Wednesday, August 3, 2016

Moon Express licensed for lunar expedition in 2017

Moon Express unique torus bus approaches lunar vicinity in notional representation [Moon Express].
Mike Wall
Senior Writer

For the first time ever, a private company has permission to land on the moon.

The U.S. government has officially approved the planned 2017 robotic lunar landing of California-based Moon Express, which aims to fly commercial missions to Earth's nearest neighbor and help exploit its resources, company representatives announced today .

"This is not only a milestone, but really a threshold for the entire commercial space industry," Moon Express co-founder and CEO Bob Richards told

Previously, companies had been able to operate only on or around Earth. The new approval, while exclusive to Moon Express, could therefore serve as an important regulatory guide for deep-space commercial activity in general, Richards said.

"Nobody's had a deep-sea voyage yet. We're still charting those waters," he said. "Somebody had to be first."

Moon Express submitted an application to the U.S. Federal Aviation Administration (FAA) on April 8. The document then made its way through the U.S. State Department, the U.S. Department of Defense, NASA, the National Oceanic and Atmospheric Administration, and the Federal Communications Commission, Richards said.

View the full article, HERE.

Monday, March 21, 2016

Desolate magnificence -The Space Review

LRO images on display at the Smithsonian Air & Space Museum [Dwayne Day/The Space Review].
Dwayne Day

Right now Washington, DC’s museums are filled with the noise of hormonal teenagers on their spring break trips to the nation’s capital. They run around aimlessly, oblivious to their surroundings, or sprawl on the dirty carpet absorbed in their own little worlds. Later, in May, the senior class trips will show up, and those older students are a little less noisy, a little more focused, but they too will probably not be all that interested in the actual museums, even if they take their noses out of their cellphones for more than a second or two. But just maybe, perhaps, one or two of them may accidentally wander into one of the National Air and Space Museum’s new exhibits and they might quiet down for a moment and see something both familiar and alien.

The exhibit is titled “A New Moon Rises” and it is a display of large format photographs from NASA’s Lunar Reconnaissance Orbiter featuring the Moon in all its panchromatic glory. You could look at most of these photos on your computer screen, but seeing them enlarged and displayed on a museum wall like works of art is an entirely different experience.

The Lunar Reconnaissance Orbiter, or LRO, was launched in 2009 and has been chugging away ever since. If nothing breaks, in four or five years the spacecraft will probably run out of fuel and, because the Moon’s gravity field is uneven, it will ultimately fall and silently crash into the surface after more than a decade in orbit.

- Read the full article online, in the latest issue of The Space Review, HERE.

Tuesday, February 16, 2016

Stunning pictures of the Moon over London skyline

Photographer James Burns has spent the past year capturing various lunar spectacles in London. Some of the result is part of thirteen images posted in a London Evening Standard slideshow, HERE [james Burns@London_Rooftops].
Liz Connor and Gareth Richman

From September’s supermoon rising to the magnificent lunar eclipse, photographer James Burns captures some of the most breathtaking states of the moon over London.

His Lunar London project emerged after various evenings of photographing the capital’s skyline led to a string of chance encounters with the moon.

“I had a growing fascination with how I could capture it in the same way I had been the shooting the rising and setting sun for some years”, James told the Evening Standard.

“2015 was a lucky year for moongazing in London. Despite cloud cover across most of Europe, September's supermoon lunar eclipse was visible in perfectly clear skies over London and was an otherworldly joy to behold.”

Read the full feature and view the Gallery HERE.

Monday, February 15, 2016

Plans for Moon resort in California

Artist conception of the proposed Moon USA resort and entertainment complex in Coachella Valley near Indio,  California.Renderings courtesy of Moon World Resorts, Inc. feature at
Danny Jensen

Dust off your moon boots because a Canadian developer is aiming to build a $4 billion, five-star lunar resort, known as Moon USA, in the city of Coachella, just down the road from where the music fest is held in Indio. That kind of awesomeness is obviously what has been missing from all of our lives.

View details and artist renderings HERE.

Friday, February 12, 2016

Israeli GLXP team 'all in' for Reiner Gamma

Israeli President Reuven Rivlinlooks on as SpaceIL's GLXP lunar lander prototype is unveiled [Alon Hadar].
Abigail Klein Leichman
New Jersey Jewish Standard

Why is a team from the tiniest country in the Middle East joining an international race to the moon?

