Space Exploration Archives

March 24, 2013June 5, 2022 by Ken Kremer

Curiosity is Back! Snapping Fresh Martian Vistas

Curiosity's raised robotic arm and drill are staring at you in this new panoramic vista of Yellowknife Bay basin snapped on March 23, Sol 223 by the rover's navigation camera system. The raw images were stitched by Marco Di Lorenzo and Ken Kremer and colorized. Credit: NASA/JPL-Caltech/Marco Di Lorenzo/KenKremer (kenkremer.com)

Curiosity is back! After a multi-week hiatus forced by a computer memory glitch, NASA’s mega rover is back to full operation.

And the proof is crystal clear in the beautiful new panoramic view (above) snapped by Curiosity this weekend from Yellowknife Bay, showing the robot’s arm and drill elevated and aiming straight at you – raring to go and ready to feast on something deliciously Martian.

“That drill is hungry, looking for something tasty to eat, and ‘you’ (loaded with water and organics) are it,” I thought with a chuckle as Curiosity seeks additional habitats and ingredients friendly to life.

So my imaging partner Marco Di Lorenzo and I celebrated the great news by quickly creating the new panoramic mosaic assembled from images taken on Saturday, March 23, or Sol 223, by the robot’s navigation cameras. Our new Curiosity mosaic was first featured on Saturday at NBC News Cosmic Log by Alan Boyle – while I was hunting for Comet Pan-STARRS.

So the fact that Curiosity is again snapping images and transmitting fresh alien vistas and new science data is a relief to eagerly waiting scientists and engineers here on Earth.

Drilling goes to the heart of the mission. It was absolutely essential to the key finding of Curiosity’s Martian foray thus far – that Mars possesses an environment where alien microbes could once have thrived in the distant past when the Red Planet was warmer and wetter.

Curiosity accomplished Historic 1st drilling into Martian rock at John Klein outcrop on Feb 8, 2013 (Sol 182), shown in this context mosaic view of the Yellowknife Bay basin taken on Jan. 26 (Sol 169) where the robot is currently working. The robotic arm is pressing down on the surface at John Klein outcrop of veined hydrated minerals – dramatically back dropped with her ultimate destination; Mount Sharp. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo

Curiosity has found widespread evidence for repeated episodes of flowing liquid water on the floor of her Gale Crater landing site – an essential prerequisite to life as we know it.

After coring and analyzing the first powder ever drilled from the interior of a Martian rock in February 2013, NASA’s Curiosity robot discovered some of the key chemical ingredients necessary to support life on early Mars billions of years ago.

Curiosity found that the fine-grained, sedimentary mudstone rock at the rovers current worksite inside the Yellowknife Bay basin possesses significant amounts of phyllosilicate clay minerals; indicating the flow of nearly neutral liquid water and a habitat friendly to the possible origin of simple Martian life forms eons ago.

Curiosity's First Sample Drilling hole is shown at the center of this image in a rock called "John Klein" on Feb. 8, 2013, or Sol 182 operations. The image was obtained by Curiosity’s Mars Hand Lens Imager (MAHLI). The sample-collection hole is 0.63 inch (1.6 centimeters) in diameter and 2.5 inches (6.4 centimeters) deep. The “mini drill” test hole near it is the same diameter, with a depth of 0.8 inch (2 centimeters). Credit: NASA/JPL-Caltech/MSSS — Curiosity’s First Sample Drilling hole is shown at the center of this image in a rock called “John Klein” on Feb. 8, 2013, or Sol 182 operations. The image was obtained by Curiosity’s Mars Hand Lens Imager (MAHLI). The sample-collection hole is 0.63 inch (1.6 centimeters) in diameter and 2.5 inches (6.4 centimeters) deep. The “mini drill” test hole near it is the same diameter, with a depth of 0.8 inch (2 centimeters). Credit: NASA/JPL-Caltech/MSSS

The rovers 7 foot (2.1 meter) long robotic arm fed aspirin sized samples of the gray, pulverized powder into the miniaturized CheMin and SAM analytical instruments on Feb. 22 and 23, or Sols 195 and 196. The samples were analyzed on Sol 200 and then the rover experienced her first significant problems since landing on Aug. 5, 2012.

The Chemistry and Mineralogy (CheMin) instrument and Sample Analysis at Mars (SAM) instruments test the Martian soil and rock samples to determine their chemical composition and search for traces of organic molecules – the building blocks of life

No organics have been found thus far.

The rover’s science mission has been on hold for nearly a month since “a memory glitch on the A-side computer on Feb. 27, which prompted controllers to command a swap from the A-side computer to the B-side computer,” according to a NASA statement.

“That operator-commanded swap put Curiosity into safe mode for two days. The rover team restored the availability of the A-side as a backup and prepared the B-side to resume full operations.”

The memory issue may have been caused by a cosmic ray strike. The rover suffered another minor setback last week, briefly reentering ‘safe mode’. And in between, a solar storm forced the team to shut Curiosity down for a few more days.

All appears well now.

The next step is to reanalyze those 1st gray rock tailings to continue the hunt for traces of organic molecules.

But the next solar conjunction will interrupt communications starting around April 4 for several weeks. More on that shortly.

After conjunction, Curiosity will resume her drilling campaign

Ken Kremer

…………….

Learn more about Curiosity’s groundbreaking discoveries and NASA missions at Ken’s upcoming lecture presentations:

April 20/21 : “Curiosity and the Search for Life on Mars – (in 3-D)”. Plus Orion, SpaceX, Antares, the Space Shuttle and more! NEAF Astronomy Forum, Suffern, NY

April 28: “Curiosity and the Search for Life on Mars – (in 3-D)”. Washington Crossing State Park, Titusville, NJ, 130 PM

Rover self portrait MAHLI mosaic taken this week has Curiosity sitting on the flat rocks of the “John Klein” drilling target area within the Yellowknife Bay depression. Note gradual rise behind rover. Credit: NASA/JPL-Caltech/MSSS/Marco Di Lorenzo/www.KenKremer.com. — Rover self portrait MAHLI mosaic taken this week has Curiosity sitting on the flat rocks of the “John Klein” drilling target area within the Yellowknife Bay depression. Note gradual rise behind rover. Credit: NASA/JPL-Caltech/MSSS/Marco Di Lorenzo/Ken Kremer (kenkremer.com)

March 23, 2013December 23, 2015 by Ken Kremer

Powerful Private Rocket Crucial to ISS Set for Maiden April Blast Off from Virginia – Launch Pad Gallery

The first stage of the privately developed Antares rocket stands on the pad at NASA's Wallops Flight Facility. Credit: Ken Kremer (kenkremer.com)

The first stage of the privately developed Antares rocket stands erect at newly constructed Launch Pad 0-A at NASA’s Wallops Flight Facility during exclusive launch complex tour by Universe Today. Maiden Antares test launch is scheduled for mid-April 2013. Later operational flights are critical to resupply the ISS.
Credit: Ken Kremer (kenkremer.com)
See Antares photo gallery below[/caption]

The most powerful rocket ever to ascend near major American East Coast population centers is slated to blast off soon from the eastern Virginia shore on its inaugural test flight in mid April.

