Missions Archives

December 18, 2013December 23, 2015 by Bob King

Smack! A New Crater Appears on the Moon/ Yutu Rover Update

Before and after views of the March 17, 2013 impact taken by the LRO camera. Credit: NASA/GSFC/Arizona State University

Where there’s smoke, there’s fire, or in this instance, a new hole in the moon. NASA’s Lunar Impact Monitoring Program recorded the brightest meteoroid impact ever in its 8-year history on March 17 this year. The flash of light, as luminous as a 4th magnitude star and lasting about one second, was caught on video striking the moon in the Sea of Rains (Mare Imbrium) not far from the prominent crater Copernicus. Some time after the event, the Lunar Reconnaissance Orbiter (LRO) swept in for a closer look and spied a brand new impact crater.

Since 2005 the program has detected over 300 flashes which are presumed to be from meteoroid impacts.

Bright impact flash made by a foot-wide rock that struck the moon on March 17, 2013. The moon was a crescent in the evening sky at the time. The impact occurred in the dark, earthlit part of the moon away from the sun-lit crescent. Click photo to see video about the event. Credit: NASA

Based on the flash brightness and duration of the St. Pat’s Day smack, the space boulder measured between one to 1.5 feet long (0.3-0.4 meters) and struck the moon traveling at 56,000 mph with a force of 5 tons of TNT. Scientists predicted then that the impact could produce a crater up to 65 feet (20 meters) in diameter.

Left: Fresh material brought to the surface makes the new 59-foot-wide crater look like it was spray painted white. Credit: NASA/GSFC/Arizona State University. Right: The meteoroid strike occurred near the prominent crater Copernicus in Mare Imbrium. Credit: Bob King — Left: Fresh material brought to the surface makes the new 59-foot-wide crater look like it was spray painted white. Credit: NASA/GSFC/Arizona State University. Right: The meteoroid strike occurred near the familiar crater Copernicus in the Sea of Rains (Mare Imbrium). Credit: Bob King

Well, guess what? When LRO dropped by for a look and compared images taken of the flash site before and after March 17. Staring it in the face was a brand new crater 59 feet across (18 meters). Wow! Just look at how reflective the crater and its rays of ejecta appear. That’s all unweathered, fresh dust and rock excavated from beneath the surface courtesy of 5 tons of extraterrestrial TNT. While impressive from LRO’s 31-mile altitude, the “St. Pat” crater is unfortunately invisible in even the largest telescopes from Earth.

Over time, cosmic rays, solar irradiation and micrometeoroids darken and redden the lunar soil. Millions of years from now, the once brilliant crater will blend into the moonscape. Can you imagine how bright larger craters like Tycho and Copernicus must have looked once upon a time?

Now it's the Chinese Yutu rover's turn to take a photo of the lander. Credit: CCTV — Now it’s the Chinese Yutu rover’s turn to take a photo of the lander. Credit: CCTV

The March 17 impact wasn’t the first new crater seen by LRO, but it does appear to be one of the largest. The LRO camera team has been systematically searching its archive of before and after images for many more lunar landscape changes. Some of those results – including these photos – were presented at the American Geophysical Union Fall Meeting last week; more new craters will be announced in the near future.

Left: The lander's new location in northern Mare Imbrium. Right: LRO scientists have so far nailed down the lander's position somewhere inside the red box on the rim of a small crater with exposed rocky outcrops. Picture is about 1,750 feet side to side. Credit: NASA — Left: The lander’s new location in northern Mare Imbrium. Right: LRO scientists have so far nailed down the lander’s position somewhere inside the red box on the rim of a small crater with exposed rocky outcrops. Picture is about 1,750 feet side to side. Credit: NASA

While we’re on the topic of flyover discoveries, NASA will photograph the Chinese Yutu rover and lander when LRO orbits over western Mare Imbrium on Dec. 24 and 25. As it turns out, the lander didn’t land in Sinus Iridium as reported earlier but in nearby Mare Imbrium, a good distance east of the original site but still within the official “landing box”.

Fortuitously, this location turns out to be a great spot to examine young lavas not sampled during the Apollo missions. All the Apollo rocks ranged in age from 3.1 to 3.8 billion years old. Based on crater counts and the flow’s relatively fresh appearance, Yutu sits at the northern edge of a lava sheet dated at between 1 and 2.5 billion years. In lunar years, that’s fresh!

Flow lobes in the lavas of Mare Imbrium. Chang’e 3 landed at the extreme northern end of this sequence of lavas, which are very young in lunar terms. Credit: NASA / Apollo 15

Younger flows experience less erosion, so the lunar bedrock isn’t buried beneath as much rock as at the Apollo sites. Where Yutu sits, the lunar soil or regolith goes down some 6-7 feet (2 meters) instead of 10-26 feet (3-8 meters) at other landing sites. That means easier excavation of much sought after lunar bedrock. We may even be seeing blocks of bedrock littered about the ~35 foot wide crater (10 meters) in one of the first photos sent back to Earth by the Chinese lander.

The boulders strewn about the crater rim at the Chang'e 3 landing site might be samples of lunar bedrock. Credit: CCTV — The boulders strewn about the crater rim at the Chang’e 3 landing site might be samples of lunar bedrock. Credit: CCTV

For a great analysis of the Chang’e 3 landing site, I recommend reading A New Site to Explore on the Moon by lunar geologist Paul D. Spudis

December 17, 2013December 23, 2015 by Ken Kremer

How to See Spectacular Prime Time Night Launch of Antares Commercial Rocket to ISS on Dec. 19

Antares Launch – Maximum Elevation Map
The Antares nighttime launch will be visible to millions of spectators across a wide area of the Eastern US -weather permitting. This map shows the maximum elevation (degrees above the horizon) that the Antares rocket will reach during the Dec 19, 2013 launch depending on your location along the US east coast. Credit: Orbital Sciences[/caption]

UPDATE: The launch of Cygnus has been delayed until no earlier than January 7, 2014 due to the coolant leak at the International Space Station and necessary spacewalks to fix the problem. You can read more about the issue here and here.

