Mars Archives

November 7, 2014December 23, 2015 by Matt Williams

Canadian Micro-Rover and Lander “Northern Light” Aim for Launch to Mars in 2018

Artist's concept of the Norther Light Lander on the Martian surface. Credit: Mars Rocks

The first Canadian mission to Mars could be blasting off towards the Red Planet in just three years time. At least, that is what Thoth Technology, a Canadian aerospace company from Pembroke, Ontario, hopes to accomplish. And two days ago, they launched an Indiegogo campaign to raise the 1.1 million dollars needed to pay for all the hardware needed to make the mission happen.

If it is successful, it would be first Canadian mission to the surface of Mars.

The project for this Canadian mission would involve sending the Northern Light lander and Beaver rover in space and land them on Mars. Once there, the Beaver rover will be deployed and begin conducting surveys of the Martian surface, alongside the many other robotic rovers and orbiters studying the Martian landscape.

“I think it’s important to do big things,” said Ben Quine, principal investigator for the mission. “Mars is the only other habitable planet in the solar system, and if we want to survive, we need to be a multi-planet species.”

Quine is the technical director and chair of the board at Thoth Technology and a professor of space engineering at York University, which is a partner on the project, houses a lot of the space testing facilities, and will analyze the data from the mission.

*Northern Light Lander and Robotic Arm (concept art). Credit: Mars Rocks/Indiegogo*

The main goal of the mission is to expand upon the efforts being made by NASA’s Curiosity, Spirit, and Opportunity rovers, which have only explored a half dozen sites on Mars. By exploring more areas, they hope to find other signs of life on the harsh landscape, and using knowledge gleaned from studies in the Canadian Arctic no less.

According to Quine, in Antarctica and the Canadian Arctic, photosynthetic microbes can be found in a layer a millimeter or two below the surface of the rock. Here, they are protected from the harshest of the sun’s UV rays, but can still use sunlight to produce energy.

Northern Light will look for similar life on Mars by using the lander’s robotic arm to grind away the surface of rocks. It will then use a device called a photometer to scan for different shades of green that may indicate the presence of photosynthetic organisms. Quine and his colleagues also hope to determine what future technologies will be required to sustain a future human presence.

“If we are serious about living on Mars,” he said, “we need to explore it much more thoroughly. We probably need hundreds of landers to pepper the surface prior to sending people so we know exactly what it is that we’re up against, where we’d find things like minerals and where we’d want to live.”

Intrinsic to the company’s plan is the widespread exploration of Mars using low cost, off-the-shelf technology. For example, the Northern Light lander probe has a mass under 50 kg (including payload) and is made of an advanced composite material that includes thermal shielding and shock absorption. The probe includes solar arrays to generate power for the instrumentation and lander avionics.

*The Beaver Rover prototype. Credit: Thoth Technologies/Indiegogo*

As for the Beaver rover, its small size and low-cost mask the fact that it is like no other rover that has ever gone to Mars. For one thing, it weighs just six kilograms (13 pounds). In comparison, NASA’s Curiosity rover weighs in at a hefty 900 kilograms (1980 pounds, close to an imperial ton), forcing it to rely largely on nuclear power to lug its bulk around.

The NASA rovers, which are controlled from Earth, also move very slowly and cover only a few dozen meters per day because their commands take 15 minutes to reach Mars from Earth. By contrast, the Beaver rover is designed to be quicker, in part by being more independent.

“We’re going to embed intelligence into the rover,” Quine said, “and the rover is going to be tasked to drive around and explore the environment using autonomous algorithms built into the rover to determine things like when it should make a maneuver to avoid falling into a hole or run into a rock.”

Quine said he has already spent 12 years working on the project and his team has spent half a million dollars developing and testing prototypes of the lander and micro-rover. They’ve also performed space tests on some of the instruments by flying them on satellites in low-Earth orbit.

*Northern Light Ground Station at the Algonquin Radio Observatory. Credit: Mars Rocks/Indiegogo*

Thoth Technologies also recently spent $1 million leasing and repairing the Algonquin Radio Observatory from the federal government, which they plan to use as a ground station to communicate with the lander and rover when they are on Mars.

