An Amazing Capture of Jupiter and its Moons

Astrophotographer Michael Phillips with the gear used to capture the Jupiter rotation animation. Credit-Michael Phillips

It’s always a thrill to watch the action at Jupiter, as its moons pass in front of and behind the gas giant planet. We wrote recently about this month’s opposition of Jove on January 5th, marking the start of the Jupiter evening viewing season for 2014. 

Astrophotographer Michael A. Philips also recently undertook a challenging series of sequences of Jupiter and its moons Io and Ganymede, with stunning results. You can see the motion of Jupiter’s rotation, the Great Red Spot and even a bit of cloud swirl as Io disappears behind Jupiter and Ganymede begins to transit in front and cast a shadow back onto the Jovian cloud tops.

Concerning the capture, Michael wrote on his blog:

“This night was a lucky night. I had not looked at the weather forecast enough to know if it would be good or not. Cold temps aside, I decided earlier in the day to set up and go out with the 14” f/4.5 scope named Akule. As an added bonus, Mitchell Duke tipped me off to a transit of the Jovian moon, Ganymede.”

Note that Jupiter and its moons are currently casting their shadows nearly straight back from our perspective. Expect that to change, however, in the coming months,as Jupiter heads towards eastern dusk quadrature on April 1st and we see the action from a sideways angle. Watch the video in full screen mode and you’ll note that Mike captured some detail on the surface of Ganymede as well! Generally, at the eyepiece, the moons of Jupiter disappear entirely due to low contrast against the bulk of the planet, with only the black dot of the shadow seen… this video capture gives the ingress of Ganymede at the start of the transit a great 3-D appearance.

Webcam imaging of planets has really taken off in the past decade, with backyard astronomers now routinely capturing images that far surpass professional and textbook images from just a decade prior. Great images can be taken using nothing more than a telescope, a laptop, free image stacking software such as Registax, and a webcam converted to fit into an eyepiece holder… you may find that you’ve got the gear sitting around to image Jupiter, tonight.

Mr. Phillips rig, however, is a little more advanced. He notes in the description of the video that he’s using a Flea3 camera from PointGrey Research with a 5x Barlow lens yielding a 9200mm focal length. He’s also shooting at 120 frames per second, and taking successive red, green and blue images for 30 seconds. Finally, a derotation of Jupiter – yes, it really rotates that quickly, even in a short sequence – is accomplished using a sophisticated program named WINJupos.

Video stacking gives processors the ability to “freeze” and nab the best moments of seeing from thousands of frames. Some imagers hand select frames one by one, though many programs, such as Registax, use algorithms to nab the best frames from a preselected percentage of the total shot.

Local seeing conditions also play a key role in image capturing.

“I moved far away from the house as possible, and I think that helped some,” Michael noted. “I also started cooling the spit out of the mirror, aggressively. Even when cooled for a few hours in the winter, the heat in the Pyrex mirror comes back. I think there’s a small heat engine inside the beast!”

For best results, imagers tend to go after planets when they’re at their highest in the sky, and viewed through the least amount of turbulent atmosphere. This is when a planet is transiting the local north to south meridian, and when it’s at opposition, which Jupiter is this month. At opposition, a planet transits at local midnight. The same goes for the best opportunities for visual observing as well.

Shadow transits of Jupiter’s moons are also just plain fun to watch. In an often unchanging universe, they offer a chance to see something unfolding in real time. Jupiter has the fastest rotation of any planet at 9.9 hours, and the large Galilean moons of Io, Europa, Ganymede and Callisto are tidally locked in their rotation, keeping one hemisphere permanently turned towards Jupiter like the Moon does orbiting the Earth. The inner three moons also keep a 1:2:4 orbital resonance, assuring you’ll never see more than three of the four Galilean moons transiting from your line of sight at once. You can see two of the inner three moons, plus Callisto in transit, but never all four at the same time! A triple transit last occurred on October 12th, 2013, and will next occur for observers in eastern Europe and Africa this year on June 3rd.

