Like Yoda This Moon Shadow Looks. Yes, hmmm?

An oblique view from the Lunar Reconnaissance Orbiter of Icarus Crater on the Moon. The shadow created by the unusual central peak in the crater is reminiscent of a certain Star Wars character. Icarus is approximately 94 km in diameter. Credit: NASA/GSFC/Arizona State University.

Scientists from the Lunar Reconnaissance Orbiter say that Icarus Crater is one of a kind on the Moon because its central peak rises higher than about half its rim. Most central peaks rise only about halfway to the crater rim. But at just the ring angle and lighting conditions, the shadow this central peak creates on the rolling and jagged crater rim looks like the Star Wars Character Yoda. Interestingly, this crater is located on what some people erroneously call the “Dark Side” of the Moon – what is actually the lunar farside.

Yoda meditates about moons. Via Blastr.com
Yoda meditates about moons. Via Blastr.com

Below you can see a closeup of the central peak of Icarus crater rising out of the shadows to greet a new lunar day.

The central peak of Icarus Crater on the Moon’s farside, as seen by LROC. Image width is approximately 10 km, north is to the right. Credit: NASA/GSFC/Arizona State University.
The central peak of Icarus Crater on the Moon’s farside, as seen by LROC. Image width is approximately 10 km, north is to the right. Credit: NASA/GSFC/Arizona State University.

Icarus is located just west of Korolev crater on the lunar farside. The light-colored plains surrounding the craters were deposited during the formation of the Orientale basin, which is located over 1500 km away.

Image from LRO’s Wide Angle Camera of Icarus crater and vicinity. Image width is approximately 365 km. Credit: NASA/GSFC/Arizona State University.
Image from LRO’s Wide Angle Camera of Icarus crater and vicinity. Image width is approximately 365 km. Credit: NASA/GSFC/Arizona State University.

Find out more about these images from LRO and see larger versions at the LROC website.

Martian Dune Buggy Curiosity Adopts New Driving Mode to Save Wheels from Rough Rocks

Curiosity looks back eastward to ‘Dingo Gap’ sand dune inside Gale Crater. After crossing over the 3 foot (1 meter) tall dune on Sol 539, Feb. 9, 2014 the rover drove westward into the ‘Moonlight Valley’. The parallel rover wheel tracks are 9 feet (2.7 meters) apart. Assembled from Sol 539 colorized navcam raw images. Credit: NASA/JPL/ Ken Kremer- kenkremer.com/Marco Di Lorenzo

Curiosity looks back eastward to ‘Dingo Gap’ sand dune inside Gale Crater
After crossing over the 3 foot (1 meter) tall dune on Sol 539, Feb. 9, 2014 the rover drove westward into the ‘Moonlight Valley’. The parallel rover wheel tracks are 9 feet (2.7 meters) apart. Assembled from Sol 539 colorized navcam raw images. Credit: NASA/JPL/ Ken Kremer- kenkremer.com/Marco Di Lorenzo
See Dune and Wheel mosaics below – Story updated [/caption]

The team directing the epic trek of NASA’s Curiosity rover across the floor of Gale Crater has adopted new driving strategies and a new way forward in response to the unexpected wheel damage caused by driving over fields of rough edged Red Planet rocks in recent months.

This week, engineers directed dune buggy Curiosity to drive backwards for a lengthy distance over the Martian surface for the first time since landing.

The SUV sized vehicle apparently passed the reverse driving feasibility test with flying colors and is now well on the way to the exciting journey ahead aiming for the sedimentary layers at the base of towering Mount Sharp – the primary mission destination – which reaches 3.4 miles (5.5 km) into the Martian sky and possesses water altered minerals.

“We wanted to have backwards driving in our validated toolkit because there will be parts of our route that will be more challenging,” said Curiosity Project Manager Jim Erickson of NASA’s Jet Propulsion Laboratory, Pasadena, Calif, in a statement.

On Tuesday, Feb. 18, Curiosity not only drove in reverse, but the 329 feet (100.3 meters) distance covered marked her farthest one-day advance in over three months.

And she is also now roving over the much sought after smoother Martian terrain, as hoped, when the team decided to alter the traverse route based on high resolution imaging observations collected by the telescopic camera on NASA’s Mars Reconnaissance Orbiter (MRO) circling overhead.

The goal is to minimize wear and tear on the 20 inch diameter wheels.

This map shows the route driven and route planned for NASA's Curiosity Mars rover from before reaching "Dingo Gap" -- in upper right -- to the mission's next science waypoint, "Kimberley" (formerly referred to as "KMS-9") -- in lower left.   Credit: NASA/JPL-Caltech/Univ. of Arizona
This map shows the route driven and route planned for NASA’s Curiosity Mars rover from before reaching “Dingo Gap” — in upper right — to the mission’s next science waypoint, “Kimberley” (formerly referred to as “KMS-9”) — in lower left. Credit: NASA/JPL-Caltech/Univ. of Arizona

Engineers were forced to devise new driving techniques and consider a new route forward after the aluminum wheels accumulated significant punctures and rips during the past few months of driving over fields strewn with sharp edged Martian rocks.

“We have changed our focus to look at the big picture for getting to the slopes of Mount Sharp, assessing different potential routes and different entry points to the destination area,” Erickson said.

“No route will be perfect; we need to figure out the best of the imperfect ones.”

But to reach the smooth terrain and the science rich targets located on the pathway ahead, the six wheeled rover first had to pass through a gateway known as the ‘Dingo Gap’ sand dune.

Curiosity’s View Past Tall Dune at edge of ‘Dingo Gap’  This photomosaic from Curiosity’s Navigation Camera (Navcam) taken at the edge of the entrance to the Dingo Gap shows a 3 foot (1 meter) tall dune and valley terrain beyond to the west, all dramatically back dropped by eroded rim of Gale Crater. View from the rover’s current position on Sol 528 (Jan. 30, 2014). The rover team may decide soon whether Curiosity will bridge the dune gap as a smoother path to next science destination. Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer- kenkremer.com
Curiosity’s View Past Tall Dune at edge of ‘Dingo Gap’
This photomosaic from Curiosity’s Navigation Camera (Navcam) taken at the edge of the entrance to the Dingo Gap shows a 3 foot (1 meter) tall dune and valley terrain beyond to the west, all dramatically back dropped by eroded rim of Gale Crater. View from the rover’s current position on Sol 528 (Jan. 30, 2014). The rover team may decide soon whether Curiosity will bridge the dune gap as a smoother path to next science destination. Credit: NASA/JPL-Caltech/Marco Di Lorenzo/Ken Kremer- kenkremer.com

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

Curiosity crossed through the 3 foot (1 meter) tall Dingo Gap sand dune with ease on Feb. 9 and roved on to targets in the “Moonlight Valley” and the region beyond.

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

“We’re seeing recessive bedrock.”

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

Since passing through the Dingo Gap gateway, Curiosity has traveled another 937 feet (285.5 meters) for a total mission odometry of 3.24 miles (5.21 kilometers) since the nail biting landing on Aug. 6, 2012.

“After we got over the dune, we began driving in terrain that looks like what we expected based on the orbital data. There are fewer sharp rocks, many of them are loose, and in most places there’s a little bit of sand cushioning the vehicle,” Erickson said.

Curiosity looks back to ‘Dingo Gap’ sand dune after crossing over, backdropped by Mount Sharp on Sol 540, Feb. 12, 2014.  Rear hazcam fisheye image linearized and colorized.  Credit: NASA/JPL/Marco Di Lorenzo/Ken Kremer- kenkremer.com
Curiosity looks back to ‘Dingo Gap’ sand dune after crossing over, backdropped by Mount Sharp on Sol 540, Feb. 12, 2014. Rear hazcam fisheye image linearized and colorized. Credit: NASA/JPL/Marco Di Lorenzo/Ken Kremer- kenkremer.com

Curiosity’s near term goal is to reach her next science waypoint, named Kimberly (formerly called KMS-9) which lies about two-thirds of a mile (about 1.1 kilometers) ahead.

