This Mountain on Mars Is Leaking

Seasonal flows spotted by HiRISE on northwestern slopes in Hale Crater. (NASA/JPL/University of Arizona)

As the midsummer Sun beats down on the southern mountains of Mars, bringing daytime temperatures soaring up to a balmy 25ºC (77ºF), some of their slopes become darkened with long, rusty stains that may be the result of water seeping out from just below the surface.

The image above, captured by the HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter on Feb. 20, shows mountain peaks within the 150-km (93-mile) -wide Hale Crater. Made from data acquired in visible and near infrared wavelengths the long stains are very evident, running down steep slopes below the rocky cliffs.

These dark lines, called recurring slope lineae (RSL) by planetary scientists, are some of the best visual evidence we have of liquid water existing on Mars today – although if RSL are the result of water it’s nothing you’d want to fill your astro-canteen with; based on the first appearances of these features in early Martian spring any water responsible for them would have to be extremely high in salt content.

According to HiRISE Principal Investigator Alfred McEwen “[t]he RSL in Hale have an unusually “reddish” color compared to most RSL, perhaps due to oxidized iron compounds, like rust.”

See a full image scan of the region here, and watch an animation of RSL evolution (in another location) over the course of a Martian season here.

Perspective view of Hale crater made from data acquired by ESA's Mars Express. Credit: ESA/DLR/FU Berlin (G. Neukum)
Perspective view of Hale crater made from data acquired by ESA’s Mars Express. Credit: ESA/DLR/FU Berlin (G. Neukum)
Channels in the southeastern ejecta of Hale crater. Credit: NASA/JPL-Caltech/Arizona State University. (Source.)
THEMIS image of channels in the southeastern ejecta of Hale crater. Credit: NASA/JPL-Caltech/Arizona State University. (Source.)

Hale Crater itself is likely no stranger to liquid water. Its geology strongly suggests the presence of water at the time of its formation at least 3.5 billion years ago in the form of subsurface ice (with more potentially supplied by its cosmic progenitor) that was melted en masse at the time of impact. Today carved channels and gullies branch within and around the Hale region, evidence of enormous amounts of water that must have flowed from the site after the crater was created. (Source.)

The crater is named after George Ellery Hale, an astronomer from Chicago who determined in 1908 that sunspots are the result of magnetic activity.

Read more on the University of Arizona’s HiRISE site here.

Sources: NASA, HiRISE and Alfred McEwen

UPDATE April 13: Conditions for subsurface salt water (i.e., brine) have also been found to exist in Gale Crater based on data acquired by the Curiosity rover. Gale was not thought to be in a location conducive to brine formation, but if it is then it would further strengthen the case for such salt water deposits in places where RSL have been observed. Read more here.

How Dense is the Asteroid Belt?

How Dense is the Asteroid Belt?

We’ve seen way too many science fiction episodes that show asteroid belts as dense fields of tumbling boulders. How dense is the asteroid belt, and how to spacecraft survive getting through them?

For the purposes of revenue, lazy storytelling, and whatever it is Zak Snyder tells himself to get out of bed in the morning, when it comes to asteroids, Science fiction and video games creators have done something of disservice to your perception of reality.

Take a fond trip down sci-fi memory lane, and think about the time someone, possibly you, has had to dogfight or navigate through yet another frakkin’ asteroid belt. Huge space rocks tumbling dangerously in space! Action! Adventure! Only the skilled pilot, with her trusty astromecha-doplis ship can maneuver through the dense cluster of space boulders, dodging this way and that, avoiding certain collision.

And then she shoots her pew pew laser breaking up larger asteroids up into smaller ones, possibly obliterating them entirely depending on the cg budget. Inevitably, there’s bobbing and weaving. Pursuit craft will clip their wings on asteroids, spinning off into nearby tango. Some will fly straight into a space boulder.

Finally you’ll thread the needle on a pair of asteroids and the last ship of the whatever they’re called clicky clacky mantis Zorak bug people will try and catch you, but he/it won’t be quite so lucky. Poetically getting squashed like… a… bug. Sackhoff for the win, pilot victorious.

Okay, you probably knew the laser part is totally fake. I mean, everybody knows you can’t hear sounds in space. Outside of Starbuck being awesome, is that at all realistic? And if so, how does NASA maneuver unmanned spacecraft through that boulder-strewn grand canyon death trap to reach the outer planets?

The asteroid belt is a vast region between the orbits of Mars and Jupiter. Our collection of space rocks starts around 300 million kilometers from the Sun and ends around 500 million kilometers. The first asteroid, the dwarf planet Ceres which measures 950 km across, was discovered in 1801, with a “That’s funny.”. Soon after astronomers turned up many more small objects orbiting in this region at the “Oooh neat!” stage.

