Universe Today

February 13, 2014March 8, 2017 by Fraser Cain

How Fast Do Black Holes Spin?

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.

The Universe is a crazy place.

February 13, 2014December 23, 2015 by Elizabeth Howell

Martian Spacecraft Busts A Move To Glimpse Possible Water Flows

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 — 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.”

Sources: NASA Jet Propulsion Laboratory and Arizona State University

February 13, 2014December 23, 2015 by Nancy Atkinson

Astrophoto: Stunning Wide-Field Mosaic of the Milky Way

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.

February 13, 2014December 23, 2015 by David Dickinson

What to Wear? The History and Future of Spacesuits

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.

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.

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-20^th 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.

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.

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.

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.

February 13, 2014December 23, 2015 by Elizabeth Howell

When Doves Fly: Swarm Of Tiny Satellites Shot From Space Station

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

Flock 1 is a customer of the NanoRacks CubeSats program. CubeSats are small satellites that heavily rely on computer miniaturization to do the job of Earth observation and telecommunication that previously was the province of much larger and more expensive satellites. NanoRacks provides space both inside and outside the station for research experiments.

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.)

February 13, 2014December 23, 2015 by Ken Kremer

China’s Yutu Moon Rover Alive and Awake for 3rd Lunar Day of Exploration despite Malfunction

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

Yutu Lives!

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) — 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.

“Yutu went into sleep under an abnormal status,” Pei said.

“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 — 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 — 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.

Ken Kremer

February 12, 2014April 26, 2016 by Nancy Atkinson

Arecibo Observatory Undergoing Emergency Repairs After Earthquake Causes Damage

The Arecibo radio telescope in Puerto Rico.

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.

You can get more information about the Arecibo Observatory here, and here, or at the observatory’s Facebook page.

February 12, 2014December 23, 2015 by Nancy Atkinson

Mars’ Dingo Gap Seen From Orbit and the Ground

An orbital view from the Mars Reconnaissance Orbiter of the Curiosity rover's traverse through the Dingo Gap area of Gale crater, (top), along with a ground view from Curiosity's mastcam. Credit: NASA/JPL/University of Arizona.

Thanks to the Mars Reconnaissance Orbiter and the HiRISE camera, we have an orbital view of Dingo Gap, an opening between two low scarps which is spanned by a single dune. This gap and dune are visible both from the ground and from orbit. The Curiosity Mars rover has now crossed the gap and is continuing its travels toward enticing science destinations, including interesting veins and mineral fractures.

In the orbital image from HiRISE, the rover itself is not in this image as it was acquired before MSL landed. However, the imagery was likely used to help the rover team decide on the way to travel.

Below are more images of Dingo gap before and after the rover plowed its way through the sand.

The Curiosity rover looks back at the tracks it left after crossing through the Dingo Gap sand dune. Credit: NASA/JPL, Caltech. Via Doug Ellison on Twitter.

The series of nine images making up this animation were taken by the rear Hazard-Avoidance Camera (rear Hazcam) on NASA’s Curiosity Mars rover as the rover drove over a dune spanning “Dingo Gap” on Mars. Image credit: NASA/JPL-Caltech

The orbital view of Gale Crater and the Dingo Gap region. Credit: NASA/JPL/University of Arizona.

Curiosity looks back to ‘Dingo Gap’ sand dune after crossing over, backdropped by Mount Sharp on Sol 535, Feb. 5, 2014. Hazcam fisheye image linearized and colorized. Credit: NASA/JPL/Marco Di Lorenzo/Ken Kremer- kenkremer.

Curiosity’s view to valley beyond after crossing over ‘Dingo Gap’ sand dune. This photomosaic was taken after Curiosity drove over the 1 meter tall Dingo Gap sand dune and shows dramatic scenery in the valley beyond, back dropped by eroded rim of Gale Crater. Assembled from navigation camera (navcam) raw images from Sol 535 (Feb. 6, 2104) Credit: NASA/JPL-Caltech/Ken Kremer- kenkremer.com/Marco Di Lorenzo

February 12, 2014April 26, 2016 by Elizabeth Howell

Who Wants A One-Way Trip To Mars? Meet Three People Applying For Mars One

Three Mars One applicants that made it to the second round. From left, Max Fagin, Brian Hinson and Andrew Rader. (All pictures provided by the respective subjects of the photos).