We’re also currently in the midst of a series of shadow transits for the outermost Galilean moon Callisto, which end in July 2016. Can you identify the different moons by the size and hue of shadows they cast? Sky & Telescope publishes a great table for the ingress and egress of Jupiter’s moons. You can also check them out using the freeware program Stellarium.

The double shadow transit of February 6th as seen at 11:22 UT. Created by the author using Starry Night Education software.
The double shadow transit of February 6th as seen at 11:22 UT. Created by the author using Starry Night Education software.

Can’t wait that long? A double shadow transit involving Europa and Callisto occurs in just a few weeks for western North America from 10:20 UT-12:44UT on the morning of February 6th, a chance for another stunning animation sequence…

Congrats to Michael Phillips on a great capture!

Astrophoto: Jupiter Meets Moon Halo

Gorgeous shot of the Moon-Jupiter conjunction on January 14, 2014 and a beautiful lunar halo, as seen from Ankara, Turkey. Credit and copyright: M. Ra?id Tu?ral

Last night, the Moon and Jupiter snuggled up together in the evening sky, passing within 4°51′ of each other. Folks in Ankara, Turkey got an added benefit to the conjunction, a gorgeous lunar halo. This shot by M. Rasid Tugral is just lovely. The duo stayed together through the night, and you MUST see below for another awesome view of the conjunction at dawn as seen from Pennsylvania in the US:

The morning's setting Moon and Jupiter, on January 15th, 2014. Photo taken near White Haven, Pennsylvania.  Credit and copyright: Tom Wildoner.
The morning’s setting Moon and Jupiter, on January 15th, 2014. Photo taken near White Haven, Pennsylvania. Credit and copyright: Tom Wildoner.

So many things make this such a great photo: the conjunction, of course, but the colors, the shadow of the photographer, and the landscape all combine for a simply stunning image.

Thanks to both of our photographers for sharing, and you can always see more great astrophotos at our Flickr page.

If you’re looking for more conjunctions with the Moon, there are a couple coming up: On Wednesday, Jan 22, 2014 mars will be near the Moon, and on Saturday January 25, 2014 the Moon will meet up with Saturn. Find out more at In-The-Sky.org.

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.

Up Close Launch Pad Cameras capture Spectacular Sound and Fury of Antares/Cygnus Jan. 9 Blast off to Space Station – Video Gallery

Antares rocket blastoff on Jan. 9 from Launch Pad 0A at NASA Wallops Flight Facility, VA lofting the Cygnus resupply vehicle on a mission for NASA bound for the International Space Station. Docking at ISS planned for Jan. 9. Both vehicles built by Orbital Sciences. Photo taken by remote camera at launch pad. Credit: Alan Walters/AmericaSpace/awaltersphoto.com


Video caption: Antares ORB-1 Launch Pad Camera on south side of pad 0A being hammered from Orbital Sciences Antares rocket launch at 1:07 p.m. EST on January 9th 2014, from NASA’s Wallops Flight Facility, VA, carrying the Cygnus resupply spacecraft to the ISS. Credit: Mike Killian/Jeff Seibert/Mike Barrett/AmericaSpace.com/MikeKillianPhotography.com/Wired4Space.com

What’s it like to be standing at a rocket launch pad? Especially when it’s a private spaceship embarking on a history making flight to the space station that’s blasting the opening salvos of the new ‘commercial space era’ heard round the world?

Thrilling beyond belief!

And what’s it like to be standing at the launch pad when the engines ignite and the bird begins soaring by guzzling hundreds of thousands of pounds of burning fuel, generating intense heat and deadly earsplitting noise?

Well for a first-hand, up-close adventure to hear the deafening sound and feel the overwhelming fury, I’ve collected a gallery of videos from the Jan. 9 blastoff of the privately built Antares rocket from NASA’s Wallops Flight Facility, VA on a historic mission to the International Space Station (ISS).

The videos were created by a team of space journalists from a variety of space websites working together to create the best possible products for everyone’s enjoyment- including Alan Walters, Mike Killian, Matt Travis, Jeff Seibert, Mike Barrett and Ken Kremer representing AmericaSpace, Zero-G News, Wired4Space and Universe Today.


