While we’re unsure about the status of chocolates and flowers in locations far beyond Earth, there certainly is no lack of hearts for us to look at to enjoy Valentine’s Day. If you look at enough geologic features or gas clouds, statistically some of them will take on shapes that we recognize (such as faces).
Below, we’ve collected some hearts on Mars and other places in the universe. Have we missed any? Share other astronomy hearts in the comments!
This heart-shaped feature on Mars “is actually a pit formed by collapse within a straight-walled trough known in geological terms as a graben,” wrote Malin Space Systems in 1999. Picture taken by Mars Global Surveyor. Credit: Malin Space Science Systems, MGS, JPL, NASAA heart-shaped mesa captured by Mars Global Surveyor in 1999, in the Promethei Rupes region. Credit: Malin Space Science Systems, MGS, JPL, NASAThe Heart and Soul nebulae in an infrared mosaic from NASA’s Wide-field Infrared Survey Explorer (WISE). It is located about about 6,000 light-years from Earth. Credit: NASA/JPL-Caltech/UCLA
This visible image of the winter storm over the U.S. south and East Coast was taken by NOAA's GOES-13 satellite on Feb. 13 at 1455 UTC/9:45 a.m. EST. Snow covered ground can be seen over the Great Lakes region and Ohio Valley. Image Credit: NASA/NOAA GOES Project
This visible image of the winter storm over the U.S. south and East Coast was taken by NOAA’s GOES-13 satellite on Feb. 13 at 1455 UTC/9:45 a.m. EST. Snow covered ground can be seen over the Great Lakes region and Ohio Valley. Image Credit: NASA/NOAA GOES Project
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A deadly monster storm is battering virtually the entire US Eastern seaboard today, Thursday, Feb. 13, as it moves from the Southeast to the Northeast and into the New England states, wreaking havoc and causing miserable weather conditions for over 100 million Americas.
This afternoon, NASA and NOAA published a new image taken by a GOES satellite that showed the extent of the clouds associated with the massive winter storm over the US East Coast – see above and below.
Blizzard, white out and slippery conditions have already caused more than 18 deaths.
The killer storm has brought relentless waves of snow, sleet and ice over the past two days covering a vast swath stretching from inland to coastal areas as it moved up from the southern to northern states.
More than a foot of snow has already fallen in many areas today stretching from the Mid-Atlantic into the entire Northeast region.
Several states have declared states of emergency.
This is the season’s 12th snow storm. In many Northeast localities, the accumulated snowfall totals are three times the normal average. As a result many municipalities are running out of road salt.
And to add insult to injury, much more icy snow is falling overnight into Friday on top of the massive existing mounds and piles of frozen ice and snow that’s accumulated over the past few weeks of subfreezing temperatures.
There are also predictions for patches of “thunder snow” — which is a snow storm mixed with thunder and lightning!
Full disk image of the winter storm over the U.S. south and East Coast was taken by NOAA’s GOES-13 satellite on Feb. 13 at 1455 UTC/9:45 a.m. EST. Credit: NASA/NOAA GOES Project
Incredibly, another round of snow is forecast for Saturday.
Much of the I-95 corridor where I also live has been especially hard hit.
The image above was created from data captured by NOAA’s GOES-East satellite today, Feb. 13 at 1455 UTC/9:45 a.m. EST by a team from the NASA/NOAA’s GOES Project at NASA’s Goddard Space Flight Center in Greenbelt, Md.
“The clouds and fallen snow data from NOAA’s GOES-East satellite were overlaid on a true-color image of land and ocean created by data from the Moderate Resolution Imaging Spectroradiometer or MODIS instrument that flies aboard NASA’s Aqua and Terra satellites,” said NASA in a statement.
An eight months pregnant 36 year old women was tragically killed in New York City accident today by a snowplow. Thank God the unborn baby was saved and delivered by cesarean section.
The storm has caused thousands of traffic accidents and several deaths.