If you were to find yourself on the Red Planet, what would you do when you get there? Those who made the second round of the Mars One mission (which aims to establish a colony on Mars in the next decade) are a step closer to answering that question. In interviews with Universe Today, applicants Andrew Rader, Max Fagin and Brian Hinson explained what they’ll do if they embark on a planned one-way trip to the Red Planet.

It’s impossible in three interviews to capture the diversity of more than 1,000 second-round applicants, so we encourage you to head over to Mars One’s website to browse the full list of people. As for these three would-be Marstronauts, we have their application videos and their plans for Mars exploration below the jump.

Max Fagin, 26, United States

With a resume including the NASA Academy and the Mars Desert Research Station, you’d expect that Fagin would be interested in the conventional astronaut program. He wants to try for Mars One first, however, because the Red Planet is the destination he prefers.

“Applying to become an astronaut at NASA is still an option, but at the moment they don’t have Mars as a destination,” he said. “Right now it’s the asteroids, which is cool, I’d love to see that, but it’s not something I’m willing to risk my life over.” Going to Mars would provide a greater payoff, he added, in that a new home base could be established for humanity.

One question intriguing Fagin is how to make a vehicle that travels to Mars better optimized to be used on the surface. He believes that the design will need to be changed somehow post-landing to make it possible to perform agriculture and do other duties on station. (He is in fact doing graduate engineering work at Indiana’s Purdue University right now to study more about this problem.)

Fagin is looking forward to diversifying his training if he does get selected. He’s strong in engineering, he said, but feels that learning medical skills, for example, will position all crew members well to work on the surface.

Brian Hinson, 44, United States

As you can see by the application video, Hinson is not afraid of standing out. He’s been to 39 countries and describes himself as experienced in learning about different cultures. He’s a private pilot and has also tested himself physically, for example by mountain-climbing to altitudes above 19,685 feet (6,000 meters).

“The whole Mars thing came up, and it sounds like the greatest adventure of all time,” said Hinson, who co-founded the company Skin Beautiful Dermaceuticals with his wife, Kathleen Eickholt (who is supportive of the Mars mission, but doesn’t necessarily want him to leave, he adds).

Hinson is a lifelong space enthusiast, but says his math capabilities weren’t enough to consider the NASA astronaut program. He would contribute to the mission as an engineer: “I think I could help out with hydroponics, recycle the water and everything else … [and also] picking up samples for scientists back home.”

From spending as long as 2.5 weeks on trips with strangers, Hinson added that he thinks psychological aspects will be key to success of the crew. He added that he expects the Mars One training process will include extended periods of time in isolation, perhaps something similar to the six months a science crew typically spends in Antarctica.

Andrew Rader, 34, Canada

Rader’s skills span both the technical and the human, as he earned a Ph.D. in aerospace engineering from the Massachusetts Institute of Technology and also was crowned “Canada’s Greatest Know-It-All” in a reality show competition hosted by the Discovery Channel. Mars One will only succeed as a venture if it can be “sold” to the public as a worthy endeavor, he said, adding that space enthusiasts will be among the hardest to convince because of their knowledge.

“Mars One could possibly happen if it gains enough support, if everyone donated a dollar, or space enthusiasts donated a hundred dollars [each], or billionaires donated a chunk, it could happen,” he added.

He characterizes the first few years of the colony as a time when people need to focus on the basic parts of Maslow’s hierarchy of needs. Keeping people safe and fed will come before scientific return for the first bit. His first goal on the surface will be to make the base as self-sustaining as possible. If that works out, he’d be happy to do things such as maintain rovers to pick up samples for people to analyze back at a Mars “lab”. (Having robots do surface exploration would reduce the risk of radiation, he said.)