As for the tricky task of getting to Mars, Quine and his colleagues hope to barter their way aboard one of the many missions heading to Mars in 2018. These include the joint Russian-European Space Agency ExoMars rover mission and an Indian Space Research Organization mission that will likely include a lander and rover.

In exchange for hitching a ride on one of these rockets, they will collect and relay other agencies’ data from Mars via the ARO ground station, which can collect them at times of day when places like Russia and India are facing away from Mars.

Those who are interested in supporting their campaign are being incentivized with a chance to help choose the landing site for the mission, and will get rewards ranging from a Frisbee for $20 or the chance to name the lander for $1 million.

The company has also launched a social campaign – featuring Ed Robertson of the “Barenaked Ladies” – urging people to create and upload their own “Mars dance” video to marsrocks.ca.

To find out more, check out their promotional video or click on the link below:

Further Reading: Mars Rocks

November 6, 2014December 23, 2015 by Bob King

Curiosity Rover Sees a Pixel’s-Worth of Comet Siding Spring

In this panoramic view taken by NASA's Curiosity Rover on October 19th shortly after local sunset (6:11 p.m.), Comet Siding Spring is the single bright pixel at far upper left. Click for a high resolution version. Credit: NASA/JPL-Caltech/Malin Space Science Systems/James Sorenson

When Comet Siding Spring skimmed just 84,500 miles from Mars last month, NASA’s Opportunity and Curiosity Rovers – along with several orbiting Mars spacecraft – readied their cameras to record the historic flyby. Opportunity’s photos revealed a small, fuzzy blob against the stars of Cetus the Whale, but most of us searched in vain to find any trace of the comet among the blizzard of noise in pictures snapped by Curiosity. Yet it may be there after all.

In this before and after animation, you can see how much noise needed to be cleaned from one of the original photos to uncover the the comet. Credit: NASA/JPL-Caltech/Malin Space Science Systems/James Sorenson — In this before-and-after animation, you can see how much noise needed to be cleaned from the original photos to uncover the the comet. Credit: NASA/JPL-Caltech/Malin Space Science Systems/James Sorenson

In this panoramic image at top, assembled and processed by James Sorenson to remove the pervasive noise in the original photos, we see with a twilit landscape just after sundown. Look closely in the upper left hand corner and you’ll see a speck of light. That’s it! Combined with positional information, Sorenson tentatively identified that pixel as Comet C/2013 A1 Siding Spring. OK, it’s not much to look at but may be our best candidate for the hoped-for photo from Curiosity.

Comet Siding Spring near Mars in a composite image by the Hubble Space Telescope, capturing their positions between Oct. 18 8:06 a.m. EDT (12:06 p.m. UTC) and Oct. 19 11:17 p.m. EDT (Oct. 20, 3:17 a.m. UTC). Credit: NASA, ESA, PSI, JHU/APL, STScI/AURA

Remember that conditions were far from ideal when the picture was taken. There was considerable dust and haze in the Martian atmosphere over Gale Crater. Dust effectively absorbs and also scatters light. The bright twilight sky only made the comet more difficult to discern. If you’ve ever struggled to see Mercury at dusk on a hazy summer evening, you’ll understand what our robot was up against.

This animation combines multiple images that were acquired by the HRSC camera on board Mars Express during the comet Siding Spring flyby on October 19, 2014. Click to animate Credit: ESA/DLR/FU Berlin — This single image is one of series that were acquired by the HRSC camera on board Mars Express during the comet Siding Spring flyby on October 19, 2014. Click to animate. Credit: ESA/DLR/FU Berlin

The European Space Agency’s Mars Express orbiter also chimed in with a recent set of comet images. As it flew by, Siding Spring was traveling at around 35 miles per second (56 km/sec) relative to Mars. Images were acquired at 17-second intervals at a resolution of 10.5 miles (17 km) per pixel. What do they show? The irregular shape might make you might think you’re seeing the actual shape of the comet’s nucleus. Unfortunately, that’s impossible because it’s less than a kilometer across and each pixel in the photo spans 17 km. Instead, we’re seeing the combined light of the nucleus and extended coma, the surrounding cloud of gas and dust. Why the images are pure black and white with no grey tones is unclear.