And Universe Today took an exclusive inspection tour around the privately developed Antares rocket and NASA Wallops Island launch complex just days ago.

NASA announced that the maiden flight of the commercial Antares rocket from Orbital Sciences is slated to soar to space between April 16 to 18 from the newly constructed seaside launch pad dubbed 0-A at the Mid-Atlantic Regional Spaceport (MARS) at NASA’s Wallops Flight Facility in Virginia.

The two stage Antares rocket is absolutely pivotal to NASA’s plans to ship essential cargo to the International Space Station (ISS) in the wake of the shutdown of the Space Shuttle program in July 2011.

No admittance to the Orbital Sciences Corp. Antares rocket without permission from the pad manager! Credit: Ken Kremer (kenkremer.com) — No admittance to the Orbital Sciences Corp. Antares rocket without permission from the pad manager. Credit: Ken Kremer (kenkremer.com)

Antares stands 131 feet tall and serves as the launcher for the unmanned commercial Cygnus cargo spacecraft.

Both Antares and Cygnus were developed by Orbital Sciences Corp under NASA’s Commercial Orbital Transportation Services (COTS) program to replace the ISS cargo resupply capability previously tasked to NASA’s now retired Space Shuttle’s. The goal is to achieve safe, reliable and cost-effective transportation to and from the ISS and low-Earth orbit (LEO).

I visited NASA Wallops for an up close personal tour of the impressive Antares 1st stage rocket erected at the launch pad following the successful 29 second hot fire engine test that cleared the last hurdle to approve the maiden flight of Antares. Umbilical lines were still connected to the rocket.

Antares rocket 1st stage and umbilicals at NASA Wallops Flight Facility. Credit: Ken Kremer (kenkremer.com) — Antares rocket 1st stage and umbilical lines at NASA Wallops Flight Facility. Credit: Ken Kremer (kenkremer.com)

The pads protective seawall was rebuilt following significant damage from Hurricane Sandy, NASA Wallops spokesman Keith Koehler told me.

Launch Complex 0-A sits just a few hundred yards (meters) from Virginia’s eastern shore line on the Atlantic Ocean. It’s hard to believe just how close the low lying pad complex is to the beach and potentially destructive tidal surges.

Barely 400 meters (1300 feet) away lies the adjacent Launch Pad 0-B – from which Orbital’s new and unflown solid fueled Minotaur 5 rocket will boost NASA’s LADEE lunar science probe to the Moon in August 2013 – see my upcoming article.

The maiden Antares test flight is called the A-One Test Launch Mission. It will validate the medium class rocket for the actual follow-on flights to the ISS topped with the Cygnus cargo carrier starting later this year with a demonstration docking mission to the orbiting lab complex.

The Antares first stage is powered by dual liquid fueled AJ26 first stage rocket engines that generate a combined total thrust of some 680,000 lbs. The upper stage features a Castor 30 solid rocket motor with thrust vectoring. Antares can loft payloads weighing over 5000 kg to LEO.

The launch window opens at 3 p.m. and extends for a period of time since this initial test flight is not docking at the ISS, Orbital spokesman Barry Boneski told Universe Today.

Antares will boost a simulated version of the Cygnus carrier – known as a mass simulator – into a target orbit of 250 x 300 kilometers and inclined 51.6 degrees.

Antares A-One will fly on a southeast trajectory and the Cygnus dummy will be instrumented to collect flight and payload data.

The simulated Cygnus will separate from the upper stage 10 minutes after liftoff for orbital insertion.

“All launches are to the south away from population centers. Wildlife areas are nearby,” said Koehler.

The goal of the ambitious A-One mission is to fully demonstrate every aspect of the operational Antares rocket system starting from rollout of the rocket and all required functions of an operational pad from range operation to fueling to liftoff to payload delivery to orbit.

Orbital Sciences Antares rocket and Launch Complex 0-A at the edge of Virginia’s shore at NASA Wallops are crucial to resupply the International Space Station (ISS). Credit: Ken Kremer (kenkremer.com) — Orbital Sciences Antares rocket and Launch Complex 0-A at the edge of Virginia’s shore at NASA Wallops are crucial to resupply the International Space Station (ISS). . Credit: Ken Kremer (kenkremer.com)

Antares/Cygnus will provide a cargo up mass service similar to the Falcon 9/Dragon system developed by SpaceX Corporation – which has already docked three times to the ISS during historic linkups in 2012 and earlier this month following the tension filled March 1 liftoff of the SpaceX CRS-2 mission.

The Dragon is still docked to the ISS and is due to make a parachute assisted return to Earth on March 26.

Orbital has eight commercial resupply missions manifested under a $1.9 Billion contact with NASA to deliver approximately 20,000 kilograms of supplies and equipment to the ISS, Orbital spokesman Barry Boneski told me.

Tens of millions of American East Coast residents in the Mid-Atlantic and Northeast regions have never before had the opportunity to witness anything as powerful as an Antares rocket launch in their neighborhood.

Watch for my continuing reports through liftoff of the Antares A-One Test flight.

Ken Kremer

March 20, 2013April 26, 2016 by David Dickinson

U.S. To Restart Plutonium Production for Deep Space Exploration

A marshmellow-sized Pu-238 pellet awaits a space mission. (Credit: The Department of Energy).

The end of NASA’s plutonium shortage may be in sight. On Monday March 18^th, NASA’s planetary science division head Jim Green announced that production of Plutonium-238 (Pu-238) by the United States Department of Energy (DOE) is currently in the test phases leading up to a restart of full scale production.

“By the end of the calendar year, we’ll have a complete plan from the Department of Energy on how they’ll be able to satisfy our requirement of 1.5 to 2 kilograms a year.” Green said at the 44^th Lunar and Planetary Science Conference being held in Woodlands, Texas this past Monday.

This news comes none too soon. We’ve written previously on the impending Plutonium shortage and the consequences it has for future deep space exploration. Solar power is adequate in most cases when you explore the inner solar system, but when you venture out beyond the asteroid belt, you need nuclear power to do it.

