Natural Planetary Defense Against Solar Storms

Matthew Francis (@DrMRFrancis, BowlerHatScience.org):
Using gravitational lensing to measure a spinning quasar
CosmoAcademy classes

Casey Dreier (Planetary.org):
The 2015 NASA Budget Request
NASA Kinda Embraces Exploring Europa

Jason Major (@JPMajor, LightsInTheDark.com):
That’s the way the asteroid crumbles

Brian Koberlein (@briankoberlein, briankoberlein.com):
*Possible* evidence for dark matter WIMPs
Black Holes exceed Eddington limit
Using quasars in a quantum experiment

We record the Weekly Space Hangout every Friday at 12:00 pm Pacific / 3:00 pm Eastern. You can watch us live on Google+, Universe Today, or the Universe Today YouTube page.

TV Show ‘Cosmos’ Gets An Epic Reboot This Sunday

Poster for Cosmos: A Spacetime Odyssey.

Sunday is going to be a once-in-a-generation moment. For those of us who were too young to remember the original Cosmos (writer puts hand up) or those who are eager to see the classic 1980 Carl Sagan series updated with discoveries since then, we’re all in luck. A new series starring astronomer Neil deGrasse Tyson is premiering on Fox.

NASA hosted a sneak preview of the series at several NASA centers, and the early reviews on Twitter indicated a heck of a lot of excited people in the audience. In the video above, you can watch the Q&A with the main players after the premiere concluded.

“Watching Cosmos, I saw a Brooklyn-born researcher pull back the curtain on a world of seemingly dense scientific concepts, which, with the flair of P.T. Barnum, he managed to present in ways that made them accessible to those of us lacking a degree in mathematics or physics,” Seth MacFarlane, the executive producer of Cosmos (who is best known for creating Family Guy), said in a statement.

“He was able to make a discussion of the most distant stellar objects suddenly become relevant to our small, day-to-day lives. And he did so with such obvious passion, enthusiasm, and love for the knowledge he imparted that even those who had little interest in science found it impossible not to want to go along for the ride.”

The original Cosmos series premiered in 1980 and won three primetime Emmys. Sagan — who was involved in NASA missions such as the Voyagers — combined his worktime experiences with more meditative thoughts on the cosmos, the role of intelligence and the future of the universe. It’s still easy to purchase the original series, despite its age, so we’re sure Fox is hoping for the same kind of longevity with the reboot.

deGrasse Tyson, for those who don’t know, is the engaging director of the Hayden Planetarium in New York. Like Sagan, he’s a New York City-based popularizer of science who appears regularly on shows that aren’t necessarily science focused — such as The Colbert Report, where he has spoken several times and is often cited as one of Colbert’s most-returning guests, if not the most returning one.

We’ll be eagerly watching the series as it comes out. For more information, you can check out Fox’s website.

Giant Planet May Be Lurking In ‘Poisonous’ Gas Around Beta Pictoris

Artist's conception of a hypothetical giant planet (left) in Beta Pictoris. The gas giant would sweep up comets into a swarm, causing frequent collisions. Astronomers using the Atacama Large Millimeter Array (ALMA) are calling this the "preferred model" for observations they made. Credit: Goddard Space Flight Center/F. Reddy

A Saturn-mass planet might be lurking in the debris surrounding Beta Pictoris, new measurements of a debris field around the star shown. If this could be proven, this would be the second planet found around that star.

The planet would be sheparding a giant swarm of comets (some in front and some trailing behind the planet) that are smacking into each other as often as every five minutes, new observations with the Atacama Large Millimeter/submillimeter Array (ALMA) show. This is the leading explanation for a cloud of carbon monoxide gas visible in the array.

“Although toxic to us, carbon monoxide is one of many gases found in comets and other icy bodies,” stated Aki Roberge, an astrophysicist at NASA’s Goddard Space Flight Center in Maryland who participated in the research. “In the rough-and-tumble environment around a young star, these objects frequently collide and generate fragments that release dust, icy grains and stored gases.”

ALMA captured millimeter-sized light from carbon monoxide and dust around Beta Pictoris, which is about 63 light-years from Earth (relatively close to our planet). The gas seems to be most prevalent in an area about 8 billion miles (13 kilometers) from the star — the equivalent distance of three times the length of Neptune’s location from the sun. The carbon monoxide cloud itself makes up about one-sixth the mass of Earth’s oceans.

Ultraviolet light from the star should be breaking up the carbon monoxide molecules within 100 years, so the fact there is so much gas indicates something must be replenishing it, the researchers noted. Their models showed that the comets would need to be destroyed every five minutes for this to happen (unless we are looking at the star at an unusual time).

While the researchers say they need more study to see how the gas is concentrated, their hypothesis is there is two clumps of gas and it is due to a big planet behaving similarly to what Jupiter does in our solar system. Thousands of asteroids follow behind and fly in front of Jupiter due to the planet’s massive gravity. In this more distant system, it’s possible that a gas giant planet would be doing the same thing with comets.

If the gas turns out to be in just one clump, however, another scenario would suggest two Mars-sized planets (icy ones) smashing into each other about half a million years ago. This “would account for the comet swarm, with frequent ongoing collisions among the fragments gradually releasing carbon monoxide gas,” NASA stated.

The research was published yesterday (March 6) in the journal Science and is led by Bill Dent, a researcher at the Joint ALMA Office in  Chile. You can read more information in press releases from NASA, the National Radio Astronomy Observatory and European Southern Observatory.