Curiosity Crosses Dingo Gap Dune – Gateway to ‘Moonlight Valley’ and Mountain Destinations Beyond

Curiosity scans Moonlight Valley beyond Dingo Gap Dune. Curiosity’s view to “Moonlight 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

Curiosity scans Moonlight Valley beyond Dingo Gap Dune.
Curiosity’s view to “Moonlight 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
See below more before/after Dingo Gap imagery
Story updated[/caption]

NASA’s Curiosity mega rover has successfully crossed over the ‘Dingo Gap’ sand dune- opening the gateway to the science rich targets in the “Moonlight Valley” and Martian mountain beyond.

“I’m over the moon that I’m over the dune! I successfully crossed the “Dingo Gap” sand dune on Mars,” Curiosity tweeted overnight Thursday.

“Moonlight Valley” is the name of the breathtaking new locale beyond Dingo, Curiosity Principal Investigator John Grotzinger, of Caltech, told Universe Today.

Curiosity drove westward over the 1 meter ( 3 foot) tall Dingo Gap dune in stellar style on Thursday, Feb. 6, on Sol 535.

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 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.com

Dramatic before and after photos reveal that the rover passed over the Red Planet dune without difficulty. They also show some interesting veins and mineral fractures are visible in the vicinity just ahead.

“Moonlight Valley has got lots of veins cutting through it,” Grotzinger told me.

“We’re seeing recessive bedrock.”

The Martian dune lies between two low scarps sitting at the north and south ends.

“The rover successfully traversed the dune in Dingo Gap,” wrote science team member Ken Herkenhoff in an update.

“The data look good.”

Curiosity Crosses ‘Dingo Gap’ sand dune - Looking forward and back. Credit:  NASA
Curiosity Crosses ‘Dingo Gap’ sand dune – Looking forward and back on Sol 535. Hazcam camera images. Credit: NASA

Since arriving at the picturesque “Dingo Gap” sand dune about a week ago, Curiosity’s handlers had pondered whether to breach the dune as an alternate pathway into the smoother terrain of the valley beyond as a work around to avoid fields of rough rocks that have been ripping holes into the robots six aluminum wheels in recent months.

“We’re guessing it will be softer on the wheels,” Grotzinger informed me.

Before giving the go ahead to move forward, engineers took a few days to carefully assess the dune’s integrity and physical characteristics with the rovers science instruments and cameras to insure there wasn’t the potential to get irretrievably stuck in a deep sand trap.

The team even commanded Curiosity to carry out a toe dip by gently rolling the 20 inch (50 cm) diameter wheels back and forth over the crest on Tuesday, Feb. 4 to insure it was safe to mount.

They won’t take any chances with safety, recalling that rover Spirit’s demise occurred when she because mired in a hidden sand trap in 2010 from which there was ultimately no escape. She froze to death during the bitter Martin winter – more than 6 years into her 90 day mission.

Opportunity also got wedged at the seemingly endless dune field at “Purgatory Dune”, that nearly doomed her early in the now decade long trek. Engineers spent weeks on the extrication effort.

Curiosity does a “toe dip” wheel motion test at Dingo Gap sand dune on Sol 534, Feb 5, 2014 before crossing dune on Sol 535. Hazcam image linearized and colorized. Credit: NASA/JPL/Marco Di Lorenzo/Ken Kremer- kenkremer.com
Curiosity does a “toe dip” wheel motion test at Dingo Gap sand dune on Sol 534, Feb 5, 2014 before crossing dune on Sol 535. Hazcam image linearized and colorized. Credit: NASA/JPL/Marco Di Lorenzo/Ken Kremer- kenkremer.com

Since last summer, Curiosity has been traveling on a southwestward route to the breathtaking foothills of Mount Sharp, her ultimate science destination.

The westward route though Dingo will soon lead Curiosity to a spot dubbed “KMS-9” where the team hopes to conduct the first rock drilling operations since departing the Yellowknife Bay quadrant in July 2013, into areas of intriguing bedrock.

“At KMS-9, we see three terrain types exposed and a relatively dust-free surface,” said science team collaborator Katie Stack of the California Institute of Technology, Pasadena.

The missions science focus has shifted to “search for that subset of habitable environments which also preserves organic carbon,” says Curiosity Principal Investigator John Grotzinger, of the California Institute of Technology in Pasadena.

But first, with the dune now safely in the rear view mirror, the team plans a busy weekend of research activities.

A big science program using the X-Ray spectrometer and high resolution MAHLI camera on the robotic arm is already planned for this weekend.

“The arm will be deployed to investigate some interesting veins or minerals filling fractures in front of the rover,” says Herkenhoff.

“ChemCam will search for frost early on the morning of Sol 538 (Saturday), then analyze targets Collett and Mussell along the vein/fracture fill later in the day.”

Thereafter Curiosity will continue on its journey across the floor of Gale Crater, taking images and atmospheric measurements along the way to the sedimentary layers at the base of Mount Sharp.

Curiosity has already accomplished her primary goal of discovering a habitable zone on Mars that could support Martian microbes if they ever existed.

And be sure to check out Curiosity’s first ever image of Earth from Mars in my new story – here.

To date Curiosity’s odometer stands at nearly 5 kilometers and she has taken over 118,000 images.

The robot has about another 5 km to go to reach Mount Sharp.

Meanwhile, NASA’s sister Opportunity rover is exploring clay mineral outcrops by the summit of Solander Point on the opposite side of Mars at the start of her 2nd Decade investigating the Red Planet’s mysteries.

And a pair of new orbiters are streaking to the Red Planet to fortify Earth’s invasion fleet- NASA’s MAVEN and India’s MOM.

Stay tuned here for Ken’s continuing Curiosity, Opportunity, Chang’e-3, SpaceX, Orbital Sciences, LADEE, MAVEN, MOM, Mars and more planetary and human spaceflight news.