Production of the isotope Pu-238 was a fortunate consequence of the Cold War. First produced by Glen Seaborg in 1940, the weapons grade isotope of plutonium (-239) is produced via bombarding neptunium (which itself is a decay product of uranium-238) with neutrons. Use the same target isotope of Neptunium-237 in a fast reactor, and Pu-238 is the result. Pu-238 produces 280x times the decay heat at 560 watts per kilogram versus weapons grade Pu-239 and is ideal as a compact source of energy for deep space exploration.

Since 1961, over 26 U.S. spacecraft have been launched carrying Multi-Mission Radioisotope Thermoelectric Generators (MMRTG, or formerly simply RTGs) as power sources and have explored every planet except Mercury. RTGs were used by the Apollo Lunar Surface Experiments Package (ALSEP) science payloads left on by the astronauts on the Moon, and Cassini, Mars Curiosity and New Horizons enroute to explore Pluto in July 2015 are all nuclear powered.

Plutonium powered RTGs are the only technology that we have currently in use that can carry out deep space exploration. NASA’s Juno spacecraft will be the first to reach Jupiter in 2016 without the use of a nuclear-powered RTG, but it will need to employ 3 enormous 2.7 x 8.9 metre solar panels to do it.

The plutonium power source inside the Mars Science Laboratory's MMRTG during assembly at the Idaho National Laboratory. (Credit: Department of Energy?National Laboratory image under a Creative Commons Generic Attribution 2.0 License). — The plutonium power source inside the Mars Science Laboratory’s MMRTG during assembly at the Idaho National Laboratory. (Credit: Department of Energy/Idaho National Laboratory image under a Creative Commons Generic Attribution 2.0 License).

The problem is, plutonium production in the U.S. ceased in 1988 with the end of the Cold War. How much Plutonium-238 NASA and the DOE has stockpiled is classified, but it has been speculated that it has at most enough for one more large Flag Ship class mission and perhaps a small Scout class mission. Plus, once weapons grade plutonium-239 is manufactured, there’s no re-processing it the desired Pu-238 isotope. The plutonium that currently powers Curiosity across the surface of Mars was bought from the Russians, and that source ended in 2010. New Horizons is equipped with a spare MMRTG that was built for Cassini, which was launched in 1999.

Technicians handle an RTG at the Payload Hazardous Servicing Facility at the Kennedy Space Center for the Cassini spacecraft. (Credit: NASA).

As an added bonus, plutonium powered missions often exceed expectations as well. For example, the Voyager 1 & 2 spacecraft had an original mission duration of five years and are now expected to continue well into their fifth decade of operation. Mars Curiosity doesn’t suffer from the issues of “dusty solar panels” that plagued Spirit and Opportunity and can operate through the long Martian winter. Incidentally, while the Spirit and Opportunity rovers were not nuclear powered, they did employ tiny pellets of plutonium oxide in their joints to stay warm, as well as radioactive curium to provide neutron sources in their spectrometers. It’s even quite possible that any alien intelligence stumbles upon the five spacecraft escaping our solar system (Pioneer 10 & 11, Voyagers 1 & 2, and New Horizons) could conceivably date their departure from Earth by measuring the decay of their plutonium power source. (Pu-238 has a half life of 87.7 years and eventually decays after transitioning through a long series of daughter isotopes into lead-206).

New Horizons in the Payload Hazardous Servicing Facility at the Kennedy Space Center. Note the RTG (black) protruding from the spacecraft. (Credit: NASA/Uwe W.)

The current production run of Pu-238 will be carried out at the Oak Ridge National Laboratory (ORNL) using its High Flux Isotope Reactor (HFIR). “Old” Pu-238 can also be revived by adding newly manufactured Pu-238 to it.

“For every 1 kilogram, we really revive two kilograms of the older plutonium by mixing it… it’s a critical part of our process to be able to utilize our existing supply at the energy density we want it,” Green told a recent Mars exploration planning committee.

Still, full target production of 1.5 kilograms per year may be some time off. For context, the Mars rover Curiosity utilizes 4.8 kilograms of Pu-238, and New Horizons contains 11 kilograms. No missions to the outer planets have left Earth since the launch of Curiosity in November 2011, and the next mission likely to sport an RTG is the proposed Mars 2020 rover. Ideas on the drawing board such as a Titan lake lander and a Jupiter Icy Moons mission would all be nuclear powered.

Engineers perform a fit check of the MMRTG on Curiousity at the Kennedy Space Center. The final installation of the MMRTG occured the evening prior to launch. (Credit: NASA/Cory Huston). — Engineers perform a fit check of the MMRTG on Curiosity at the Kennedy Space Center. The final installation of the MMRTG occurred the evening prior to launch. (Credit: NASA/Cory Huston).

Along with new plutonium production, NASA plans to have two new RTGs dubbed Advanced Stirling Radioisotope Generators (ASRGs) available by 2016. While more efficient, the ASRG may not always be the device of choice. For example, Curiosity uses its MMRTG waste heat to keep instruments warm via Freon circulation. Curiosity also had to vent waste heat produced by the 110-watt generator while cooped up in its aero shell enroute to Mars.

Cutaway diagram of the Advanced Stirling Radioisotope Generator. (Credit: DOE/NASA).

And of course, there are the added precautions that come with launching a nuclear payload. The President of the United States had to sign off on the launch of Curiosity from the Florida Space Coast. The launch of Cassini, New Horizons, and Curiosity all drew a scattering of protesters, as does anything nuclear related. Never mind that coal fired power plants produce radioactive polonium, radon and thorium as an undesired by-product daily.

An RTG (in the foreground on the pallet) left on the Moon by astronauts during Apollo 14. (Credit: NASA/Alan Shepard).

Said launches aren’t without hazards, albeit with risks that can be mitigated and managed. One of the most notorious space-related nuclear accidents occurred early in the U.S. space program with the loss of an RTG-equipped Transit-5BN-3 satellite off of the coast of Madagascar shortly after launch in 1964. And when Apollo 13 had to abort and return to Earth, the astronauts were directed to ditch the Aquarius Landing Module along with its nuclear-powered science experiments meant for the surface of the Moon in the Pacific Ocean near the island of Fiji. (They don’t tell you that in the movie) One wonders if it would be cost effective to “resurrect” this RTG from the ocean floor for a future space mission. On previous nuclear-equipped launches such as New Horizons, NASA placed the chance of a “launch accident that could release plutonium” at 350-to-1 against Even then, the shielded RTG is “over-engineered” to survive an explosion and impact with the water.

But the risks are worth the gain in terms of new solar system discoveries. In a brave new future of space exploration, the restart of plutonium production for peaceful purposes gives us hope. To paraphrase Carl Sagan, space travel is one of the best uses of nuclear fission that we can think of!