Kimberly is of interest to the science team because it sits at an the intersection of different rock layers.

The 1 ton robot may be directed to drill into another rock at Kimberly.

If approved, Kimberly would be her first since drilling operation since boring into Cumberland rock target last spring and since departing the Yellowknife Bay region in July 2013 where she discovered a habitable zone.

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

To date Curiosity’s odometer stands at 5.2 kilometers and she has taken over 118,000 images. The robot has about another 5 km to go to reach the foothills of Mount Sharp.

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

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

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

Ken Kremer

Up close photomosaic view shows lengthy tear in rover Curiosity’s left front wheel caused by recent driving over sharp edged Martian rocks on the months long trek to Mount Sharp. Raw images taken by the MAHLI camera on Curiosity’s arm on Jan. 31, 2014 (Sol 529) were assembled to show some recent damage to several of its six wheels   Credit: NASA / JPL / MSSS / Marco Di Lorenzo / Ken Kremer- kenkremer.com  See below complete 6 wheel mosaic and further wheel mosaics for comparison
Up close photomosaic view shows lengthy tear in rover Curiosity’s left front wheel caused by recent driving over sharp edged Martian rocks on the months long trek to Mount Sharp. Raw images taken by the MAHLI camera on Curiosity’s arm on Jan. 31, 2014 (Sol 529) were assembled to show some recent damage to several of its six wheels Credit: NASA / JPL / MSSS / Marco Di Lorenzo / Ken Kremer- kenkremer.com

Private Cygnus Cargo Carrier departs Space Station Complex

The Cygnus private cargo craft built by Orbital Sciences Corp. was released from the station's robotic arm at 6:41am EST, Feb 18. It will burn up in Earth's atmosphere on Wednesday, Feb. 19, 2014. Credit: NASA TV

Following a picture perfect blastoff from NASA’s frigid Virginia spaceport and a flawless docking at the International Space Station (ISS) in mid-January, the privately built Cygnus cargo resupply vehicle has completed its five week long and initial operational station delivery mission and departed the facility early this morning, Tuesday, Feb. 18.

The Expedition 38 crewmembers Michael Hopkins of NASA and Koichi Wakata of the Japan Aerospace Exploration Agency (JAXA) demated the Orbital Sciences Cygnus commercial spacecraft from the Earth-facing port of the Harmony node using the Canadian built robotic arm at about 5:15 a.m. EST.

The cylindrically shaped ship was released from the grappling snare on the terminus of the 57 foot long extended arm at about 6:41 a.m. EST and with a slight shove as both vehicles were flying at 17500 mph and some 260 miles (415 km) altitude above Earth over the southern tip of Argentina and the South Atlantic Ocean.

The astronauts were working at a robotics work station in the windowed Cupola module facing the Earth. The arm was quickly pulled back about 5 feet (1.5 m) after triggering the release from the grappling pin.

NASA TV carried the operation live. Station and arm cameras provided spectacular video views of the distinctive grey cylindrical Cygnus back dropped by the massive, cloud covered blue Earth as it was released and sped away.

The Cygnus private cargo craft built by Orbital Sciences Corp. was released from the station's robotic arm at 6:41am EST, Feb 18. It will burn up in Earth's atmosphere on Wednesday, Feb. 19, 2014. Credit: NASA TV
The Cygnus private cargo craft built by Orbital Sciences Corp. was released from the station’s robotic arm at 6:41am EST, Feb 18. It will burn up in Earth’s atmosphere on Wednesday, Feb. 19, 2014. Credit: NASA TV

Cygnus was commanded to fire its jets for the departure maneuvers to quickly retreat away from the station. It was barely a speck only 5 minutes after the arm release maneuver by Wakata and Hopkins.

“The departure was nominal,” said Houston mission control. “Cygnus is on its way.”

The solar powered Cygnus is America’s newest commercial space freighter and was built by Orbital Sciences Corporation with seed money from NASA in a public-private partnership aimed at restoring the cargo up mass capabilities lost following the retirement of NASA’s space shuttles in 2011.

Cygnus, as well as the SpaceX Dragon cargo vessel, functions as an absolutely indispensable “lifeline” to keep the massive orbiting outpost alive and humming with the science for which it was designed.

The Cygnus private cargo craft built by Orbital Sciences Corp. was released from the station's robotic arm at 6:41am EST, Feb 18. It will burn up in Earth's atmosphere on Wednesday, Feb. 19, 2014. Credit: NASA TV
The Cygnus private cargo craft built by Orbital Sciences Corp. was released from the station’s robotic arm at 6:41am EST, Feb 18. It will burn up in Earth’s atmosphere on Wednesday, Feb. 19, 2014. Credit: NASA TV

The freighter delivered a treasure trove of 1.5 tons of vital research experiments, crew provisions, two dozen student science projects, belated Christmas presents, fresh fruit and more to the million pound orbiting lab complex and its six man crew.

The milestone flight dubbed Orbital 1, or Orb-1, began with the flawless Jan. 9 blast off of Cygnus mounted atop Orbital Sciences’ two stage, private Antares booster on the maiden operational launch from NASA’s Wallops Flight Facility along Virginia’s eastern shore. See a gallery of launch photos and videos – here and here.

“Today’s launch gives us the cargo capability to keep the station going,” said Frank Culbertson, executive vice president and general manager of Orbital’s advanced spaceflight programs group, and former Space Shuttle astronaut.

Antares soars to space on Jan. 9, 2014 from NASA Wallops on Virginia coast on the Orb-1 mission to the ISS.  Photo taken by remote camera at launch pad. Credit: Ken Kremer - kenkremer.com
Antares soars to space on Jan. 9, 2014 from NASA Wallops on Virginia coast on the Orb-1 mission to the ISS. Photo taken by remote camera at launch pad. Credit: Ken Kremer – kenkremer.com

And NASA’s commercial cargo initiative is even more important following the recent extension of station operations to at least 2024.

“I think it’s fantastic that the Administration has committed to extending the station,” Culbertson told me following the launch at NASA Wallops.

“So extending it gives not only commercial companies but also researchers the idea that Yes I can do long term research on the station because it will be there for another 10 years. And I can get some significant data.”

Following a two day orbital chase the Cygnus spacecraft reached the station on Jan. 12.

The ship is named in honor of NASA shuttle astronaut C. Gordon Fullerton who passed away in 2013.

Science experiments weighing 1000 pounds accounted for nearly 1/3 of the cargo load.

Among those were 23 student designed experiments representing over 8700 K-12 students involving life sciences topics ranging from amoeba reproduction to calcium in the bones to salamanders.

The students are participants of the Student SpaceFlight Experiments Program (SSEP) sponsored by the National Center for Earth and Space Science Education (NCESSE).

Over 20 of the students attended the launch at Wallops. The student experiments selected are from 6 middle school and high school teams from Washington, DC, Traverse, MI, Downingtown and Jamestown, PA, North Charleston, SC and Hays County, TX.

Student Space Flight teams at NASA Wallops Science experiments from these students representing six schools across  America were selected to fly aboard the Cygnus spacecraft which launched to the ISS from NASA Wallops, VA, on Jan . 9, 2014, as part of the Student Spaceflight Experiments Program (SSEP).  Credit: Ken Kremer - kenkremer.com
Student Space Flight teams at NASA Wallops
These are among the students benefiting from ISS extension
Science experiments from these students representing six schools across America were selected to fly aboard the Cygnus spacecraft which launched to the ISS from NASA Wallops, VA, on Jan . 9, 2014, as part of the Student Spaceflight Experiments Program (SSEP). Credit: Ken Kremer – kenkremer.com

“More than half the student experiments were activated within four days of arrival,” Dr. Jeff Goldstein, Director of the NCESSE, told Universe Today exclusively.

Ant colonies from three US states were also on board to study “swarm behavior.” The “ants in space” experiment was among the first to be unloaded from Cygnus to insure they are well fed for their expedition on how they fare and adapt in zero gravity.

33 cubesats were also aboard. Several of those were deployed last week from the Japanese Experiment Module airlock.