Ken Kremer

You are here! As an Evening Star in the Martian Sky. This evening-sky view taken by NASA's Mars rover Curiosity shows the  Earth and Earth's moon as seen on Jan. 31, 2014, or Sol 529 shortly after sunset inside Gale Crater. Credit: NASA/JPL-Caltech/MSSS/TAMU
You are here! As an Evening Star in the Martian Sky
This evening-sky view taken by NASA’s Mars rover Curiosity shows the Earth and Earth’s moon as seen on Jan. 31, 2014, or Sol 529 shortly after sunset at the Dingo Gap inside Gale Crater. Credit: NASA/JPL-Caltech/MSSS/TAMU
Curiosity’s View Past Tall Dune at edge of ‘Dingo Gap’  This photomosaic from Curiosity’s Navigation Camera (Navcam) taken at the edge of the entrance to the Dingo Gap shows a 3 foot (1 meter) tall dune and valley terrain beyond to the west, all dramatically back dropped by eroded rim of Gale Crater. View from the rover’s current position on Sol 528 (Jan. 30, 2014). The rover team may decide soon whether Curiosity will bridge the dune gap as a smoother path to next science destination. Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer- kenkremer.com
Curiosity’s View Past Tall Dune at edge of ‘Dingo Gap’
This photomosaic from Curiosity’s Navigation Camera (Navcam) taken at the edge of the entrance to the Dingo Gap shows a 3 foot (1 meter) tall dune and valley terrain beyond to the west, all dramatically back dropped by eroded rim of Gale Crater. View from the rover’s overlook position on Sol 528 (Jan. 30, 2014). The rover team has now commanded Curiosity to bridge the dune gap as a smoother path to next science destination. Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer- kenkremer.com
Up close view of hole in one of rover Curiosity’s six wheels caused by recent driving over rough Martian rocks. Mosaic assembled from Mastcam raw images taken on Dec. 22, 2013 (Sol 490).  Credit: NASA/JPL/MSSS/Ken Kremer - kenkremer.com/Marco Di Lorenzo
Up close view of hole in one of rover Curiosity’s six wheels caused by recent driving over rough Martian rocks. Mosaic assembled from Mastcam raw images taken on Dec. 22, 2013 (Sol 490). Credit: NASA/JPL/MSSS/Ken Kremer – kenkremer.com/Marco Di Lorenzo

Milky Way-Mapping Telescope Nabs Its First Pictures In Space

The Large Magellanic Cloud is visible in this calibration image for the European Space Agency's Gaia telescope taken in 2014. Credit: ESA/DPAC/Airbus DS

From a lonely outpost in space, the European Space Agency’s Gaia telescope is getting ready to map out the Milky Way. It will take some time to calibrate the instruments to make sure they’re ready for work, however, and that’s why you’re looking at the image above.

Controllers aimed the telescope at the Large Magellanic Cloud, which is a satellite galaxy to our own Milky Way, and snapped this picture of star cluster NGC 1818.

“This test picture, taken as part of commissioning the mission to ‘fine tune’ the behaviour of the instruments, is one of the first proper ‘images’ to be seen from Gaia, but ironically, it will also be one of the last, as Gaia’s main scientific operational mode does not involve sending full images back to Earth,” ESA stated.

This is one crucial step along the road to making sure Gaia’s measurements are accurate. In the next five years, it will examine a billion stars (an astounding number, but still only 1 percent of the galaxy’s population). Gaia will build up a database of key stellar properties such as brightness, what it is made of and temperature.

For more information on Gaia, check out this past Universe Today story from its Dec. 19 launch as well as the official Gaia blog.

Source: ESA

Mariner 10: Best Venus Image and 1st Ever Planetary Gravity Assist – 40 Years Ago Today

On Feb. 5, 1974, NASA's Mariner 10 mission took this first close-up photo of Venus during 1st gravity assist flyby. Credit: NASA

Exactly 40 Years ago today on Feb. 5, 1974, Mariner 10, accomplished a history making and groundbreaking feat when the NASA science probe became the first spacecraft ever to test out and execute the technique known as a planetary gravity assisted flyby used to alter its speed and trajectory – in order to reach another celestial body.

Mariner 10 flew by Venus 40 years ago to enable the probe to gain enough speed and alter its flight path to eventually become humanity’s first spacecraft to reach the planet Mercury, closest to our Sun.

Indeed it was the first spacecraft to visit two planets.

During the flyby precisely four decades ago, Mariner 10 snapped its 1st close up view of Venus – see above.

From that moment forward, gravity assisted slingshot maneuvers became an extremely important technique used numerous times by NASA to carry out planetary exploration missions that would not otherwise have been possible.

For example, NASA’s twin Voyager 1 and 2 probes launched barely three years later in 1977 used the gravity speed boost to conduct their own historic flyby expeditions to our Solar Systems outer planets.

Mariner 10's Mercury.  This is a photomosaic of images collected by Mariner 10 as it flew past Mercury on 29 March 1974.  It shows the southern hemisphere.  The spacecraft took more than 7,000 images of Mercury, Venus, the Earth, and the moon during its mission.  Credit: NASA
Mariner 10’s Mercury.
This is a photomosaic of images collected by Mariner 10 as it flew past Mercury on 29 March 1974. It shows the southern hemisphere. The spacecraft took more than 7,000 images of Mercury, Venus, the Earth, and the moon during its mission. Credit: NASA

Without the flyby’s, the rocket launchers thrust by themselves did not provide sufficient interplanetary speed to reach their follow on targets.

NASA’s Juno Jupiter orbiter just flew back around Earth this past October 9, 2013 to gain the speed it requires to reach the Jovian system.

The Mariner 10 probe used an ultraviolet filter in its imaging system to bring out details in the Venusian clouds which are otherwise featureless to the human eye – as you’ll notice when viewing it through a telescope.

Venus surface is completely obscured by a thick layer of carbon dioxide clouds.

The hellish planet’s surface temperature is 460 degrees Celsius or 900 degrees Fahrenheit.

Diagram of Mariner 10 which flew by Venus and Mercury in 1974 and 1975. This photo identifies various parts of the spacecraft and the science instruments, which were used to study the atmospheric, surface, and physical characteristics of Venus and Mercury. This was the sixth in the series of Mariner spacecraft that explored the inner planets beginning in 1962. Credit: Jet Propulsion Laboratory
Diagram of Mariner 10 which flew by Venus and Mercury in 1974 and 1975. This photo identifies various parts of the spacecraft and the science instruments, which were used to study the atmospheric, surface, and physical characteristics of Venus and Mercury. This was the sixth in the series of Mariner spacecraft that explored the inner planets beginning in 1962. Credit: Jet Propulsion Laboratory

Following the completely successful Venus flyby, Mariner 10 eventually went on to conduct a trio of flyby’s of Mercury in 1974 and 1975.