March 18, 2013December 23, 2015 by David Dickinson

Stalking the Lunar X

The Lunar X, captured by the author on June 8th, 2011.

This week offers observers a shot at capturing a fascinating but elusive lunar feature.

But why study the Moon? It’s a question we occasionally receive as a backyard astronomer. There’s a sort of “been there, done that” mentality associated with our nearest natural neighbor in space. Keeping one face perpetually turned Earthward, the Moon goes through its 29.5 synodic period of phases looking roughly the same from one lunation to the next. Then there’s the issue of light pollution. Many deep sky imagers “pack it in” during the weeks surrounding the Full Moon, carefully stacking and processing images of wispy nebulae and dreaming of darker times ahead…

But fans of the Moon know better. Just think of life without the Moon. No eclipses. No nearby object in space to give greats such as Sir Isaac Newton insight into celestial mechanics 101. In fact, there’s a fair amount of evidence to suggest that life arose here in part because of our large Moon. The Moon stabilizes our rotational axis and produces a large tidal force on our planet. And as all students of lunar astronomy know, not all lunations are exactly equal.

A daytime capture of the Lunar X. (Photo by Author).

This week, we get a unique look at a feature embedded in the lunar highlands which demonstrates this fact. The Lunar X, also sometimes known as the Purbach cross or the Werner X reaches a decent apparition on March 19^th at 11:40UT/7:40EDT favoring East Asia and Australia. This feature is actually the overlapping convergence of the rims of Blanchinus, La Caille and Purbach craters. The X-shaped feature reaches a favorable illumination about six hours before 1^st Quarter phase and six hours after Last Quarter phase. It is pure magic watching the X catch the first rays of sunlight while the floor of the craters are still immersed in darkness. For about the span of an hour, the silver-white X will appear to float just beyond the lunar terminator.

Visibility of the Lunar X for the Remainder of 2013.
Lunation	Date	Time	Phase	Favors
1116	March 19^th	11:40UT/7:40EDT	Waxing	East Asia/Australia
1116	April 3^rd	3:20UT/23:20EDT*	Waning	Africa/Europe
1117	April 17^th	23:47UT/19:47EDT	Waxing	Eastern North America
1117	May 2^nd	16:19UT/12:19EDT	Waning	Central Pacific
1118	May 17^th	10:51UT/6:51EDT	Waxing	East Asia/Australia
1118	June 1^st	4:31UT/0:31EDT	Waning	Western Africa
1119	June 15^th	21:21UT/17:21EDT	Waxing	South America
1119	June 30^th	16:04UT/12:04EDT	Waning	Western Pacific
1120	July 15^th	7:49UT/3:49EDT	Waxing	Australia
1120	July 30^th	3:16UT/23:16EDT*	Waning	Africa/Western Europe
1121	August 13^th	18:50UT/14:50EDT	Waxing	South Atlantic
1121	August 28^th	14:27UT/10:27EDT	Waning	Central Pacific
1122	September 12^th	9:50UT/5:50EDT	Waxing	East Asia/Australia
1122	September 27^th	2:00UT/22:00EDT*	Waning	Middle East/East Africa
1123	October 11^th	19:52UT/15:52EDT	Waxing	Atlantic Ocean
1123	October 26^th	14:12UT/10:12EDT	Waning	Central Pacific
1124	November 10^th	10:03UT/5:03EST	Waxing	East Asia/Australia
1124	November 25^th	3:14UT/22:14EST*	Waning	Africa/Europe
1125	December 10^th	00:57UT/19:57EST	Waxing	Western North America
1126	December 24^th	17:07UT/12:07EST	Waning	Western Pacific
Times marked in bold* denote visibility in EDT/EST the evening prior.

Fun Factoid: All lunar apogees and perigees are not created equal either. The Moon also reaches another notable point tonight at 11:13PM EDT/ 3:13 UT as it arrives at its closest apogee (think “nearest far point”) in its elliptical orbit for 2013 at 404,261 kilometres distant. Lunar apogee varies from 404,000 to 406,700 kilometres, and the angular diameter of the Moon appears 29.3’ near apogee versus 34.1’ near perigee. The farthest and visually smallest Full Moon of 2013 occurs on December 17^th.

The first sighting of the Lunar X feature remains a mystery, although modern descriptions of the curious feature date back to an observation made by Bill Busler in June 1974. As the Sun rises across the lunar highlands the feature loses contrast. By the time the Moon reaches Full, evidence of the Lunar X vanishes all together. With such a narrow window to catch the feature, many longitudes tend to miss out during successive lunations. Note that it is possible to catch the 1^st and Last Quarter Moon in the daytime.

A 1st Quarter Moon with the Lunar X (inset). (Photo by Author).

Compounding the dilemma is the fact that the lighting angle for each lunation isn’t precisely the same. This is primarily because of two rocking motions of the Moon known as libration and nutation. Due to these effects, we actually see 59% of the lunar surface. We had to wait for the advent of the Space Age and the flight of the Soviet spacecraft Luna 3 in 1959 to pass the Moon and look back and image its far side for the first time.

We actually managed to grab the Lunar X during a recent Virtual Star Party this past February. Note that another fine example of lunar pareidolia lies along the terminator roughly at the same time as the Lunar X approaches favorable illumination. The Lunar V sits near the center of the lunar disk near 1^st and Last Quarter as well and is visible right around the same time. Formed by the confluence of two distinct ridges situated between the Mare Vaporum and Sinus Medii, it is possible to image both the Lunar X and the Lunar V simultaneously!

A simultaneous capture of the Lunar X & the Lunar V features. (Photo by Author).

This also brings up the interesting possibility of more “Lunar letters” awaiting discovery by keen-eyed amateur observers… could a visual “Lunar alphabet be constructed similar to the one built by Galaxy Zoo using galactic structures? Obviously, the Moon has no shortage of “O’s,” but perhaps “R” and “Q” would be a bit more problematic. Let us know what you see!

-Thanks to Ed Kotapish for providing us with the calculations for the visibility of the Lunar X for 2013.

March 12, 2013December 23, 2015 by Ken Kremer

Curiosity Discovers Environment Where Life Could have Thrived on Ancient Mars

This set of images shows the results from the rock abrasion tool from Opportunity (left) and the drill from NASA's Curiosity rover (right). Note how the rock grindings from Opportunity are brownish red, indicating the presence of hematite, a strongly oxidized iron-bearing mineral. Such minerals are less supportive of habitability and also may degrade organic compounds. On the right is the hole produced by Curiosity during the first drilling into a rock on Mars to collect a sample from inside the rock. In this case, the rock produced gray tailings -- not red -- suggesting the presence of iron that is less oxidized. Curiosity also found clay minerals that form in more neutral water friendly to the formation of life. Credit: NASA

After analyzing the first powder ever drilled from the interior of a Martian rock, NASA’s Curiosity rover discovered some of the key chemical ingredients necessary for life to have thrived on early Mars billions of years ago.