WALLOPS ISLAND, VA – Orbital Sciences Corp. is marching forward with plans for a spectacular night blastoff of the firms privately developed Antares rocket and Cygnus cargo spacecraft on Thursday, Dec. 19 from a seaside pad at Wallops Island, Virginia on a mission for NASA that’s bound for the International Space Station (ISS).

The nighttime Antares liftoff is currently scheduled for prime time – at 9:19 p.m. EST from Launch Pad 0A at the Mid-Atlantic Regional Spaceport (MARS) at NASA Wallops Island, Virginia. It should be easily visible to tens of millions of residents along a wide swath of the US East Coast spanning from South Carolina to southern Maine – weather permitting.

Here’s our guide on “How to See the Antares/Cygnus Dec. 19 Night Launch” – with your own eyes – complete with viewing maps and trajectory graphics from a variety of prime viewing locations; including Philadelphia, NYC, Baltimore and historic landmarks in Washington, DC.

Update: launch postponed to mid-January 2014 to allow NASA astronauts to conduct 3 EVA’s to swap out the ammonia pump module and restore full cooling capacity to the ISS

It will be visible to spectators inland as well, stretching possibly into portions of West Virginia and western Pennsylvania.

For example; Here’s the expected view from Rocky’s famous workout on the steps of the Philadelphia Art Museum.

The viewing maps are courtesy of Orbital Sciences, the private company that developed both the Antares rocket and Cygnus resupply vessel aimed at keeping the ISS fully stocked and operational for science research.

Up top is the map showing the maximum elevation the rocket will reach in the eastern United States.

The flight is designated the Orbital-1, or Orb-1 mission.

Orb-1 is the first of eight commercial cargo resupply missions to the ISS by Orbital according to its Commercial Resupply Services (CRS) contract with NASA.

Of course you can still view the launch live via the NASA TV webcast.

This marks the maiden night launch of the two stage Antares rocket following a pair of daytime test and demonstration launches earlier this year, in April and September.

It’s important to note that the Dec. 19 liftoff is still dependent on NASA engineers resolving the significant issue with the ammonia cooling system that popped up late last week when a critical flow control valve malfunctioned.

If the pump valve can’t be brought back online, two American astronauts may make two or three unscheduled spacewalks starting later this week.

So in the event spacewalks are required, Antares launch could still slip a few days to the end of the launch window around Dec. 21 or Dec. 22. Thereafter the launch would be postponed until January 2014.

Here’s your chance to witness a mighty rocket launch – from the comfort of your home and nearby locations along the east coast.

And its smack dab in the middle of the Christmas and holiday season resplendent with shining bright lights.

Weather outlook appears rather promising at this time – 95% favorable chance of lift off.

The rocket was rolled out to the Wallops launch pad this morning by Orbital’s technicians.

Cygnus is loaded with approximately 1465 kg (3,230 lbs.) of cargo for the ISS crew for NASA.

NASA Television coverage of the Antares launch will begin at 8:45 p.m. on Dec. 19 – www.nasa.gov/ntv

Stay tuned here for Ken’s Antares launch reports from NASA Wallops Flight Facility, VA.

Ken Kremer

December 16, 2013December 23, 2015 by Nancy Atkinson

Oh, the Places We’ve Been: 21 Spacecraft Trajectories Plotted in One Picture

One image from an infographic showing trajectories of 21 different unmanned spacecraft. Click for full image. Credit: Kevin Gill.

Want to know the orbital paths where different spacecraft have traveled and where they are now? A great new infographic put together by Kevin Gill is a visualization of where 21 different unmanned spacecraft have traveled through the Solar System. “The spacecraft data and planet orbital data is derived from NASA/JPL Horizons ephemeris,” said Gill on G+. “The image was rendered using a modified version of my Orbit Viewer WebGL application and put into infographic form using Photoshop. Body and spacecraft positions are as of December 15, 2013.”

By the way, Kevin’s orbit viewer is really fun to play with!

See the full infographic below or on Kevin’s website here:

Paths range from the earliest vector data available, typically just following launch, to either the latest data available or December 15, 2013, whichever is earlier.

“Originally intended as an animation, my browser was not too amused with the quantity of data being thrown at it,” Kevin said via G+. “In the new year, given sufficient demand, I may optimize the modeling and animation algorithms and either produce the animation or release it as a distinct WebGL visualization.”

We certainly look forward to that!

Three different views of our Solar System and the paths of unmanned spacecraft trajectories from their launches to Dec. 15, 2013. Credit: Kevin Gill.

December 15, 2013December 23, 2015 by Ken Kremer

Chinese rover & lander beam back Portraits with China’s Flag shining on Moon’s Surface

Yutu rover emblazoned with Chinese Flag as seen by the Chang'e 3 lander on the moon on Dec. 15, 2013. Credit: China Space

Yutu rover emblazoned with Chinese Flag as seen by the Chang’e-3 lander on the moon on Dec. 15, 2013. Notice the rover tire tracks left behind in the loose lunar topsoil. Credit: China Space
Story updated[/caption]

China’s ambitious lunar space exploration program achieved another stunning success Sunday night, Dec 15, when the countries inaugural Chang’e-3 lunar lander and rover beamed back portraits of one another snapped from the Moon’s surface – that also proudly displayed the brilliant red Chinese national flag shining atop an extraterrestrial body for the very first time in human history.

“I announce the complete success of the Chang’e-3 mission,” said Ma Xingrui, chief commander of China’s lunar program, during a live CCTV broadcast as the portraits were shown to a worldwide audience from huge screens mounted at the mission control at the Beijing Aerospace Control Center (BACC) in Beijing.

Chinese President Xi Jinping was on hand to personally witness the momentous events in real time.

A wave of cheers and high fives rocked around mission control as the startling imagery of the ‘Yutu’ rover and Chang’e-3 lander nestled atop the Moon’s soil in the Bay of Rainbows was received around 11:42 p.m. Sunday, local Beijing time, 10:42 a.m. EST, via China’s own deep space tracking network.

Xi Jinping’s presence was a clear demonstration of China’s confidence in its lunar team and the importance of this space spectacular to China’s prestige and technological prowess.

China thus became 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.