Video caption: Close up camera captures Antares liftoff carrying the Cygnus Orb-1 ISS resupply spacecraft. This was composed of 59 images taken by a Canon Rebel xti and 18 mm lens of the Antares Orbital 1 launch to the ISS on Jan. 9, 2013 at NASA Wallops Island, VA. Credit: Ken Kremer/Alan Walters/Matthew Travis/kenkremer.com

Wallops is located along the eastern shore of Virginia at America’s newest space port.

Because the launch pad is near the most heavily populated ares of the US, millions have a chance to view the launch along the US eastern seaboard.

And the pad sits almost directly on the Atlantic Ocean, so you can hear the waves constantly crashing on shore.

Well we always want to be as close as possible. But as you’ll see, it’s really not a very good idea to be right there.


North Side Launch Pad Camera Captures Antares Rocket Launch With Orbital Sciences Cygnus Orb-1 To ISS on Jan. 9, 2013 from NASA Wallops. A GoPro Hero 2 camera captures the launch of Orbital Sciences Antares rocket carrying the Cygnus spacecraft on the Orb-1 mission to resupply the International Space Station. Credit: Matt Travis/Mike Killian/MikeKillianPhotography.com/ZeroGnews.com/AmericaSpace.com

Virtually every camera on the south side got creamed and was blown over by the approaching fiery exhaust fury seen in the videos.

Amazingly they continued taking pictures of the exhaust as they were violently hit and flung backwards.

Luckily, as they were knocked over and fell to the ground, the lenses were still facing skyward and snapping away showing the sky and exhaust plume swirling around and eventually dissipating.

Our cameras capture the experience realistically.

We’ve set them up around the north and side sides at NASA’s Wallops Launch Pad 0A on the Mid-Atlantic Regional Spaceport (MARS).

Antares soars to space on Jan. 9, 2014 from NASA Wallops on Virginia coast on the Orb-1 mission to the ISS.  Photo taken by remote camera at launch pad. Credit: Ken Kremer - kenkremer.com
Antares soars to space on Jan. 9, 2014 from NASA Wallops on Virginia coast on the Orb-1 mission to the ISS. Photo taken by remote camera at launch pad. Credit: Ken Kremer – kenkremer.com

How do the cameras, called remotes, collect the imagery?

They are activated either by sound triggers or timers.

It takes a lot of hard work and equipment and doesn’t always work out as planned.

But the payoff when it does is absolutely extraordinary.

The Jan. 9 blast off of Orbital Sciences’ private Antares booster delivered the firm’s Cygnus Orbital-1 cargo freighter to orbit.

Orbital Sciences' Cygnus cargo spacecraft, with the moon seen in the background, is moved into installation position by astronauts using a robotic arm aboard the International Space Station Jan. 12. Credit: NASA
Orbital Sciences’ Cygnus cargo spacecraft, with the moon seen in the background, is moved into installation position by astronauts using a robotic arm aboard the International Space Station Jan. 12. Credit: NASA

Following a two day orbital chase and an intricate series of orbit raising maneuvers, the Cygnus vessel reached the station on Sunday, Jan. 12, and was berthed by astronauts maneuvering the robot arm at an Earth-facing port on the massive orbiting lab complex.

The Orbital -1 spaceship is conducting the first of 8 operational cargo logistics flights scheduled under Orbital Sciences’ multi-year $1.9 Billion Commercial Resupply Services contract (CRS) with NASA that runs through 2016.

SpaceX likewise has a contract with NASA to deliver cargo to the ISS via their Dragon spaceship. The next SpaceX launch is slated for Feb. 22.

Stay tuned here for Ken’s continuing Orbital Sciences, SpaceX, commercial space, Chang’e-3, LADEE, Mars and more news.