Curiosity has achieved her goal of discovering a habitable environment on the Red Planet, mission scientists reported today at a briefing held at NASA headquarters in Washington, D.C.

Data collected by Curiosity’s two analytical chemistry labs (SAM and CheMin) confirm that the gray powder collected from inside the sedimentary rock where the rover is exploring – near an ancient Martian stream bed – possesses a significant amount of phyllosilicate clay minerals; indicating an environment where Martian microbes could once have thrived in the distant past.

“We have found a habitable environment which is so benign and supportive of life that probably if this water was around, and you had been on the planet, you would have been able to drink it,” said John Grotzinger, the chief scientist for the Curiosity Mars Science Laboratory mission at the California Institute of Technology in Pasadena, Calif.

Curiosity cored the rocky sample from a fine-grained, sedimentary outcrop named “John Klein” inside a shallow basin named Yellowknife Bay, and delivered pulverized powered to the Sample Analysis at Mars (SAM) and Chemistry and Mineralogy (CheMin) instruments inside the robot.

The presence of abundant phyllosilicate clay minerals in the John Klein drill powder indicates a fresh water environment. Further evidence derives from the veiny sedimentary bedrock shot through with calcium sulfate mineral veins that form in a neutral to mildly alkaline pH environment.

This side-by-side comparison shows the X-ray diffraction patterns of two different samples collected from the Martian surface by NASA's Curiosity rover. These images were obtained by Curiosity's Chemistry and Mineralogy instrument (CheMin) and show the patterns obtained from a drift of windblown dust and sand called "Rocknest" and from a powdered rock sample drilled from the "John Klein" bedrock wherer Curiosty corted the frist interior rock samples. The presence of abundant clay minerals in the John Klein drill powder and the lack of abundant salt suggest a fresh water environment. The presence of calcium sulfates suggests a neutral to mildly alkaline pH environment. NASA/JPL-Caltech/Ames — This side-by-side comparison shows the X-ray diffraction patterns of two different samples collected from the Martian surface by NASA’s Curiosity rover. These images were obtained by Curiosity’s Chemistry and Mineralogy instrument (CheMin) and show the patterns obtained from a drift of windblown dust and sand called “Rocknest” (left) and from a powdered rock sample drilled by Curiosity from the “John Klein” bedrock (right). The presence of abundant phyllosilicate clay minerals in the John Klein drill powder suggest a fresh water environment. The presence of calcium sulfates suggests a neutral to mildly alkaline pH environment. NASA/JPL-Caltech/Ames

“Clay minerals make up at least 20 percent of the composition of this sample,” said David Blake, principal investigator for the CheMin instrument at NASA’s Ames Research Center in Moffett Field, Calif.

The rovers 7 foot (2.1 meter) long robotic arm fed aspirin sized samples of the gray, pulverized powder into the miniaturized CheMin SAM analytical instruments on Feb. 22 and 23, or Sols 195 and 196. The samples were analyzed on Sol 200.

Scientists were able to identify carbon, hydrogen, oxygen, nitrogen, sulfur and phosphorus in the sample – all of which are essential constituents for life as we know it based on organic molecules.

“The range of chemical ingredients we have identified in the sample is impressive, and it suggests pairings such as sulfates and sulfides that indicate a possible chemical energy source for micro-organisms,” said Paul Mahaffy, principal investigator of the SAM suite of instruments at NASA’s Goddard Space Flight Center in Greenbelt, Md.

The discovery of phyllosilicates on the floor of Gale crater was unexpected and has delighted the scientists. Based on spectral observations from Mars orbit. Grotzinger told me previously that phyllosilicates had only been detected in the lower reaches of Mount Sharp, the 3 mile (5 km) high mountain that is Curiosity’s ultimate destination.

Grotzinger said today that Curiosity will remain in the Yellowknife Bay area for several additional weeks or months to fully characterize the area. The rover will also conduct at least one more drilling campaign to try and replicate the results, check for organic molecules and search for new discoveries.

Ken Kremer

March 12, 2013April 26, 2016 by Jason Major

Saturn to Shed its Spooky Spokes for Summer

Cassini image of Saturn's rings from Dec. 20, 2012 (NASA/JPL-Caltech/SSI)

As Saturn steadily moves along its 29.7-year-long orbit toward summertime in its northern hemisphere NASA’s Cassini spacecraft is along for the ride, giving astronomers a front-row seat to seasonal changes taking place on the ringed planet.

One of these fluctuations is the anticipated disappearance of the “spokes” found in the rings, a few of which can be seen above in an image captured on Dec. 20 of last year.

First identified by Voyager in 1980, spokes are ghostly streaks of varying size and brightness that stretch radially across Saturn’s ring system. They orbit around the planet with the ring particles and can last for hours before fading away.

*Under the right lighting conditions spokes can appear dark, as seen in this image from Jan. 2010 (NASA/JPL/SSI)*

One of the most elusive and transient of features found on Saturn, spokes are thought to be made up of larger microscopic particles of ice — each at least a micron or more — although exactly what makes them gather together isn’t yet known.

They are believed to be associated with interactions between ring particles and Saturn’s electromagnetic field.

“The spokes are most prominent at a point in the rings where the ring particles are moving at the same speed as Saturn’s electromagnetic field,” said Brad Wallis, Cassini rings discipline scientist. “That idea and variations of it are still the most prominent theories about the spokes.”

Other researchers have suggested that they may be caused by electron beams issuing outwards along magnetic field lines from lightning storms in Saturn’s atmosphere.

Regardless of how they are created, spokes are more often observed when sunlight is striking the rings edge-on — that is, during the spring and autumn equinoxes. Perhaps the increased solar radiation along Saturn’s equator increases the formation of lightning-generating storms, in turn creating more spokes? It’s only a guess, but Cassini — and astronomers — will be watching to see if these furtive features do in fact fail to appear during Saturn’s northern summer, the height of which arrives in 2016.

NASA’s KaBOOM Experimental Asteroid Radar Aims to Thwart Earth’s Kaboom

Installation of new KaBOOM asteroid detection radar dish antenna system at the Kennedy Space Center, Florida. Credit: Ken Kremer (kenkremer.com)

Over the past month, about a half dozen rather large asteroids have careened nearby our home planet and in one case caused significant injury and property damage with no forewarning – showcasing the hidden lurking dangers from lackluster attitudes towards Asteroid Detection & Planetary Defense.