China’s ‘Yutu’ rover had just rolled majestically onto the Moon’s soil hours earlier on Sunday, Dec. 15, at 4:35 a.m. Beijing local time – barely seven hours after the Chang’e-3 mothership touched down atop the lava filled plains of the Bay of Rainbows on Dec. 14.

The rover’s wheels left behind noticeable tire tracks as it drove across the loose lunar topsoil.

Read my earlier detailed accounts of the Dec. 15 drive by Yutu onto the lunar surface illustrated with an extensive photo gallery – here; and of the stunning Dec. 14 landing – here.

CCTV showed China’s President gleefully shaking hands and extending congratulations with many members of the mission team at BACC after seeing the high resolution photos of the Chang’e-3 rover emblazoned with China’s flag for himself.

Chang'e 3 lander as seen by the rover Yutu on the moon on Dec. 15, 2013. Credit: China Space — Chang’e 3 lander as seen by the rover Yutu on the moon on Dec. 15, 2013. Credit: China Space

It’s been nearly four decades since the prior lunar landing was accomplished by 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 ago.

“The Central Committee of the Communist Party and the Central Military Commission [responsible for China’s space program] sends congratulations to all the staff that participated in the successful completion of the mission and China’s first soft landing on the moon,” said the Chinese vice premier Ma Kai during the CCTV broadcast.

“The rover and lander are working properly and reaching the goals set.”

“Chang’e-3 is China’s most complicated space mission,” said Kai. “This shows China is dedicated to the peaceful uses of space.”

“There are many more complicated and difficult tasks ahead.”

Chang'e-3 lander imaged by the rover Yutu on the moon on Dec. 15, 2013. Note landing ramp at bottom. Credit: CCTV — Chang’e-3 lander imaged by the rover Yutu on the moon on Dec. 15, 2013. Note landing ramp at bottom. Credit: CCTV

Indeed so far the Chang’e-3 mission has been primarily a highly successful demonstration of the extremely challenging engineering required to accomplish China’s first lunar landing.

Now the science phase can truly begin.

Over 4600 images have already been transmitted by Chang’e-3 since the Dec. 14 touchdown.

After rolling all six wheels into the dirt, Yutu – which translates as Jade Rabbit – drove to a location about nine meters north of the lander, according to CCTV commentators.

The rover then turned around so that the red Chinese flag emblazoned on the front side would be facing the lander’s high resolution color cameras for the eagerly awaited portraits of one another.

Yutu is nearly the size of a golf cart. It measures about 1.5 m x 1 m on its sides and stands about 1.5 m (nearly 5 feet) tall – nearly human height.

The 120 kg Yutu rover will now begin driving in a circle around the right side of the 1200 kg Chang’e-3 lander – for better illumination – at a distance ranging from 10 to 18 meters.

The rover will snap further photos of the lander as it traverses about from 5 specific locations – showing the front, side and back – over the course of the next 24 hours.

See the accompanying graphic – written in Chinese.

Yutu and the Chang'e 3 lander are scheduled to take photos of each other soon from locations outlined in this artists concept. Credit: China Space — Yutu and the Chang’e 3 lander are scheduled to take photos of each other soon from locations outlined in this artists concept. Credit: China Space

Thereafter Yutu will depart the landing site forever and begin its own lunar trek that’s expected to last at least 3 months.

So the rover and lander will soon be operating independently.

They are equipped with eight science instruments including multiple cameras, spectrometers, an optical telescope, ground penetrating radar and other sensors to investigate the lunar surface and composition.

The radar instrument installed at the bottom of the rover can penetrate 100 meters deep below the surface to study the Moon’s structure and composition in unprecedented detail, according to Ouyang Ziyuan, senior advisor of China’s lunar probe project, in an interview on CCTV.

A UV camera will study the earth and its interaction with solar wind and a telescope will study celestial objects. This is done during the lunar day.

It will also investigate the moon’s natural resources for use by potential future Chinese astronauts.

China's first lunar rover separates from Chang'e-3 moon lander early Dec. 15, 2013. Screenshot taken from the screen of the Beijing Aerospace Control Center in Beijing. Credit: CCTV — China’s first lunar rover separates from Chang’e-3 moon lander early Dec. 15, 2013. Screenshot taken from the screen of the Beijing Aerospace Control Center in Beijing. Credit: CCTV

The two probes are now almost fully operational. Most of the science instruments are working including at least three cameras and the ground penetrating radar.

And although they have survived the harsh lunar environment thus far, they still face massive challenges. They must prove that they can survive the extremely cold lunar night and temperature fluctuations of more than 300 degrees Celsius – a great engineering challenge.

The rover will hibernate during the two week long lunar night.

A radioisotopic heater will provide heat to safeguard the rovers computer and electronics – including the alpha particle X-ray instrument on the rover’s robotic arm.

The Bay of Rainbows, or Sinus Iridum region, is located in the upper left portion of the moon as seen from Earth. You can see the landing site with your own eyes.

Chang’e 3 targeted lunar landing site in the Bay of Rainbows or Sinus Iridum

It was imaged in high resolution by China’s prior lunar mission – the Chang’e-2 lunar orbiter and is shown in graphics herein.

China’s Chang’e-3 probe joins NASA’s newly arrived LADEE lunar probe which entered lunar orbit on Oct. 6 following a spectacular night time blastoff from NASA’s Wallops Flight Facility in Virginia.

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

Ken Kremer

December 14, 2013December 23, 2015 by Ken Kremer

China Scores Historic Success as Chang’e-3 Rover Lands on the Moon Today

Photo taken on Dec. 14, 2013 shows a picture of the moon surface taken by the on-board camera of lunar probe Chang’e-3 on the screen of the Beijing Aerospace Control Center in Beijing. This marks the first time that China has sent a spacecraft to soft land on the surface of an extraterrestrial body. Credit: Xinhua/CCTV
Story updated[/caption]

China scored a stunning, history making success with the successful touchdown of the ambitious Chang’e-3 probe with the ‘Yutu’ rover on the surface of the Moon today, Dec. 14, on the country’s first ever attempt to conduct a landing on an extraterrestrial body.

The dramatic Chang’e-3 soft landing on the lava filled plains of the Bay of Rainbows occurred at about 8:11 am EST, 9:11 p.m. Beijing local time, 1311 GMT today.