Ken Kremer

This Cygnus launched atop Antares on Jan. 9 and docked on Jan. 12   Cygnus pressurized cargo module – side view – during exclusive visit by  Ken Kremer/Universe Today to observe prelaunch processing by Orbital Sciences at NASA Wallops, VA. ISS astronauts will open this hatch to unload 2780 pounds of cargo.  Docking mechanism hooks and latches to ISS at left. Credit: Ken Kremer – kenkremer.com
This Cygnus launched atop Antares on Jan. 9 and docked on Jan. 12 Cygnus pressurized cargo module – side view – during exclusive visit by Ken Kremer/Universe Today to observe prelaunch processing by Orbital Sciences at NASA Wallops, VA. ISS astronauts will open this hatch to unload 2780 pounds of cargo. Docking mechanism hooks and latches to ISS at left. Credit: Ken Kremer – kenkremer.com
Space journalists Ken Kremer/Universe Today (left) and Mike Killian  and Alan Walters  of AmericaSpace (center, right) setting remote cameras at Antares launch pad amidst bone chilling cold for the photos featured herein.  Credit: Ken Kremer - kenkremer.com
Space journalists Ken Kremer/Universe Today (left) and Mike Killian and Alan Walters of AmericaSpace (center, right) setting remote cameras at Antares launch pad amidst bone chilling cold for the imagery featured herein. Credit: Ken Kremer – kenkremer.com

Stunning Footage from SpaceShipTwo’s Third Rocket-Powered Flight

Image from the "tail cam" on SpaceShipTwo of engine ignition. Credit: Virgin Galactic.

Virgin Galactic released video from SpaceShipTwo’s flight test last Friday, January 10, 2014. This was the third supersonic, rocket-powered test of the Virgin Galactic system after dozens of successful subsonic test flights. The pilots Dave Mackay and Mark Stucky tested the spaceship’s Reaction Control System, the newly installed thermal protection coating on the vehicle’s tail booms, and the “feather” re-entry system, all with great success.

See some images from the flight below.

You can read our coverage from Friday’s test flight here.

Image from SpaceShipTwo's third powered flight on January 10, 2014. Credit: Virgin Galactic.
Image from SpaceShipTwo’s third powered flight on January 10, 2014. Credit: Virgin Galactic.
Feathered Flight during Virgin Galactic's SpaceShipTwo's third powered flight on January 10,  2014 over the Mojave desert. This image was taken by MARS Scientific as part of the Mobile Aerospace Reconnaissance System optical tracking system.
Feathered Flight during Virgin Galactic’s SpaceShipTwo’s third powered flight on January 10, 2014 over the Mojave desert. This image was taken by MARS Scientific as part of the Mobile Aerospace Reconnaissance System optical tracking system.

Fly Over the Floodplains of Mars

A mosaic of 67 images from the Mars Express spacecraft of Kasei Valles on Mars. Credit: ESA/DLR/FU (G. Neukum)

Over 3 billion years ago, dramatic flood events likely carved this gigantic channel system on Mars. It extends some 3,000 km and covers over 1.55 million square kilometers. ESA released this flyover video today, on the 10th anniversary of the Mars Express spacecraft’s launch to the Red Planet on January 14, 2004.

ESA describes the scene in the video:

The scene spans 987 km in the north–south direction, 19–36°N, and 1550 km in the east–west direction (280–310°E). It covers 1.55 million square kilometers, an area equivalent to the size of Mongolia.

Kasei Valles splits into two main branches that hug a broad island of fractured terrain — Sacra Mensa — rising 2 km above the channels that swerve around it. While weaker materials succumbed to the erosive power of the fast-flowing water, this hardier outcrop has stood the test of time.

Slightly further downstream, the flood waters did their best to erase the 100 km-wide Sharonov crater, crumpling its walls to the south. Around Sharonov many small streamlined islands form teardrop shapes rising from the riverbed as water swept around these natural obstacles.

Source: ESA

Astrophoto: Space Station on the Moon

The International Space Station captured as it passed in front of the Moon on Dec. 6, 2013, as seen from Puerto Rico. Credit and copyright: Juan Gonzalez-Alicea.

We can dream, right? … because we’d all love to have a space station on the Moon. But this is as close as we’re going to get for the foreseeable future, anyway. Juan Gonzalez-Alicea of Sociedad de Astronomia del Caribe in Puerto Rico captured this great image of the International Space Station crossing in front of the crescent Moon on Dec. 6, 2013. He used a Canon 7D with a 300 mm lens, and actually got a fair amount of detail. A shot like this is tricky, as from our vantage point on Earth, it takes just a half second for the International Space Station to fly across the face of the Moon, so timing is everything!