Now in a prescient coincidence of timing, NASA is funding an experimental asteroid radar detection array called ‘KaBOOM’ that may one day help thwart Earth’s untimely Ka-boom – and which I inspected first-hand this past week at the Kennedy Space Center (KSC),following the SpaceX Falcon 9 blastoff for the ISS.

“KaBOOM takes evolutionary steps towards a revolutionary capability,” said Dr. Barry Geldzahler, KaBOOM Chief Scientist of NASA Headquarters, in an exclusive interview with Universe Today.

If successful, KaBOOM will serve as a prelude to a US National Radar Facility and help contribute to an eventual Near Earth Object (NEO) Planetary Defense System to avert Earth’s demise.

“It will enable us to reach the goal of tracking asteroids farther out than we can today.”

First some background – This weekend a space rock the size of a city block whizzed past Earth at a distance of just 2.5 times the distance to our Moon. The asteroid – dubbed 2013 ET – is noteworthy because it went completely undetected until a few days beforehand on March 3 and measures about 460 feet (140 meters) in diameter.

KaBOOM experimental asteroid radar array at KSC consists of three 12 meter wide dish antennas mounted on pedestals at the Kennedy Space Center in Florida. Credit: Ken Kremer (kenkremer.com)

2013 ET follows close on the heels of the Feb. 15 Russian meteor that exploded violently with no prior warning and injured over 1200 people on the same day as Asteroid 2012 DA 14 zoomed past Earth barely 17,000 miles above the surface – scarcely a whisker astronomically speaking.

Had any of these chunky asteroids actually impacted cities or other populated areas, the death toll and devastation would have been absolutely catastrophic – potentially hundreds of billions of dollars !

Taken together, this rash of uncomfortably close asteroid flybys is a wake-up call for a significantly improved asteroid detection and early warning system. KaBOOM takes a key step along the path to those asteroid warning goals.

KaBOOM asteroid radar under construction near alligator infested swamps at the Kennedy Space Center Visitor Complex in Florida. Credit: Ken Kremer (kenkremer.com) — KaBOOM asteroid radar under construction near alligator infested swamps at the Kennedy Space Center in Florida. Credit: Ken Kremer (kenkremer.com)

‘KaBOOM’ – the acronym stands for ‘Ka-Band Objects Observation and Monitoring Project’ – is a new test bed demonstration radar array aimed at developing the techniques required for tracking and characterizing Near Earth Objects (NEO’s) at much further distances and far higher resolution than currently available.

“The purpose of KaBOOM is to be a ‘proof of concept’ using coherent uplink arraying of three widely spaced antennas at a high frequency; Ka band- 30 GHz,” KaBOOM Chief Scientist Geldzahler told me.

Currently the KaBOOM array consists of a trio of 12 meter wide radar antennas spaced 60 meters apart – whose installation was just completed in late February at a remote site at KSC near an alligator infested swamp.

I visited the array just days after the reflectors were assembled and erected, with Michael Miller, KaBOOM project manager of the Kennedy Space Center. “Ka Band offers greater resolution with shorter wavelengths to image smaller space objects such as NEO’s and space debris.”

“The more you learn about the NEO’s the more you can react.”

“This is a small test bed demonstration to prove out the concept, first in X-band and then in Ka band,” Miller explained. “The experiment will run about two to three years.”

Miller showed how the dish antennae’s are movable and can be easily slewed to different directions as desired.

“The KaBOOM concept is similar to that of normal phased arrays, but in this case, instead of the antenna elements being separated by ~ 1 wavelength [1 cm], they are separated by ~ 6000 wavelengths. In addition, we want to correct for the atmospheric twinkling in real time,” Geldzahler told me.

Why are big antennae’s needed?

“The reason we are using large antennas is to send more powerful radar signals to track and characterize asteroids farther out than we can today. We want to determine their size, shape, spin and surface porosity; is it a loose agglomeration of pebbles? composed of solid iron? etc.”

Such physical characterization data would be absolutely invaluable in determining the forces required for implementing an asteroid deflection strategy in case the urgent need arises.

How does KaBOOM compare with and improve upon existing NEO radars in terms of distance and resolution?

“Currently at NASA¹s Goldstone 70 meter antenna in California, we can track an object that is about 0.1 AU away [1 astronomical unit is the average distance between the Earth and the sun, 93 million miles, so 0.1 AU is ~ 9 million miles]. We would like to track objects 0.5 AU or more away, perhaps 1 AU.”

“In addition, the resolution achievable with Goldstone is at best 400 cm in the direction along the line of sight to the object. At Ka band, we should be able to reduce that to 5 cm – that’s 80 times better !”

“In the end, we want a high power, high resolution radar system,” Geldzahler explained.

Thumbs Up for Science & Planetary Defense ! Ken Kremer; Universe Today and Mike Miller; NASA KSC KaBOOM project manager. Credit: Ken Kremer (kenkremer.com) — Thumbs Up for Science & Planetary Defense !
Ken Kremer; Universe Today and Mike Miller; NASA KSC KaBOOM project manager. Credit: Ken Kremer (kenkremer.com)

Another significant advantage compared to Goldstone, is that the Ka radar array would be dedicated 24/7 to tracking and characterizing NEO’s and orbital debris, explained Miller.

Goldstone is only available about 2 to 3% of the time since it’s heavily involved in numerous other applications including deep space planetary missions like Curiosity, Cassini, Deep Impact, Voyager, etc.

‘Time is precious’ at Goldstone – which communicates with some 100 spacecraft per day, says Miller.

“If/when the proof of concept is successful, then we can envision an array of many more elements that will enable us to reach the goal of tracking asteroids farther out than we can today,” Geldzahler elaborated.

A high power, high resolution radar system can determine the NEO orbits about 100,000 times more precisely than can be done optically.

Lead KaBOOM scientist Barry Geldzahler ‘assists’ with dish antenna installation at the Kennedy Space Center; - I’m from Headquarters and I’m here to help’ - is Barry’s mantra. Credit: NASA — Lead KaBOOM scientist Barry Geldzahler ‘assists’ with dish antenna installation at the Kennedy Space Center; – ‘I’m from Headquarters and I’m here to help’ – is Barry’s mantra. Credit: NASA/KSC

So – what are the implications for Planetary Defense ?

“If we can track asteroids that are up to 0.5 AU rather than 0.1 AU distant, we can track many more than we can track today.”

“This will give us a better chance of finding potentially hazardous asteroids.”

“If we were to find that a NEO might hit the Earth, NASA and others are exploring ways of mitigating the potential danger,” Geldzahler told me.