Space is the long-term solution to the survival of our species, Rader adds, with the ultimate destination being outside the solar system. To get there first, however, you need stepping stones, and he believes Mars is the most likely destination for humans. “Mars is a very challenging place to go for us, but it is within our technological capabilities, and going there would create the technological incentives to go further.”

February 12, 2014March 8, 2017 by Fraser Cain

What are Hot Jupiters?

This artist's conception illustrates the brown dwarf named 2MASSJ22282889-431026. NASA's Hubble and Spitzer space telescopes observed the object to learn more about its turbulent atmosphere. Brown dwarfs are more massive and hotter than planets but lack the mass required to become sizzling stars. Their atmospheres can be similar to the giant planet Jupiter's. Spitzer and Hubble simultaneously observed the object as it rotated every 1.4 hours. The results suggest wind-driven, planet-size clouds. Image credit: — This artist's conception illustrates what a "hot jupiter" might look like.

When astronomers first discovered other planets, they were completely unlike anything we’ve ever found in the Solar System. These first planets were known as “hot jupiters”, because they’re giant planets – even more massive than Jupiter – but they orbit closer to their star than Mercury. Dr. Heather Knutson, a professor at Caltech explains these amazing objects.

“My name is Heather Knutson, and I’m a professor in the planetary science department here at Caltech. I study the properties of extrasolar planets, which are planets that orbit stars other than the sun, so mostly these are our closest exoplanetary neighbors. We’re not talking about planets in other galaxies – we’re mostly talking about planets which are in the same part of our own corner of our galaxy. So these are around some of the closest stars to the sun.”

What is a hot jupiter?

“The planets that I’ve found the most surprising, out of all of the ones I’ve discovered so far, I guess the sort of classic example, is that we’ve see these sorts of giant planets which are very similar to Jupiter, but orbit very much closer in than Mercury is to our sun, so these planets orbit their sun every two or three days and are absolutely getting roasted. We know that they couldn’t have formed there – they had to have formed farther out and migrated in, so what we’re still trying to understand are what are the forces that caused them to migrate in, whereas Jupiter seems to have migrated a little bit but more or less stayed put in our own solar system.”

What do hot jupiters mean for our understanding our own Solar System?

“The implications of these “hot jupiters” as we call them are actually huge for our own solar system, because if you want to know how many potentially habitable earthlike planets are out there, having one of these giant planets just rampage their way though the inner part of the planetary system, and it could toss out your habitable earth and put it into either a much closer orbit or a much further orbit. So knowing how things have moved around will tell you a lot about where you might find interesting planets.”

What is their atmosphere like?

“So, the atmospheres of hot jupiters are very exotic, by solar system standards. They typically have temperatures of a thousand to several thousand Kelvin, so at these temperatures these planets could have clouds of molten rock, for example. They have atmospheric compositions that would seem very exotic to us – they’re actually more similar to the compositions of relatively cool stars, so we have to adapt to describe these planets – we actually use stellar models to describe their atmospheres. We think that they’re also probably also tidally locked, which is very interesting because it means that one side of the planet is getting all of the heat and the other side is sort of in permanent night. And one thing we do is to try and understand the effect that has on the weather patterns on these planets, so you have winds that are pretty good at carrying that around the night side and mixing everything up, or do these planets have these just extreme temperature gradients between the day side and the night side.”

How’d they get there?

“So, we have a couple of theories for how hot jupiters may have ended up in their present day orbits. One theory is, that after they formed, that they were still embedded in the gas disc where they formed, and maybe they interacted with the disc as such that it kind of torqued and pulled them and so that’s kind of an early migration theory. There’s also a late migration theory version where when after the disc had gone away, these planets had interacted with a third body in the system, so maybe you had another distant massive planet or maybe you had a planet that was part of a binary star system, and those three body interactions excited a large orbital eccentricity in the innermost planet, and once it starts coming in closer to the star, the tides start to damp out the eccentricities, so what you end up with is something which is a gas giant planet in a very short period circular orbit.

So that’s kind of a more complicated story, but there are some clues in the data that might be true for at least a subset of the hot jupiters that we study.”