Video Caption: This animation of NOAA’s GOES satellite data shows the progression of the major winter storm in the U.S. south from Feb. 10 at 1815 UTC/1:15 p.m. EST to Feb. 12 to 1845 UTC/1:45 p.m. EST. Credit: NASA/NOAA GOES Project, Dennis Chesters
Hundreds of thousands of customers have lost power due to fallen tree limbs on exposed power lines, mostly in the southeast. In recent days, hundreds of thousands of us here in the Northeast lost power after a severe ice storm.
Mountains of snow inundate the Northeast. Credit: Mark Usciak
Most of those affected were left with no heat in subfreezing temperatures. It’s definitely no fun when you can see you exhaled breath – indoors.
Many school districts were closed today. But not in NYC where the new Mayor Bill DeBlasio kept schools open, and faced a hail of criticism – including from NBC News weatherman Al Roker.
Over 6500 airplane flights have been cancelled, stranding over a half million people.
So after days of shoveling, even more is on tap for the morning. Be careful, pace yourself and don’t overdo it – as several people died from heart attacks digging out the heavy slushy mess
Here is this evenings forecast (Feb 13) from the National Weather Service (NWS):
STORM SUMMARY NUMBER 09 FOR SOUTHERN PLAINS TO EAST COAST WINTER STORM
NWS WEATHER PREDICTION CENTER COLLEGE PARK MD – – 1000 PM EST THU FEB 13 2014
…LOW PRESSURE CENTER HAS MOVED OFF THE NEW JERSEY COAST AND IS
RAPIDLY INTENSIFYING…HEAVY SNOW BANDS IMPACTING INTERIOR
NORTHEAST AND I 95 CORRIDOR…WINDS INCREASING ACROSS THE AFFECTED
REGION…
WINTER STORM WARNINGS AND WINTER WEATHER ADVISORIES ARE IN EFFECT
FOR THE NORTHERN MID ATLANTIC AND NORTHEAST….
FOR A DETAILED GRAPHICAL DEPICTION OF THE LATEST
WATCHES…WARNINGS AND ADVISORIES…PLEASE SEE WWW.WEATHER.GOV
AT 900 PM EST…THE MAIN CENTER OF A RAPIDLY INTENSIFYING LOW
PRESSURE SYSTEM WITH ESTIMATED CENTRAL PRESSURE OF 986 MB…29.12
INCHES…WAS LOCATED JUST EAST OF THE SOUTHERN NEW JERSEY COAST.
NATIONAL WEATHER SERVICE DOPPLER RADAR AND SURFACE OBSERVATIONS
INDICATED THAT OVER THE PAST FEW HOURS…A BAND OF HEAVY SNOW WAS
IMPACTING CENTRAL PENNSYLVANIA ACROSS NORTHERN NEW ENGLAND TO
NORTHERN MAINE. MEANWHILE…ANOTHER BAND OF MODERATE TO HEAVY
SNOW WAS LOCATED ALONG THE I 95 CORRIDOR FROM WASHINGTON DC TO NEW YORK CITY. EAST OF I 95 THE PRECIPITATION TYPE IS MAINLY RAIN…BUT A CHANGEOVER BACK TO SNOW IS EXPECTED.
Stay tuned here for Ken’s continuing planetary and human spaceflight news.
Recent ice and snow storms caused hundreds of thousands to lose power and heat in the Northeast in subfreezing temperatures. Credit: Ken KremerMountains of snow inundate the Northeast. Credit: Mark Usciak
USS Enterprise-D, a starship of the Star Trek: The Next Generation era. Credit: MemoryAlpha.Org/Paramount Pictures/CBS Studios
I have a new exercise routine where I watch Star Trek: The Next Generation most mornings of the week while doing my thing. Besides serving as awesome distraction, the episodes do get me thinking about how humans would talk to extraterrestrials. It likely wouldn’t be as easy as the show portrays to zoom across space to conduct diplomatic negotiations at the planet “Parliament”, for example, so interstellar communication would be a problem.