It imaged nearly half of the planets moon-like surface, found surprising evidence of a magnetic field, discovered that a metallic core comprised nearly 80 percent of the planet’s mass, and measured temperatures ranging from 187°C on the dayside to minus 183°C on the nightside.

Mercury was not visited again for over three decades until NASA’s MESSENGER flew by and eventually orbited the planet – and where it remains active today.

Mariner 10 was launched on Nov. 3, 1973 from the Kennedy Space Center atop an Atlas-Centaur rocket.

Mosaic of the Earth from Mariner 10 after launch. Credit: NASA
Mosaic of the Earth from Mariner 10 after launch. Credit: NASA
Shortly after blastoff if also took photos of the Earth and the Moon.

Ultimately it was the last of NASA’s venerable Mariner planetary missions hailing from the dawn of the Space Age.

Mariner 11 and 12 were descoped due to congressional budget cuts and eventually renamed as Voyager 1 and 2.

The Mariner 10 science team was led by Bruce Murray of the Jet Propulsion Laboratory (JPL), Pasadena, Calif.

Murray eventually became the Director of JPL. After he passed away in 2013, key science features on Martian mountain climbing destinations were named in his honor by the Opportunity and Curiosity Mars rover science teams.

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

Ken Kremer

Mariner 10 trajectory and timeline to Venus and Mercury. Credit: NASA
Mariner 10 trajectory and timeline to Venus and Mercury. Credit: NASA
Diagram of the Mariner series of spacecraft and launch vehicle. Mariner spacecraft explored Mercury, Venus and Mars. Credit: Jet Propulsion Laboratory
Diagram of the Mariner series of spacecraft and launch vehicle. Mariner spacecraft explored Mercury, Venus and Mars. Credit: Jet Propulsion Laboratory
This false color composite shows more than half of Earth’s disk over the coast of Argentina and the South Atlantic Ocean as the Juno probe slingshotted by on Oct. 9, 2013 for a gravity assisted acceleration to Jupiter. The mosaic was assembled from raw images taken by the Junocam imager. Credit: NASA/JPL/SwRI/MSSS/Ken Kremer/Marco Di Lorenzo
Mosaic of Earth from Juno gravity assist Flyby in 2013 –
compare to Mariner 10 Earth mosaic above from 1973 to see advances in space technology
This false color composite shows more than half of Earth’s disk over the coast of Argentina and the South Atlantic Ocean as the Juno probe slingshotted by on Oct. 9, 2013 for a gravity assisted acceleration to Jupiter. The mosaic was assembled from raw images taken by the Junocam imager. Credit: NASA/JPL/SwRI/MSSS/Ken Kremer/Marco Di Lorenzo

NASA Extends LADEE Dust Explorer for Bonus Lunar Science

Depiction of NASA's Lunar Atmosphere and Dust Environment Explorer (LADEE) observatory as it approaches lunar orbit.Credit: NASA Ames/Dana Berry

Depiction of NASA’s Lunar Atmosphere and Dust Environment Explorer (LADEE) observatory as it approaches lunar orbit.Credit: NASA Ames/Dana Berry
LADEE will now orbit far lower than ever before – details below![/caption]

LADEE, NASA’s latest lunar orbiter, is getting a new lease on life and will live a little longer to study the mysteries of the body’s tenuous atmosphere, or exosphere, and make surprising new discoveries while hugging Earth’s nearest neighbor even tighter than ever before, the team told Universe Today.

NASA has announced that the Lunar Atmosphere and Dust Environment Explorer (LADEE) mission will be granted a month long extension since the residual rocket fuel is more than anticipated due to the expertise of LADEE’s navigation engineers.

This is great news because it means LADEE’s three research instruments will collect a big bonus of science measurements about the pristine lunar atmosphere and dust during an additional 28 days in an ultra tight low orbit skimming around the Moon.

And the extension news follows closely on the heels of LADEE being photographed in lunar orbit for the first time by a powerful camera aboard NASA’s five year old Lunar Reconnaissance Orbiter (LRO), her orbital NASA sister – detailed here.

This dissolve  animation compares the LRO image (geometrically corrected) of LADEE  captured on Jan 14, 2014 with a computer-generated and labeled image of LADEE .  LRO and LADEE are both NASA science spacecraft currently in orbit around the Moon. Credit:  NASA/Goddard/Arizona State University
This dissolve animation compares the LRO image (geometrically corrected) of LADEE captured on Jan 14, 2014 with a computer-generated and labeled image of LADEE . LRO and LADEE are both NASA science spacecraft currently in orbit around the Moon. Credit: NASA/Goddard/Arizona State University

LADEE is currently flying around the moon’s equator at altitudes ranging barely eight to 37 miles (12-60 kilometers) above the surface which crosses over from lunar day to lunar night approximately every two hours.

During the extended mission lasting an additional full lunar cycle, LADEE will fly even lower to within a few miles (km) thereby allowing scientists an exceptional vantage point to unravel the mysteries of the moon’s atmosphere.

Just how low will LADEE fly?

I asked Rick Elphic, LADEE project scientist at NASA Ames Research Center, Moffett Field, Calif.

“We will be taking LADEE from its nominal 20 to 50 kilometer periapsis right down to the treetops — we want to get data from 5 kilometers or even less!” Elphic told me.

“So far we’ve been keeping a healthy margin for spacecraft safety, but after the nominal mission is completed, we will relax those requirements in the interest of new science.”

With the measurements collected so far the science team has already established a baseline of data for the tenuous lunar atmosphere, or exosphere, and dust impacts, says NASA.

Therefore the LADEE team is free to fly the spacecraft much lower than ever before.

And why even go to lower altitudes? I asked Elphic.

Basically because the team hopes to see changes in the particle density and composition.

“The density depends on the species. For instance, argon-40 is heavier than neon-20, and has a lower scale height. That means we should see a big increase in argon compared to neon.”

“And we may see the heavier species for the first time at these really low altitudes.”

“It’s remotely possible we’ll see krypton, for instance.”