The Orbital-1 mission was the first of 8 operational cargo logistics flights scheduled under Orbital Sciences’ multi-year $1.9 Billion Commercial Resupply Services contract (CRS) with NASA to deliver 20,000 kg (44,000 pounds) of cargo through 2016.

Cygnus was berthed at the ISS for some 37 days.

After fully unpacking the 2,780 pounds (1,261 kilograms) of supplies packed inside Cygnus, the crew reloaded it with all manner of no longer need trash and have sent it off to a fiery and destructive atmospheric reentry to burn up high over the Pacific Ocean on Feb. 19.

“The cargo ship is now a trash ship,” said NASA astronaut Cady Coleman.

“Getting rid of the trash frees up a lot of valuable and much needed space on the station.”

When it reaches a sufficiently safe separation distance from the ISS, mission controllers will fire its engines two times to slow the Cygnus and begin the final deorbit sequence starting at about 8:12 a.m. on Wednesday.

This Cygnus launched atop Antares on Jan. 9 and docked on Jan. 12   Cygnus pressurized cargo module – side view – during exclusive visit by  Ken Kremer/Universe Today to observe prelaunch processing by Orbital Sciences at NASA Wallops, VA. ISS astronauts will open this hatch to unload 2780 pounds of cargo.  Docking mechanism hooks and latches to ISS at left. Credit: Ken Kremer – kenkremer.com
This Cygnus launched atop Antares on Jan. 9 and docked on Jan. 12
Cygnus pressurized cargo module – side view – during exclusive visit by Ken Kremer/Universe Today to observe prelaunch processing by Orbital Sciences at NASA Wallops, VA. ISS astronauts will open this hatch to unload 2780 pounds of cargo. Docking mechanism hooks and latches to ISS at left. Credit: Ken Kremer – kenkremer.com

Cygnus departure is required to make way for the next private American cargo freighter – the SpaceX Dragon, which is now slated to blast off from Cape Canaveral, Florida on March 16 atop the company’s upgraded Falcon 9 booster.

Two additional Antares/Cygnus flights are slated for this year.

They are scheduled to lift off around May 1 and early October, said Culbertson.

Indeed there will be a flurry of visiting vehicles to the ISS throughout this year and beyond – creating a space traffic jam of sorts.

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

Ken Kremer

ISS Astronauts grapple Orbital Sciences Cygnus spacecraft with robotic arm and guide it to docking port. Credit: NASA TV
ISS Astronauts grapple Orbital Sciences Cygnus spacecraft with robotic arm and guide it to docking port. Credit: NASA TV

100 Days of MOM – India’s 1st Mars Mission Streaking to Red Planet Rendezvous

India’s Mars Orbiter Mission (MOM) completes 100 days in space on February 12, 2014 on its journey to reach the Red Planet on Sept 24, 2014. Credit ISRO

India’s maiden Mars explorer, the Mars Orbiter Mission or MOM, celebrated 100 days speeding through space this past week, racing outwards on its historic journey to the Red Planet.

After streaking through space for some ten and a half months, the 1,350 kilogram (2,980 pound) MOM probe will rendezvous with the Red Planet on September 24, 2014 – where she will study the atmosphere and sniff for signals of methane.

Feb. 12, 2014 marked ‘100 Days of MOM’ since the picture perfect blast off on Nov. 5, 2013 from India’s spaceport at the Satish Dhawan Space Centre, Sriharikota, atop the nations indigenous Polar Satellite Launch Vehicle (PSLV) which placed the probe into its initial Earth parking orbit.

First ever image of Earth Taken by Mars Color Camera aboard India’s Mars Orbiter Mission (MOM) spacecraft while orbiting Earth and before the Trans Mars Insertion firing on Dec. 1, 2013. Image is focused on the Indian subcontinent.  Credit: ISRO
First ever image of Earth Taken by Mars Color Camera aboard India’s Mars Orbiter Mission (MOM) spacecraft while orbiting Earth and before the Trans Mars Insertion firing on Dec. 1, 2013. Image is focused on the Indian subcontinent. Credit: ISRO

A series of six subsequent orbit raising maneuvers ultimately culminated with the liquid fueled main engine firing on Dec. 1, 2013 for the Trans Mars Injection(TMI) maneuver that successfully placed MOM on a heliocentric elliptical trajectory to the Red Planet.

The TMI, affectionately dubbed ‘The mother of all slingshots’ finally provided the craft with sufficient thrust to achieve escape velocity and blast free of the Earth’s sphere of influence forever and begin her nearly yearlong momentous voyage to Mars.

The first of four in flight Trajectory Correction Maneuvers, TCM-1, was conducted by firing the 22 Newton Thrusters for a duration of 40.5 seconds on December 11, 2013. A trio of additional TCM firings are planned around April 2014, August 2014 and September 2014.

Trans Mars Injection (TMI), carried out on Dec 01, 2013 at 00:49 hrs (IST) has moved the spacecraft in the Mars Transfer Trajectory (MTT). With TMI the Earth orbiting phase of the spacecraft ended and the spacecraft is now on a course to encounter Mars after a journey of about 10 months around the Sun. Credit: ISRO
Trans Mars Injection (TMI), carried out on Dec 01, 2013 at 00:49 hrs (IST) has moved the spacecraft in the Mars Transfer Trajectory (MTT). With TMI the Earth orbiting phase of the spacecraft ended and the spacecraft is now on a course to encounter Mars after a journey of about 10 months around the Sun. Credit: ISRO

MOM was designed and developed by the Indian Space Research Organization’s (ISRO) at a cost of $69 Million and marks India’s inaugural foray into interplanetary flight.

During the first 100 days, the probe has traveled about 190 million kilometers and has a little less than 500 million kilometers and 205 days to go during her journey of some 680 million kilometers (400 million miles) overall.

A health check on February 6, 2014 confirmed that the 15 kg (33 lb) science payload comprising five Indian built instruments was turned “ON” and is operating well.

MOM is currently some 16 million km distant from Earth and one way radio signals take approximately 55 seconds.

“The round trip time is almost 2 minutes for a communication signal to go to MOM and come back, about the same time mom takes to make noodles!” ISRO noted humorously in a Facebook mission posting.

“Keep going MOM!”

MOM's first Trajectory Correction Manoeuver in Baiju Raj's imagination.
MOM’s first Trajectory Correction Manoeuver in Baiju Raj’s imagination.

Following the ten month cruise through space the orbital insertion engine will fire for the do or die burn on September 24, 2014 placing MOM into an 377 km x 80,000 km elliptical orbit around Mars.

MOM is not alone in the frigid vacuum of space. She is joined by NASA’s MAVEN orbiter in pursuit of Mars.

MOM will reach Mars vicinity just two days after the arrival MAVEN on Sept. 22, 2014.

To date MAVEN has flown over 137 million miles (221 million km) of its total 442 million miles (712 million km) path to Mars.

If all continues to goes well, India will join an elite club of only four who have launched probes that successfully investigated the Red Planet from orbit or the surface – following the Soviet Union, the United States and the European Space Agency (ESA).

Both MAVEN and MOM’s goal is to study the Martian atmosphere, unlock the mysteries of its current atmosphere and determine how, why and when the atmosphere and liquid water was lost – and how this transformed Mars climate into its cold, desiccated state of today.

Together, MOM and MAVEN will fortify Earth’s invasion fleet at Mars. They join 3 current orbiters from NASA and ESA as well as NASA’s pair of sister surface roversCuriosity and Opportunity.

Although they were developed independently and have different suites of scientific instruments, the MAVEN and MOM science teams will “work together” to unlock the secrets of Mars atmosphere and climate history, MAVEN’s top scientist told Universe Today.

“We have had some discussions with their science team, and there are some overlapping objectives,” Bruce Jakosky told me. Jakosky is MAVEN’s principal Investigator from the University of Colorado at Boulder.

“At the point where we [MAVEN and MOM] are both in orbit collecting data we do plan to collaborate and work together with the data jointly,” Jakosky said.