Two photos of comet C/2013 A1 Siding Spring taken 37 minutes apart by the CRISM imager. The subtle coloration of the comet indicates the abundance of different molecules. Credit: NASA / JPL / JHUAPL — Two photos of comet C/2013 A1 Siding Spring taken 37 minutes apart by the CRISM imager when the comet was closest to Mars. The subtle colors seen are likely related to dust grain size or composition. The nucleus itself is not resolved. Credit: NASA/JPL/JHUAPL

Besides the the close-up photo taken with the HiRISE camera on NASA’s Mars Reconnaissance Orbiter, its Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) got busy photographing the dusty inner coma generated when sunlight warms and vaporizes dust-laden ice in the nucleus. The scale of the left image is approximately 2.5 miles (4 km) per pixel; for the right image, it is about 3 miles (5 km) per pixel.

According to NASA, CRISM observed 107 different wavelengths of light in each pixel. Here, only three colors are shown. Researchers think the appearance of color variations in the inner coma could be due to the properties of the comet’s dust, possibly dust grain size or composition. More photos and results from all the spacecraft will appear in the weeks and months ahead as scientists continue their analyses.

Comet Siding Spring shows a condensed coma and a short, faint tail in this photo taken on November 5, 2014. Credit: Alfons Diepvens — Comet Siding Spring shows a condensed coma and hint of a tail in this photo taken on November 5, 2014. Credit: Alfons Diepvens

Comet Siding Spring has left Mars and its crew of robotic eyes behind as it crawls north into the constellation Serpens low in the southwest at dusk. Amateur astronomers are still keen to photograph it at every opportunity. Recent observations indicate a temporary re-brightening, though the comet remains a dim 11th magnitude object.

November 6, 2014December 23, 2015 by Elizabeth Howell

Mars Habitability? Curiosity Rover Spots Intriguing Mineral On Red Planet

A view from the Curiosity rover on Sol 794 (Oct. 31, 2014) from its outpost at the base of Mount Sharp (Aeolis Mons). Credit: NASA/JPL-Caltech

NASA’s Curiosity rover has struck hematite — an iron-oxide mineral often associated with water-soaked environments — in its first drill hole inside the huge Mount Sharp (Aeolis Mons) on Mars. While in this case oxidization is more important to its formation, the sample’s oxidization shows that the area had enough chemical energy to support microbes, NASA said.

Hematite is not a new discovery for Curiosity or Mars rovers generally, but what excites scientists is this confirms observations from the Mars Reconnaissance Orbiter that spotted hematite from orbit in the Pahrump Hills, the area that Curiosity is currently roving.

“This connects us with the mineral identifications from orbit, which can now help guide our investigations as we climb the slope and test hypotheses derived from the orbital mapping,” stated John Grotzinger, Curiosity project scientist at the California Institute of Technology in Pasadena.

This is the latest in a series of finds for the rover related to habitability. In December 2013, scientists announced it found a zone (dubbed Yellowknife Bay) that was likely an ancient lakebed. But Yellowknife’s mineralogy eluded detection from orbit, likely due to dust covering the rocks.

Photo mosaic shows NASA’s Curiosity Mars rover in action reaching out to investigate rocks at a location called Yellowknife Bay on Sol 132, Dec 19, 2012 in search of first drilling target. The view is reminiscent of a dried up shoreline. Curiosity’s navigation camera captured the scene surrounding the rover with the arm deployed and the APXS and MAHLI science instruments on tool turret collecting microscopic imaging and X-ray spectroscopic data. The mosaic is colorized. See the full 360 degree panoramic and black & white versions below. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo — Photo mosaic shows NASA’s Curiosity Mars rover in action reaching out to investigate rocks at a location called Yellowknife Bay on Sol 132, Dec 19, 2012, in search of first drilling target. The view is reminiscent of a dried up shoreline. Curiosity’s navigation camera captured the scene surrounding the rover with the arm deployed and the APXS and MAHLI science instruments on tool turret collecting microscopic imaging and X-ray spectroscopic data. The mosaic is colorized. See the full 360 degree panoramic and black & white versions below. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo

Hematite is perhaps most closely associated with spherical rocks called “blueberries” that the Opportunity rover discovered on Mars in 2004. While Opportunity’s discovery showed clear evidence of water, the new Curiosity find is more closely associated with oxidization, NASA said.