Luckily for non-engineers such as me, there are folks out there (on Earth, at least) that are examining the problem of talking between stars. David Messerschmitt, of the University of California at Berkeley, is one of those people. A new paper by him on Arxiv examines the issue. Note this is a preprint site and not a peer-reviewed journal, but all the same it provides an intriguing addition to how to communicate outside of Earth.
Messerschmitt explains that humans already communicate with probes that are a fair distance from Earth (say, Voyager 1 in interstellar space) at radio frequencies, and there is some usage now of laser/optical communications (namely between the Earth and the moon).
Across greater distances, however, you lose information, the interstellar medium gets in the way, and stars shift due to relative motion. Besides all that, at first you wouldn’t know how the other civilization designs its systems and you could therefore send a message that wouldn’t be picked up.
This sequence of images, showing a region where fewer stars are forming near the constellation of Perseus, illustrates how the structure and distribution of the interstellar medium can be distilled from the images obtained with Planck. Credit: ESA / HFI and LFI Consortia
He further explains that starships and civilizations would have different communications requirements. Starship communication would be two-way and based on a similar design, so success comes by having high “uplink and downlink transmit times”. The more information, the better it would be for scientific observations and keeping down errors.
Civilization-to-civilization chats, however, would present headaches. As with all diplomatic negotiations, crafting suitable messages would take time. Then we’d have to send the message out repeatedly to make sure it is heard (which actually means that reliability is not as big of a problem.) Then the ISM would have to be contended with (something that pulsar astronomers and astrophysicists are already working on, he said).
In either case — talking to starships or other civilizations — one can assume there’d be a lot of energy involved, he added. “Starships are likely to be much closer than the nearest civilizations, but the cost of either a large transmit antenna or transmit energy is likely to be considerably greater for the starship than for a terrestrial-based transmitter,” he said, suggesting that a solution would be to minimize the energy delivered to the receiver. Other civilizations may have found more efficient ways to overcome this problem, he added.
You can read more details of the research on Arxiv, where Messerschmitt talks about Gaussian noise, channel coding and other parameters to keep in mind during communication.
There is nothing in the Universe more awe inspiring or mysterious than a black hole. Because of their massive gravity and ability to absorb even light, they defy our attempts to understand them. All their secrets hide behind the veil of the event horizon.
What do they look like? We don’t know. They absorb all the radiation they emit. How big are they? Do they have a size, or could they be infinitely dense? We just don’t know. But there are a few things we can know. Like how massive they are, and how fast they’re spinning.
Wait, what? Spinning?
Consider the massive star that came before the black hole. It was formed from a solar nebula, gaining its rotation by averaging out the momentum of all the individual particles in the cloud. As mutual gravity pulled the star together, through the conservation of angular momentum it rotated more rapidly. When a star becomes a black hole, it still has all that mass, but now compressed down into an infinitesimally smaller space. And to conserve that angular momentum, the black hole’s rate of rotation speeds up… a lot.The entire history of everything the black hole ever consumed, averaged down to a single number: the spin rate.
If the black hole could shrink down to an infinitely small size, you would think that the spin rate might increase to infinity too. But black holes have a speed limit.
“There is a speed limit to the spin of a black hole. It’s sort of set by the faster a black hole spins, the smaller is its event horizon.”
That’s Dr. Mark Morris, a professor of astronomy at UCLA. He has devoted much of his time to researching the mysteries of black holes.
“There is this region, called the ergosphere between the event horizon and another boundary, outside. The ergosphere is a very interesting region outside the event horizon in which a variety of interesting effects can occur.”
Scientists measure the spin rates of supermassive black holes by spreading the X-ray light into different colors. Image credit: NASA/JPL-Caltech
Imagine the event horizon of a black hole as a sphere in space, and then surrounding this black hole is the ergosphere. The faster the black hole spins, the more this ergosphere flattens out.
“The speed limit is set by the event horizon, eventually, at a high enough spin, reaches the singularity. You can’t have what’s called a naked singularity. You can’t have a singularity exposed to the rest of the Universe. That would mean that the singularity itself could emit energy or light and somebody outside could actually see it. And that can’t happen. That’s the physical limitation of how fast it can spin. Physicists use units for angular momentum that are cast in terms of mass, which is a curious thing, and the speed limit can be described as the angular momentum equals the mass of the black hole, and that sets the speed limit.”