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

Ken Kremer

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Mystery of the Martian ‘Jelly Doughnut’ Rock – Solved

This image from the panoramic camera (Pancam) on NASA’s rover Opportunity shows the location of a rock called "Pinnacle Island" before it appeared in front of the rover in early January 2014. Arrow at lower left. This image was taken during Sol 3567 of Opportunity's work on Mars (Feb. 4, 2014). Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.

The mystery of the world famous “Jelly Doughnut” rock on Mars has at last been solved by diligent mission scientists toiling away in dank research labs on Earth.

The “Jelly Doughnut” rock achieved worldwide fame, or better yet infamy, when it suddenly appeared out of nowhere in pictures taken by NASA’s renowned Red Planet rover Opportunity in January.

And the answer is – well it’s not heretofore undetected Martian beings or even rocks falling from the sky.

Rather its ‘Alien Space Invaders’ – in some sense at least.

And that ‘Alien Space Invader’ is from – Earth! And her name is – Opportunity!

Indeed sister rover Curiosity may have unwittingly pointed to the culprit and helped resolve the riddle when she snapped a brand new photo of Earth – home planet to Opportunity and Curiosity and all their makers! See the evidence for yourselves – lurking here!

It turns out that the six wheeled Opportunity unknowingly ‘created’ the mystery herself when she drove over a larger rock, crushing it with the force from the wheels and her 400 pound (185 kg) mass.

Fragments were sent hurtling across the summit of the north facing Solander Point mountain top, where she is currently climbing up ‘Murray Ridge’ along the western rim of a vast crater named Endeavour that spans some 22 kilometers (14 miles) in diameter. See traverse map below.

One piece unwittingly rolled downhill.

That rock fragment – now dubbed ‘Pinnacle Island’ – suddenly appeared in pictures taken by Opportunity’s cameras on Jan, 8, 2014 (Sol 3540).

Mosaic of Opportunity and mysterious Pinnacle Island rock by Solander Point peak.  Mysterious Pinnacle Island rock suddenly appeared out of nowhere in images snapped on Sol 3540.  It was absent in earlier images on Sol 3528.  This mosaic shows the rock nearby the solar panels of NASA’s Opportunity rover.  Assembled from Sol 3528 and 3540 pancam raw images.  Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com
Mosaic of Opportunity and mysterious Pinnacle Island rock by Solander Point peak. Mysterious Pinnacle Island rock suddenly appeared out of nowhere in images snapped on Sol 3540. It was absent in earlier images on Sol 3528. This mosaic shows the rock nearby the solar panels of NASA’s Opportunity rover. Assembled from Sol 3528 and 3540 pancam raw images. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com

And that exact same spot had been vacant of debris in photos taken barely 4 days earlier – during which time the rover didn’t move a single millimeter.

Pinnacle Island measures only about 1.5 inches wide (4 centimeters) with a noticeable white rim and red center – hence its jelly doughnut nickname.

The Martian riddle was finally resolved when Opportunity roved a tiny stretch and took some look back photographs to document the ‘mysterious scene’ for further scrutiny.

“Once we moved Opportunity a short distance, after inspecting Pinnacle Island, we could see directly uphill an overturned rock that has the same unusual appearance,” said Opportunity Deputy Principal Investigator Ray Arvidson of Washington University in St. Louis, in a NASA statement.

“We drove over it. We can see the track. That’s where Pinnacle Island came from.”

New pictures showed another fragment of the rock – dubbed ‘Stuart Island’ – eerily similar in appearance to the ‘Pinnacle Island’ doughnut.

Opportunity by Solander Point peak – 2nd Mars Decade Starts here!  NASA’s Opportunity rover captured this panoramic mosaic on Dec. 10, 2013 (Sol 3512) near the summit of “Solander Point” on the western rim of Endeavour Crater where she starts Decade 2 on the Red Planet. She is currently investigating outcrops of potential clay minerals formed in liquid water on her 1st mountain climbing adventure. Assembled from Sol 3512 navcam raw images. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com
Opportunity by Solander Point peak – 2nd Mars Decade Starts here! NASA’s Opportunity rover captured this panoramic mosaic on Dec. 10, 2013 (Sol 3512) near the summit of “Solander Point” on the western rim of Endeavour Crater where she starts Decade 2 on the Red Planet. She is currently investigating outcrops of potential clay minerals formed in liquid water on her 1st mountain climbing adventure. Assembled from Sol 3512 navcam raw images. Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Ken Kremer-kenkremer.com

To gather some up-close clues before driving away, the rover deployed its robotic arm to investigate ‘Pinnacle Island’ with her microscopic imager and APXS mineral mapping spectrometer.

The results revealed high levels of the elements manganese and sulfur “suggesting these water-soluble ingredients were concentrated in the rock by the action of water,” says NASA.

“This may have happened just beneath the surface relatively recently,” Arvidson noted, “or it may have happened deeper below ground longer ago and then, by serendipity, erosion stripped away material above it and made it accessible to our wheels.”

This before-and-after pair of images of the same patch of ground in front of NASA's Mars Exploration Rover Opportunity 13 days apart documents the arrival of a bright rock onto the scene.  Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.
This before-and-after pair of images of the same patch of ground in front of NASA’s Mars Exploration Rover Opportunity 13 days apart documents the arrival of a bright rock onto the scene. Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.

The Solander Point mountaintop is riven with outcrops of minerals, including clay minerals, that likely formed in flowing liquid neutral water conducive to life – potentially a scientific goldmine.

Opportunity
is NASA’s 1st ever ‘Decade Old’ living Mars rover.

She has been uncovering and solving Mars’ billion years old secrets for over 10 years now since landing back on January 24, 2004 on Meridiani Planum – although she was only expected to function a mere 90 days!

Today, Feb 15, marks Opportunity’s 3578th Sol or Martian Day roving Mars.

So far she has snapped over 188,700 amazing images on the first overland expedition across the Red Planet.

Her total odometry stands at over 24.07 miles (38.73 kilometers) since touchdown on Jan. 24, 2004 at Meridiani Planum.

Read more about sister Spirit – here and here.

Meanwhile on the opposite side of Mars, Opportunity’s younger sister rover Curiosity is trekking towards gigantic Mount Sharp and just crested over the Dingo Gap sand dune. She celebrated 500 Sols on Mars on New Years Day 2014.

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

Finally, China’s Yutu rover has awoken for her 3rd workday on the Moon.

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

Ken Kremer

Traverse Map for NASA’s Opportunity rover from 2004 to 2014  This map shows the entire path the rover has driven during a decade on Mars and over 3560 Sols, or Martian days, since landing inside Eagle Crater on Jan 24, 2004 to current location by Solander Point summit at the western rim of Endeavour Crater. Rover will spend 6th winter here atop Solander. Opportunity discovered clay minerals at Esperance – indicative of a habitable zone. Credit: NASA/JPL/Cornell/ASU/Marco Di Lorenzo/Ken Kremer – kenkremer.com
Traverse Map for NASA’s Opportunity rover from 2004 to 2014
This map shows the entire path the rover has driven during a decade on Mars and over 3560 Sols, or Martian days, since landing inside Eagle Crater on Jan 24, 2004 to current location by Solander Point summit at the western rim of Endeavour Crater. Rover will spend 6th winter here atop Solander. Opportunity discovered clay minerals at Esperance – indicative of a habitable zone. Credit: NASA/JPL/Cornell/ASU/Marco Di Lorenzo/Ken Kremer – kenkremer.com

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

This composite view shows China’s Yutu rover heading south and away forever from the Chang’e-3 landing site about a week after the Dec. 14, 2013 touchdown at Mare Imbrium. This cropped view was taken from the 360-degree panorama. See complete 360 degree landing site panorama herein. Chang’e-3 landers extreme ultraviolet (EUV) camera is at right, antenna at left. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com. See our complete Yutu timelapse pano at NASA APOD Feb. 3, 2014: http://apod.nasa.gov/apod/ap140203.htm

Yutu Lives!

The little ‘rabbit’ beloved worldwide has now phoned home and actually survived the perils of the long lunar night and is alive and awake to start a 3rd day of scientific exploration despite suffering a serious malfunction as it entered the latest hibernation period two weeks ago.