The new find, contained in a pinch of dust analyzed in Curiosity’s internal Chemistry and Mineralogy (CheMin) instrument, yielded 8% and 4% magnetite. The latter mineral is one way that hematite can be created, should magnetite be placed in “oxidizing conditions”, NASA stated. Previous samples en route to Mount Sharp had concentrations only as high as 1% hematite, but more magnetite. This shows more oxidization took place in this new sample, NASA stated.

Curiosity will likely stick around Pahrump Hills for at least weeks, perhaps months, until it climbs further up the mountain. Among Mount Sharp’s many layers is one that contains so much hematite (as predicted from orbit) that NASA calls it “Hematite Ridge.”

Source: NASA

November 3, 2014December 23, 2015 by Matt Williams

Welcome to Mars! – Hi-SEAS and Mars Society Kick Off New Season of Missions

The Hawaii Space Exploration Analog and Simulation (aka. Hi-SEAS) – a human spaceflight analog for Mars located on the slopes of the Mauna Loa volcano in Hawaii – just kicked off its third research mission designed to simulate manned missions on Mars.

Located at an elevation of 2500 meters (8,200 feet) above sea level, the analog site is located in a dry, rocky environment that is very cold and subject to very little precipitation. While there, the crew of Mission Three will conduct detailed research studies to determine what is required to sustain a space flight crew during an extended mission to Mars and while living on Mars.

The six-member team includes Martha Lenio (Commander), Allen Mirkadyrov, Sophie Milam, Neil Sheibelhut, Jocelyn Dunn, and Zak Wilson, with Ed Fix and Micheal Castro in Reserve. This crew will spend the next 254 days living in conditions that closely resemble those present on the Martian surface.

Research into food, crew dynamics, behaviors, roles and performance, and other aspects of space flight and a mission on Mars itself is the primary focus. This will be the third of four research missions conducted by Hi-SEAS and funded by the NASA Human Research Program. The information gleaned from these research studies, it is hoped, will one day help NASA conduct its own manned missions to the Red Planet.

*Artist conception of a Hi-SEAS habitation dome. Credit: Blue Planet Research/Bryan Christie Design*

For the course of their research studies, the crew will be living in a dome that is 11 meters (36 feet) in diameter and has a living area of about 93 square meters (1000 square feet). The dome also has a second level that is loftlike – providing a high-ceiling is crucial to combating long-term feelings of claustrophobia.

The six crew members will sleep in pie-slice-shaped staterooms, each of which contains a mattress, desk and stool. Their clothing is stored under the bed, which sits at the wide side of the slice. They do their business in a series of composting toilets that turn their repurposed feces (the pathogens are removed) into a potential source of fertilizer for the next mission.

A workout area provides the astronauts with an opportunity to stay in shape with such exercises as video aerobics, juggling, and balloon volleyball. And communications are conducted through NASA-issued email addresses – with an artificial delay to simulate the time lag from Mars – and access to a web made of cached, nondynamic pages.

To complete the illusion of being on Mars, when the crew are not in their pressurized habitation dome, they will be walking around in space suits. The mission will conclude on July 14th, 2015, with a fourth and final mission to take place at a so-far undetermined date.

Image Credit: Mars Society MRDS — *The Mars Society’s Mars Desert Research Station in southern Utah.*
*Credit: Mars Society MRDS*

In related news, the Mars Society announced yesterday that Crew 142 arrived at the Mars Desert Research Station (MDRS) in southern Utah to begin the 2014-15 MDRS field season. Crew 142, consisting of seven people, is the first of three crews composed of finalists for the planned Mars Arctic 365 (MA365) mission that will serve at MDRS for two weeks of training and testing.

Once their training is complete, crew 142 will be shipping off to the Flashline Mars Arctic Research Station (FMARS) located on Devon Island in northern Canada, followed shortly behind by the other MA365 finalists, for a year-long research stint.