It’s not just the promise of a Google Lunar XPRIZE of $20 million to the first team (and $5 million to the second team) that lands an unmanned spacecraft on the moon by December 31, 2017, and then moves it 500 meters across the lunar surface as it sends high-definition images and videos back to earth.

The Israelis’ participation has much to do with a cultural passion to accomplish the seemingly impossible. It also is fueled by a desire to make history, inspire Jewish pride, and encourage more young people to pursue careers that will sustain Israel’s leading position in the high-tech world.

Still image from YouTube video detailing the SpaceIL ballistics. the Israeli team intends to utilize graduated orbital phases to attain increasing apogee in graduated stages, similar to the polar orbit method previously employed by both ESA and the ISRO. The team has chosen the Reiner Gamma swirl and magnetic anomaly north of the lunar equator in Oceanua Procellarum as its eventual landing site.
“Only global superpowers with billion-dollar space programs — the United States, Russia, and China — have soft-landed a rover on the surface of the moon,” said SpaceIL’s CEO, Dr. Eran Privman, last October, when SpaceIL became the first Google Lunar XPRIZE (GLXP) team to sign a verified launch contract for a privately funded mission to the moon.

On February 17, Yonatan Winetraub — one of three young Israeli engineers who founded the nonprofit organization SpaceIL in 2010 to enter the GLXP competition — will speak about the ambitious project at Rutgers University in New Brunswick.

Read the full and unusually detailed write-up HERE.

Thursday, February 11, 2016

Lunar Survival game concept 'revealed'

Hat Tip to for news of "Lunar Survival," a "first-person survival adventure game with horror elements," developers frankly admit is barely 'a work in progress.'

"The gameplay is designed as a combination of survival-action, map quests, realistic Apollo mission technologies and various Moon mysteries. Players will need to take in consideration of the different technical aspects to pass missions, such as the amount of oxygen, electricity, stamina and the space suit temperature. Players will be able to repair, fix and build different mechanisms and upgrade their suit which will help them to spend more time on missions without coming back to the Lunar Space Module to recover."

Interesting how the concept Surveyor artifact features artfully edged and updated landing pods.

Perhaps someone in the community could help the developers out.

They might begin with the amazingly stubborn 'dark side and light side of the Moon' fallacy, before these guys embarrass themselves repeating what every Pink Floyd fan has accepted as false since 1973.

Some will laugh at the early stage vaporware feel to this concept, which seems to borrow heavily from Apollo 18 (2011),

Is it possible they totally missed that movie? Of course it is.

Still this game's development is, at least, claimed to be 'in progress' and is, therefore, making a better pace than Congress, for example

Sadly, none of this raises any hope that search results, using YouTube especially, will soon start to separate science from urban legend for those using criteria that includes 'NASA' or 'Apollo.'

Saturday, February 6, 2016

Edgar Mitchell (1930-2016)

Edgar Mitchell, sixth human to visit the lunar surface, takes a live panorama of the close horizon using the first color television camera successfully operated on the Moon; at Fra Mauro, south of Copernicus, February 1971. Photograph by Apollo 14 commander Alan Shepard [NASA/JSC].
Astronaut Edgar Mitchell, lunar module pilot on Apollo 14, passed away Thursday in West Palm Beach, Florida,  and on the eve of the 45th anniversary of his lunar expedition in 1971.

Mitchell joined Apollo 14 commander Alan Shephard, Jr., the first American in space, in the lunar module Antares, which touched down February 5, 1971, in the Fra Mauro highlands. Shepard and Mitchell were assigned to traverse the lunar surface to deploy scientific instruments and perform a communications test on the surface, as well as photograph the lunar surface and any deep space phenomena. It was Mitchell’s only spaceflight.

Mitchell and Shephard set mission records for the time of the longest distance traversed on the lunar surface; the largest payload returned from lunar surface; and the longest lunar stay time (33 hours). They were also the first to transmit color TV from the lunar surface. Mitchell helped collect 94 pounds of lunar rock and soil samples that were distributed across 187 scientific teams in the United States and 14 other countries for analysis.

Read the full NASA release HERE.