The monumental feat is the first landing on the Moon by any entity in nearly four decades. It was broadcast live on CCTV, China’s state run television network.

Note: Read my related new story with a photo gallery of Yutu’s 6 wheels rolling onto lunar soil – here

This maiden Chinese moon landing marks a milestone achievement for China and clearly demonstrates the country’s technological prowess.

A tidal wave of high fives was unleashed by the huge teams of Chinese space engineers teams controlling the flight from the Beijing Aerospace Control Center (BACC).

There was also a huge sense of relief from the nail biting tension upon confirmation of the successful soft landing following many years of hard work and intense planning.

The Chang’e-3 mission entails the first soft landing on the Moon by anyone since the Soviet Union’s unmanned Luna 24 sample return vehicle touched down back in 1976.

Artists concept of the rocket assisted landing of China’s lunar probe Chang'e-3. — Artists concept of the rocket assisted landing of China’s lunar probe Chang’e-3.

China now joins an elite club of three, including the United States, who have mastered the critical technology required to successfully touch down on Earth’s nearest neighbor.

China’s space vision also stands in total contrast to the utter lack of vision emanating from so called political leaders in Washington, DC who stymie NASA and US science at every opportunity!

‘Yutu’ could very well serve as a forerunner for testing the key technologies required for a Chinese manned lunar landing in the next decade.

In one of its first acts from the surface, the landers life giving solar panels were deployed as planned within minutes of touchdown

The Chang’e-3 mission is comprised of China’s ‘Yutu’ lunar lander riding piggyback atop a much larger four legged landing vehicle.

The Chang’e-3 lander transmitted its first images of the moon in real time during its approach to the lunar surface during the final stages of the ongoing landing operation carried live by CCTV.

A total of 59 images were received instead of the 10 expected, said a CCTV commentator.

The voyage from the Earth to the Moon began 12 days ago with the flawless launch of Chang’e-3 atop China’s Long March 3-B booster at 1:30 a.m. Beijing local time, Dec. 2, 2013 (12:30 p.m. EST, Dec. 1) from the Xichang Satellite Launch Center, in southwest China.

Chang’e-3 made a rocket powered descent to the Moon’s surface today by firing the landing thrusters starting at the altitude of 15 km (9 mi) for a soft landing targeted to a preselected area on the Bay of Rainbows.

The powered descent was autonomous and took about 12 minutes.

The variable thrust engine can continuously vary its thrust power between 1,500 to 7,500 newtons. It was the biggest ever used by China in space said a commentator on CCTV.

The variable thrust engine enabled Chang’e-3 to reduce its deceleration as it approached the moon.

The descent was preprogrammed and controlled by the probe itself, not from the ground.

A descent camera was mounted on the lander’s belly

The 1200 kg lander is equipped with unprecedented terrain recognition equipment and software to hover above the landing site and confirm it was safe. This enabled the craft to avoid rock and boulder fields that could spell catastrophe even in the final seconds before touchdown if the vehicle were to land directly on top of them.

The descent engine fired until the lander was about hovering 100 meters above the lunar surface.

After determining it was safe to proceed, the lander descended further to about 3 meters. The engine then cut off and the lander free fell the remaining distance. The impact was cushioned by shock absorbers.

The solar panels soon unfurled. They are the most efficient Chinese solar panels available, said a CCTV commentator.

The Bay of Rainbows, or Sinus Iridum region, is located in the upper left portion of the moon as seen from Earth. You can see the landing site with your own eyes.

It was imaged in high resolution by China’s prior lunar mission – the Chang’e-2 lunar orbiter – and is shown in graphics herein.

The Yutu rover is also unfurling its solar panels and mast today.

Yutu, which translates as Jade Rabbit, stands 150 centimeters high, or nearly 5 feet – human height.

It weighs approximately 120 kilograms and sports a robotic arm equipped with advanced science instruments.

On Sunday, the six-wheeled ‘Yutu’ rover with a rocker bogie suspension similar to NASA’s Mars rovers will be lowered in stages to the moon’s surface in a complex operation and then drive off a pair of landing ramps to explore the moon’s terrain for at least three months.

In what promises to be a space spectacular, the lander and rover are expected to photograph one another soon after Yutu rolls onto the Bay of Rainbows.

They will work independently.

The rover and lander are equipped with multiple cameras, spectrometers, an optical telescope, ground penetrating radar and other sensors to investigate the lunar surface and composition.

The Chang’e-3 lander is powered by a combination of solar arrays and a nuclear battery said CCTV, in order to survive the two week long lunar nights.

Chinese space officials expect the lander will function a minimum of 1 year.

ESA’s network of tracking stations are providing crucial support to China for Chang’e-3 from launch to landing.

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

Ken Kremer

December 13, 2013December 23, 2015 by Ken Kremer

China’s Chang’e-3 Moon Rover Descends to Lower Orbit Sets Up Historic Soft Landing

All systems appear to be “GO” for the world’s first attempt to soft land a space probe on the Moon in nearly four decades.

China’s maiden moon landing probe – Chang’e-3 – is slated to attempt the history making landing this weekend on a lava plain in the Bay of Rainbows, or Sinus Iridum region.

Chinese space engineers at the Beijing Aerospace Control Center (BACC) paved the way for the historic touchdown by successfully commanding Chang’e-3 to descend from the 100 km-high lunar circular orbit it reached just one week ago on Dec. 6, to “an elliptical orbit with its nearest point about 15 km away from the moon’s surface”, according to a statement from China’s State Administration of Science, Technology and Industry for National Defense (SASTIND).

UPDATE: CCTV is providing live landing coverage

The first pictures taken from the alien lunar surface in some 37 years are expected to be transmitted within days or hours of touchdown planned as early as Saturday, Dec. 14, at 9:40 p.m. Beijing local time, 8:40 a.m. EST.

CCTV, China’s state run network, carried the launch live. It remains to be seen whether they will have live coverage of the landing since there have been no programming announcements.

SASTIND said the orbit lowering thruster firing was “conducted above the dark side of the moon at 9:20 p.m.” on Dec. 10, Beijing local time.