Kaboom’s ‘First light’ is on schedule for late March 2013.

Lessons From a Space Dummy

Ivan Ivanovich, currently on display at the Smithsonian National Air and Space Museum. Credit: Eric Long, courtesy of the National Air and Space Museum.

Before a man could head into space, the Russians felt a mannequin needed to get there first.

It was on this day (March 9) in 1961 that Ivan Ivanovich — the mannequin, or space dummy — made his first flight in a Sputnik. He then took another turn in space later that month before being placed into storage for decades. United States businessman (and failed presidential candidate) Ross Perot bought him at auction in the 1990s, and lent him to the Smithsonian National Air and Space Museum. He’s on display there today.

Universe Today caught up with Cathleen Lewis, the museum’s curator of international space programs and spacesuits in the division of space history. She explained that the mannequin was actually designed and built by three organizations:

– Zvezda (aka JSC Zvezda and RD&PE Zvezda), a firm known for high-altitude suits and spacesuits;

– The Institute for Bio-Medical Problems, which performed aerospace medicine research;

– The Moscow Institute for Prosthetics, which built the mannequin using specifications from the first two groups.

Yuri Gagarin - first human in space. Credit: Russian Archives — Yuri Gagarin – first human in space. Credit: Russian Archives

Here are some of the lessons the Russians learned from Ivan Ivanovich’s flight, according to Lewis:

– What the environment is like inside the spacecraft. While the Soviets had already sent dogs and other animals into space in that time, Lewis said they were sent up in their own self-contained canisters. The chest cavity of Ivan included accelerator and angular rate changes to see what gravity changes he was experiencing. He also measured the level of radiation. Notably, Ivan actually went up twice before the first man in space (Yuri Gagarin), but the reasons are still unclear. “One assumes that because they did do it twice, they weren’t satisfied with the result the first time,” Lewis said. “But there were not a lot of modifications [between flights], so it might have been a testing failure or ambiguity in the results.”

– The communications network. During the early years of the space program, the Americans had a number of ground and ship stations scattered around the world. These stations allowed constant, but not completely continuous, contact with the astronauts. The Soviets had a much smaller network, and wanted to know exactly when the cosmonauts would be audible to ground control. The solution? Recorded singing. “They were broadcasting a song, a folk song from the spacecraft,” she said. The song had an unintended consequence: those listening in from other countries thought there was an actual cosmonaut on board, leading to rumors that other cosmonauts died before Gagarin’s flight, she said.

– Limited public outreach. In the closed Soviet society of the time, public broadcasts of missions generally happened after the fact. Engineers had to figure out how not to alarm the locals if Ivanovich ended up falling nearby a populated area and officials could not retrieve him first. They therefore wrote the word “mannequin” on Ivan to make sure people understood what was going on. It turned out the precaution was never needed, though. “He was more on target than Gagarin,” Lewis said.

March 9, 2013December 23, 2015 by Ken Kremer

Plastic Wrapped Shuttle Atlantis Slated for Grand Public Unveiling in June

Space Shuttle Atlantis enveloped in plastic shrink-wrap for protection from ongoing construction debris inside her magnificent new futuristic museum pavilion home at the Kennedy Space Center Visitor complex in Florida. She will be unveiled to the public in June 2013. Credit: Ken Kremer (kenkremer.com)

Imagine visiting Star Fleet headquarters in the 23nd Century and being engulfed by a holodeck journey to a 21st century NASA Space Shuttle; complete with a full sized Hubble Space Telescope – perhaps the important science instrument ever constructed and an outstanding legacy of the Space Shuttle Program.

Well that’s the thrilling new experience awaiting the visiting public and space enthusiasts alike starting this summer at the Kennedy Space Center Visitor Complex (KSCVC) in Florida – after the ghostlike Space Shuttle Atlantis (see photo album above & below) is unveiled from a thick coating of shrink wrapped plastic.

But – there is one important caveat regarding the holodeck dream sequence.

Starting on June 29 you will be seeing the ‘real deal’, an actual space flown NASA Space Shuttle Orbiter – not a high tech imaginary glimpse, engineering reproduction or holodeck recreation.

During the recent SpaceX CRS-2 launch events, I was very fortunate to take a behind the scenes inspection tour all around of the new ‘Space Shuttle Atlantis’ pavilion that’s been under construction at the Kennedy Visitor Complex for a year and is now racing towards completion.

And Atlantis is still supremely impressive beneath that white plastic wrap – unlike any shuttle view I’ve see over the years.

Scan through my photo album walking around Atlantis – covered in 16,000 square feet of shrink wrap plastic – and the Star Fleet like pavilion that truly reminded me of an exciting Star Trek adventure ; to see what’s in store soon. The orange exterior pavilion facade is meant to evoke the scorching heat of reentry into the Earth’s atmosphere.

Shrink-wrapped Space Shuttle Atlantis inside museum home under construction at the Kennedy Space Center Visitor complex in Florida - mounted on pedestals. Credit: Ken Kremer (kenkremer.com) — Shrink-wrapped Space Shuttle Atlantis inside museum home under construction at the Kennedy Space Center Visitor complex in Florida – mounted on steel pedestals. Credit: Ken Kremer (kenkremer.com)

The plastic wrap is protecting the orbiter from construction debris and will be unfurled in May. Then the payload bay doors will be carefully opened and the Canadian built remote manipulator system (RMS) — or robotic arm — will be installed and extended.

Inside her new 90,000-square-foot home, everyone will be treated to breathtaking, up close views of the real ‘Space Shuttle Atlantis’ mounted high on steel pedestals – tilted at exactly 43.21 degrees – simulating the outlook as though she was ‘in flight’ orbiting Earth and approaching the International Space Station (ISS).

The ISS and Hubble are the primary legacies of the Space Shuttle program. Atlantis flew 33 total space missions, spent 307 days in orbit and conducted the final flight of the shuttle era.

Rear-side view of plastic wrapped Space Shuttle Atlantis inside museum home under construction at the Kennedy Space Center Visitor complex in Florida. Credit: Ken Kremer (kenkremer.com) — Rear-side view of plastic wrapped Space Shuttle Atlantis inside museum home under construction at the Kennedy Space Center Visitor complex in Florida. Walkways will provide exquisite up close viewing access. Credit: Ken Kremer (kenkremer.com)

You’ll gaze from stem to stern and from above and below – and all while peering down into the humongous open cargo bay, up to the heat shield tiles, or across to the engines, wings, tail and crew flight deck. Walkways will provide exquisite up close viewing access.

Atlantis rises some 30 feet off the ground. Although her nose soars 26.5 feet above ground the portside wingtip sits only 7.5 feet from the floor. The wing tip top soars 87 feet from the ground.