Artist’s concept of Dawn in its survey orbit at dwarf planet Ceres. Credit: NASA/JPL-Caltech
Artist’s concept of Dawn in its survey orbit at dwarf planet Ceres. Credit: NASA/JPL-Caltech

They realized it was a vast belt of material orbiting the Sun, with I suspect a “We’re all gonna die.”. To date, almost half a million asteroids have been discovered, most of which are in the main belt.

As mentioned in a another video, gathering up all the material in the asteroid belt and gluing it together makes a mass around 4% of the Moon. So, in case one of your friends gets excited and suggests it was a failed planet, you can bust out that stat and publicly shame them for being so 1996, Goodwill Hunting style. You like asteroids? How about them asteroids?

There’s a few hundred larger than 100 km across, and tens of millions of rocks a hundred meters across. Any one of these could ruin a good day, or bring a bad day to a welcome firey close for either a depressed wayfaring spacecraft or a little bluegreen speck of a planet. Which sounds dangerous all the way around.

Fortunately, our asteroid belt is a vast region of space. Let’s wind up the perspective-o-meter. If you divide the total number of objects in the field by the volume of space that asteroid belt takes up, each space rock is separated by hundreds of thousands of kilometers. Think of it as gravity’s remarkably spacious zen rock garden.

Ceres compared to asteroids visited to date, including Vesta, Dawn's mapping target in 2011. Image by NASA/ESA. Compiled by Paul Schenck.
Ceres compared to asteroids visited to date, including Vesta, Dawn’s mapping target in 2011. Image by NASA/ESA. Compiled by Paul Schenck.

As a result, when NASA engineers plot a spacecraft’s route through the asteroid belt, they don’t expect to make a close encounter with any asteroids – in fact, they’ll change its flight path to intercept asteroids en route. Because hey look, asteroid!

Even though Ceres was discovered in 1801, it’s never been observed up close, until now. NASA’s Dawn spacecraft already visited Asteroid Vesta, and by the time you’re watching this video, it will have captured close-up images of the surface of Ceres.

Once again, science fiction creatives sold us out to drama over hard science. If you’re passing through an asteroid belt, you won’t need to dodge and weave to avoid the space rocks. In fact, you probably wouldn’t even know you were passing through a belt at all. You’d have to go way the heck over there to even get a nearby look at one of the bloody things. So we’re safe, our speck is safe, and all the little spacecraft are safe…. for now.

Which dramatic version of “asteroids” are you most fond of? Tell us in the comments below.

Weekly Space Hangout – March 27, 2015: Dark Matter Galaxy “X” with Dr. Sukanya Chakrabarti

Host: Fraser Cain (@fcain)
Special Guest: Dr. Sukanya Chakrabarti, Lead Investigator for team that may have discovered Dark Matter Galaxy “X”.

Guests:
Morgan Rehnberg (cosmicchatter.org / @MorganRehnberg )
Dave Dickinson (@astroguyz / www.astroguyz.com)
Brian Koberlein (@briankoberlein)
Continue reading “Weekly Space Hangout – March 27, 2015: Dark Matter Galaxy “X” with Dr. Sukanya Chakrabarti”

Helicopter Drones on Mars

Mars helicopter drone
A small drone helicopter currently being developed by engineers at NASA's Jet Propulsion Laboratory could serve as a reconnaissance scout for future Mars rovers, greatly enhancing their effectiveness. Credit NASA JPL

NASA’s Jet Propulsion Laboratory recently announced that it is developing a small drone helicopter to scout the way for future Mars rovers. Why would Mars rovers need such a robotic guide? The answer is that driving on Mars is really hard.

Here on Earth, robots exploring volcanic rims, or assisting rescuers, can be driven by remote control, with a joystick. This is because radio signals reach the robot from its control center almost instantly. Driving on the moon isn’t much harder. Radio signals traveling at the speed of light take about two and half seconds to make the round trip to the moon and back. This delay isn’t long enough to seriously interfere with remote control driving. In the 1970’s Soviet controllers drove the Lunokhod moon rovers this way, successfully exploring more than 40 km of lunar terrain.

Driving on Mars is much harder, because it is so much further away. Depending on its position with respect to Earth, signals can take between 8 and 42 minutes for the round trip. Pre-programmed instructions must be sent to the rover, which it then executes on its own. Each Martian drive takes hours of careful planning. Stereo images taken by the rover’s navigation cameras are carefully scrutinized by engineers. Images from spacecraft orbiting Mars sometimes provide additional information.

A rover can be programmed either to simply execute a list of driving commands sent from Earth, or it can use images taken by its navigation cameras and processed by its on-board computers to measure speed and detect obstacles or hazards by itself. It can even plot its own safe path to a specified goal. Drives based on instructions from the ground are the fastest.

The Mars Exploration Rovers Spirit and Opportunity could drive up to 124 meters in an hour this way. This corresponds to about the length of an American football field. But this mode was also the least safe.

When the rover actively guides itself with its cameras, progress is safer, but much slower because of all the image processing needed. It may progress by as little as 10 meters an hour, which is about the distance from the goal line to the 10 yard line on an American football field. This method must be used whenever the rover doesn’t have a clear view of the route ahead, which is often the case due to rough and hilly terrain.