Confirmation of the Chang’e-3 probes new, lower orbit was received four minutes later.

China's lunar probe Chang'e-3 entered an orbit closer to the moon on Dec. 10, 2013. (Xinhua) — China’s lunar probe Chang’e-3 entered an orbit closer to the moon on Dec. 10, 2013. Credit: Xinhua

If successful, the Chang’e-3 mission will mark the first soft landing on the Moon since the Soviet Union’s unmanned Luna 24 sample return vehicle landed back in 1976.

China would join an elite club of three, including the United States, who have mastered the critical technology to successfully touch down on Earth’s nearest neighbor.

The Chang’e-3 mission is comprised of China’s ‘Yutu’ lunar lander riding piggyback atop a much larger four legged landing probe.

Artists concept of the Chinese Chang'e 3 lander and rover on the lunar surface. Credit: Beijing Institute of Spacecraft System Engineering — Artists concept of the Chinese Chang’e-3 lander and rover on the lunar surface. Credit: Beijing Institute of Spacecraft System Engineering

Chang’e-3 will make a powered descent to the Moon’s surface on Dec. 14 by firing the landing thrusters at the altitude of 15 km (9 mi) for a soft landing in a preselected area on the Bay of Rainbows.

The powered descent will take about 12 minutes.

The variable thrust engine can continuously vary its thrust power between 1,500 to 7,500 newtons, according to Xinhua.

The Bay of Rainbows is located in the upper left portion of the moon as seen from Earth. It was imaged in high resolution by China’s prior lunar mission – the Chang’e-2 lunar orbiter.

The 1200 kg lander is equipped with terrain recognition equipment and software to avoid rock and boulder fields that could spell catastrophe even in the final seconds before touchdown if the vehicle were to land directly on top of them.

Chang’e-3 is powered by a combination of solar arrays and a nuclear device in order to survive the two week long lunar nights.

The six-wheeled ‘Yutu’ rover, with a rocker bogie suspension, will be lowered in stages to the moon’s surface in a complex operation and then drive off a pair of landing ramps to explore the moon’s terrain.

Yutu measures 150 centimeters high and weighs approximately 120 kilograms and sports a robotic arm equipped with science instruments.

The rover and lander are equipped with multiple cameras, spectrometers, an optical telescope, ground penetrating radar and other sensors to investigate the lunar surface and composition.

The radar instrument installed at the bottom of the rover can penetrate 100 meters deep below the surface to study the Moon’s structure and composition in unprecedented detail.

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

Ken Kremer

December 12, 2013December 23, 2015 by David Dickinson

IRIS Glimpses an Elusive Region of the Sun

An innovative solar observatory is adding a key piece to the puzzle of the enigma that is our Sun.

Its two of key questions in heliophysics: why does our Sun have a corona? And why is the temperature of the corona actually higher than the surface of the Sun?

This week, researchers released results from the preliminary first six months of data from NASA’s Interface Region Imaging Spectrograph, known as IRIS. The findings were presented at the Fall American Geophysical Union Meeting this past Monday.

IRIS was launched on June 27^th of this year on a Pegasus-XL rocket deployed from the belly of a Lockheed L-1011 aircraft flying out of Vandenberg Air Force Base. IRIS can focus in on a very specific interface region of the Sun sandwiched between the dazzling solar photosphere and the transition to the corona. To accomplish this, IRIS employs an ultraviolet slit spectrograph looking at ionized gas spectra.

IRIS in the clean room. The spacecraft is only about 2 metres in length, about the height of a person. (Credit: Lockheed Martin).

“The quality of images and spectra we are receiving is amazing,” IRIS Principal Investigator Alan Title said in a recent press release from the NASA Goddard Space Flight Center. While other missions may take over a decade to go from the drawing board to the launch pad, IRIS was developed and deployed into Low Earth Orbit in just 44 months.

IRIS offers scientists a new tool to probe the Sun and a complimentary instrument to platforms such as Hinode, the Solar Heliospheric Observatory (SOHO) and NASA’s Solar Dynamics Observatory. In fact, IRIS has a better resolution than SDO’s AIA imagers or Hinode when it comes to this key solar interface region. IRIS has a 20x greater resolution in time, and 25x the spatial resolution of any former space-based UV spectrometer deployed.

“We are seeing rich and unprecedented images of violent events in which gases are accelerated to very high velocities while being rapidly heated to hundreds of thousands of degrees,” said Lockheed Martin science lead on the IRIS mission Bart De Pontieu. These observations are key to backing up theoretical models of solar dynamics as well as testing and formulating new ones of how our Sun works.

IRIS bridges this crucial gap between the photosphere and the lower chromosphere of the Sun. While the solar surface roils at relatively placid 6,000 degrees Celsius, temperatures rise into the range of 2-3 million degrees Celsius as you move up through the transition region and into the corona.

Two key solar phenomena that are of concern to solar researchers can be examined by IRIS in detail. One is the formation of prominences, which show up as long looping swirls of solar material rising up from the surface of the Sun. Prominences can be seen from backyard telescopes at hydrogen alpha wavelengths. IRIS can catch and track their early modeling with unprecedented resolution. Images released from IRIS show the fine structure of targeted prominences as they evolve and rise off the surface of the Sun. When a prominence and accompanying coronal mass ejection is launched in our direction, disruption of our local space environment caused by massive solar storm can result.

Slit jaw spectra images (the two strips to the left) and imaging a spicules 9to the right as seen by IRIS. (Credit: NASA/IRIS). — Slit jaw spectra images (the two strips to the left) and imaging of spicules (to the right) as seen by IRIS. (Credit: NASA/IRIS).

The second phenomenon targeted by IRIS is the formation of spicules, which are giant columns of gas rising from the photosphere. Although the spicules look like hair-fine structures through Earth-based solar telescopes, they can be several hundred kilometres wide and as long as the Earth. Short-lived, spicules race up from the surface of the Sun at up to 240,000 kilometres per hour and seem to play a key role in energy and heat transfer from the solar surface up through the atmosphere. IRIS is giving us a view of the evolution of spicules for the first time, and they’re proving to be even more complex than theory previously suggested.