Just imagine. The black hole spins up to the point that it’s just about to reveal itself. But that’s impossible. The laws of physics won’t let it spin any faster. And here’s the amazing part. Astronomers have actually detected supermassive black holes spinning at the limits predicted by these theories.
One black hole, at the heart of galaxy NGC 1365 is turning at 84% the speed of light. It has reached the cosmic speed limit, and can’t spin any faster without revealing its singularity.
Artist's conception of the Mars Odyssey spacecraft. Credit: NASA/JPL
Just a few days ago, we posted about possibly salty water flows on Mars. Of note, the NASA press release noted, moisture is likely more prevalent in the morning and the Mars Reconnaissance Orbiter does most observations in the afternoon, local time. That’s too bad, we thought. But wait! It turns out that NASA Mars Odyssey spacecraft is going to change its orbit to get a better look.
It’s going to take nearly two years for NASA to maneuver the long-running Odyssey to the right spot, but at that point mission managers expect the spacecraft still has another decade of observations ahead of it based on current fuel consumption. That’s great considering that the spacecraft has been beaming back images since 2001!
Odyssey will be the first spacecraft to do dedicated morning observations of the planet since any NASA orbiter of the 1970s, which dates observations back to the Viking era (except for a few glimpses by European Space Agency spacecraft and previous NASA orbiters). Advances in imaging mean we will get a far clearer view of the ground than ever before.
“The change will enable observation of changing ground temperatures after sunrise and after sunset in thousands of places on Mars,” NASA stated. “Those observations could yield insight about the composition of the ground and about temperature-driven processes, such as warm-season flows observed on some slopes, and geysers fed by spring thawing of carbon-dioxide ice near Mars’ poles.”
Morning water-ice clouds on Mars spotted by Viking 1 in 1976. Mars Odyssey’s new orbit will reveal more of these types of morning observations. Credit: NASA/JPL
The first maneuver took place Tuesday (Feb. 11) when a brief firing of Odyssey’s engines got the spacecraft pushing faster for an orbital shift. It will drift in that direction until November 2015, when controllers will do another maneuver to keep it in a stable location.
Right now, Odyssey is in a near-polar orbit that keeps local daylight at the same time below it. There have been a few changes to the timing over its dozen years of operation:
First six years (approx. 2001-2007): The orbit was mostly at 5 p.m. local solar time (as it flew north to south) and 5 a.m. local solar time on the south-to-north orbit. “That orbit provided an advantage for the orbiter’s Gamma Ray Spectrometer to have its cooling equipment pointed away from the sun,” NASA stated. At that time, the spectrometer found evidence of water ice, through the spectrum of hydrogen.
Next five years (approx. 2007-2012): The orbit shifted to 4 p.m. local solar time on north-to-south, and 4 a.m. south to north. While this allowed the Thermal Emission Imaging System to examine warm ground that made the mineral signatures in infrared pop out more easily, on the flip side of the planet Odyssey’s power system was under more strain because the solar panels couldn’t work as well in predawn light. Odyssey remained in that orbit until about the 2012 landing of the Curiosity rover, then was sent on a maneuver to move its orbit to later in the day to keep the battery functioning.
What’s next: Once Odyssey is in the right spot, the spacecraft will flip its daylight observations to scan the ground at 6:45 a.m. on the south-to-north part of the orbit. The spacecraft was in fact going in that direction already, but the new maneuver gets it there a bit sooner.
“We don’t know exactly what we’re going to find when we get to an orbit where we see the morning just after sunrise,” stated Philip Christensen of Arizona State University, who is THEMIS principal investigator and the person who suggested the move. “We can look for seasonal differences. Are fogs more common in winter or spring? We will look systematically. We will observe clouds in visible light and check the temperature of the ground in infrared.”