As of early 2015, the farthest Curiosity has driven in a single day is 144 meters. Opportunity’s longest daily drive was 224 meters, a distance the length of two American football fields.

If ground controllers could get a better view of the path ahead, they could devise instructions allowing a future rover to safely drive much further in a day.

That’s where the idea of a drone helicopter comes in. The helicopter could fly out ahead of the rover every day. Images made from its aerial vantage point would be invaluable to ground controllers for identifying points of scientific interest, and planning driving routes to get there.

Flying a helicopter on Mars poses special challenges. One advantage is that Martian gravity is only 38% as strong as that of Earth, so that the helicopter wouldn’t need to generate as much lift as one of the same mass on Earth. A helicopter’s propeller blades generate lift by pushing air downward. This is harder to do on Mars than on Earth, because the Martian atmosphere is on hundred times thinner. To displace enough air, the propeller blades would need to spin very quickly, or to be very large.

The copter must be capable of flying on its own, using prior instructions, maintaining stable flight along a pre-specified route. It must land and take off repeatedly in rocky Martian terrain. Finally it must be capable of surviving the harsh conditions of Mars, where the temperature plummets to 100 degrees Fahrenheit or lower every night.

The JPL engineers designed a copter with a mass of 1 kilogram; a tiny fraction of the 900 kg mass of the Curiosity rover. Its propeller blades span 1.1 meters from blade tip to blade tip, and are capable of spinning at 3400 rotations per minute. The body is about the size of a tissue box.

The copter is solar powered, with a disk of solar cells gathering enough power every day to power a flight of two to three minutes and to heat the vehicle at night. It can fly about half a kilometer in that time, gathering images for transmission to ground control as it goes. Engineers expect that the reconnaissance that the drone copter gathers will be invaluable in planning a rover’s drives, tripling the distance that can be traveled in a day.

References and further reading:
Thanks to Mark Maimone of NASA Jet Propulsion Laboratory for information about the daily driving distances of Curiosity and Opportunity.

J.J. Biesiadecki, P. C. Leger, and M.W. Maimone (2007), ‘tradeoffs between directed and autonomous driving on the Mars exploration rovers’, The International Journal of Robotics Research, 26(1), 91-104

E. Howell, Opportunity Mars rover treks past 41 kilometers towards ‘Marathon Valley’, Universe Today, Dec. 2014.

T. Reyes, An incredible journey, Mars Curiosity rover reaches base of Mount Sharp. Universe Today, Sept. 2014.

Helicopter could be ‘scout’ for Mars rovers. NASA Jet Propulsion Laboratory Press release. January 22, 2015.

Crazy Engineering: The Mars helicopter. NASA Jet Propulsion Laboratory video.

Curiosity- Mars Science Laboratory, NASA.

Mars- Future rover plans. NASA

World’s Most Powerful Solid Booster Set for Space Launch System Test Firing on March 11

Orbital ATK’s five segment rocket motor is assembled in its Promontory, Utah, test stand where it is being conditioned for the March 11 ground test. Credit: Orbital ATK

All systems are go for the inaugural ground test firing on March 11 of the world’s most powerful solid rocket booster ever built that will one day power NASA’s mammoth new Space Launch System (SLS) heavy lift rocket and propel astronauts to deep space destinations.

The booster known as qualification motor, QM-1, is the largest solid rocket motor ever built and will be ignited on March 11 for a full duration static fire test by prime contractor Orbital ATK at the newly merged firms test facility in Promontory, Utah.

Ignition of the horizontally mounted motor is planned for 11:30 a.m. EDT (9:30 a.m. MDT) on Wednesday, March 11 on the T-97 test stand.

The test will be broadcast live on NASA TV.

Engineers at Orbital ATK in Promontory, Utah, prepare to test the booster that will help power NASA’s Space Launch System to space to begin missions to deep space, including to an asteroid and Mars. A test on March 11 is one of two that will qualify the booster for flight.  Image Credit:  Orbital ATK
Engineers at Orbital ATK in Promontory, Utah, prepare to test the booster that will help power NASA’s Space Launch System to space to begin missions to deep space, including to an asteroid and Mars. A test on March 11 is one of two that will qualify the booster for flight. Image Credit: Orbital ATK

The two minute long, full duration static test firing of the motor marks a major milestone in the ongoing development of NASA’s SLS booster, which is the most powerful rocket ever built in human history.

The 5-segment booster produces 3.6 million lbs of maximum thrust which equates to more than 14 Boeing 747-400s at full takeoff power!

The new 5-segment booster is directly derived from the 4-segment booster used during NASA’s three decade long Space Shuttle program. One segment has been added and therefore the new, longer and more powerful booster must be requalified to launch the SLS and humans.

A second test is planned a year from now and will qualify the boosters for use with the SLS.