“But the real boon will be in the dust measurements.”

“LDEX (The Lunar Dust Experiment) will be measuring dust densities very close to the surface, and we will see if something new shows up. Each time we’ve dropped our orbit down to lower altitudes, we’ve been surprised by new things,” Elphic told Universe Today.

The Neutral Mass Spectrometer (NMS) instrument will measure the identity and abundances of the exospheres constituents, such as argon, neon and krypton.

LADEE Science Instrument locations
LADEE Science Instrument locations

With the extension, LADEE is expected to continue capturing data in orbit until about April 21, 2014, depending on the usage of the declining on board fuel to feed its maneuvering thrusters.

“LADEE is investigating the moons tenuous exosphere, trace outgases like the sodium halo and lofted dust at the terminator,” Jim Green, Planetary Science Division Director at NASA HQ, told me earlier in an exclusive interview.

“The spacecraft has a mass spectrometer to identify the gases, a physical dust detector and an imager to look at scattered light from the dust. These processes also occur at asteroids.”

The Lunar Dust Experiment (LDEX) recorded dust impacts as soon as its cover opened, says NASA and is also seeing occasional bursts of dust impacts caused by meteoroid showers, such as the Geminids.

By studying the raised lunar dust, scientists also hope to solve a 40 year old mystery – Why did the Apollo astronauts and early unmanned landers see a glow of rays and streamers at the moon’s horizon stretching high into the lunar sky.

The science mission duration had initially been planned to last approximately 100 days and finish with a final impact on the Moon on about March 24th.

And the team had told me before launch that an extension was rather unlikely since the spacecraft would be flying in such a very low science orbit of about 50 kilometers altitude above the moon that it will require considerable fuel to maintain.

“LADEE is limited by the amount of onboard fuel required to maintain orbit,” Doug Voss, launch manager, Wallops, told me.

So what accounts for the extension?

Basically it’s because of the expert navigation by NASA’s engineers and the Orbital Sciences Minotaur V rocket and upper stages following the spectacular night time LADEE blastoff from NASA Wallops, VA, on Sept. 6, 2013 and subsequent insertion into lunar orbit.

“The launch vehicle performance and orbit capture burns using LADEE’s onboard engines were extremely accurate, so the spacecraft had significant propellant remaining to enable extra science,” said Butler Hine, LADEE project manager at NASA’s Ames where the mission was designed, built, tested, in a NASA statement.

“This extension represents a tremendous increase in the amount of science data returned from the mission.”

Launch of NASA’s LADEE lunar orbiter on Friday night Sept. 6, at 11:27 p.m. EDT on the maiden flight of the Minotaur V rocket from NASA Wallops, Virginia, viewing site 2 miles away. Antares rocket launch pad at left.  Credit: Ken Kremer/kenkremer.com
Launch of NASA’s LADEE lunar orbiter on Friday night Sept. 6, at 11:27 p.m. EDT on the maiden flight of the Minotaur V rocket from NASA Wallops, Virginia, viewing site 2 miles away. Antares rocket launch pad at left. Credit: Ken Kremer/kenkremer.com

“LADEE launched with 134.5 kilograms of fuel. After the third lunar orbit insertion burn (LOI-3), 80% of our fuel had been consumed,” said Dawn McIntosh, LADEE deputy project manager at NASA Ames Research Center, in an exclusive interview with Universe Today.

“Additional orbit-lowering maneuvers with the orbital control system (OCS) and reaction control system (RCS) of approximately 40 seconds were used to get LADEE into the science orbit.

And LADEE’s orbit capture was accomplished amidst the ridiculous US government shutdown with a skeleton crew.

The spacecraft finally entered its planned two hour science orbit around the moon’s equator on Nov. 20.

So LADEE’s orbital lifetime depends entirely on the remaining quantity of rocket fuel.

“LADEE has about 20 kg of propellant remaining today,” Butler Hine told Universe Today.

The 844 pound (383 kg) robot explorer is the size of a couch and was assembled at NASA’s Ames Research Center, Moffett Field, Calif., and is a cooperative project with NASA Goddard Spaceflight Center in Maryland.

Full scale model of NASA’s LADEE lunar orbiter on display at the free visitor center at NASA’s Wallops Flight Facility in Virginia. Credit: Ken Kremer/kenkremer.com
Full scale model of NASA’s LADEE lunar orbiter on display at the free visitor center at NASA’s Wallops Flight Facility in Virginia. Credit: Ken Kremer/kenkremer.com

The $280 million probe is built on a revolutionary ‘modular common spacecraft bus’, or body, that could dramatically cut the cost of exploring space and also be utilized on space probes to explore a wide variety of inviting targets in the solar system.

“LADEE is the first in a new class of interplanetary exploration missions,” NASA Ames Center Director Pete Worden told me in an interview. “It will study the pristine moon to study significant questions.”

“This is probably our last best chance to study the pristine Moon before there is a lot of human activity there changing things.”

To date LADEE has traveled over 1 million miles and in excess of 1200 equatorial orbits around the Moon.

LADEE is also searching for any changes caused to the exosphere and dust by the landing of China’s maiden Chang’e-3 lander and Yutu moon rover in December 2013.

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

Ken Kremer

LADEE_Poster_01

Paul Mahaffy, LADEE Neutral Mass Spectrometer (NMS) instrument, principal investigator, and Ken Kremer/Universe Today discuss LADEE science at NASA Wallops Flight Facility, VA. Credit: Ken Kremer/kenkremer.com
Paul Mahaffy, LADEE Neutral Mass Spectrometer instrument, principal investigator, and Ken Kremer/Universe Today discuss LADEE science at NASA Wallops Flight Facility, VA. Credit: Ken Kremer/kenkremer.com

Close Encounters of the Lunar Kind – LRO images LADEE

This dissolve animation compares the LRO image (geometrically corrected) of LADEE captured on Jan 14, 2014 with a computer-generated and labeled image of LADEE . LRO and LADEE are both NASA science spacecraft currently in orbit around the Moon. Credit: NASA/Goddard/Arizona State University

This dissolve animation compares the LRO image (geometrically corrected) of LADEE captured on Jan 14, 2014 with a computer-generated and labeled image of LADEE . LRO and LADEE are both NASA science spacecraft currently in orbit around the Moon. Credit: NASA/Goddard/Arizona State University
Story updated[/caption]

A pair of NASA spacecraft orbiting Earth’s nearest celestial neighbor just experienced a brief ‘Close Encounter of the Lunar Kind’.