“We know that in places, carbon dioxide frost forms overnight,” he added. “And then it sublimates immediately after sunrise. What would this process look like in action? How would it behave? We’ve never observed this kind of phenomenon directly.”
A mosaic of two wide field images taken from the Nevada desert, with the view stretching from Cepheus to the Milky Way core in Sagittarius. Credit and copyright: Tanja Sund.
This gorgeous view of the Milky Way was taken by astrophotographer Tanja Sund during a trip to the desert in Nevada. Made from just two images, this long exposure (180 seconds) mosaic has incredible detail and stunning clarity. You seriously need to click on this image to see a larger version!
See more of Tanja’s work at her Flickr page. She has some beautiful night sky and aurora photos, as well as some striking landscape 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.
The issue of “what to wear?” takes on an extra dimension of life and death when it comes to space travel. Upon exiting a spacecraft on a spacewalk, an astronaut becomes his very own personal satellite in orbit about the Earth and must rely on the flimsy layer of his suit to provide them with a small degree of protection from radiation and extreme fluctuations of heat and cold.
We recently had a chance to see the past, present and future of space suit technology in the Smithsonian Institutions’ touring Suited for Space exhibit currently on display at the Tampa Bay History Center in Tampa, Florida.
Tampa Bay History Center Director of Marketing Manny Leto recently gave Universe Today an exclusive look at the traveling display. If you think you know space suits, Suited for Space will show you otherwise, as well as give you a unique perspective on a familiar but often overlooked and essential piece of space hardware. And heck, it’s just plain fascinating to see the design and development of some of these earlier suits as well as videos and stills of astronauts at work – and yes, sometimes even at play – in them.
One of the highlights of the exhibit are some unique x-ray images of iconic suits from space travel history. Familiar suits become new again in these images by Smithsonian photographer Mark Avino, which includes a penetrating view of Neil Armstrong’s space suit that he wore on Apollo 11.
X-ray images of Neil Armstrong’s historic suit on display in Suited for Space. (Photo by author).
Space suits evolved from pressure suits developed for high-altitude flights in the 1950’s, and Suited for Space traces that progression. It was particularly interesting to see the depiction of Wiley Post’s 1934 suit, complete with steel cylindrical helmet and glass portal! Such early suits resembled diving bell suits of yore — think Captain Nemo in a chemsuit. Still, this antiquated contraption was the first practical full pressure suit that functioned successfully at over 13,000 metres altitude.
Wiley Post’s 1934 “rubber bladder suit.” (Photo by author).
No suit that has been into space is allowed to tour due to the fragility of many historic originals that are now kept at the Smithsonian, though several authentic suits used in training during the U.S. space program are on display. We thought it was interesting to note how the evolution of the spacesuit closely followed the development of composites and materials through the mid-20th century. You can see the progression from canvas, glass and steel in the early suits right up though the advent of the age of plastic and modern fabrics. Designs have flirted with the idea of rigid and semi-rigid suits before settling on the modern day familiar white astronaut suit.
A x-ray photo of an EX-1A spacesuit. (Photo by author).
Spacesuit technology has also always faced the ultimate challenge of protecting an astronaut from the rigors of space during Extra-Vehicular Activity, or EVA.
Cosmonaut Alexey Leonov performed the first 12 minute space walk during Voskhod 2 back in 1965, and NASA astronaut Ed White became the first American to walk in space on Gemini 4 just months later. Both space walkers had issues with over-heating, and White nearly didn’t make it back into his Gemini capsule.
Early evolution of space suits on display at the Suited for Space exhibit. (Photo by author).
Designing a proper spacesuit was a major challenge that had to be overcome. In 1962, Playtex (yes THAT Playtex) was awarded a contract to develop the suits that astronauts would wear on the Moon. Said suits had 13 distinct layers and weighed 35 kilograms here on Earth. The Playtex industrial division eventually became known as the International Latex Corporation or ILC Dover, which still makes spacesuits for ISS crewmembers today. It’s also fascinating to see some of the alternate suits proposed, including one “bubble suit” with arms and legs (!) that was actually tested but, thankfully, was never used.