Teams of engineers, operators, inspectors and program managers across Orbital ATK’s Flight Systems Group have spent months getting ready for the QM-1 test. To prepare they started countdown tests on Feb 25.

“The crew officially starts daily countdown test runs of the systems this week, at T-15 days,” said Kevin Rees, director, Test & Research Operations at Orbital ATK.

“These checks, along with other test stand calibrations, will verify all systems are ready for the static test. Our team is prepared and we are proud to play such a significant role on this program.”

The first qualification motor for NASA's Space Launch System's booster is installed in ATK's test stand in Utah and is ready for a March 11 static-fire test.   Credit:  ATK
The first qualification motor for NASA’s Space Launch System’s booster is installed in ATK’s test stand in Utah and is ready for a March 11 static-fire test. Credit: ATK

The QM-1 booster is being conditioned to 90 degrees and the static fire test will qualify the booster design for high temperature launch conditions. It sits horizontally in the test stand and measures 154 feet in length and 12 feet in diameter and weighs 801 tons.

The static fire test will collect data on 103 design objectives as measured through more than 534 instrumentation channels on the booster it is firing.

The second booster test in March 2016 will be conducted at lower temperature to qualify the lower end of the launch conditions at 40 degrees F.

The first stage of the SLS will be powered by a pair of the five-segment boosters and four RS-25 engines that will generate a combined 8.4 million pounds of liftoff thrust.

The SLS is designed to propel the Orion crew capsule to deep space destinations, including the Moon, asteroids and the Red Planet.

The maiden test flight of the SLS is targeted for no later than November 2018 and will be configured in its initial 70-metric-ton (77-ton) version with a liftoff thrust of 8.4 million pounds. It will boost an unmanned Orion on an approximately three week long test flight beyond the Moon and back.

NASA plans to gradually upgrade the SLS to achieve an unprecedented lift capability of 130 metric tons (143 tons), enabling the more distant missions even farther into our solar system.

The first SLS test flight with the uncrewed Orion is called Exploration Mission-1 (EM-1) and will launch from Launch Complex 39-B at the Kennedy Space Center.

Solid rocket boosters separate from SLS core stage in this artists concept. Credit: NASA
Solid rocket boosters separate from SLS core stage in this artists concept. Credit: NASA

Orion’s inaugural mission dubbed Exploration Flight Test-1 (EFT) was successfully launched on a flawless flight on Dec. 5, 2014 atop a United Launch Alliance Delta IV Heavy rocket Space Launch Complex 37 (SLC-37) at Cape Canaveral Air Force Station in Florida.

Orion’s inaugural mission dubbed Exploration Flight Test-1 (EFT) was successfully launched on a flawless flight on Dec. 5, 2014 atop a United Launch Alliance Delta IV Heavy rocket Space Launch Complex 37 (SLC-37) at Cape Canaveral Air Force Station in Florida.

NASA’s first Orion spacecraft blasts off at 7:05 a.m. atop United Launch Alliance Delta 4 Heavy Booster at Space Launch Complex 37 (SLC-37) at Cape Canaveral Air Force Station in Florida on Dec. 5, 2014.   Launch pad remote camera view.   Credit: Ken Kremer - kenkremer.com
NASA’s first Orion spacecraft blasts off at 7:05 a.m. atop United Launch Alliance Delta 4 Heavy Booster at Space Launch Complex 37 (SLC-37) at Cape Canaveral Air Force Station in Florida on Dec. 5, 2014. Launch pad remote camera view. Credit: Ken Kremer – kenkremer.com

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

Ken Kremer

. ………….

Learn more about MMS, Mars rovers, Orion, SpaceX, Antares, NASA missions and more at Ken’s upcoming outreach events:

Mar 9-11: “MMS, Orion, SpaceX, Antares, Curiosity Explores Mars,” Kennedy Space Center Quality Inn, Titusville, FL, evenings

NASA Administrator Charles Bolden officially unveils world’s largest welder to start construction of core stage of NASA's Space Launch System (SLS) rocket at NASA Michoud Assembly Facility, New Orleans, on Sept. 12, 2014. SLS will be the world’s most powerful rocket ever built.  Credit: Ken Kremer - kenkremer.com
NASA Administrator Charles Bolden officially unveils world’s largest welder to start construction of core stage of NASA’s Space Launch System (SLS) rocket at NASA Michoud Assembly Facility, New Orleans, on Sept. 12, 2014. SLS will be the world’s most powerful rocket ever built. Credit: Ken Kremer – kenkremer.com

Mars Loses an Ocean But Gains the Potential for Life

NASA scientists have determined that a primitive ocean on Mars held more water than Earth's Arctic Ocean and that the Red Planet has lost 87 percent of that water to space. Credit: NASA/GSFC

It’s hard to believe it now looking at Mars’ dusty, dessicated landscape that it once possessed a vast ocean. A recent NASA study of the Red Planet using the world’s most powerful infrared telescopes clearly indicate a planet that sustained a body of water larger than the Earth’s Arctic Ocean.