Tuesday, January 19, 2016

Re-entry debris traced to Lunar Prospector in '98

The highly-economical science probe Lunar Prospector mated to the payload assist module prior to launch in 1998. The  man-sized tran-lunar ejection module (Bottom)  may have made a fiery return to Earth, last year [NASA].
Traci Watson

The piece of space junk that made a fiery plunge into the Indian Ocean two months ago was most likely the remains of a rocket motor that propelled a NASA probe to the Moon in 1998, researchers studying the event have concluded.

The junk’s identity is by no means certain, but the “leading candidate” is the translunar injection module of Lunar Prospector, says Paul Chodas, an asteroid tracker at the CalTech/Jet Propulsion Laboratory in Pasadena, California. The module nudged the probe out of Earth orbit and then detached from the main spacecraft, which orbited the Moon for 19 months before it was deliberately slammed into the lunar south pole in July 1999.

Speculation about the source of the debris, known as WT1190F, ran rampant even before it plummeted through the atmosphere on 13 November. The only artificial object to make an uncontrolled re-entry at a precisely predicted place and moment, it presented a unique chance to witness such an event in real time. Researchers took advantage of the opportunity, monitoring the debris from a chartered jet as well as from ground-based observatories.

Catch the full article HERE.

Thorium concentrations in ppm, among the many elemental maps gather from data collected during the pioneering and economy-driven Lunar Prospector mission over its eighteen months in lunar orbit in 1998 and 1999 [Spudis/NASA].

After ISS, lunar 'village' is next -Woerner

For ESA's 3D-printed lunar base concept, Foster+Partners devised a weight-bearing ‘catenary’ dome design with a cellular structured wall to shield against micrometeoroids and space radiation, incorporating a pressurised inflatable to shelter astronauts [ESA/Foster & Partners].
Katherine Derla

European Space Agency's head Jan Woerner released the vision outline for the Moon Village, which could replace the International Space Station as early as 2030. The lunar village will be composed of structures created by 3D printers and robots using Moon dusts as raw materials.

Woerner became the ESA head in July 2015 and made the Moon mission the space agency's central project. Woerner added that this lunar project is a crucial step towards the future flight to Mars.

"I looked into the requirements I see for a project after ISS. As of today, I see the Moon Village as the ideal successor of the International Space Station for [space] exploration," said Woerner.

The Moon Village project could be a collaboration of several nations and space exploration groups including Russia, China, NASA and ESA. Experts around the world could contribute advanced technology, knowledge and even manpower (astronauts) for the Mars mission preparations. The same can be done for the ongoing biology and physics explorations that are currently being conducted onboard the ISS.

In 2014, the U.S. announced they intend to keep the ISS in operation until 2024, which pushed back the station's retirement by at least four years. Several European nations raised concerns over the extended operation's perceived costs, challenging if the extension would be worthwhile. On the other hand, Russia is considering the option of building its own space station.

Read the full-article HERE.

Wednesday, October 14, 2015

APOD: A Gegenschein Lunar Eclipse

Lunar Eclipse through elusive Gegenschein light from Namibia [Petr Horálek/NASA/APOD].
Explanation: Is there anything interesting to see in the direction opposite the Sun? One night last month, there were quite a few things. First, the red-glowing orb on the lower right of the original image is the full moon, darkened and reddened because it has entered Earth's shadow. Beyond Earth's cone of darkness are backscattering dust particles orbiting the Sun that standout with a diffuse glow called the gegenschein, visible as a faint band rising from the central horizon and passing behind the Moon. A nearly horizontal stripe of green airglow is also discernable just above the horizon, partly blocked by blowing orange sand. 

View of Petr Horálek's original "dark Namibian eclipse in the Gegenschein," featured NASA ASTRONOMY PICTURE of the DAY," October 14, 2015 [NASA/APOD/Petr Horálek].
Visible in the distant sky as the blue dot near the top of the image is the star Sirius, while the central band of our Milky Way galaxy arches up on the image left and down again on the right. 

The fuzzy light patches just left of center are the Large and Small Magellanic Clouds. Red emission nebulas too numerous to mention are scattered about the sky, but are labelled in a companion annotated image. In the image foreground is the desolate Deadvlei region of the Namib-Naukluft National Park in Namibia, featuring the astrophotographer himself surveying a land and sky so amazing that he described it as one of the top experiences of his life.
Context, by  Judy Schmidt.