“Yutu has come back to life!” said Pei Zhaoyu, the spokesperson for China’s lunar probe program, according to a breaking news report by the state owned Xinhua news agency.

“Experts are still working to verify the causes of its mechanical control abnormality.”

The Chang’e-3 mothership lander and piggybacked Yutu surface rover soft landed on the Moon on Dec. 14, 2013 at Mare Imbrium (Sea of Rains) – marking China’s first successful spacecraft landings on an extraterrestrial body in history.

Yutu’s new lease on life also comes after Monday’s (Feb. 11) premature report of the robots demise by the state owned China News Service, reported here.

However, “Yutu failed to power-up Monday [Feb 11] and data about its current condition and repair progress is still being collected and analyzed,” Xinhua and CCTV (China state run television) reported.

This indicates that Yutu was in fact feared lost for some time by the mission team, until further efforts finally resulted in the detection of a signal from the spacecraft – and a welcome reversal of yesterdays news!

The robot “has now been restored to its normal signal reception function,” says Pei.

Side by side screenshot photos of the Chang'e-3 moon lander (L) and the Yutu moon rover during the mutual-photograph process, at the Beijing Aerospace Control Center in Beijing, on Dec. 15, 2013. The moon rover and the moon lander took photos of each other  marking the complete success of the Chang'e-3 lunar probe mission. (Xinhua/Ding Lin)
Side by side screenshot photos of the Chang’e-3 moon lander (L) and the Yutu moon rover during the mutual-photograph process, at the Beijing Aerospace Control Center in Beijing, on Dec. 15, 2013. The moon rover and the moon lander took photos of each other marking the complete success of the Chang’e-3 lunar probe mission. (Xinhua/Ding Lin)

Earlier today (Feb. 12) amateur radio operators at UHF-satcom reported detection of a signal from Yutu.

But much technical work remains ahead for the engineering and science teams to ascertain why it malfunctioned and whether the six wheeled rover can be restored to partial or full functionality.

As night fell on Jan. 25, the rover entered its second two week long period of dormancy just as the rover “experienced a mechanical control abnormality,” according to a report by China’s official government newspaper, The People’s Daily.

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

“Experts were initially concerned that it might not be able to survive the extremely low temperatures during the lunar night.”

360-degree time-lapse color panorama from China’s Chang’e-3 lander This 360-degree time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at three different positions during its trek over the Moon’s surface at its landing site from Dec. 15-22, 2013 during the 1st Lunar Day. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com.  See our Yutu timelapse pano at NASA APOD Feb. 3, 2014: http://apod.nasa.gov/apod/ap140203.htm
360-degree time-lapse color panorama from China’s Chang’e-3 lander
This 360-degree time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at three different positions during its trek over the Moon’s surface at its landing site from Dec. 15-22, 2013 during the 1st Lunar Day. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com. See our Yutu timelapse pano at NASA APOD Feb. 3, 2014: http://apod.nasa.gov/apod/ap140203.htm

Each lunar day and night lasts for alternating periods of 14 Earth days.

During each long night, the Moon’s temperatures plunge dramatically to below minus 180 Celsius, or minus 292 degrees Fahrenheit.

Both solar powered probes must enter hibernation mode during each lunar night to conserve energy and protect their science instruments and control mechanisms, computers and electronics.

“The rover stands a chance of being saved now that it is still alive,” Pei stated.

Yutu, which translates as ‘Jade Rabbit’ is named after the rabbit in Chinese mythology that lives on the Moon as a pet of the Moon goddess Chang’e.

‘Jade Rabbit’ had departed the landing site forever, and was journeying southwards as the anomoly occurred – about six weeks into its planned 3 month long moon roving expedition to investigate the moon’s surface composition and natural resources.

The 140 kg Yutu robot is located some 100 m south of the lander.

Traverse Path of Yutu rover from Dec. 14 landing to Dec. 21. Landscape textured with Chang'e 3 imagery from space and ground.  Credit: CNSA/BACC
Traverse Path of Yutu rover from Dec. 14 landing to Dec. 21. Landscape textured with Chang’e 3 imagery from space and ground. Credit: CNSA/BACC

Definitive word about the Chang’e-3 lander has not yet been announced. But it is expected to survive since no malfunctions have been reported. It has a 1 year design lifetime.

Xinhua stated that Chinese space officials will comment on the landers status soon.

The 1200 kg stationary lander is expected to return science data about the Moon and conduct telescopic observations of the Earth and celestial objects for at least one year.

Chang’e-3 and Yutu landed on a thick deposit of volcanic material.

The inaugural pair of probes could be the forerunners to a manned Chinese Moon landing mission a decade from now.

China’s current plans call for the Chang’e-4 Moon lander/rover to launch in 2016, perhaps with some upgrades and lessons learned from the ongoing mission.

China is only the 3rd country in the world to successfully soft land a spacecraft on Earth’s nearest neighbor after the United States and the Soviet Union.

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

Ken Kremer

Time for Earth to bid China’s Yutu Moon Rover Farewell ?

Farewell Yutu - artistic impression of Earthrise over Yutu at lunar landing site. This composite photomosaic combines farewell view of China’s Yutu rover with Moon’s surface terrain at Mare Imbrium landing site and enlarged photo of Earth, all taken by Chang’e-3 lander. Not a science image. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com

Farewell Yutu – artistic impression of Earthrise over Yutu at lunar landing site. This composite timelapse photomosaic combines farewell view of China’s Yutu rover with Moon’s surface terrain at Mare Imbrium landing site and enlarged photo of Earth – all actual images taken by Chang’e-3 lander. Not a science image. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com
See complete Yutu timelapse panorama below and at NASA APOD Feb. 3, 2014:http://apod.nasa.gov/apod/ap140203.html
Story and Headline revised and updated[/caption]

Update: There might yet be hope for Yutu. Amateur radio operators at UHF-satcom reported detection of a signal from Yutu today. But no update has been reported on the China News Service website or other official state media. Yutu’s fate is unknown.]

Update 2: Yutu is alive. story and headline revised. Further details – here
………..

For a time, it seemed China’s maiden moon rover ‘Yutu’, beloved by millions worldwide, had been lost.

The apparently unfortunate and sad breaking news was just reported today in an ultra brief dispatch by the English language version of Chinadaily – with the headline “Loss of lunar rover.”

But the death notice by Chinese officials turned out to be premature when a signal was detected a day later.

It had been thought that Yutu froze to death due to a pre-hibernation mechanical malfunction and failed to wake up and communicate with China’s mission controllers in Beijing on Monday, Feb. 10, when daylight returned to the rovers Moon landing site at Mare Imbrium (Sea of Rains) at the start of what would have been Lunar Day 3 for the mission.

“China’s first lunar rover, Yutu, could not be restored to full function on Monday [Feb. 10] as expected,” wrote the state owned Chinadaily.com, China News Service agency.

The cause of the pre-hibernation malfunction may perhaps be traced back to a buildup of abrasive lunar dust, but no one knows at this time.

Note: This story has been updated as further details emerged.

Portrait photo of Yutu moon rover taken by camera on the Chang'e-3 moon lander on Dec. 15, 2013 shortly after rolling all 6 wheels onto lunar surface.  Credit: Chinese Academy of Sciences
Portrait photo of Yutu moon rover taken by camera on the Chang’e-3 moon lander on Dec. 15, 2013 shortly after rolling all 6 wheels onto lunar surface. Credit: Chinese Academy of Sciences

Yutu has touched the hearts of countless Earthlings since the history making landing on the desolate gray plains of the the Moon atop the Chang’e-3 lander two month ago on Dec. 14, 2013.

See our timelapse mosaic, artistic impression of Earthrise over Yutu – above – by the image processing team of Ken Kremer and Marco Di Lorenzo.

It combines real images of the Moon’s surface terrain with an intentionally enlarged photo of Earth – all snapped by the Chang’e-3 lander – as a homage to the mission.

See the complete timelapse mosaic herein and featured at NASA APOD on Feb 3, 2013.