And sitting right beside Atlantis will be a co-orbiting, high fidelity full scale replica of NASA’s Hubble Space Telescope which was deployed and upgraded by the astronaut crews of six space shuttle missions.

ISS module mockups, simulators and displays will tell the story of the massive stations intricate assembly by several dozen shuttle crews.

Star Fleet like headquarters- still under construction - is the permanent new home for Space Shuttle Atlantis due to open in June 2013 the Kennedy Space Center Visitor Complex in Florida. Credit: Ken Kremer (kenkremer.com) — Star Fleet like headquarters- still under construction – is the permanent new home for Space Shuttle Atlantis due to open in June 2013 at the Kennedy Space Center Visitor Complex in Florida. Credit: Ken Kremer (kenkremer.com)

More than 60 exhibits, hands- on activities and artifacts surrounding Atlantis will tell the complete story of the three-decade long Space Shuttle program and the thousands of shuttle workers who prepared all five orbiters for a total of 135 space missions spanning from 1981 to 2011.

Atlantis has been lovingly preserved exactly as she returned upon touchdown at the shuttle landing strip at the conclusion of her last space mission, STS-135, in July 2011 – dings, dents, scorch marks, you name it. And that is exactly as it should be in my opinion too.

Rear view of plastic wrapped Space Shuttle Atlantis with soaring tail at the Kennedy Space Center Visitor complex in Florida. Credit: Ken Kremer (kenkremer.com)

Shuttle Atlantis was towed to the Visitor Complex in November. The orbiter is housed inside a spanking new six- story museum facility constructed at a cost of $100 million that dominates the skyline at the largely revamped Kennedy Space Center Visitor Complex.

Rear view of plastic wrapped Space Shuttle Atlantis and 3 main engines at the Kennedy Space Center Visitor Complex in Florida. Credit: Ken Kremer (kenkremer.com)

Standing tall right outside the entry to the museum pavilion, visitors will see full scale replicas of the twin solid rocket boosters mated to the orange external fuel tank, suspended 24 feet above ground – and reaching to a top height of 185 feet. They will be erected vertically, precisely as they were at the Shuttle Launch Pads 39 A and 39 B. It will give a realistic sense of what it looked like atop the actual shuttle launch complex.

The mighty steel framework for holding the boosters in place (in case of hurricane force winds up to 140 MPH) was coming together piece by piece as workers maneuvered heavy duty cranes before my eyes during my pavilion museum tour just days ago.

Well, get set to zoom to space as never before beginning on June 29 with the last shuttle orbiter that ever flew in space.

Ken Kremer

Plastic wrapped Space Shuttle Atlantis tilted at 43.21 degrees and mounted on pedestals at the Kennedy Space Center Visitor Complex in Florida. Credit: Ken Kremer (kenkremer.com)

Workers install steel braces for outside display of twin shuttle Solid Rocket Boosters at new Space Shuttle Atlantis pavilions due to open in June 2013 the Kennedy Space Center Visitor Complex in Florida. Credit: Ken Kremer (kenkremer.com)

A full-scale space shuttle external fuel tank and twin solid rocket boosters will serve as a gateway at the entry to Space Shuttle Atlantis. The metallic “swish” on the outside of the new exhibit building is representative of the shuttle’s re-entry to Earth. Image credit: PGAV Destinations

Steel trusses being installed as braces for outside vertical display of full size twin, full size shuttle Solid Rocket Boosters at the Kennedy Space Center Visitor Complex in Florida. Credit: Ken Kremer (kenkremer.com) — Steel trusses being installed as braces for outside vertical display of twin, full size shuttle Solid Rocket Booster replicas at the Kennedy Space Center Visitor Complex in Florida. Credit: Ken Kremer (kenkremer.com)

March 8, 2013December 23, 2015 by Ken Kremer

Solar Storm Blasting to Mars Shuts Down Curiosity – 1st Rocky Sample Results on tap

Curiosity Rover snapped this self portrait mosaic with the MAHLI camera while sitting on flat sedimentary rocks at the “John Klein” outcrop where the robot conducted historic first sample drilling inside the Yellowknife Bay basin, on Feb. 8 (Sol 182) at lower left in front of rover. The photo mosaic was stitched from raw images snapped on Sol 177, or Feb 3, 2013, by the robotic arm camera - accounting for foreground camera distortion. Credit: NASA/JPL-Caltech/MSSS/Marco Di Lorenzo/KenKremer (kenkremer.com)

Due to a fast approaching solar storm, NASA has temporarily shut down surface operations of the Curiosity Mars Science Lab (MSL) rover.

NASA took the precautionary measure because ‘a big coronal mass ejection’ was predicted to hit Mars over the next few days starting March 7, or Martian Sol 207 of the mission, researchers said.

The rover team wants to avoid a repeat of the computer memory glitch that afflicted Curiosity last week, and caused the rover to enter a protective ‘safe mode’.

“The rover was commanded to go to sleep,” says science team member Ken Herkenhoff of the US Geological Survey (USGS).

“Space weather can by nasty!”

This is the 2nd shutdown of the 1 ton robot in a week. Curiosity had just been returned to active status over the weekend.

A full resumption of science operations had been anticipated for next week, but is now on hold pending the outcome of effects from the solar storm explosions.

“We are making good progress in the recovery,” said Mars Science Laboratory Project Manager Richard Cook, of NASA’s Jet Propulsion Laboratory, prior to the new solar flare.

“Storm’s a-comin’! There’s a solar storm heading for Mars. I’m going back to sleep to weather it out,” tweeted Curiosity.

Solar flares cause intense bursts of radiation that can damage spacecraft and also harm space faring astronauts, and require the installation of radiation shielding and hardening on space based assets.

Since Mars lacks a magnetic field, the surface is virtually unprotected from constant bombardment by radiation.

NASA’s other spacecraft exploring Mars were unaffected by the solar eruptions – including the long lived Opportunity rover and the orbiters; Mars Odyssey & Mars Reconnaissance Orbiter.

Curiosity has been in the midst of analyzing the historic 1st samples of gray rocky powder ever cored from the interior of a Martian rock about a month ago.

Eventually, the six-wheeled mega rover will set off on a nearly year long trek to her main destination – the sedimentary layers of the lower reaches of the 3 mile (5 km) high mountain named Mount Sharp – some 6 miles (10 km) away.

So far Curiosity has snapped over 48,000 images and traveled nearly 0.5 miles.

Curiosity’s goal is to assess whether the Gale Crater area on Mars ever offered a habitable zone conducive for Martian microbial life, past or present.

Ken Kremer