If spread evenly across the Martian globe, it would have covered the entire surface to a depth of about 450 feet (137 meters). More likely, the water pooled into the low-lying plains that cover much of Mars’ northern hemisphere. In some places, it would have been nearly a mile (1.6 km) deep. 

Three of the best infrared observatories in the world were used to study normal to heavy water abundances in Mars atmosphere, especially the polar caps, to create a global map of the planet's water content and infer an ancient ocean. Credit: NASA/ GSFC
Three of the best infrared observatories in the world were used to study normal to heavy water abundances in Mars atmosphere, especially the polar caps, to create a global map of the planet’s water content and infer an ancient ocean. Credit: NASA/ GSFC

Now here’s the good part. Before taking flight molecule-by-molecule into space, waves lapped the desert shores for more than 1.5 billion years – longer than the time life needed to develop on Earth. By implication, life had enough time to get kickstarted on Mars, too.

A hydrogen atom is made up of one proton and one electron, but its heavy form, called deuterium, also contains a neutron. HDO or heavy water is rare compared to normal drinking water, but being heavier, more likely to stick around when the lighter form vaporizes into space. Credit: NASA/GFSC
A hydrogen atom is made up of one proton and one electron, but its heavy form, called deuterium, also contains a neutron. HDO or heavy water is rare compared to normal drinking water, but being heavier, more likely to stick around when the lighter form vaporizes into space. Credit: NASA/GFSC

Using the three most powerful infrared telescopes on Earth – the W. M. Keck Observatory in Hawaii, the ESO’s Very Large Telescope and NASA’s Infrared Telescope Facility – scientists at NASA’s Goddard Space Flight Center studied water molecules in the Martian atmosphere. The maps they created show the distribution and amount of two types of water – the normal H2O version we use in our coffee and HDO or heavy water, rare on Earth but not so much on Mars as it turns out.

Maps showing the distribution of H20 and HDO across the planet made with the trio of infrared telescopes. Credit: NASA/GSFC
Maps showing the distribution of H20 and HDO (heavy water) across the planet made with the trio of infrared telescopes. Credit: NASA/GSFC

In heavy water, one of the hydrogen atoms contains a neutron in addition to its lone proton, forming an isotope of hydrogen called deuterium. Because deuterium is more massive than regular hydrogen, heavy water really is heavier than normal water just as its name implies. The new “water maps” showed how the ratio of normal to heavy water varied across the planet according to location and season. Remarkably, the new data show the polar caps, where much of Mars’ current-day water is concentrated, are highly enriched in deuterium.

It's thought that
It’s thought that the decay of Mars’ once-global magnetic field, the solar wind stripped away much of the planet’s early, thicker atmosphere, allowing solar UV light to break water molecules apart. Lighter hydrogen exited into space, concentrating the heavier form. Some of the hydrogen may also departed due to the planet’s weak gravity. Credit: NASA/GSFC

On Earth, the ratio of deuterium to normal hydrogen in water is 1 to 3,200, but at the Mars polar caps it’s 1 to 400.  Normal, lighter hydrogen is slowly lost to space once a small planet has lost its protective atmosphere envelope, concentrating the heavier form of hydrogen. Once scientists knew the deuterium to normal hydrogen ratio, they could directly determine how much water Mars must have had when it was young. The answer is A LOT!

Goddard scientists estimate that only 13% of Mars' original water reserves are still around today, concentrated in the icy polar caps. The rest took off for space. Credit: NASA/GSFC
Goddard scientists estimate that only 13% of Mars’ original water reserves are still around today, concentrated in the icy polar caps. The rest took off for space. Credit: NASA/GSFC

Only 13% of the original water remains on the planet, locked up primarily in the polar regions, while 87% of the original ocean has been lost to space. The most likely place for the ocean would have been the northern plains, a vast, low-elevation region ideal for cupping huge quantities of water. Mars would have been a much more earth-like planet back then with a thicker atmosphere, providing the necessary pressure, and warmer climate to sustain the ocean below.

Mars at the present time has little to no liquid water on its cold, desert-like surface. Long ago, the Sun saw its reflection from wave-rippled lakes and a northern ocean. Credit: NASA/GSFC
Mars at the present time has little to no liquid water on its cold, desert-like surface. Long ago, the Sun almost certainly saw its reflection from wave-rippled lakes and a northern ocean. Credit: NASA/GSFC

What’s most exciting about the findings is that Mars would have stayed wet much longer than originally thought. We know from measurements made by the Curiosity Rover that water flowed on the planet for 1.5 billion years after its formation. But the new study shows that the Mars sloshed with the stuff much longer. Given that the first evidence for life on Earth goes back to 3.5 billion years ago – just a billion years after the planet’s formation – Mars may have had time enough for the evolution of life.