Although definitive word about the Chang’e-3 lander has not yet been announced, it is expected to survive and has a 1 year design lifetime.

Potentially bad news about Yutu’s fate was not unexpected however, after Chinese space officials disclosed that the rover “experienced a mechanical control abnormality” two weeks ago, just as her 2nd lunar night was to begin, according to a report by China’s official government newspaper, The People’s Daily.

“Yutu experienced mechanical problems on Jan 25 and has been unable to function since then,” according to Chinadaily.com, China News service.

360-degree time-lapse color panorama from China’s Chang’e-3 lander This 360-degree time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at three different positions during its trek over the Moon’s surface at its landing site from Dec. 15-22, 2013 during the 1st Lunar Day. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com
360-degree time-lapse color panorama from China’s Chang’e-3 lander
This 360-degree time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at three different positions during its trek over the Moon’s surface at its landing site from Dec. 15-22, 2013 during the 1st Lunar Day.
Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo – kenkremer.com
See our Yutu timelapse pano also at NASA APOD Feb. 3, 2014:
http://apod.nasa.gov/apod/ap140203.html

Each lunar day and night lasts for alternating periods of 14 Earth days.

The six wheeled Yutu rover and Chang’e-3 mothership lander had just finished sleeping through the terribly frigid two week long lunar night since they entered their second hibernation period on Jan. 24th and 25th respectively, and Chinese space engineers had hoped to reawaken both probes in the past few days.

No communications are possible during the period of nighttime dormancy.

This time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at two different positions during its trek over the Moon’s surface at its landing site from Dec. 15-18, 2013. This view was taken from the 360-degree panorama. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo.   See our complete Yutu timelapse pano at NASA APOD Feb. 3, 2014:  http://apod.nasa.gov/apod/ap140203.htm
This time-lapse color panorama from China’s Chang’e-3 lander shows the Yutu rover at two different positions during its trek over the Moon’s surface at its landing site from Dec. 15-18, 2013. This view was taken from the 360-degree panorama, herein. Credit: CNSA/Chinanews/Ken Kremer/Marco Di Lorenzo. See our complete Yutu timelapse pano also at NASA APOD Feb. 3, 2014: http://apod.nasa.gov/apod/ap140203.htm

Yutu, which translates as ‘Jade Rabbit’ is named after the rabbit in Chinese mythology that lives on the Moon as a pet of the Moon goddess Chang’e.

The piggybacked pair of Chinese probes safely touched down on the Moon at Mare Imbrium near the Bay of Rainbows on Dec. 14, 2013.

Photo of Chang'e-3 moon lander emblazoned with Chinese national flag taken by the panoramic camera on the Yutu moon rover on Dec. 22, 2013. Credit: CNSA
Photo of Chang’e-3 moon lander emblazoned with Chinese national flag taken by the panoramic camera on the Yutu moon rover on Dec. 22, 2013. Credit: CNSA

Apparently one of Yutu’s solar panels did not fold back properly over the instrument laden mast after it was lowered to a horizontal position into a warmed electronics box where it is shielded and insulated from the extremely frigid lunar night time temperatures.

Dust accumulation on the rover and gears may possibly be to blame for the failure to retract, based on unofficial accounts.

China has not released any official or detailed information on the cause of the malfunction or recovery actions taken by Chinese space engineers.

Such a malfunction could spell doom for the fragile electronic and computer components in the unprotected mast mounted instruments and systems, including the color and navigation cameras and the high gain antenna.

During each 14 Earth-day long night, the Moon’s temperatures plunge dramatically to below minus 180 Celsius, or minus 292 degrees Fahrenheit.

‘Jade Rabbit’ had departed the landing site forever, and was journeying southwards as the incident occurred – about six weeks into its planned 3 month long moon roving expedition to investigate the moon’s surface composition and natural resources.

The 140 kg Yutu robot drove off a pair of ramps and onto the moon seven hours after the Dec. 14, 2013 touchdown.

The 1200 kg stationary lander is expected to return science data about the Moon and telescopic observations of the Earth and celestial objects for at least one year.

Chang’e-3 and Yutu landed on a thick deposit of volcanic material.

Chang’e-3 lander and Yutu rover – from Above And Below  Composite view shows China’s Chang’e-3 lander and Yutu rover from Above And Below (orbit and surface) – lander color panorama (top) and orbital view from NASA’s LRO orbiter (bottom). Chang’e-3 lander color panorama shows Yutu rover after it drove down the ramp to the moon’s surface and began driving around the landers right side to the south. Yellow lines connect craters seen in the lander panorama and the LROC image from LRO (taken at a later date after the rover had moved), red lines indicate approximate field of view of the lander panorama. Credit: CNSA/NASA/Ken Kremer/Marco Di Lorenzo/Mark Robinson
Chang’e-3 lander and Yutu rover – from Above And Below
Composite view shows China’s Chang’e-3 lander and Yutu rover from Above And Below (orbit and surface) – lander color panorama (top) and orbital view from NASA’s LRO orbiter (bottom). Chang’e-3 lander color panorama shows Yutu rover after it drove down the ramp to the moon’s surface and began driving around the landers right side to the south. Yellow lines connect craters seen in the lander panorama and the LROC image from LRO (taken at a later date after the rover had moved), red lines indicate approximate field of view of the lander panorama. Credit: CNSA/NASA/Ken Kremer/Marco Di Lorenzo/Mark Robinson

They were designed to conduct their science investigations and work independently of one another.

China can be proud of its magnificent space flight accomplishment.

Chang’e-3 was the first spacecraft from Earth to soft land on the Moon in nearly four decades since the touchdown of the Soviet Union’s Luna 24 sample return spacecraft back in 1976.

America’s last visit to the Moon’s surface occurred with the manned Apollo 17 landing mission – crewed by astronauts Gene Cernan and Harrison ‘Jack’ Schmitt , who coincidentally ascended from the lunar soil on Dec. 14, 1972 – exactly 41 years before Chang’e-3.

China’s follow on Chang’e-4 Moon lander is due to blastoff in 2015.

Surely the science and engineering team will incorporate valuable lessons learned.

China is only the 3rd country in the world to successfully soft land a spacecraft on Earth’s nearest neighbor after the United States and the Soviet Union.

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

Ken Kremer

Landing site of Chinese lunar probe Chang'e-3 on Dec. 14, 2013.
Landing site of Chinese lunar probe Chang’e-3 on Dec. 14, 2013.

Science Instruments Perfect as NASA’s MAVEN Orbiter Speeds to Red Planet

MAVEN is NASA’s next Mars Orbiter and will investigate how the planet lost most of its atmosphere and water over time. Credit: NASA

NASA’s newest Mars orbiter, the Mars Atmosphere and Volatile Evolution (MAVEN) probe passed a significant interplanetary milestone with the announcement that all of the craft’s science instruments were activated and passed their initial checkout.

“I’m delighted that we’re operating in space so well,” Bruce Jakosky, MAVEN’s Principal Investigator told Universe Today.

“We’re on our way!”

Earth is now clearly in the rear view mirror and fading with each passing day.

The $671 Million MAVEN spacecraft’s goal is to study Mars upper atmosphere to explore how the Red Planet may have lost its atmosphere and water over billions of years.

The MAVEN probe carries nine sensors in three instrument suites to study why and exactly when did Mars undergo the radical climatic transformation.

“I’m really looking forward to getting to Mars and starting our science!” Jakosky told me.

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MAVEN aims to discover the history of water and habitability stretching back over billions of years on Mars.

It will measure current rates of atmospheric loss to determine how and when Mars lost its atmosphere and water.

MAVEN thundered to space nearly three months ago on Nov. 18, 2013 following a flawless blastoff from Cape Canaveral Air Force Station’s Space Launch Complex 41 atop a powerful Atlas V rocket and thus began a 10 month interplanetary voyage from Earth to the Red Planet.