“We see discrepancies between these observations and the models, and that is great news for advancing knowledge. By seeing something we don’t understand, we have a chance of learning something new,” Said University of Oslo astrophysicist Mats Carlsson.

Like SDO and SOHO, data and images from IRIS are free for the public to access online. Though the field of view for IRIS is a narrow 2’ to 4’ arc minutes on a side – the solar disk spans about 30’ as seen from the Earth – IRIS gives us a refined view of “where the action is.”

Where is IRIS looking? This snapshot gives some context of the IRIS field of view (green and red boxes) and black and white insets versus SDO's AIA full disk view of the Sun. (Credit: NASA/SDO/IRIS). — Where is IRIS looking? This snapshot gives some context of the IRIS field of view (green and red boxes) and black and white insets versus SDO’s AIA full disk view of the Sun. (Credit: NASA/SDO/IRIS).

And this all comes at an interesting time, as our nearest star crosses the sputtering solar maximum for Cycle #24.

The equivalent of 50 million CPU hours were utilized in constructing and modeling what IRIS sees. The reconstruction was an international effort, spanning the Partnership for Advanced Computing in Europe, the Norwegian supercomputing collaboration, and NASA’s Ames Research Center.

IRIS also faced the additional challenge of weathering a 2.5 week period of inactivity due to the U.S. government shutdown this fall. Potential impacts due to sequestration remain an issue, though small explorer missions such as IRIS demonstrate how we can do more with less.

“We’ve made a giant step forward in characterizing the heat transfer properties of this region between the visible surface and the corona, which is key to understanding how the outer atmosphere of the Sun exists, and is key to understanding the outer atmosphere that the Earth lies in,” said Alan Title, referring to the tenuous heliosphere of the Sun extending out through the solar system.

Understanding the inner working of our Sun is vital: no other astronomical body has as big an impact on life here on Earth.

IRIS is slated for a two-year mission, though as is the case with most space-based platforms, researchers will work to get every bit of usefulness out of the spacecraft that they can. And it’s already returning some first-rate science at a relatively low production cost. This is all knowledge that will help us as a civilization live with and understand our often tempestuous star.

December 11, 2013December 23, 2015 by Elizabeth Howell

Is There Martian Salty Water At The Red Planet’s Equator? These Lines May Be The Smoking Gun

A series of images from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter show how the appearance of dark markings on Martian slope changes with the seasons. Image credit: NASA/JPL-Caltech/Univ. of Arizona.

Get ready, because here are some more findings about possible water on Mars. This picture above from the Mars Reconnaissance Orbiter is a series showing changing dark lines on an equatorial hillside — which could be an indication of salty water, scientists said.

As MRO circled the planet and peered at the lines with its High Resolution Imaging Science Experiment (HiRISE) camera, it tracked these changes at five locations in Valles Marineris, the biggest canyon our solar system has to offer. The lines were on slopes that faced the north and the south, and most intriguingly, they activated when the sun hit their respective sides.

“The equatorial surface region of Mars has been regarded as dry, free of liquid or frozen water, but we may need to rethink that,” stated Alfred McEwen of the University of Arizona in Tucson.

“The explanation that fits best is salty water is flowing down the slopes when the temperature rises,” added McEwen, who is HiRISE principal investigator. “We still don’t have any definite identification of water at these sites, but there’s nothing that rules it out, either.”

A 2010 image of ice excavated on Mars after a recent meteorite impact. Image from the Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE) camera. Credit: NASA/JPL-Caltech/Univ. of Arizona — A 2010 image of ice excavated on Mars after a recent meteorite impact. Image from the Mars Reconnaissance Orbiter’s High Resolution Imaging Science Experiment (HiRISE) camera. Credit: NASA/JPL-Caltech/Univ. of Arizona

Scientists first spotted these types of features two years ago in the mid-latitudes of Mars, but in that case these were small features (usually less than 16 feet or five meters wide). The slopes observed here range as wide as 4,000 feet (1,200 meters).

Salt can keep water flowing even in temperatures where more pure water gets frozen, and also reduce the evaporation rate. NASA also noted it used data from two other MRO instruments (Compact Reconnaissance Imaging Spectrometer for Mars and the Context Camera) and the Mars Oddysey’s Thermal Emission Imaging System.

That’s not all, however. Scientists also reported 15 fresh craters that excavated ice that used to be hidden underneath the soil of Mars.

A radar on NASA's Mars Reconnaissance Orbiter has detected widespread deposits of glacial ice in the mid-latitudes of Mars.NASA/JPL-Caltech/ASI/University of Rome/Southwest Research Institute — A radar on NASA’s Mars Reconnaissance Orbiter has detected widespread deposits of glacial ice in the mid-latitudes of Mars.NASA/JPL-Caltech/ASI/University of Rome/Southwest Research Institute

“The more we find, the more we can fill in a global map of where ice is buried,” stated Colin Dundas of the United States Geological Survey in Flagstaff, Ariz.

“We’ve now seen icy craters down to 39 degrees north, more than halfway from the pole to the equator. They tell us that either the average climate over several thousand years is wetter than present or that water vapor in the current atmosphere is concentrated near the surface. Ice could have formed under wetter conditions, with remnants from that time persisting today, but slowly disappearing.”

Results were presented at the American Geophysical Union’s fall meeting this week.

Source: NASA

December 10, 2013December 23, 2015 by Ken Kremer

Mars One Proposes First Privately Funded Robotic Mars Missions – 2018 Lander & Orbiter

Mars One proposes Phoenix-like lander for first privately funded mission to the Red Planet slated to blastoff in 2018. This film solar array experiment would provide additional power. Credit: Mars One

The Mars One non-profit foundation that aims to establish a permanent human settlement on the Red Planet in the mid-2020’s – with colonists volunteering for a one-way trip – took a major step forward today, Dec. 10, when they announced plans to launch the first ever privately funded space missions to Mars in 2018; as forerunners to gather critical measurements.

Bas Lansdorp, Mars One Co-founder and CEO announced plans to launch two missions to the Red Planet in 2018 – consisting of a robotic lander and an orbiting communications satellite; essential for transmitting the data collected on the Red Planet’s surface.

And he has partnered with a pair of prestigious space companies to get started.