So while we might bemoan the loss of so wonderful a thing as an ocean, we’re left with the tantalizing possibility that it was around long enough to give rise to that most precious of the universe’s creations – life.

To quote Charles Darwin: “… from so simple a beginning endless forms most beautiful and most wonderful have been, and are being, evolved.

Illustration showing Mars evolving from a wet world to the present-day Red Planet. Credit: NASA/GSFC
Illustration showing Mars evolving from a wet world to the present-day where liquid water can’t pond on its surface without vaporizing directly into the planet’s thin air. As Mars lost its atmosphere over billions of years, the remaining water, cooled and condensed to form the north and south polar caps. Credit: NASA/GSFC

The Night Mars Was Closest to Earth

On Earth, Don Parker’s Mars images were hard to beat, but the Hubble Space Telescope—six times larger than his 16-inch ‘scope and, more importantly, above the atmosphere—easily pulled it off. In this pair of images taken around the time of the planet’s closest approach in 2003, the giant volcano Olympus Mons is the small, bright circular feature above center. Image courtesy Andrew Chaikin.

Editor’s note: On August 27, 2003 Mars was closer to Earth than at any time in human history. Author Andrew Chaikin asked Universe Today to tell the story of how he was fortunate enough to enjoy the event with Don Parker, a “superb planetary photographer and wonderful guy,” Chaikin wrote. “I first met Don, a retired anesthesiologist from Coral Gables, Florida, several weeks earlier when I journeyed with my telescope to Florida to photograph the Moon passing in front of Mars, an event called an occultation. I’d seen Don’s work for decades in Sky & Telescope magazine, but until the occultation we’d never met. I certainly had never imagined that he would turn out to be as much fun as he was, with a warped, wickedly bawdy sense of humor. Standing under the moon and Mars we bonded, and soon we were making plans for me to come down to his place for the closest approach.”

Don passed away on February 22, 2015. In his memory here’s an excerpt from Chaikin’s book, A Passion for Mars.

Godspeed, Don. See you on Mars.

Don Parker with his 16-inch telescope, which he used to take thousands of superb images of the planets. Photo by Sean Walker.
Don Parker with his 16-inch telescope, which he used to take thousands of superb images of the planets. Photo by Sean Walker.

ON PAPER, Don Parker’s life story is pretty ordinary: Born in 1939, he grew up in an Italian neighborhood in Chicago. He spent a few years in the navy, went to medical school, and ended up living in Florida with his wife, Maureen, and their children, working as an anesthesiologist in a Miami hospital. Looking at his résumé you’d never know about his other life, the one dominated by a lifelong obsession with Mars. By the time he went to see Invaders from Mars and War of the Worlds as a teenager in 1953, he was building his first telescope, a three-inch refractor with lenses from Edmund Scientific and a body made from a stovepipe his dad got for him.

He was subscribing to Sky & Telescope magazine and following the continuing debate over whether the canals on Mars really existed. That was a question that only a handful of professional astronomers cared about, but amateur observers, like the ones whose drawings were printed in the magazine, seemed to be on the case. Parker got serious about observing Mars himself around 1954, when he tried to create a homemade reflector, but failed when he had trouble with the mirror. His aunt Hattie came to the rescue that Christmas by giving him a hundred dollar bill — quite a bit of money in those days — which he used to buy a professionally made eight-inch mirror. With help from his dad, he assembled the new telescope, using pipe fittings for the mounting.

In the summer of 1956, when Mars made its famously close appearance, he was at the eyepiece making drawings of his own, until a dust storm engulfed much of the planet that September, just as Mars came closest to Earth. “Mars looked like a cue ball,” Parker remembers. “There was nothing on it. It was very disappointing for me.” At the time, he thought the problem was with his instrument. “I even took the mirror out of the telescope,” he recalls. “You know,‘What the hell is going on here?’” Only much later, when information on Martian dust storms began to show up in the amateur astronomy literature, did he realize his view had been spoiled by an event happening on Mars.

Gullies on a Martian sand dune in this trio of images from NASA's Mars Reconnaissance Orbiter deceptively resemble features on Earth that are carved by streams of water. However, these gullies likely owe their existence to entirely different geological processes apparently related to the winter buildup of carbon-dioxide frost. Image Credit: NASA/JPL-Caltech/University of Arizona
Gullies on a Martian sand dune in this trio of images from NASA’s Mars Reconnaissance Orbiter deceptively resemble features on Earth that are carved by streams of water. However, these gullies likely owe their existence to entirely different geological processes apparently related to the winter buildup of carbon-dioxide frost. Image Credit: NASA/JPL-Caltech/University of Arizona

By that time Parker was in high school, and soon Martian canals became much less important than more earthly matters. “Football and blondes were my major,” he quips. Then it was off to college, and his telescope sat unused in its wooden shelter in the backyard. When it came time for his internship he convinced his wife, Maureen, that they should move to Florida so he could pursue his interest in scuba diving.