NASA’s Mars bound MAVEN spacecraft launches atop Atlas V booster at 1:28 p.m. EST from Space Launch Complex 41 at Cape Canaveral Air Force Station on Nov. 18, 2013. Image taken from the roof of the Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center.  Credit: Ken Kremer/kenkremer.com
NASA’s Mars bound MAVEN spacecraft launches atop Atlas V booster at 1:28 p.m. EST from Space Launch Complex 41 at Cape Canaveral Air Force Station on Nov. 18, 2013. Image taken from the roof of the Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center. Credit: Ken Kremer/kenkremer.com

“I can’t tell you how exciting this is to be now only seven and a half months from getting to Mars,” Jakosky gushed.

Further instrument checkouts are planned as the orbiter streaks closer to Mars including tesating to the Electra communications package that will serve as a critical relay for NASA’s surface rovers including Curiosity, Opportunity and the planned 2020 rover.

“The second Trajectory Correction Maneuver (TCM-2) is scheduled for Feb. 26,” said Jakosky.

MAVEN’s trajectory from Earth to Mars. MAVEN arrives at Mars on Sept. 22, 2014 some ten months after launch on Nov. 18, 2013.  Credit: NASA
MAVEN’s trajectory from Earth to Mars. MAVEN arrives at Mars on Sept. 22, 2014 some ten months after launch on Nov. 18, 2013. Credit: NASA

TCM thruster firings insure that the spacecraft is exactly on course for the do or die orbital insertion maneuver when MAVEN arrives on September 22, 2014.

To date MAVEN has flown over 137 million miles (221 million km) of its total 442 million miles (712 million km) path to Mars. It is speeding around the sun at 69,480 mph or 31.06 kps.

“The performance of the spacecraft and instruments to date bears out all the hard work the team put into testing the system while it was on the ground,” said David Mitchell, MAVEN project manager at NASA’s Goddard Space Flight Center in Greenbelt, Md, in a statement.

“The way that the operations team has performed while flying the system has been nothing short of outstanding. We have big events ahead of us before we can claim success but I am very pleased with how things have gone thus far.”

MAVEN is not alone in the frigid vacuum of space. She is joined by India’s Mars Orbiter Mission (MOM) orbiter in pursuit of Mars to fortify Earth’s invasion fleet.

MOM will reach Mars vicinity on Sept. 24, just two days after the arrival MAVEN on Sept. 22, 2014.

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

Ken Kremer

NASA’s MAVEN Mars orbiter, chief scientist Prof. Bruce Jakosky of CU-Boulder and Ken Kremer of Universe Today inside the clean room at the Kennedy Space Center on Sept. 27, 2013. MAVEN launches to Mars on Nov. 18, 2013 from Florida. Credit: Ken Kremer/kenkremer.com
NASA’s MAVEN Mars orbiter, chief scientist Prof. Bruce Jakosky of CU-Boulder and Ken Kremer of Universe Today inside the clean room at the Kennedy Space Center on Sept. 27, 2013. MAVEN launched to Mars on Nov. 18, 2013 from Florida. Credit: Ken Kremer/kenkremer.com

A Mesmerizing Look at Year 4 of the Solar Dynamics Observatory

Coronal Mass Ejection as viewed by the Solar Dynamics Observatory on June 7, 2011. A similar type of outburst triggered aurorae during a strong geomagnetic storm in February 1872. Image Credit: NASA/SDO
Coronal Mass Ejection as viewed by the Solar Dynamics Observatory on June 7, 2011. A similar type of outburst triggered aurorae during a strong geomagnetic storm in February 1872. Image Credit: NASA/SDO

Four years ago today, the Solar Dynamics Observatory embarked on a five-year mission to boldly go where no Sun-observing satellite has gone before. SDO uses its three instruments to look constantly at the Sun in ten different wavelengths. Called the “Crown Jewel” of NASA’s fleet of solar observatories, SDO is a technologically advanced spacecraft that takes images of the sun every 0.75 seconds. Each day it sends back about 1.5 terabytes of data to Earth — the equivalent of about 380 full-length movies.

SDO launched on Feb. 11, 2010, and it has since captured the amazing views of the ever-changing face of the Sun — the graceful dance of solar material coursing through the Sun’s the corona, massive solar explosions and giant sunspot shows. Enjoy this latest highlight video from year 4 from SDO!

I was priveldged to be able to attend the launch of SDO, and you can read our article about the launch here.

The launch included a little “special effects” that wowed the crowd. The Atlas rocket soared close to a sundog just as the spacecraft reached Max-Q, and a ripple effect was created around the spacecraft. You can watch the launch below to see what happened:

Enter the Red Planet: A Guide to the Upcoming Mars 2014 Opposition Season

Astrophotographers are already getting some great images of Mars, such as this sequence captured by Efrain Morales Rivera on January 9th, 2014.

Get those telescopes ready: the coming months offer Earthbound viewers some great views of the planet Mars.

Mars reaches opposition for 2014 on April 8th. This is approaching season represents the best time to observe Mars, as the Red Planet is closest to us in April and rises in the east as the Sun sets opposite to it in the west.  Mars reaches 10” in apparent size this week. Mars is already beginning to show surface detail through a moderate-sized telescope as it continues to grow. In mid-February, Mars currently rises at around midnight local, and rides high to the south at local sunrise.

Mars imaged by Leo Aerts on February 3rd. Shot using a Celestron 14" scope, DMK 21AU618 webcam with a 2.5 powermate projection and a RGB Baader filter set.
Mars imaged by Leo Aerts on February 3rd. Shot using a Celestron 14″ scope, DMK 21AU618 webcam with a 2.5 powermate projection and a RGB Baader filter set.

The 2014 opposition of Mars offers a mixed bag for observers. Hanging around 5-10 degrees south of the celestial equator just east of the September equinoctial point in Virgo, viewing opportunities are roughly equal for both northern and southern hemisphere observers. At opposition, Mars will shine at magnitude -1.5 and present a 15.2” disk, only slightly larger than the near minimum apparition of 2012, when it appeared 13.9” across. This is a far cry from the historic 2003 appearance, when Mars nearly maxed out at 25.1” across.

Why such a difference? Because the planet Mars has an exceptionally eccentric orbit. In fact, the eccentricity for Mars is 9.3% compared to 1.7% for the relatively sedate Earth.

A decade of Mars oppositions.
A decade plus of Mars oppositions, from 2012 through 2025. Graphic created by the author.

This guarantees that all oppositions of Mars – which occur roughly 26 months/780 days apart – are not created equal. In our current epoch, Mars can pass anywhere from 0.683 to 0.373 Astronomical Units (A.U.s) from the Earth. This year’s passage sees Mars overtake us at 0.62 A.U.s or over 96 million kilometres from Earth on the night of opposition. Mars is slightly closer to us at 0.618 A.U.s six nights later on April 14th.

Why the slight difference? Well, the speedier Earth is on the inside track headed towards aphelion in July, while Mars is lagging but headed slightly inward towards perihelion just afterwards in September. This combined motion makes for a slightly closer approach just after opposition until the Earth begins to pull away.

And this also means that Mars will make its apparent retrograde loop through Virgo on the months surrounding opposition:

Mars retrograde credit-Starry Night
The motion of Mars through Virgo from March 1st through July 31st. Created by the author using Starry Night Education software.

Now for the good news. Oppositions of Mars also follow a rough 15-year cycle, meaning that they get successively closer or more distant with every two year passage. For example, the 1999 opposition of Mars had a very similar geometry to this year’s, as will to the future opposition in 2029.

And we’re currently on an improving trend: the next opposition in 2016 is much better than this year’s at 18.6” in size, and during the 2018 opposition, Mars will present a disc 24.3” across and will be nearly as favorable as the one in 2003!

It’s also worth noting that Mars sits within four degrees of the rising Moon on the evening of April 14th. The bright star Spica also sits even closer to the Full Moon on the same evening, at less than two degrees away. This particular evening is also noteworthy as it hosts the first of two lunar eclipses for 2014, both of which favor North America.

Mars April 14th.
Mars, the Full Moon and Spica rising in the east on April 14th. Created using Stellarium.

Can you catch Mars near the Moon before sundown on the 14th using binoculars? The Moon will also occult Mars on July 6th for viewers across central and South America.