To see another great shot of the ISS crossing in front of the Moon, check out Theirry Legault’s photo from 2010, which shows absolutely incredible detail.

And to see more great astrophotos, check out our Flickr page.

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.

A Possible Meteor Shower from Comet ISON?

Credit-Stellarium

Hey, remember Comet C/2012 S1 ISON? Who can forget the roller-coaster ride that the touted “Comet of the Century” took us on last year. Well, ISON could have one more trick up its cosmic sleeve –although it’s a big maybe — in the form of a meteor shower or (more likely) a brief uptick in meteor activity this week.

In case you skipped 2012 and 2013, or you’re a time traveler who missed their temporal mark, we’ll fill you in on the story thus far.

Comet ISON was discovered by Artyom Novichonok and Vitali Nevski on September 21st, 2012 as part of the ongoing International Scientific Optical Network (ISON) survey. Shortly after its discovery, researchers knew they had spotted something special: a sungrazing comet already active at over 6.4 Astronomical Units (A.U.s) from the Sun. The Internet then did what it does best, and promptly ran with the story. There were no shortage of Comet ISON conspiracy theories for science writers to combat in 2013. It’s still amusing to this day to see predictions for comet ISON post-perihelion echo through calendars, almanacs and magazines compiled and sent to press before its demise.

ISON back in the day. Credit-Efrain Morales Rivera, Jaicoa Observatory Aguadilla, Puerto Rico
ISON back in the day. Credit-Efrain Morales Rivera, Jaicoa Observatory Aguadilla, Puerto Rico

The frenzy for all things ISON reached a crescendo on U.S. Thanksgiving Day November 28th 2013, as ISON passed just 1.1 million kilometres from the surface of the Sun. Unfortunately, what emerged was a sputtering ember of the comet formerly known as ISON, which faded from view just as it was slated to reenter the dawn sky.

Hey, we were crestfallen as well… we had our semi-secret dark sky site pre-selected for ISON imaging post-perihelion and everything. Despite heroic searches by ground and space-based assets, we’ve yet to see any compelling recoveries of Comet ISON post-perihelion.

This week, however, Comet ISON may put on its last hurrah, in the form of a minor meteor shower. We have to say from the outset that we’re highly skeptical that an “ISON-id meteor outburst” will grace the skies. Known annual showers are fickle enough, and it’s nearly impossible to predict just what might happen during a meteor shower with no past track record.

But you won’t see anything if you don’t try. If anything is set to occur, the night of January 15th into the 16th might just be the time to watch. This is because the Earth will cross the orbital plane of ISON’s path right around 9:00 PM EST/2:00 UT. Last year, ISON passed within 3.3 million kilometres of the Earth’s orbit on its inbound leg. Earlier last year, ISON was estimated to have been generating a prodigious amount of dust, at a rate of about 51,000 kilograms per minute. Any would-be fragments of ISON outbound would’ve passed closest to the Earth at 64 million kilometres distant on the day after Christmas last year. Veteran sky observer Bob King wrote about the prospects for catching ISON one last time during this month back in December 2013.

Credit: NASA/JPL Solar System Dynamics Small Body Database Browser.
A simulation showing Earth crossing the plane of Comet ISON’s orbit early on January 16th. Credit: NASA/JPL Solar System Dynamics Small Body Database Browser.

Another idea out there that is even more unlikely is the proposal that dust from Comet ISON may generate an uptick in noctilucent cloud activity. And already, a brief search of the internet sees local news reports attempting to tie every meteor observed to ISON this week, though no conclusive link to any observed fireball has been made.

The radiant to watch for any possible “ISON-ids” sits near the +3.5 magnitude star Eta Leonis in the sickle of Leo. Robert Lundsford of the American Meteor Society notes in a recent posting that any ISON-related meteors would pass through our atmosphere at a moderate 51 kilometres a second, with a visible duration of less than one second.

Note that meteor activity has another strike against it, as the Moon reaches Full on the same night. In fact, the Full Moon of Wednesday January 15th sits in the constellation Gemini,just 32 degrees away from the suspect radiant!