These suits were used by astronauts on the Moon, to repair Hubble, build the International Space Station and much more. Al Worden recounts performing the “most distant EVA ever” on the return from the Moon in his book Falling to Earth. This record will still stand until the proposed asteroid retrieval mission in the coming decade, which will see astronauts performing the first EVA ever in orbit around Earth’s Moon.
An A5-L Spacesuit. Credit: Smithsonian/Suited for Space.
And working in a modern spacesuit during an EVA is anything but routine. CSA Astronaut Chris Hadfield said in his recent book An Astronaut’s Guide to Life on Earth that “Spacewalking is like rock climbing, weightlifting, repairing a small engine and performing an intricate pas de deux – simultaneously, while encased in a bulky suit that’s scraping your knuckle, fingertips and collarbone raw.”
And one only has to look at the recent drama that cut ESA astronaut Luca Parmitamo’s EVA short last year to realize that your spacesuit is the only thin barrier that exists between yourself and the perils of space.
“We’re delighted to host our first Smithsonian Institution Travelling Exhibition Service (SITES) and we think that Florida’s close ties to NASA and the space program make it a great fit for us,” said Rodney Kite-Powell, the Tampa Bay History Center’s Saunders Foundation Curator of History.
Be sure to catch this fascinating exhibit coming to a city near you!
-And you can see these suits in action on the up and coming future EVAs for 2014.
-Here’s the schedule for Suited for Space Exhibit tour.
-Astronaut Nicole Stott (veteran of STS-128, -129, -133, & ISS Expeditions 20 and 21) will also be on hand at the Tampa Bay History Center on March 2014 (Date to be Announced) to present Suited for Space: An Astronaut’s View.
– Follow the Tampa Bay History Museum of Twitter as @TampaBayHistory.
NanoRacks CubeSats deployed from the International Space Station in February 2014, during Expedition 38. Credit: NASA
Astronauts fired up the International Space Station’s Yard-a-Pult (actually, we mean the Japanese Kibo arm’s satellite launcher) this week to send out a flock of Doves or tiny satellites that take pictures of the Earth below. An incredible 28 satellites from Planet Labs of San Francisco are expected to swarm into orbit — the largest fleet yet, NASA says — but there have been delays in launching some of them.
The aim? To provide Earth observation information for any purpose that is needed, whether it’s disaster relief or looking to learn more about the Earth’s environment. Planet Labs and NASA say that commercial applications could include real estate, mapping, construction and oil and gas monitoring.
Deployments of two satellites each began on Tuesday and Wednesday, but NASA noted there are “glitches” (which the agency didn’t specify) that are holding up the launch of other ones. There’s no estimated date yet for sending out the rest of the satellites.
“We believe that the democratization of information about a changing planet is the mission that we are focused on, and that, in and of itself, is going to be quite valuable for the planet,” stated Robbie Schingler, co-founder of Planet Labs.
The Japanese Kibo robotic arm on the International Space Station deploys CubeSats during February 2014. The arm was holding a Small Satellite Orbital Deployer to send out the small satellites during Expedition 38. Credit: NASA
Expedition 38’s Rick Mastracchio and Koichi Wakata both commented on the unusual launches. “Two small satellites are deployed from our launcher here on the space station. Each a little bigger than loaf of bread,” Mastracchio tweeted, while Wakata wrote, “Congratulations on the successful deploy of the satellites by the NanoRacks CubeSat Deployer and Kibo robotics!”
For more information on Flock 1, check out the Planet Labs website. You can also check out an animation of how NanoRacks CubeSats deploy in the animation below (which includes a clip from the song “We Are Young” by Fun.)
This composite view shows China’s Yutu rover heading south and away forever from the Chang’e-3 landing site about a week after the Dec. 14, 2013 touchdown at Mare Imbrium. This cropped view was taken from the 360-degree panorama. See complete 360 degree landing site panorama herein. 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
The little ‘rabbit’ beloved worldwide has now phoned home and actually survived the perils of the long lunar night and is alive and awake to start a 3rd day of scientific exploration despite suffering a serious malfunction as it entered the latest hibernation period two weeks ago.