Needless to say he had no time for astronomy then, or during his residency. Then came a stint in the navy, and by the early 1970s he was back in Florida, beginning his career as an anesthesiologist and raising a family. By the time Mars made another close approach in 1973 Parker had brought his telescope down from Chicago; his parents had asked him to take it out of the backyard so they could put in a birdbath, and a few months after that, he remembers, “Maureen said, ‘Can you get that thing out of the garage?’”

He didn’t expect it to do him much good outside, however. The conventional wisdom was that south Florida, with its clouds and frequent storms, was a terrible place to do astronomy. But he found out differently that summer, when he trained his telescope on Mars. “I went, ‘Holy shit.’ It was just absolutely steady. I couldn’t believe it.”

Parker returned to his old practice of making drawings at the eyepiece to record as much detail as possible. He sent some of his work to Charles “Chick” Capen, an astronomer at Arizona’s Lowell Observatory and coordinator of Mars observations for the Association of Lunar and Planetary Observers. Soon he and Capen were in frequent contact, and from him Parker learned about the latest techniques for planetary photography.

In the 1970s that was a time-consuming process; he used professional-grade film ordered directly from Kodak and developed it with special, highly toxic chemicals that had to be laboriously prepared for each session. But that became a part of his life’s routine: off to the hospital in the morning, sailing with Maureen in the afternoon, nights at the telescope, and the rest of the time developing and printing his pictures. Returning to work after a beautiful Florida weekend, he says, “Everybody would come in with a nice tan; I’d come in looking like a bed sheet. Forty-eight hours in the darkroom! People would say, ‘Are you ill?’”

All that effort paid off. Parker’s planetary photos were now appearing frequently in Sky & Telescope. But they still couldn’t record the kind of details a good observer could see at the eyepiece. Soon Chick Capen was steering him, gently, toward more ambitious Martian observing projects—especially the exacting task of monitoring the planet’s north polar ice cap. Using a measuring device called a filar micrometer attached to their telescopes, Parker and fellow amateur Jeff Beish studied the cap as it shrank during the Martian spring and summer. Observations going back to the early years of the twentieth century showed that the north polar cap always shrank at the same predictable rate, but in the 1980s Parker and Beish found a surprise: The cap shrank more quickly, and to a smaller size, than ever before. Years before most people had even heard the term “global warming” (and more than a decade before evidence from NASA’s Mars Global Surveyor mission) Parker and Beish had found evidence that it was taking place on Mars.

Hubble images show cloud formations (left) and the effects of a global dust storm on Mars (Credit: NASA/Hubble)
Hubble images show cloud formations (left) and the effects of a global dust storm on Mars (Credit: NASA/Hubble)

Soon their observations were being reinforced by several kinds of data from other astronomers, a convergence that Parker remembers as tremendously thrilling. “All this stuff began to come together,” Parker says. “The dust storm frequencies, the cloud study frequencies, the polar cap shit. And it’s almost better than sex. And it came in from a lot of different observers, different times. It’s really kind of cool—when you’re in a science and something all of a sudden falls into place that you don’t expect. It’s really neat. Nothing’s better than sex, but it’s close.” His work with Beish and other observers was later published, to Parker’s great satisfaction, in the professional planetary science journal Icarus. For Parker it epitomizes the rewards of all those hours at the eyepiece. “It’s the thrill of the hunt,” he says. “That’s really the only thing that’s kept me going. Taking pretty pictures is fine and fun, but doing that for thirty years, it wears after a while. You’ve taken one pretty picture, you’ve taken them all.”

In the 1990s, though, the pictures started to get really pretty. For the first time, amateurs had access to electronic cameras using charged-coupled devices (CCDs), like the ones in NASA spacecraft and professional observatories. Around 1990 fellow amateur astronomer Richard Berry convinced Parker to invest in one of these new cameras, but he had a tough time getting used to it. “I hooked it up,” he remembers. “I didn’t know what to do with it. I was afraid of it. So I went back to film.”

Don Parker's image of Jupiter and the Great Red Spot, taken in 2012. Credit: Don Parker.
Don Parker’s image of Jupiter and the Great Red Spot, taken in 2012. Credit: Don Parker.

Some months later Berry came for a visit and showed Parker what he’d been missing. They pointed Parker’s sixteen-inch telescope at Jupiter, and when the first image came up on his computer screen, “It was ten times better than anything I’d ever gotten with film. The detail was amazing. It was really exciting.”

Before long Parker had completely switched over to using his electronic imager, and he never looked back. Unlike film, it offered instant gratification; no longer did he have to spend hours in the darkroom before he could see results. Even more important, the extraordinary sensitivity of CCDs allowed much shorter exposure times than film, making it possible to record a planet during those brief moments of good seeing. He could even create remarkably detailed color images by taking separate exposures through red, green, and blue filters, then combining the results in newly developed programs like Adobe Photoshop.