Proof of the rare orbital tryst has now been revealed by NASA in the form of spectacular imagery (see above and below) just released showing NASA’s recently arrived Lunar Atmosphere and Dust Environment Explorer (LADEE) lunar orbiter being photographed by a powerful camera aboard NASA’s five year old Lunar Reconnaissance Orbiter (LRO) – as the two orbiters met for a fleeting moment just two weeks ago.

See above a dissolve animation that compares the LRO image (geometrically corrected) of LADEE captured on Jan. 14, 2014 with a computer-generated and labeled LADEE image.

All this was only made possible by a lot of very precise orbital calculations and a spacecraft ballet of sorts that had to be nearly perfectly choreographed and timed – and spot on to accomplish.

This subsection of the LRO image, expanded four times, shows the smeared view of LADEE against the lunar background..   LADEE is about 2 meters in the long direction. Lunar scene about 81 meter wide.  Credit:  NASA/Goddard/Arizona State University
This subsection of the LRO image, expanded four times, shows the smeared view of LADEE against the lunar background. LADEE is about 2 meters in the long direction. Lunar scene about 81 meter wide. Credit: NASA/Goddard/Arizona State University

Both sister orbiters were speeding along at over 3600 MPH (1,600 meters per second) while traveling perpendicularly to one another!

So the glimpse was short but sweet.

LADEE flies in an equatorial orbit (east-to-west) while LRO travels in a polar orbit (south-to-north). LADEE achieved lunar orbit on Oct. 6, 2013 amidst the federal government shutdown.

Thus their orbits align only infrequently.

The LRO orbiter did a pirouette to precisely point its high resolution narrow angle camera (NAC) while hurtling along in lunar orbit, barely 5.6 miles (9 km) above LADEE.

And it was all over in less than the wink of an eye!

LADEE entered LRO’s Narrow Angle Camera (NAC) field of view for 1.35 milliseconds and a smeared image of LADEE was snapped. LADEE appears in four lines of the LROC image, and is distorted right-to-left.

Both spacecraft are tiny – barely two meters in length.

“Since LROC is a pushbroom imager, it builds up an image one line at a time, thus catching a target as small and fast as LADEE is tricky!” wrote Mark Robinson, LROC principal investigator of Arizona State University.

So the fabulous picture was only possible as a result of close collaboration and extraordinary teamwork between NASA’s LADEE, LRO and LROC camera mission operations teams.

NASA’s LRO imaged NASA’s LADEE, about 5.6 miles (9 km) beneath it, at 8:11 p.m. EST on Jan. 14, 2014. (LROC NAC image M1144387511LR).  Image width is 821 meters, or about 898 yards.)   Credit:   NASA/Goddard/Arizona State University
NASA’s LRO imaged NASA’s LADEE, about 5.6 miles (9 km) beneath it, at 8:11 p.m. EST on Jan. 14, 2014. (LROC NAC image M1144387511LR). Image width is 821 meters, or about 898 yards.) Credit: NASA/Goddard/Arizona State University

LADEE passed directly beneath the LRO orbit plane a few seconds before LRO crossed the LADEE orbit plane, meaning a straight down LROC image would have just missed LADEE, said NASA.

LRO spacecraft (top) protected by gray colored blankets is equipped with 7 science instruments located at upper right side of spacecraft. LRO cameras are pointing to right. LRO is piggybacked atop NASA’s LCROSS spacecraft.  Payload fairing in background protects the spacecraft during launch and ascent. Credit: Ken Kremer
LRO spacecraft (top) protected by gray colored blankets is equipped with 7 science instruments located at upper right side of spacecraft. LRO cameras are pointing to right. LRO is piggybacked atop NASA’s LCROSS spacecraft. Payload fairing in background protects the spacecraft during launch and ascent. Credit: Ken Kremer

Therefore, LRO was rolled 34 degrees to the west so the LROC detector (one line) would be precisely oriented to catch LADEE as it passed beneath.

“Despite the blur it is possible to find details of the spacecraft. You can see the engine nozzle, bright solar panel, and perhaps a star tracker camera (especially if you have a correctly oriented schematic diagram of LADEE for comparison),” wrote Robinson in a description.

See the LADEE schematic in the lead image herein.

LADEE was launched Sept. 6, 2013 from NASA Wallops in Virginia on a science mission to investigate the composition and properties of the Moon’s pristine and extremely tenuous atmosphere, or exosphere, and untangle the mysteries of its lofted lunar dust.

Since LADEE is now more than halfway through its roughly 100 day long mission, timing was of the essence before the craft takes a death dive into the moon’s surface.

You can see a full scale model of LADEE at the NASA Wallops visitor center, which offers free admission.

Full scale model of NASA’s LADEE lunar orbiter on display at the free visitor center at NASA’s Wallops Flight Facility in Virginia. Credit: Ken Kremer/kenkremer.com
Full scale model of NASA’s LADEE lunar orbiter on display at the free visitor center at NASA’s Wallops Flight Facility in Virginia. Credit: Ken Kremer/kenkremer.com

LRO launched Sept. 18, 2009 from Cape Canaveral, Florida to conduct comprehensive investigations of the Moon with seven science instruments and search for potential landing sites for a return by human explorers. It has collected astounding views of the lunar surface, including the manned Apollo landing sites as well as a treasure trove of lunar data.

In addition to NASA’s pair of lunar orbiters, China recently soft landed two probes on the Moon.

So be sure to read my new story detailing how LRO took some stupendous Christmas time 2013 images of China’s maiden lunar lander and rover; Chang’e-3 and Yutu from high above- here.