Another caveat is in order for any remaining dooms-dayers: no substantial fragments of ISON are (or ever were) inbound and headed towards our fair planet. Yes, we’re seeing rumblings to this effect in the pseudoscience netherworlds of ye ole Internet, along with ideas that ISON secretly survived, NASA “hid” ISON, ISON cloaked like a Romulan Bird of Prey, you name it. Just dust grains, folks… a good show perhaps, but nothing more.

As near as we can tell, talk of a possible meteor shower generated from Comet ISON goes all the way back to a NASA Science News article online from April 2013. Radio observers of meteor showers should be alert for a possible surge in activity this week as well, and it may be the case that more radio “pings” will be noted than visual activity what with the light-polluting Full Moon in the sky. The radiant for any would-be “ISON-ids” transits highest in the sky for northern hemisphere observers at around 2 AM local.

But despite what it has going against it, we’d be thrilled if ISON put on one last show anyhow. It’s always worth watching for meteor activity and noting the magnitude and from whence the meteor came to perhaps note the pedigree as to the shower it might belong to.

The next annual dependable meteor shower won’t be until the night of April 21st to the 22nd, when the Spring Lyrids are once again active. And this year may just offer a special treat on May 24th, when researchers have predicted that the Earth may encounter debris streams laid down by Comet 209P LINEAR way back in 1803 and 1924… Camelopardalids, anyone? Now, that’s an exotic name for a meteor shower that we’d love to see trending!

-Catch sight of any “ISON-ids?” we’d love to see ‘em… be sure to post said pics at Universe Today’s Flickr pool.

 

 

China’s Historic Moon Robot Duo Awaken from 1st Long Frigid Night and Resume Science Operations

Photo of Chang'e-3 moon lander emblazoned with Chinese national flag taken by the panoramic camera on the Yutu moon rover on Dec. 22, 2013. Credit: CNSA

Chinese Moon Robots Wake up
Photo of Chang’e-3 moon lander emblazoned with Chinese national flag taken by the panoramic camera on the Yutu moon rover on Dec. 22, 2013. Credit: CNSA
Story updated[/caption]

Chinese Moon Robots Wake up!

China’s history making moon robots – the Chang’e-3 lander and Yutu rover – have just awoken from the forced slumber of survival during their first, long frigid lunar night and have now resumed full operations – marking a major milestone in the mission.

This landmark achievement offers a realistic prognosis that the best is yet to come for this new dynamic duo of robots dispatched from Earth!

The stationary lander and six wheeled rover were autonomously revived from their dormant mode this weekend.

Both were then placed back into full working science mode in response to commands issued by Chinese space engineers at the Beijing Aerospace Control Center (BACC), according to CCTV, China’s official government broadcast network.

Portrait photo of Yutu moon rover taken by camera on the Chang'e-3 moon lander on Dec. 15, 2013 shortly after rolling all 6 wheels onto lunar surface.  Credit: Chinese Academy of Sciences
Portrait photo of Yutu moon rover taken by camera on the Chang’e-3 moon lander on Dec. 15, 2013 shortly after rolling all 6 wheels onto lunar surface. Credit: Chinese Academy of Sciences

Yutu woke up first on Saturday, Jan. 11, at 5:09 a.m. Beijing local time.

The Chang’e-3 lander was awoken on Sunday, Jan. 12, at 8:21 a.m. Beijing local time, according to a BACC statement.

Both vehicles depend on their life giving solar panels to produce power in order to function and accomplish their scientific tasks.

They went to sleep to conserve energy since there is no sunlight to generate power with the solar arrays during the lunar night.

During the nocturnal hiatus they were kept alive by a radioisotopic heat source that kept their delicate computer and electronics subsystems warmed inside a box below the deck. It was maintained at a temperature of about minus 40 degrees Celsius to prevent debilitating damage

The simple fact that both spacecraft survived half a month through the extremely harsh lunar night time environment when temperatures plunged to below minus 180 degrees Celsius, or minus 292 degrees Fahrenheit, and then restarted intact, proves the resiliency and robustness of China’s space technology.