Much like the Hi-SEAS project, the Mars Society is a non-profit space advocacy organization that is dedicated to promoting the human exploration and settlement of Mars. Established by Dr. Robert Zubrin and colleagues in 1998, the organization works to educate the public, the media, and government on the benefits of Mars exploration and the importance of planning a manned mission in the coming decade.

For the next two weeks, the seven finalists will be engaged in activities designed to simulate conditions on another planet. For the duration, they will be living and working in the Mars Analog Research Stations (MARS) – a prototype of the habitat that the Mars Society plans to eventually land on Mars and serves as the crew’s main base as they explore the harsh Martian environment.

*FMARS hab with Mars flag in foreground. Credit: Mars Society*

Ultimately, these analog experiments offer NASA and other space research groups the opportunity to carry out field research in a variety of key scientific and engineering disciplines that will help prepare humans to explore Mars in the coming years.

For one, it lets research crews know what kinds of work they can physically do when fully suited up, and just how well their suits can hold up to months’ worth of activity. At the same time, it allows for psychological studies and human factor issues – like testing the effects of isolation on human beings, and whether or not the habitats will suffice for long periods of occupation.

Above all, it lets us see how human beings with different skills sets and tasks can function together as a whole in a Martian environment. On any given day, astronauts in these analog environments are tasked with working within the pressurized habitats, out in the field, or far away using pressurized rovers or un-pressurized vehicles.

At the same time, it offers the opportunity for research crews to test out being in an isolated environment, connected to mission control and the terrestrial scientific community only through official communications.

And of course, there’s also the matter of the astronauts’ being connected to each other and robots in the field. Making these different assets work together to achieve the maximum possible exploration effect requires developing a combined operations approach, which is another aim of Hi-SEAS, the Mars Society, and other research groups.

Further Reading: Hi-SEAS, Mars Society

October 24, 2014December 23, 2015 by Elizabeth Howell

Comet Siding Spring Was Bleeding Hydrogen As It Sped By Mars

Comet Siding Spring shines in ultraviolet in this image obtained by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft. Credit: Laboratory for Atmospheric and Space Physics/University of Colorado; NASA

As Comet Siding Spring passed close by Mars on Sunday (Oct. 19), NASA’s newest Mars spacecraft took a time-out from its commissioning to grab some ultraviolet pictures of its coma. What you see above is hydrogen, a whole lot of it, leaving the comet in this picture taken from 5.3 million miles (8.5 million kilometers).

The hydrogen is a product of the water ice on the comet that the Sun is slowly melting and breaking apart into hydrogen and oxygen molecules. Because hydrogen scatters ultraviolet light from the Sun, it shows up rather clearly in this picture taken by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft.

Check out more recent pictures of Siding Spring below.

Is this an image of Comet Siding Spring? It's the only fuzzy object in the field photographed on Sol 3817 (October 19) by the Opportunity Rover. Click for original raw image. — Is this an image of Comet Siding Spring? It’s the only fuzzy object in the field photographed on Sol 3817 (October 19) by the Opportunity Rover. Click for original raw image.

Another photo, just in, taken of the comet and Mars today (Oct. 19) by Rolando Ligustri. Beautiful!

Comet 2013 A1 Siding Spring on October 17, 2014, with two days to go until its Martian encounter. Very dense Milkyway starfield in the background with many darker obscured regions. Credit and copyright: Damian Peach.

October 23, 2014December 23, 2015 by Elizabeth Howell

Hubble Composite Picture Shows How Close Siding Spring Comet Was To Mars

We’ve seen spectacular images of Comet Siding Spring from Mars spacecraft, showing just how close the small body was to the Red Planet when it whizzed by Sunday (Oct. 19). But how close were the two objects actually, in the sky? This Hubble Space Telescope composite image shows just how astoundingly near they were.

Above are two separate exposures taken Oct. 18-19 EDT (Oct. 18-20 UTC) against the same starry field image from another survey. It was a complicated shot to get, NASA explains, but it does serve as a powerful illustration of the celestial close encounter.

“This is a composite image because a single exposure of the stellar background, comet Siding Spring, and Mars would be problematic. Mars is actually 10,000 times brighter than the comet, and so could not be properly exposed to show detail in the Red Planet,” NASA stated.