And to Parker’s great relief, electronic images proved as good as visual observations for monitoring Martian features like clouds, dust storms, and— thankfully—the changing polar ice caps. At last, he could put aside the filar micrometer and the tedious hours that went along with it. But there was no way around the fact that the whole experience of planetary observing had changed for serious amateurs like Parker, just as it had for professionals. He realized this during Richard Berry’s visit, as they filled his computer’s hard drive with electronic portraits of Jupiter. “I said to Richard, ‘We’ve been here for six hours and haven’t even looked through the telescope.’ And he said, ‘Yeah, now you’re a real astronomer!’”

August 26, 2003,
Coral Gables, Florida

With no time for a road trip, I’ve packed my webcam and flown to Miami. I arrive at Don Parker’s waterfront home shortly after he has awakened from yet another all-nighter at the telescope. Don is tall, pot bellied, and nearly bald, with a kind of leering, lopsided grin that spreads mischievously across his face. In his old hospital scrubs he reminds me of Peter Boyle in Young Frankenstein. Don wouldn’t mind hearing me say that; he often refers to himself as Mongo, after the character in another Mel Brooks film, Blazing Saddles. (For example: “Mongo got good pictures. Mongo happy.”)

When he was a practicing anesthesiologist he had a penchant for playing crude practical jokes in the O.R. to startle the nurses (the fart machine was a favorite). “It was like MASH,” he says. Now that he is retired there is nothing to stop him from spending every clear night at the telescope—and that is what he does, whenever Mars shines overhead. Back in 1984, when the seeing was even better than it is now, he and Jeff Beish logged 285 nights of making drawings, photos, and micrometer measurements. Parker says, “We were praying for rain. Going to the Seminole reservation to pay the guys to do a rain dance.” Two decades later, his “other life” has become his life. For months now, as Mars has grown from an orange speck in the predawn sky to its current brilliance, high overhead at midnight, Don has faithfully recorded its changing aspect, the shrinking polar cap, the comings and goings of blue hazes and yellow dust clouds, the parade of deserts and dark markings. Maureen is now a full-fledged Mars widow. Don calls it “The Curse of the Red Planet.”

For me this is the big night, and I am full of anticipation. About twelve hours from now, at 5:51am Eastern Daylight Time on August 27, Mars will be 34,646,418 million miles away from Coral Gables. An astronomer at JPL has figured out that this is closer than at any time since the year 57617 B.C., and closer than Mars will be again until the year 2287. For Don, though, this is just one more night in an unbroken string of nights that began last April and will continue into next spring. Don, of course, is far from the only one so afflicted. At any given moment this summer someone around the world is observing Mars, including a couple of twenty-something wizards in Hong
Kong and Singapore who are getting spectacular results with telescopes placed on their high-rise apartment balconies (when I mention them Don curses ruefully, then laughs).

Sitting in Don’s kitchen, we discuss the weather for the coming night— the continuing hurricane season has made things a bit iffy—as he mixes his standard brew of freeze-dried coffee, sugar, and nondairy creamer, a concoction that seems less like a beverage than a research project in polymer chemistry. Arthritis and weakening of the bones in his legs have left him with a limp so painful that he must use a cane, and as he leads me to his upstairs office he utters a string of profanities.

Seated at the computer he unveils his most recent images and I am astonished by their clarity. Even back in April, when Mars was a fraction of its current apparent size, Don was getting a remarkable amount of detail. Now his pictures are so good that they hold up in side-by-side comparisons with Mars images from the Hubble Space Telescope. If you know where to look, you can even spot the giant volcano, Olympus Mons.

When I was growing up, even the two-hundred-inch giant at Palomar couldn’t come close to the details Don has recorded with a telescope just sixteen inches in diameter.

By nightfall the sky is mercifully clear, and Don sets up a ten-inch scope for me to use. The view is amazing: The planet’s disc is shaded with subtle, dusky patterns, far more detailed than any previous view of Mars I’ve ever seen. But when I attach the webcam and fire up the laptop, the live video that appears before me is almost too good to be true. Mars is so big, so clear, that I can even see individual dark spots that must be huge, windblown craters, trailing streaks of dark sand across the pink deserts. At the south pole, the retreating ice cap gleams brilliantly, with an outlier of frosted ground distinctly visible adjacent to the larger white mass.

Long into the night, and again the next, Don and I gather our photographic records of this unprecedented encounter, he at one telescope, I at the other. I feel lucky to be alive at this moment, suspended between the time of the Neanderthals and the twenty-third century, when some of our descendants will be on Mars, looking back at Earth. Right now I am face-to-face with Mars in a way I have never been, and never will be again. It is not the Mars of my childhood picture books, or the one revealed by an armada of space probes, or the trackless world where men and women will someday leave footprints. At this moment, I am exploring Mars, and 35 million miles doesn’t seem like much, not much at all.

Andrew Chaikin.
Andrew Chaikin.

Find out more about Chaikin’s books “A Passion for for Mars,” “A Man on the Moon” and more at Chaikin’s website.