“During the lunar night, the lander and the rover were in a power-off condition and the communication with Earth was also cut off,” said Zhou Jianliang, chief engineer of the BACC, to CCTV.

The "Yutu" rover and the Chang’e-3 lander began functioning again on Jan 11 & 12, 2014 in this artists concept. Both had become dormant to ride out the harsh conditions on the moon. Credit: CNSA/CCTV
The “Yutu” rover and the Chang’e-3 lander began functioning again on Jan 11 & 12, 2014 in this artists concept. Both had become dormant to ride out the harsh conditions on the moon. Credit: CNSA/CCTV

“When the night ends, they will be started up with the power provided by sunlight and resume operation and communication according to preset programs,” Zhou said.

As night fell on the Earth’s Moon at Christmas time 2013, Yutu and the mother ship lander both entered a state of hibernation – determined to survive the utterly harsh lunar darkness upon the magnificently desolate gray plains.

The mother ship began her nap first on Christmas Day, Dec. 25. Yutu went to sleep on Dec. 26 obeying commands sent by mission control at BACC, according to China’s State Administration of Science, Technology and Industry for National Defence (SASTIND).

Just prior to hibernating, the lander snapped the first image of the Earth taken from the Moon’s surface in some four decades. See below.

The Earth from the Moon – by Chang’e-3 on Christmas Day Lander camera snapped this image on Christmas Day 2013. Credit: Chinese Academy of Sciences
The Earth from the Moon – by Chang’e-3 on Christmas Day
Lander camera snapped this image on Christmas Day 2013. Credit: Chinese Academy of Sciences

Now with the dawn of daylight the solar panels were unfurled and the instruments activated on both robots.

Yutu has already resumed roving towards pristine, unexplored lunar terrain surrounding the touchdown zone at Mare Imbrium, nearby the Bay of Rainbows, or Sinus Iridum region.

After driving in a semicircular path around the right side of the stationary lander, and snapping portraits of one another at 5 preselected locations, Yutu parked some 40 meters south of the mother ship – after touchdown and prior to the start of lunar night.

Yutu, which translates as ‘Jade Rabbit’, is departing the landing zone forever, trekking southwards for surface investigations expected to last at least 3 months – and perhaps longer depending on its robustness in the unforgiving space environment.

The Chang’e-3 lander should survive at least a year.

“They will begin to conduct scientific explorations of the geography and geomorphology of the landing spot and nearby areas, and materials like minerals and elements there,” noted Wu Weiren, chief designer of China Lunar Probe Program.

“We will also explore areas 30 meters and 100 meters beneath the lunar soil. The exploration will continue longer than we planned, because all the instruments and equipments are working very well.”

‘Jade Rabbit’ and the lander will use their suites of science instruments including cameras, telescopes, spectrometers and ground penetrating radar to survey the moon’s geological structure and composition to locate the moon’s natural resources for use by potential future Chinese astronauts.

The robotic pair safely soft landed on the Moon on Dec. 14 at Mare Imbrium, located in the upper left portion of the moon as seen from Earth. Seven hour later on Dec. 15, Yutu rolled all 6 wheels onto the moon’s surface, leaving tracks behind as it cut into the loose regolith.

Presumably they will continue exploring for about the next 14 days – the entire time span of their 2nd Lunar Day, unless they need to take a break from the high daylight temperatures.

Thereafter Yutu and Chang’e-3 will function in alternating cycles of 2 weeks on and 2 weeks off for the duration of their independent working lifetimes.

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, Orbital Sciences, SpaceX, commercial space, LADEE, Mars and more news.

Ken Kremer

Why Einstein Will Never Be Wrong

Einstein Lecturing
Albert Einstein during a lecture in Vienna in 1921. Credit: National Library of Austria/F Schmutzer/Public Domain

One of the benefits of being an astrophysicist is your weekly email from someone who claims to have “proven Einstein wrong”. These either contain no mathematical equations and use phrases such as “it is obvious that..”, or they are page after page of complex equations with dozens of scientific terms used in non-traditional ways. They all get deleted pretty quickly, not because astrophysicists are too indoctrinated in established theories, but because none of them acknowledge how theories get replaced.