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

Ken Kremer

Launch of NASA’s LADEE lunar orbiter on Friday night Sept. 6, at 11:27 p.m. EDT on the maiden flight of the Minotaur V rocket from NASA Wallops, Virginia, viewing site 2 miles away. Antares rocket launch pad at left.  Credit: Ken Kremer/kenkremer.com
Launch of NASA’s LADEE lunar orbiter on Friday night Sept. 6, at 11:27 p.m. EDT on the maiden flight of the Minotaur V rocket from NASA Wallops, Virginia, viewing site 2 miles away. Antares rocket launch pad at left. Credit: Ken Kremer/kenkremer.com

Video: These Children from Greece (and Poland) Helped Wake Up the Rosetta Spacecraft

An artist concept of the Philae lander on comet 67P/Churyumov-Gerasimenko. Credit: Astrium - E. Viktor/ESA

The European Space Agency asked for help in waking up the Rosetta spacecraft from 31 months of deep-space hibernation, and sponsored a fun video contest. The votes are in and the winning video comes from the 1,002 children of the Ellinogermaniki Agogi Primary School in Greece. Not only is the video heartwarming, but original music was composed using a “3/2 time signature symbolizing the five gravity assists that Rosetta got from the Earth and Mars. Theme ends with a perfect 5th (interval ratio 3:2) symbolizing Jupiter (5th planet), Rosetta’s ultimate orbit point.”

Wow.

There were 218 entries and 75,000 people voted. Entries came in from notables like Chris Hadfield, Bill Nye, and singer Tasmin Archer.

“We were truly impressed by the effort that all of you put into your videos, from getting your pets, friends and families involved and constructing fantastic model Rosetta spacecraft,”ESA said, “to storyboarding brilliant stop-motion animations with Lego, and writing entire songs and choreographing dance routines for dozens or even hundreds of passionate Rosetta fans.”

The top ten vote-getting videos were transmitted out to Rosetta via one of ESA’s deep-space tracking stations, and the top two video creators are invited to the control center in Darmstadt, Germany for when the Philae lander attempts landing on comet 67P/Churyumov–Gerasimenko in November 2014 after latching on with a harpoon. The second, equal award was given to Józef Dobrowolski, aged 17 student from Ostroleka, Poland, who is from the III Secondary School. He worked on his video himself, and he’s passionate about astronomy and started his hobby with observing the Perseid meteor shower:

You can see all ten winning videos here, or see a mashup of submitted videos, below.

NEOWISE Spots Mars-Crossing Comet

NASA's NEOWISE Mission takes aim at Comet A1 Siding Spring on January 16th, 2014 when the comet was 571 million kilometres distant. Credit: NASA/JPL-Caltech

One of the big ticket astronomical events of 2014 will be the close passage of Comet C/2013 A1 Siding Spring past the planet Mars in October 2014. Discovered just over a year ago from the Australian-based Siding Spring Observatory, this comet generated a surge of excitement in the astronomical community when it was discovered that it was going to pass very close to the planet Mars in late 2014.

Now, a fleet of spacecraft are poised to study the comet in unprecedented detail. Some of the first space-based observations of the comet have been conducted by NASA’s Hubble Space Telescope and the recently reactivated NEOWISE mission. And although the comet may not look like much yet in the infrared eyes of NEOWISE, its estimated 4 kilometre in diameter nucleus is already active and shedding about 100 kilograms of dust per second.

And although an impact has been since ruled out, it’s that dust that may present a hazard for Mars orbiting spacecraft, as well as a unique scientific observing opportunity.

“Our plans for using spacecraft at Mars to observe Comet A1 Siding Spring will be coordinated with plans for how the orbiters will duck and cover, if we need to do so that,” said NASA/JPL Mars Exploration Program chief scientist Rich Zurek.

The 2014 passage of Comet A1 Siding Spring through the inner solar system. Credit: NASA/JPL-Caltech
The 2014 passage of Comet A1 Siding Spring through the inner solar system. Credit: NASA/JPL-Caltech

Comet A1 Siding Spring is projected to pass within just 138,000 kilometres of Mars on October 19th, 2014. This is one-third the Earth-Moon distance, and 10 times closer than the closest recorded passage of a comet by the Earth, which was Comet D/1770 Lexell in the late 18th century. The comet will also miss the Martian moons of Phobos and Deimos, which have the closest orbits of any moons in the solar system at just 5,989 and 20,063 kilometres above the surface of Mars, respectively.

Assets in orbit around the Red Planet are also slated to observe the close approach and passage of Comet A1 Siding Spring, as well as any extraterrestrial meteor shower that its dust may generate.

“We could learn about the nucleus – its shape, its rotation, whether some areas on its surface are darker than others,” Zurek said in a recent NASA/JPL press release.

The rovers Curiosity and Opportunity are currently active on the surface of Mars. Above in orbit, we’ve got the European Space Agency’s Mars Express, and NASA’s Mars Odyssey and the Mars Reconnaissance Orbiter (MRO).  These will be joined by India’s Mars Orbiter Mission and NASA’s Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft just weeks prior to the comet’s passage.

“A third aspect for investigation could be what effect the infalling particles have on the upper atmosphere of Mars,” Zurek said. “They might heat it and expand it, not unlike the effect of a global dust storm.”

Just last year, Mars based spacecraft caught sight of the ill-fated sungrazer Comet C/2012 S1 ISON as it passed Mars. But that dim passage yielded a scant pixel-sized view in the eyes of MRO’s HiRISE camera; Comet A1 Siding Spring will pass 80 times closer than Comet ISON and could yield a view of its nucleus dozens of pixels across.

Though the tenuous Martian atmosphere will shield to surface rovers from any micro-meteoroid impacts, they may also be witness to a surreptitious meteor shower from the debris shed by the comet, a first seen from the surface of another world.

But engineers will also be assessing the potential hazards that said particles may posed to spacecraft orbiting Mars as well.

“It’s way too early for us to know how much of a threat Siding Spring will be to our orbiters,” said JPL’s Mars Exploration Program chief engineer Soren Madsen recently. “It could go either way. It could be a huge deal or it could be nothing – or anything in between.”

In a worst case scenario, Mars orbiting spacecraft would be shuttered and oriented to “shelter in place” as the dust from the comet passes. There’s precedent for this in Earth orbit, as precious assets such as the Hubble Space Telescope were closed for business during the Leonid meteor storm of 1998.

“How active will Siding Spring be in April and May? We’ll be watching that,” Madsen continued. “But if the red alarm starts sounding in May, it would be too late to start planning how to respond. That’s why we’re doing what we’re doing right now.”