Though Mars is nicknamed the Red Planet, we’ve seen it appear anywhere from a pumpkin orange to a sickly yellow hue. In fact, such a jaundiced color change can be a sign that a planet-wide dust storm is under way. Such a variation can be readily seen with the naked eye. What color does Mars appear like to you tonight?

On Mars, northern hemisphere summer starts on February 15th, 2014. This means that the northern pole cap of the planet is tipped towards us at opposition during 2014. The day on Mars is only slightly longer than Earth’s at 24 hours and 37 minutes, meaning that Mars will have seemed to rotated only an extra ~8 degrees if you observe it at the same time on each successive evening.

The white pole caps of the planet are the first feature that becomes apparent to the observer at the eyepiece. In February, Mars shows a noticeable gibbous phase in February as we get a peek at the edge of the nighttime side of the planet. Mars will be nearly “full” at opposition, after which it’ll once again take on a slightly distorted football shape.

A growing Mars.
A growing (& shrinking) Mars through the 2014 opposition season. Created by the author using Starry Night Education software.

Tracking the features of the Red Planet is also possible at moderate magnification. One of the largest features apparent is the dark area known as Syrtis Major. Sky & Telescope has an excellent and easy to use application named Mars Previewer that will show you which longitude is currently facing Earth.

Sketching the regions of Mars is a fun exercise. You’ll find that drawing planetary features at the eyepiece can sharpen your observing skills and give you a more critical eye to discern subtle detail. And this season also provides an excellent reason to turn that newly constructed planetary webcam towards Mars.

Up for a challenge? Opposition is also a great time to try and observe the moons of Mars.

moons Starry Night
The moons of Mars as seen on April 8th at around 9:00 Universal Time. Created by the author using Starry Night Education software.

Phobos and Deimos are a tough catch, but are indeed within range of amateur instruments. The chief problem lies in their close proximity to dazzling Mars: +11.5 magnitude, Phobos never strays 14” from the Red Planet in 2014, and 12.4 magnitude Deimos never travels farther than 45” away. Phobos orbits Mars once 7.7 hours — faster than the planet rotates beneath it — and Deimos orbits once every 30.3 hours. The best strategy for a successful Martian moon hunt is to either place Mars just out of the field of view at high power when a moon reaches greatest elongation or block it from view using an eyepiece equipped with an occulting bar.

Extra credit for anyone who nabs pics of the pair!

And opposition is also “Visit Mars season,” as MAVEN and India’s Mars Orbiter Mission arrive later this year. In 2016, NASA’s Mars InSight mission is slated to make the trip, and the window is fast-closing for Dennis Tito’s proposed crewed fly-by mission of Mars in 2018.

And finally, to aid you in your quest for those elusive Martian moons, reader and human astronomical calculator extraordinaire Ed Kotapish was kind enough to compile a list of favorable apparitions of the moons of Mars on the weeks surrounding opposition. (see below)

Good luck, and be sure to send in those pics of Mars and more to Universe Today!

ELONGATIONS OF THE MARTIAN MOONS
DATES AND TIMES IN UT
STARTING  3/30/2014
MAR 30
PHOBOS 0300 W
PHOBOS 0645 E
DEIMOS 0900 W
PHOBOS 1040 W
PHOBOS 1425 E
PHOBOS 1815 W
PHOBOS 2205 EMAR 31
DEIMOS 0005 E
PHOBOS 0155 W
PHOBOS 0545 E
PHOBOS 0935 W
PHOBOS 1320 E
DEIMOS 1515 W
PHOBOS 1715 W
PHOBOS 2100 E

APR 01
PHOBOS 0055 W
PHOBOS 0440 E
DEIMOS 0620 E
PHOBOS 0830 W
PHOBOS 1220 E
PHOBOS 1610 W
PHOBOS 2000 E
DEIMOS 2130 W
PHOBOS 2350 W

APR 02
PHOBOS 0340 E
PHOBOS 0730 W
PHOBOS 1115 E
DEIMOS 1235 E
PHOBOS 1510 W
PHOBOS 1855 E
PHOBOS 2245 W

APR 03
PHOBOS 0235 E
DEIMOS 0345 W
PHOBOS 0625 W
PHOBOS 1015 E
PHOBOS 1405 W
PHOBOS 1755 E
DEIMOS 1855 E
PHOBOS 2145 W

APR 04
PHOBOS 0130 E
PHOBOS 0525 W
PHOBOS 0910 E
DEIMOS 1000 W
PHOBOS 1305 W
PHOBOS 1650 E
PHOBOS 2040 W

APR 05
PHOBOS 0030 E
DEIMOS 0110 E
PHOBOS 0420 W
PHOBOS 0810 E
PHOBOS 1200 W
PHOBOS 1550 E
DEIMOS 1615 W
PHOBOS 1940 W
PHOBOS 2325 E

APR 06
PHOBOS 0320 W
PHOBOS 0705 E
DEIMOS 0725 E
PHOBOS 1055 W
PHOBOS 1445 E
PHOBOS 1835 W
PHOBOS 2225 E
DEIMOS 2230 WAPR 07
PHOBOS 0215 W
PHOBOS 0605 E
PHOBOS 0955 W
PHOBOS 1340 EDEIMOS 1340 E (Mutual)
PHOBOS 1735 W
PHOBOS 2120 E

APR 08
PHOBOS 0115 W
DEIMOS 0445 W
PHOBOS 0500 E
PHOBOS 0850 W
PHOBOS 1240 E
PHOBOS 1630 W
DEIMOS 1955 E
PHOBOS 2020 E

APR 09
PHOBOS 0010 W
PHOBOS 0355 E
PHOBOS 0750 W
DEIMOS 1100 W
PHOBOS 1135 E
PHOBOS 1530 W
PHOBOS 1915 E
PHOBOS 2305 W

APR 10
DEIMOS 0210 E
PHOBOS 0255 E
PHOBOS 0645 W
PHOBOS 1035 E
PHOBOS 1425 W
DEIMOS 1715 W
PHOBOS 1815 E
PHOBOS 2205 W

APR 11
PHOBOS 0150 E
PHOBOS 0545 W
DEIMOS 0825 E
PHOBOS 0930 E
PHOBOS 1320 W
PHOBOS 1710 E
PHOBOS 2100 W
DEIMOS 2330 W

APR 12
PHOBOS 0050 E
PHOBOS 0440 W
PHOBOS 0830 E
PHOBOS 1220 W
DEIMOS 1440 E
PHOBOS 1605 E
PHOBOS 2000 W
PHOBOS 2345 EAPR 13
PHOBOS 0340 W
DEIMOS 0550 W
PHOBOS 0725 E
PHOBOS 1115 W
PHOBOS 1505 E
PHOBOS 1855 W
DEIMOS 2055 E
PHOBOS 2245 E

APR 14
PHOBOS 0235 W
PHOBOS 0620 E
PHOBOS 1015 W
DEIMOS 1205 W
PHOBOS 1400 E
PHOBOS 1755 W
PHOBOS 2140 E

APR 15
PHOBOS 0130 W
DEIMOS 0310 E
PHOBOS 0520 E
PHOBOS 0910 W
PHOBOS 1300 E
PHOBOS 1650 W
DEIMOS 1820 W
PHOBOS 2040 E

APR 16
PHOBOS 0030 W
PHOBOS 0415 E
PHOBOS 0810 W
DEIMOS 0925 E
PHOBOS 1155 E
PHOBOS 1545 W
PHOBOS 1935 E
PHOBOS 2325 W

APR 17
DEIMOS 0035 W
PHOBOS 0315 E
PHOBOS 0705 W
PHOBOS 1055 E
PHOBOS 1445 W
DEIMOS 1540 E
PHOBOS 1830 E
PHOBOS 2225 W

APR 18
PHOBOS 0210 E
PHOBOS 0605 W
DEIMOS 0650 W
PHOBOS 0950 E
PHOBOS 1340 W
PHOBOS 1730 E
PHOBOS 2120 W
DEIMOS 2200 E