“The comet and Mars were also moving with respect to each other and so could not be imaged simultaneously in one exposure without one of the objects being motion blurred. Hubble had to be programmed to track on the comet and Mars separately in two different observations.”

The two images were blended together in this single shot, showing their separation of 1.5 arc minutes (1/20 of the Moon’s apparent diameter.) The background stars comes from data from the Palomar Digital Sky Survey “reprocessed to approximate Hubble’s resolution”, NASA stated.

While the nucleus is too small to be imaged by Hubble, you can see what it looks like in the image above from the Mars Reconnaissance Orbiter. Siding Spring passed by the Red Planet at a distance of just 87,000 miles (140,000 km).

Source: NASA

October 22, 2014December 23, 2015 by Elizabeth Howell

This 3-D Martian Picture Feels Like You’re Standing Beside The Opportunity Rover

A 3-D image of "Wdowiak Ridge" on Mars, based on images from the left and right side of the Opportunity rover's Pancam. Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.

Grab your 3-D glasses (you do have a pair handy, right?) and take a look at this latest vista from Mars. This is a view taken by the Opportunity rover that looks at a location nicknamed “Wdowiak Ridge”, on the rim of Endeavour Crater.

This mosaic was obtained Sept. 17 as Opportunity continued its journey to “Marathon Valley”, a spot that could hold clays (which would indicate a water-rich environment in the past.) The rover is more than a decade into its mission and has been sending back images amid battling Flash memory problems lately.

Check out more recent pictures below, including a probable one of Comet Siding Spring passing by Mars (which Bob King wrote about in detail earlier this week.)

“Wdowiak Ridge sticks out like a sore thumb. We want to understand why this ridge is located off the primary rim of Endeavour Crater and how it fits into the geologic story of this region,” stated Jim Rice, the Opportunity science-team of the Planetary Science Institute in Arizona.

More specifically, the team is interested in why this ridge is so prominent and sharp — they are calling it one of the most distinctive features Opportunity has ever seen. How it resisted erosion in an area so worn down is one thing scientists are hoping to learn about.

A Martian mosaic showing "Wdowiak Ridge", which the Opportunity rover imaged Sept. 17, 2014. The rover's tracks are visible at right. Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ. — A Martian mosaic showing “Wdowiak Ridge”, which the Opportunity rover imaged Sept. 17, 2014. The rover’s tracks are visible at right. Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.

The last Opportunity rover update talks about activities through Sept. 30, but NASA has released raw images available since then. Check out a selection below.

The Opportunity rover at work on Mars on Sol 3,817 in October 2014. Credit: NASA/JPL-Caltech

An image of Martian terrain with the Opportunity's rover solar panel just visible at the bottom of the panel. Picture taken Sol 3,817 in October 2014. Credit: NASA/JPL-Caltech — An image of Martian terrain with the Opportunity’s rover solar panel just visible at the bottom of the panel. Picture taken Sol 3,817 in October 2014. Credit: NASA/JPL-Caltech

A dramatic, shadowy picture showing part of the Opportunity rover on Mars lit by the Sun (at top). Picture taken Sol 3,812 in October 2014. Credit: NASA/JPL-Caltech

The Opportunity rover's tracks dominate this image taken on Mars on Sol 3,807 in October 2014. Credit: NASA/JPL-Caltech — The Opportunity rover’s tracks dominate this image taken on Mars on Sol 3,807 in October 2014. Credit: NASA/JPL-Caltech

October 22, 2014December 23, 2015 by Ken Kremer

Stunning View of Solar System’s Largest Volcano and Valles Marineris Revealed by India’s Mars Orbiter Mission

Olympus Mons, Tharsis Bulge trio of volcanoes and Valles Marineris from ISRO's Mars Orbiter Mission. Note the clouds and south polar ice cap. Credit: ISRO

India’s Mars Orbiter Mission (MOM) has delivered another sweet treat – a stunning view of our Solar System’s largest volcano and the largest canyon.

Just days ago, MOM captured a new global image of the Red Planet dominated by Olympus Mons and Valles Marineris – which is the largest known volcano and the largest known canyon in the Solar System, respectively.