Comet A1 Siding Spring was the first comet discovered in 2013 at 7.2 Astronomical Units (AUs) distant. From our Earth based perspective, the comet will reach opposition on August 25th at 0.96 AU from the Earth, and approach 7’ from Mars on October 19th in the constellation Ophiuchus in evening skies. The comet reaches perihelion just 4 days later, and is slated to be a binocular comet around that time shining at magnitude +8.

The comet nucleus itself is moving in a retrograde orbit relative to Mars. Particles from A1 Siding Spring will slam into the atmosphere of Mars — and any spacecraft that happens to be in their way — at a velocity of 56 kilometres per second. For context, the recent January Quadrantids have a more sedate atmospheric impact velocity of 41 kilometres a second.

The unfolding 2014 drama of “Mars versus the Comet” will definitely be worth keeping an eye on… more to come!

Trailer: New Horizons Gets Ready to Meet Pluto

Artist's impression of New Horizons' encounter with Pluto and Charon. Credit: NASA/Thierry Lombry

Less than a year from now, the New Horizons spacecraft will begin its encounter with Pluto. While closest approach is scheduled for July 2015, the Long Range Reconnaissance Imager or “LORRI” will begin snapping photos of the Pluto system six months earlier.

This first mission to Pluto has been a long time coming, and this new “trailer” put out by the New Horizons team recounts what it has taken to send the fastest spacecraft ever on a 5 billion km (3 billion mile) journey to Pluto, its largest moon, Charon, and the Kuiper Belt beyond. The spacecraft has been zooming towards the edge of our Solar System for over eight years since it launched on January 19, 2006.

By late April 2015, the approaching spacecraft will be taking pictures of Pluto that surpass the best images to date from Hubble. By closest approach in July 2015 –- when New Horizons will be 10,000 km from Pluto — a whole new world will open up to the spacecraft’s cameras. If New Horizons flew over Earth at the same altitude, it’s cameras could see individual buildings and their shapes.

“Humankind hasn’t had an experience like this–an encounter with a new planet–in a long time,” said Alan Stern, New Horizons’ principal investigator. “Everything we see on Pluto will be a revelation.”

It’s likely there could be some new planetary bodies discovered during the mission in addition to the five known moons: Charon, Styx, Nix, Kerberos, and Hydra.

“There is a real possibility that New Horizons will discover new moons and rings as well,” says Stern.

No matter what, Stern said, this is going to be an amazing ride.

“We’re flying into the unknown,” he said, “and there is no telling what we might find.”

See the countdown clock and find out more about the mission at the New Horizons website.

Now is Your Last Chance to Visit Inside NASA’s Iconic Vehicle Assembly Building – and maybe see an Orion

NASA’s iconic Vehicle Assembly Building (VAB) and Launch Control Center (LCC) at the Kennedy Space Center, Florida. Public access tours inside the VAB will end on Feb. 11, 2014. NASA's Apollo Saturn V Moon rockets and Space Shuttles were assembled inside. Credit: Ken Kremer - kenkremer.com

NASA’s iconic Vehicle Assembly Building (VAB) and Launch Control Center (LCC) at the Kennedy Space Center, Florida. Public access tours inside the VAB will end on Feb. 11, 2014. NASA’s Apollo Saturn V Moon rockets and Space Shuttles were assembled inside.
Credit: Ken Kremer – kenkremer.com
Story updated- Last chance to visit VAB extended to Feb. 23[/caption]

If you have ever wanted to take a personal trip inside NASA’s world famous Vehicle Assembly Building (VAB) at Kennedy Space Center in Florida, now is the time.

In fact this is your last chance. Because access to the hugely popular public tours will end very soon. And perhaps you’ll see an Orion test capsule too.

Indeed you only have until Feb. 11 [Update: now extended to Feb. 23] to enjoy the KSC “Up-Close Tour” inside the 52 story tall VAB, according to an announcement by the privately run Kennedy Space Center Visitor Complex, which organizes the VAB tours.

The VAB is an iconic world wide symbol of America’s space program.

And it’s home to many of NASA’s finest and most historic exploration achievements – including all the manned Apollo Moon landings and the three decade long Space Shuttle program that launched the Hubble Space Telescope and the International Space Station (ISS) to orbit.

Why are the interior public tours being halted, barely 2 years after they started?

Because after a bit of a lull following the termination of NASA’s Space Shuttle program, space launch activities are ramping up once again and the agency must complete much needed building renovations to prepare for the next step in human exploration of the cosmos – SLS, Orion and commercial ‘space taxis’.

Orion crew capsule, Service Module and 6 ton Launch Abort System (LAS) mock up stack inside the transfer aisle of the Vehicle Assembly Building (VAB) at the Kennedy Space Center (KSC) in Florida. Credit: Ken Kremer/kenkremer.com
Orion crew capsule, Service Module and 6 ton Launch Abort System (LAS) mock up stack inside the transfer aisle of the Vehicle Assembly Building (VAB) at the Kennedy Space Center (KSC) in Florida. Credit: Ken Kremer/kenkremer.com

The agency needs unfettered use of the VAB to prepare for assembly, lifting and stacking of the new Orion crew capsule and it’s new monster booster rocket – the Space Launch System (SLS) – slated for its maiden blastoff in 2017.

You can always see the 525 foot tall VAB from the outside, gleaming proudly from miles away.

And it’s a must see from up close outside glimpses aboard tour buses driving by all day long – resplendent with a mammoth red, white and blue American flag painted on its side.

But nothing compares to being an eyewitness to history and seeing it from the inside with your own eyes, especially if you are a space enthusiast!

The VAB is one of the largest and most voluminous buildings in the world.

Since 1978, the VAB interior had been off limits to public visitors for more than 30 years during the shuttle era. It was too hazardous to visit because of the presence of the giant shuttle solid rocket boosters loaded with fuel.

Orion Ground Test Article (GTA) recently displayed on the floor inside the Vehicle Assembly Building (VAB).    Credit: Ken Kremer - kenkremer.com
Orion Ground Test Article (GTA) recently displayed on the floor inside the Vehicle Assembly Building (VAB). Credit: Ken Kremer – kenkremer.com

Inside access was finally restored to guests at Kennedy Space Center Visitor Complex in November 2011, following the retirement of the space shuttles.