Lansdorp made the announcement at a news media briefing held today at the National Press Club in Washington, DC.

“This will be the first private mission to Mars and the lander’s successful arrival and operation will be a historic accomplishment,” said Lansdorp.

Lansdorp stated that Mars One has signed contracts with Lockheed Martin and Surrey Satellite Technology Ltd. (SSTL) to develop mission concept studies – both are leading aerospace companies with vast experience in building spacecraft.

The 2018 Mars One lander would be a technology demonstrator and include a scoop, cameras and an exotic solar array to boost power and longevity.

The spacecraft structure would be based on NASA’s highly successful 2007 Phoenix Mars lander – built by Lockheed Martin – which discovered and dug into water ice buried just inches beneath the topsoil in the northern polar regions of the Red Planet.

3 Footpads of Phoenix Mars Lander atop Martian Ice. Phoenix thrusters blasted away Martian soil and exposed water ice. Proposed Mars InSight mission will build a new Phoenix-like lander from scratch to peer deep into the Red Planet and investigate the nature and size of the mysterious Martian core. Credit: Ken Kremer, Marco Di Lorenzo, Phoenix Mission, NASA/JPL/UA/Max Planck Institute — 3 Footpads of Phoenix Mars Lander atop Martian Ice
Phoenix thrusters blasted away Martian soil and exposed water ice. Proposed Mars One 2018 mission will build a new Phoenix-like lander from scratch to test technologies for extracting water into a useable form for future human colonists. NASA’s InSight 2016 mission will build a new Phoenix-like lander to peer deep into the Red Planet and investigate the nature and size of the mysterious Martian core. Credit: Ken Kremer, Marco Di Lorenzo, Phoenix Mission, NASA/JPL/UA/Max Planck Institute

“We are excited to have been selected by Mars One for this ambitious project and we’re already working on the mission concept study, starting with the proven design of Phoenix,” said Ed Sedivy, Civil Space chief engineer at Lockheed Martin Space Systems. “Having managed the Phoenix spacecraft development, I can tell you, landing on Mars is challenging and a thrill and this is going to be a very exciting mission.”

Lockheed Martin engineers will work for the next 3 to 4 months to study mission concepts as well as how to stack the orbiter and lander on the launcher,” Sedivy said at the briefing.

“The lander will provide proof of concept for some of the technologies that are important for a permanent human settlement on Mars,” said Lansdorp.

Two examples involve experiments to extract water into a usable form and construction of a thin film solar array to provide additional power to the spacecraft and eventual human colonists.

It would include a Phoenix like scoop to collect soils for the water extraction experiment and cameras for continuous video recording transmitted by the accompanying orbiter.

Lockheed Martin is already under contract to build another Phoenix type lander for NASA that is slated to blastoff in 2016 on the InSight mission.

“They have a distinct legacy of participating in nearly every NASA mission to Mars,” said Lansdorp.

So if sufficient funding is found it seems apparent that lander construction should be accomplished in time.

However, building the science instruments from scratch to meet the tight timeline could be quite challenging.

Given that the lander is planned to launch in barely over four years, I asked Sedivy if that was sufficient time to select, design and develop the new science instruments planned for the 2018 mission.

“A typical life cycle for the Mars program provides three and a half years from commitment to design to launch. So we have about 1 year to commit to preliminary design for the 2018 launch, so that’s favorable,” Sedivy told Universe Today.

“Now as for having enough time for selecting the suite of science experiments that’s a little trickier. It depends on what’s actually selected and the maturity of those elements selected.”

“So we will provide Mars One with input as to where we see the development risks. And we’ll help guide the instrument selections to have a high probability that they will be ready in time for the 2018 launch window,” Sedivy told me.

Video caption: Mars One Crowdfunding Campaign 2018 Mars Mission

For the 2018 lander, Mars One also plans to include an experiment from a worldwide university challenge and items from several Science, Technology, Engineering and Math (STEM) challenge winners.

Surrey Satellite Technology Ltd. (SSTL) was selected to studying orbiter concepts that will provide a high bandwidth communications system in a Mars synchronous orbit and will be used to relay data and a live video feed from the lander on the surface of Mars back to Earth, according to Sir Martin Sweeting, Executive Chairman of SSTL.

There are still many unknowns at this stage including the sources for all the significant funding required by Mars One to transform their concepts into actual flight hardware.

“Crowdfunding and crowdsourcing activities are important means to do that,” said Lansdorp.

At the briefing, Lansdorp stated that Mars One has started an Indiegogo crowdfunding campaign. The goal is to raise $400,000 by Jan. 25, 2014.

Link to – Indiegogo Mars One campaign

Mars One is looking for sponsors and partners. They also plan a TV show to help select the winners of the first human crew to Mars from over 200,000 applicants from countries spread all across Earth.

The preliminary 2018 mission study contracts with Lockheed and Surrey are valued at $260,000 and $80,000 respectively.

Stay tuned here for Ken’s continuing Curiosity, Chang’e 3, LADEE, MAVEN and MOM news and his upcoming Antares launch reports from on site at NASA Wallops Flight Facility, VA.

Ken Kremer

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Learn more about Mars, Curiosity, Orion, MAVEN, MOM, Mars rovers, Antares Launch, Chang’e 3, SpaceX and more at Ken’s upcoming presentations

Dec 11: “Curiosity, MAVEN and the Search for Life on Mars”, “LADEE & Antares ISS Launches from Virginia”, Rittenhouse Astronomical Society, Franklin Institute, Phila, PA, 8 PM

Dec 15-20: “Antares/Cygnus ISS Rocket Launch from Virginia”; Rodeway Inn, Chincoteague, VA, evening

December 9, 2013December 23, 2015 by Ken Kremer

Curiosity Discovers Ancient Mars Lake Could Support Life

Outcrops in Yellowknife Bay are being exposed by wind driven erosion. These rocks record superimposed ancient lake and stream deposits that offered past environmental conditions favorable for microbial life. This image mosaic from the Mast Camera instrument on NASA's Curiosity Mars rover shows a series of sedimentary deposits in the Glenelg area of Gale Crater, from a perspective in Yellowknife Bay looking toward west-northwest. The "Cumberland" rock that the rover drilled for a sample of the Sheepbed mudstone deposit (at lower left in this scene) has been exposed at the surface for only about 80 million years. Credit: NASA/JPL-Caltech/MSSS

NASA’s Curiosity rover has discovered evidence that an ancient Martian lake had the right chemical ingredients that could have sustained microbial life forms for long periods of time – and that these habitable conditions persisted on the Red Planet until a more recent epoch than previously thought.