Situated right in between lies a vast volcanic plateau holding a trio of huge volcanoes comprising the Tharsis Bulge: Arsia Mons, Pavonis Mons, and Ascraeus Mons. All four volcanoes are shield volcanoes.

To give an idea of its enormity, Olympus Mons stands about three times taller than Mount Everest and is about the size of Arizona.

Olympus Mons from Mars orbit compared to the state of Arizona. Credit: NASA

Olympus Mons is located in Mars’ western hemisphere and measures 624 kilometers (374 miles) in diameter, 25 km (16 mi) high, and is rimmed by a 6 km (4 mi) high scarp.

Valles Marineris is often called the “Grand Canyon of Mars.” It spans about as wide as the entire United States.

The Indian Space Research Organization (ISRO), India’s space agency which designed and developed the orbiter released the image on Oct. 17, barely two days ahead of the planet’s and spacecrafts’ extremely close encounter with comet Siding Spring.

By the way, a relieved ISRO tweeted MOM’s survival of her close shave with the once-in-a-lifetime cometary passage with gusto, soon after the swingby:

“Phew! Experience of a lifetime. Watched the #MarsComet #SidingSpring whizzing past the planet. I’m in my orbit, safe and sound.”

The new global image was taken by the tri-color camera as MOM swooped around the Red Planet in a highly elliptical orbit whose nearest point to Mars (periapsis) is at 421.7 km and farthest point (apoapsis) at 76,993.6 km, according to ISRO.

To date ISRO has released four global images of the Red Planet, including a 3-D view, reported here.

Olympus Mons, the Tharsis Bulge, and Valles Marineris are near the equator.

Valles Marineris stretches over 4,000 km (2,500 mi) across the Red Planet, is as much as 600 km wide, and measures as much as 7 kilometers (4 mi) deep.

Here’s a comparison view of the region taken by NASA’s Viking 1 orbiter in the 1970s.

Global Mosaic of Mars Centered on Valles Marineris from NASA’s Viking 1 orbiter. Credit: NASA

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

The $73 million MOM mission is expected to last at least six months.

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

With MOM’s arrival, India became the newest member of an elite club of only four entities that have launched probes that successfully investigated Mars – following the Soviet Union, the United States, and the European Space Agency (ESA).

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

Ken Kremer

ISRO's Mars Orbiter Mission captures spectacular portrait of the Red Planet and swirling dust storms with the on-board Mars Color Camera from an altitude of 74500 km on Sept. 28, 2014. Credit: ISRO — ISRO’s Mars Orbiter Mission captures spectacular portrait of the Red Planet and swirling dust storms with the on-board Mars Color Camera from an altitude of 74,500 km on Sept. 28, 2014. Credit: ISRO

October 21, 2014December 23, 2015 by Elizabeth Howell

Martian Permafrost And Dust-Sculpted Surface Captured By NASA Spacecraft

Frost deposits in Louth Crater appears to remain through the year, as found in Mars Reconnaissance Orbiter HiRISE photos of the region. Credit: NASA/JPL/University of Arizona

Mars was once thought to be a fairly unchanging planet, similar to the Moon. But now we know it is a planet that was shaped by water and other forces in the past — and that these forces still come into play today.

Above is a picture of permafrost deposits just discovered in Louth Crater. This find comes from NASA’s Mars Reconnaissance Orbiter’s High Resolution Imaging Science Experiment (HiRISE) and you can see some of its latest water- and dust- shaped environments imaged below.

“A still-unexplained feature of this crater is the diffuse dark smudges visible on the crater floor,” read an update on the University of Arizona HiRISE website explaining this image. “These resemble ‘defrosting spots’ which are visible on carbon dioxide ice in the early spring, but they occur on frost-free areas and survive throughout the summer.”

The frost was caught in a HiRISE image early in the summer, and it persisted as controllers watched it through the summer — indicating that it is permanent. Its size did diminish somewhat, however. Scientists are pretty sure that this is water ice, as carbon dioxide can’t survive the summer.

See more new HiRISE photos below.