“Yutu has come back to life!” said Pei Zhaoyu, the spokesperson for China’s lunar probe program, according to a breaking news report by the state owned Xinhua news agency.
“Experts are still working to verify the causes of its mechanical control abnormality.”
The Chang’e-3 mothership lander and piggybacked Yutu surface rover soft landed on the Moon on Dec. 14, 2013 at Mare Imbrium (Sea of Rains) – marking China’s first successful spacecraft landings on an extraterrestrial body in history.
Yutu’s new lease on life also comes after Monday’s (Feb. 11) premature report of the robots demise by the state owned China News Service, reported here.
However, “Yutu failed to power-up Monday [Feb 11] and data about its current condition and repair progress is still being collected and analyzed,” Xinhua and CCTV (China state run television) reported.
This indicates that Yutu was in fact feared lost for some time by the mission team, until further efforts finally resulted in the detection of a signal from the spacecraft – and a welcome reversal of yesterdays news!
The robot “has now been restored to its normal signal reception function,” says Pei.
Side by side screenshot photos of the Chang’e-3 moon lander (L) and the Yutu moon rover during the mutual-photograph process, at the Beijing Aerospace Control Center in Beijing, on Dec. 15, 2013. The moon rover and the moon lander took photos of each other marking the complete success of the Chang’e-3 lunar probe mission. (Xinhua/Ding Lin)
Earlier today (Feb. 12) amateur radio operators at UHF-satcom reported detection of a signal from Yutu.
But much technical work remains ahead for the engineering and science teams to ascertain why it malfunctioned and whether the six wheeled rover can be restored to partial or full functionality.
As night fell on Jan. 25, the rover entered its second two week long period of dormancy just as the rover “experienced a mechanical control abnormality,” according to a report by China’s official government newspaper, The People’s Daily.
“Experts were initially concerned that it might not be able to survive the extremely low temperatures during the lunar night.”
360-degree time-lapse color panorama from China’s Chang’e-3 lander
This 360-degree time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at three different positions 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
Each lunar day and night lasts for alternating periods of 14 Earth days.
During each long night, the Moon’s temperatures plunge dramatically to below minus 180 Celsius, or minus 292 degrees Fahrenheit.
Both solar powered probes must enter hibernation mode during each lunar night to conserve energy and protect their science instruments and control mechanisms, computers and electronics.
“The rover stands a chance of being saved now that it is still alive,” Pei stated.
Yutu, which translates as ‘Jade Rabbit’ is named after the rabbit in Chinese mythology that lives on the Moon as a pet of the Moon goddess Chang’e.
‘Jade Rabbit’ had departed the landing site forever, and was journeying southwards as the anomoly occurred – about six weeks into its planned 3 month long moon roving expedition to investigate the moon’s surface composition and natural resources.
The 140 kg Yutu robot is located some 100 m south of the lander.
Traverse Path of Yutu rover from Dec. 14 landing to Dec. 21. Landscape textured with Chang’e 3 imagery from space and ground. Credit: CNSA/BACC
Definitive word about the Chang’e-3 lander has not yet been announced. But it is expected to survive since no malfunctions have been reported. It has a 1 year design lifetime.
Xinhua stated that Chinese space officials will comment on the landers status soon.
The 1200 kg stationary lander is expected to return science data about the Moon and conduct telescopic observations of the Earth and celestial objects for at least one year.
Chang’e-3 and Yutu landed on a thick deposit of volcanic material.
The inaugural pair of probes could be the forerunners to a manned Chinese Moon landing mission a decade from now.
China’s current plans call for the Chang’e-4 Moon lander/rover to launch in 2016, perhaps with some upgrades and lessons learned from the ongoing mission.
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.