Furthermore researchers have developed a novel technique allowing Curiosity to accurately date Martian rocks for the first time ever – rather than having to rely on educated guesses based on counting craters.

All that and more stems from science results just announced by members of the rover science team.

Researchers outlined their remarkable findings in a series of six new scientific papers published today (Dec. 9) in the highly respected journal Science and at talks held today at the Fall 2013 Annual Meeting of the American Geophysical Union (AGU) in San Francisco.

The Curiosity team also revealed that an investigation of natural Martian erosion processes could be used to direct the rover to spots with a higher likelihood of holding preserved evidence for the building blocks of past life – if it ever existed.

View of Yellowknife Bay Formation, with Drilling Sites. This mosaic of images from Curiosity's Mast Camera (Mastcam) shows geological members of the Yellowknife Bay formation, and the sites where Curiosity drilled into the lowest-lying member, called Sheepbed, at targets "John Klein" and "Cumberland." The scene has the Sheepbed mudstone in the foreground and rises up through Gillespie Lake member to the Point Lake outcrop. These rocks record superimposed ancient lake and stream deposits that offered past environmental conditions favorable for microbial life. Rocks here were exposed about 70 million years ago by removal of overlying layers due to erosion by the wind. Credit: NASA/JPL-Caltech/MSSS — View of Yellowknife Bay Formation, with Drilling Sites
This mosaic of images from Curiosity’s Mast Camera (Mastcam) shows geological members of the Yellowknife Bay formation, and the sites where Curiosity drilled into the lowest-lying member, called Sheepbed, at targets “John Klein” and “Cumberland.” The scene has the Sheepbed mudstone in the foreground and rises up through Gillespie Lake member to the Point Lake outcrop. These rocks record superimposed ancient lake and stream deposits that offered past environmental conditions favorable for microbial life. Rocks here were exposed about 70 million years ago by removal of overlying layers due to erosion by the wind. Credit: NASA/JPL-Caltech/MSSS

The ancient fresh water lake at the Yellowknife Bay area inside the Gale Crater landing site explored earlier this year by Curiosity existed for periods spanning perhaps millions to tens of millions of years in length – before eventually evaporating completely after Mars lost its thick atmosphere.

Furthermore the lake may have existed until as recently as 3.7 Billion years ago, much later than researchers expected which means that life had a longer and better chance of gaining a foothold on the Red Planet before it was transformed into its current cold, arid state.

NASA's Mars rover Curiosity took this self-portrait, composed of more than 50 images using its robotic arm-mounted MAHLI camera, on Feb. 3. The image shows Curiosity at the John Klein drill site. A drill hole is visible at bottom left. Credit: NASA / JPL / MSSS / Marco Di Lorenzo / Ken Kremer- kenkremer.com — NASA’s Mars rover Curiosity took this self-portrait, composed of more than 50 images using its robotic arm-mounted MAHLI camera, on Feb. 3. The image shows Curiosity at the John Klein drill site. A drill hole is visible at bottom left. Credit: NASA / JPL / MSSS / Marco Di Lorenzo / Ken Kremer- kenkremer.com

Researchers also announced that they are shifting the missions focus from searching for habitable environments to searching for organic molecules – the building blocks of all life as we know it.

Why the shift? Because the team believes they have found a way to increase the chance of finding organics preserved in the sedimentary rock layers.

“Really what we’re doing is turning the corner from a mission that is dedicated to the search for habitable environments to a mission that is now dedicated to the search for that subset of habitable environments which also preserves organic carbon,” Curiosity Principal Investigator John Grotzinger, of the California Institute of Technology in Pasadena, said at an AGU press conference today.

“That’s the step we need to take as we explore for evidence of life on Mars.”

Earlier this year, Curiosity drilled into a pair of sedimentary Martian mudstone rock outcrops at Yellowknife Bay known as “John Klein” and “Cumberland” – for the first time in history.

Grotzinger said the ancient lake at Yellowknife Bay was likely about 30 miles long and 3 miles wide.

Powdered samples deposited into the rovers miniaturized chemistry labs – SAM and CheMin – revealed the presence of significant levels of phyllosilicate clay minerals.

These clay minerals form in neutral pH water that is ‘drinkable” and conducive to the formation of life.

“Curiosity discovered that the fine-grained sedimentary rocks preserve evidence of an environment that would have been suited to support a Martian biosphere founded on chemolithoautotrophy,” according to one of the science papers co-authored by Grotzinger.

“This aqueous environment was characterized by neutral pH, low salinity, and variable redox states of both iron and sulfur species.”

The rover has detected key elements required for life including carbon, hydrogen, oxygen, sulfur nitrogen and phosphorous.

The team is still looking for signatures of organic molecules.

Right now the researchers are driving Curiosity along a 6 mile path to the base of Mount Sharp -the primary mission destination – which they hope to reach sometime in Spring 2014.

But along the way they hope to stop at a spot where wind has eroded the sedimentary rocks just recently enough to expose an area that may still preserve evidence for organic molecules – since it hasn’t been bombarded by destructive cosmic radiation for billions of years.

Stay tuned here for Ken’s continuing Curiosity, Chang’e 3, LADEE, MAVEN and MOM news.

Ken Kremer

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Learn more about Curiosity, Orion, MAVEN, MOM, Mars rovers, Chang’e 3, SpaceX, and more at Ken’s upcoming presentations

Dec 10: “Antares ISS Launch from Virginia, Mars and SpaceX Mission Update”, Amateur Astronomers Association of Princeton, Princeton University, Princeton, NJ, 8 PM

Dec 11: “Curiosity, MAVEN and the Search for Life on Mars”, “LADEE & Antares ISS Launches from Virginia”, Rittenhouse Astronomical Society, Franklin Institute, Phila, PA, 8 PM