A close-up of "chaotic terrain" in Valles Marineris imaged by the Mars Reconnaissance Orbiter's HiRISE camera. Wind or fluid may have further shaped this region, which could be related to possible signs of an ancient lake found in other regions of Valles Marineris. Credit: NASA/JPL/University of Arizona — A close-up of “chaotic terrain” in Valles Marineris imaged by the Mars Reconnaissance Orbiter’s HiRISE camera. Wind or fluid may have further shaped this region, which could be related to possible signs of an ancient lake found in other regions of Valles Marineris. Credit: NASA/JPL/University of Arizona

A section of the vast Valles Marineris ravine called Melas Chasma, a spot where sulfates (minerals formed in water) have been found before. The image shows layers of deposits that were formed before and after the formation of VAlles Marineris. Credit: NASA/JPL/University of Arizona — A section of the vast Valles Marineris ravine called Melas Chasma, a spot where sulfates (minerals formed in water) have been found before. The image shows layers of deposits that were formed before and after the formation of Valles Marineris. Credit: NASA/JPL/University of Arizona

A section of Eastern Elysium Planitia imaged by the Mars Reconnaissance Orbiter's HiRISE camera showing a possible old lava field near dust avalanches stirred up more recently. Credit: NASA/JPL/University of Arizona — A section of Eastern Elysium Planitia imaged by the Mars Reconnaissance Orbiter’s HiRISE camera showing a possible old lava field near dust avalanches stirred up more recently. Credit: NASA/JPL/University of Arizona

October 20, 2014December 23, 2015 by Bob King

MRO Spies Tiny, Bright Nucleus During Comet Flyby of Mars

Not to be outdone by the feisty Opportunity Rover, the HiRISE camera on NASA’s Mars Reconnaissance Orbiter (MRO) turned in its homework this evening with a fine image of comet C/2013 Siding Spring taken during closest approach on October 19.

The highest-resolution images were acquired by HiRISE at the minimum distance of 85,750 miles (138,000 km). The image has a scale of 453 feet (138-m) per pixel.

The top set of photos uses the full dynamic range of the camera to accurately depict brightness and detail in the nuclear region and inner coma. Prior to its arrival near Mars astronomers estimated the nucleus or comet’s core diameter at around 0.6 mile (1 km). Based on these images, where the brightest feature is only 2-3 pixels across, its true size is shy of 1/3 mile or 0.5 km. The bottom photos overexpose the comet’s innards but reveal an extended coma and the beginning of a tail extending to the right.

Annotated photo of Comet Siding Spring taken by the Opportunity Rover on October 19 when near closest approach. Credit: NASA/JPL-Caltech/Cornell Univ./ASU/TAMU

To photograph a fast-moving target from orbit, engineers at Lockheed-Martin in Denver precisely pointed and slewed the spacecraft based on comet position calculations by engineers at JPL. To make sure they knew exactly where the comet was, the team photographed the comet 12 days in advance when it was barely bright enough to register above the detector’s noise level. To their surprise, it was not exactly where orbital calculations had predicted it to be. Using the new positions, MRO succeeded in locking onto the comet during the flyby. Without this “double check” its cameras may have missed seeing Siding Spring altogether!

Meanwhile, the Jet Propulsion Lab has released an annotated image showing the stars around the comet in the photo taken by NASA’s Opportunity Rover during closest approach. From Mars’ perspective the comet passed near Alpha Ceti in the constellation Cetus, but here on Earth we see it in southern Ophiuchus not far from Sagittarius.

Comet Siding Spring continues on its way today past the planet Mars in this photo taken on October 20. Copyright: Rolando Ligustri

“It’s excitingly fortunate that this comet came so close to Mars to give us a chance to study it with the instruments we’re using to study Mars,” said Opportunity science team member Mark Lemmon of Texas A&M University, who coordinated the camera pointing. “The views from Mars rovers, in particular, give us a human perspective, because they are about as sensitive to light as our eyes would be.”

After seeing photos from both Earth and Mars I swear I’m that close to picturing this comet in 3D in my mind’s eye. NASA engineers and scientists deserve a huge thanks for their amazing and successful effort to turn rovers and spacecraft, intended for other purposes, into comet observatories in a pinch and then deliver results within 24 hours. Nice work!