Visitors could again “see firsthand where monstrous vehicles were assembled for launch, from the very first Saturn V rocket in the late 1960s to the very last space shuttle, STS-135 Atlantis, in 2011.”

Although the shuttles are now gone, there is a possibility that maybe you’ll be lucky enough to see an Orion test capsule that’s been used in real ground testing to help NASA prepare for upcoming missions.

Since the layout is constantly changing, there is no guarantee on seeing the Orion.

Possibly either an Orion boilerplate test article or the Ground Test Article (GTA) which was the first flight worthy Orion capsule to be built. The GTA is the path finding prototype for the Orion EFT-1 capsule currently in final assembly and slated to launch this Fall 2014.

Perhaps you’ll be lucky enough to snap a shot like one of mine of the Orion GTA on the floor of the main working area of the VAB – known as the transfer aisle.

You will definitely get the feel for the greatest hits in space history inside the place where the moon rockets and space shuttles were lifted, stacked and assembled for flight and then rolled out to either Launch Pad 39 A or 39 B.

Atlantis approaches the VAB for the final time. Credit: Ken Kremer
Atlantis approaches the VAB for the final time during preparations for the STS-135 flight in 2011. Credit: Ken Kremer – kenkremer.com

“Kennedy Space Center Visitor Complex has been honored to give our guests rare access to the VAB for the past two years, yet we knew that the day would come when preparations for the SLS would take precedent,” said Therrin Protze, chief operating officer for the Visitor Complex, in a statement.

“Kennedy Space Center is an operating space program facility, and preparations for the next chapter in space exploration are the utmost priority, and we are very excited about the future.”

Starting in 2017, America will again launch a mighty rocket – the SLS that will blast Americans to deep space after an unbelievable 50 year gap.

Full belly view of Space Shuttle Discovery coated with thousands of protective heat shield tiles in the transfer aisle of the VAB where it was processed for final launch on STS-133 mission.  Note two rectangular attach points holding left and right side main separation bolts. Credit: Ken Kremer - kenkremer.com
Full belly view of Space Shuttle Discovery coated with thousands of protective heat shield tiles in the transfer aisle of the VAB where it was processed for final launch on STS-133 mission. Note two rectangular attach points holding left and right side main separation bolts. Credit: Ken Kremer – kenkremer.com

So for only about the next two weeks, you can see one of the greatest treasures of America’s space program and appreciate the cavernous interior from where our astronauts once set off for the Moon as part of the “Mega Tour”.

The “Mega Tour”, which also included visits to Launch Pad 39 A and the Launch Control Center (LCC) ends on Feb. 11, the visitor complex announced.

However the visitor complex is still offering a modified “Up-Close” tour to Pad 39A and the Launch Control Center (LCC) – at this time. But that’s subject to change at any moment depending on NASA’s priorities.

View of NASA’s 52 story tall Vehicle Assembly Building (VAB) as seen from the top of Launch Pad 39 A.    Credit: Ken Kremer - kenkremer.com
View of NASA’s 52 story tall Vehicle Assembly Building (VAB) as seen from the very top of Launch Pad 39 A gantry. Credit: Ken Kremer – kenkremer.com

And don’t forget that you can also see NASA’s genuine Space Shuttle Atlantis in its new permanent exhibition hall at the Kennedy Space Center Visitor Complex.

Please check the visitor center website for complete details and admission pricing on “Up-Close” tours and everything else – www.kennedyspacecenter.com

There is one thing I can guarantee – if you don’t go you will see nothing!

Catch it if you can. It’s NOT coming back any time soon!

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

Ken Kremer

Space Shuttle Atlantis permanent display at Kennedy Space Center Visitor Complex, Florida. Credit: Ken Kremer - kenkremer.com
Space Shuttle Atlantis permanent display at Kennedy Space Center Visitor Complex, Florida. Credit: Ken Kremer – kenkremer.com
View of the Vehicle Assembly Building (VAB) and the Turn Basin adjacent to the Kennedy Space Center Press Center and the countdown clock. Credit: Ken Kremer – kenkremer.com
View of the Vehicle Assembly Building (VAB) and the Turn Basin adjacent to the Kennedy Space Center Press Center and the countdown clock. Credit: Ken Kremer – kenkremer.com

The Difficulties of Operating a Rover on Mars for 10 Years

NASA's Opportunity Mars rover recorded the component images for this self-portrait near the peak of Solander Point and about three weeks before completing a decade of work on Mars. The rover's panoramic camera (Pancam) took the images during the interval Jan. 3, 2014, to Jan. 6, 2014. Credit: NASA/JPL-Caltech/Cornell/Arizona State University

Want to get an engineer excited? Give them a challenge. And the Opportunity rover has provided plenty of challenges in the past 10 years on Mars. Fun challenges, though; amazing tests of wit and skill, doing repairs on a rover that is sometimes a hundred million kilometers away. But with the longevity of the rovers also comes some amazing science.

The Opportunity rover is celebrating ten years on Mars. While the rovers were designed for about 1 kilometer of odometry, Oppy has now traveled 38.7 kilometers (24 miles). At yesterday’s briefing, the rover scientists and engineers said Opportunity is still in very good health and still is scientifically productive.

In the recent “selfie” image below, you can see how the rover is covered with dust, almost perfectly camouflaged with its environment. That montage was taken a few weeks ago, but recently there have been some wind cleaning events that have dusted off the solar panels, improving the solar power from 47% to 60%, which is higher than it has been through the past two Martian winters. This means they can continue to drive and explore even more, perhaps even during the upcoming winter.

Dust covering the rovers’ solar panels was one of the reasons that the initial estimates of the rovers’ life was only for 90 days. The dust cleaning events have been an unexpected benefit that has allowed for the long missions for the MER rovers.

Beyond the scientific findings of potential habitability announced yesterday, John Callas, project manager for the Mars Exploration Rovers said both Spirit and Opportunity have given us a great intangible.

“Through these rovers our species has gone to work on Mars, and now a generation has grown up with these rovers and have been inspired by them,” Callas said. “Because of these rovers Earthlings have become Martians too, dual citizens, if you will. We now live in a larger world, a world than now extends beyond our own home planet these rovers have made Mars our neighborhood and our backyard, something truly remarkable.”