For example, in the late 1700s there was a theory of heat known as caloric. The basic idea of caloric was that it was a fluid that existed within materials. This fluid was self-repellant, meaning it would try to spread out as evenly as possible. We couldn’t observe this fluid directly, but the more caloric a material has the greater its temperature.

Ice-calorimeter
Ice-calorimeter from Antoine Lavoisier’s 1789 Elements of Chemistry. (Public Domain)

From this theory you get several predictions that actually work. Since you can’t create or destroy caloric, heat (energy) is conserved. If you put a cold object next to a hot object, the caloric in the hot object will spread out to the cold object until they reach the same temperature.  When air expands, the caloric is spread out more thinly, thus the temperature drops. When air is compressed there is more caloric per volume, and the temperature rises.

We now know there is no “heat fluid” known as caloric. Heat is a property of the motion (kinetic energy) of atoms or molecules in a material. So in physics we’ve dropped the caloric model in terms of kinetic theory. You could say we now know that the caloric model is completely wrong.

Except it isn’t. At least no more wrong than it ever was.

The basic assumption of a “heat fluid” doesn’t match reality, but the model makes predictions that are correct. In fact the caloric model works as well today as it did in the late 1700s. We don’t use it anymore because we have newer models that work better. Kinetic theory makes all the predictions caloric does and more. Kinetic theory even explains how the thermal energy of a material can be approximated as a fluid.

This is a key aspect of scientific theories. If you want to replace a robust scientific theory with a new one, the new theory must be able to do more than the old one. When you replace the old theory you now understand the limits of that theory and how to move beyond it.

In some cases even when an old theory is supplanted we continue to use it. Such an example can be seen in Newton’s law of gravity. When Newton proposed his theory of universal gravity in the 1600s, he described gravity as a force of attraction between all masses. This allowed for the correct prediction of the motion of the planets, the discovery of Neptune, the basic relation between a star’s mass and its temperature, and on and on. Newtonian gravity was and is a robust scientific theory.

Then in the early 1900s Einstein proposed a different model known as general relativity. The basic premise of this theory is that gravity is due to the curvature of space and time by masses.  Even though Einstein’s gravity model is radically different from Newton’s, the mathematics of the theory shows that Newton’s equations are approximate solutions to Einstein’s equations.  Everything Newton’s gravity predicts, Einstein’s does as well. But Einstein also allows us to correctly model black holes, the big bang, the precession of Mercury’s orbit, time dilation, and more, all of which have been experimentally validated.

So Einstein trumps Newton. But Einstein’s theory is much more difficult to work with than Newton’s, so often we just use Newton’s equations to calculate things. For example, the motion of satellites, or exoplanets. If we don’t need the precision of Einstein’s theory, we simply use Newton to get an answer that is “good enough.” We may have proven Newton’s theory “wrong”, but the theory is still as useful and accurate as it ever was.

Unfortunately, many budding Einsteins don’t understand this.

Binary waves from black holes. Image Credit: K. Thorne (Caltech) , T. Carnahan (NASA GSFC)
Binary waves from black holes. Image Credit: K. Thorne (Caltech) , T. Carnahan (NASA GSFC)

To begin with, Einstein’s gravity will never be proven wrong by a theory. It will be proven wrong by experimental evidence showing that the predictions of general relativity don’t work. Einstein’s theory didn’t supplant Newton’s until we had experimental evidence that agreed with Einstein and didn’t agree with Newton. So unless you have experimental evidence that clearly contradicts general relativity, claims of “disproving Einstein” will fall on deaf ears.

The other way to trump Einstein would be to develop a theory that clearly shows how Einstein’s theory is an approximation of your new theory, or how the experimental tests general relativity has passed are also passed by your theory.  Ideally, your new theory will also make new predictions that can be tested in a reasonable way.  If you can do that, and can present your ideas clearly, you will be listened to.  String theory and entropic gravity are examples of models that try to do just that.

But even if someone succeeds in creating a theory better than Einstein’s (and someone almost certainly will), Einstein’s theory will still be as valid as it ever was.  Einstein won’t have been proven wrong, we’ll simply understand the limits of his theory.