The Arecibo Observatory’s 305 meter (1,000 ft) radio telescope is undergoing emergency repair after being damaged during a 6.4 magnitude earthquake on January 13, 2014. A large cable that supports the telescope’s receiver platform had “serious damage,” according to Bob Kerr, the Director of the Arecibo Observatory.
“A protocol structural survey following the January 13 earthquake revealed serious damage to [a] short cable section, with apparent breach of several cable strands,” Kerr told Universe Today via email. “An experienced structural engineering firm was brought to assess the damage, and to consider repair options.”
The earthquake’s epicenter was located in the ocean about 60 kilometers (37 miles) northwest of Arecibo and was one of the largest to hit Puerto Rico in several years. The quake caused some floor cracking in buildings and homes on the island, as well as power outages, but no major damages or injuries, officials said. There were, however, at least 70 aftershocks with at least three of a magnitude 3.5 or greater.
The platform hangs above the Arecibo dish, supported by cables. Via Cornell University.
The famous radio observatory is located near Puerto Rico’s north coast, and opened in 1963. It was built inside a depression left by a sinkhole and is the largest curved focusing dish on Earth. The dish’s surface is made of thousands of perforated aluminum panels, each about 1 by 2 meters (3 by 6 feet), supported by a mesh of steel cables. The receiver is on a 900-ton platform suspended 137 meters (450 feet) above the dish by 18 cables running from three reinforced concrete towers.
It was one of these 18 cables that was damaged, and this particular cable was actually a known potential problem. Kerr said that during original construction of the telescope in 1962, one of the original platform suspension cables that was delivered to the observatory was too short, and another short cable section was “spliced” to provide sufficient reach to the platform.
“That cable segment and splice near the top of one of the telescope towers was consequently more rigid than the balance of the suspension system,” Kerr said. “When the earthquake shook the site, just after midnight on January 13, it is that short cable and splice that suffered damage.”
“You might say that our structural Achilles heel was exposed,” Kerr added.
Inspectors from New York’s Ammann & Whitney Bridge Construction, who have been inspecting the Arecibo observatory site since 1972, were brought in to access the situation. Kerr said a relatively low-cost (less than $100,000) repair option was designed, and materials are now being procured to complete a repair that is expected to bring the telescope back into full service.
“While the project awaits full review by the National Science Foundation, necessary steel materials for the repair are being shipped to the Observatory at this writing,” Kerr said. “Our estimated completion date for this project is March 11, 2014.”
This repair is considered temporary, however, and Kerr said a more comprehensive long-term cable repair design is being developed.
But the repair to the cable is by no means easy. The Arecibo Observatory maintenance staff will be doing the repairs themselves, working high above the ground on the 900-ton steel suspension bridge-like suspension system.
Kerr said they hope to complete this emergency repair “as expeditiously and safely as possible,” and that “it is testimony to the remarkable expertise, capability, and bravery of the Arecibo staff. I am dubious that a parallel capability exists at any other U.S. science facility.”
In the meantime, the telescope is being used only sparingly and with an “abundance of caution,” using only limited motion of the telescope. Kerr said that despite the damage, the telescope was able to continue its science mission by participation in a ten-day global ionospheric study in late January, in addition to continuing a search for pulsars in the sky above Arecibo, and searching for fast radio bursts (FRBs). Because radio telescopes can work at all times of day and in all kinds of weather, the observatory normally operates 24 hours a day. The Angel Ramos Visitor Center at the Observatory was closed for a few days, but reopened on January 22, with normal access and visiting hours.
The Observatory is recognized as one of the most important national centers for research in radio astronomy, planetary radar and terrestrial aeronomy. During its 50-plus years of use, findings from Arecibo have contributed to better understanding of the Earth’s atmosphere, the Moon, asteroids, other planets, exotic stars, our galaxy, and the large-scale galactic structure of the universe. The facility was featured in the movies “Contact” and “Golden Eye,” as well as dozens or TV shows and books, and is one of the most popular tourist attractions in Puerto Rico.
It is operated by SRI International, teaming with The Universidad Metropolitana and the Universities Space Research Association, in cooperative agreement with the National Science Foundation.