Wednesday, August 5, 2015

Moon transit from DSCOVR

This animation features actual satellite images of the far side of the moon, illuminated by the sun, as it crosses between the DSCOVR spacecraft's Earth Polychromatic Imaging Camera (EPIC) and telescope, and the Earth - one million miles away [NASA/Goddard].

Friday, June 26, 2015

LADEE analysis maps lopsided meteoric dust cloud

Artist's conception of the lunar dust exosphere surrounding the moon. The color represents the amount of material ejected from the surface, showing a peak in the apex direction. A haze of dust is shown around the moon. Gray faded circles are overlaid on the lunar surface to represent the random nature of the primary impactors. An artist's conception of the LADEE orbital inclination is also shown [UC Boulder/Daniel Morgan/Jamey Szalay].
Darryl Waller
Sharon Lozano

New science results from NASA’s LADEE mission (Lunar Atmosphere and Dust Environment Explorer) indicate the Moon is regularly engulfed in a permanent, but lopsided and transitory, dust cloud increasing in density during encounters with cometary debris, like those producing the Geminids, according to a new study led by University of Colorado Boulder.

"Knowledge about the dusty environments in space has practical applications," said CU-Boulder physics Professor Mihály Horányi. "Knowing where the dust is and where it is headed in the solar system could help mitigate hazards for future human exploration, including dust particles damaging spacecraft or harming astronauts."

The cloud was discovered using data from a detector on board LADEE called the Lunar Dust Experiment (LDEX) designed and built by CU-Boulder. LDEX charted more than 140,000 impacts during the six-month survey launched in September 2013. NASA’s Ames Research Center in Moffett Field, California was responsible for spacecraft design, development, testing and mission operations.

“The LDEX team has been painstakingly analyzing their data since the LADEE mission ended on April 18, 2014,” said LADEE project scientist at Ames, Rick Elphic. “Their results answer one of the big LADEE science questions: is there a dust component to the tenuous lunar atmosphere?  And if so, why is it there?” 

According to Horányi, the cloud is primarily made up of tiny dust grains kicked up from the moon’s surface by the impact of high-speed, interplanetary dust particles. A single dust particle from a comet striking the moon’s surface lofts thousands of smaller dust specks into the airless environment, and the lunar cloud is maintained by this sometimes predictable process of regolith "gardening."

“Identifying this permanent dust cloud engulfing the moon was a nice gift from this mission,” said Horányi, the principal investigator for the LDEX instrument and lead author of the study. “We can carry these findings over to studies of other airless bodies, like the moons of other planets and the asteroids.”

Artist's composite showing LADEE spacecraft in close orbit [NASA/JAXA/LP].
A paper on the subject appears in the June 17 issue of Nature. Co-authors Jamey Szalay, Sascha Kempf, Eberhard Grun and Zoltan Sternovsky from CU-Boulder, Juergen Schmidt from the University Oulu in Finland, and Ralf Srama from the University of Stuttgart in Germany.

The first hints of a cloud of dust around the moon came in the late 1960s when cameras functioning overnight aboard the unmanned moon lander Surveyor 7 captured bright glow hours ahead of lunar sunrise. Not long after astronauts in lunar orbit described a significant glow above the lunar surface when approaching sunrise, phenomenon brighter than the sun by itself should have been able to produce over a body with only a trace, essentially non-existent, atmosphere.

Because these new findings do not square with the Apollo reports of a thicker, higher dust cloud, conditions back then may have been somewhat different. The dust on the moon -- which is dark and sticky and regularly dirtied the suits of moonwalking astronauts -- was created over several billion years as interplanetary dust particles incessantly pounded the rocky lunar surface.

Apollo 17 commander Gene Cernan's sketches and description of horizon glow and streamers observed in lunar orbit in December 1972 [NASA].
Many of the cometary dust particles impacting lunar surface are traveling at thousands of miles per hour in a retrograde, or counterclockwise orbit around the sun, the opposite orbital direction of the solar system’s planets. This causes high-speed, near head-on collisions with the dust particles and the moon’s leading surface as the Earth-moon system travel together around the sun.

Related LADEE Posts:
LADEE impact crater found (October 29, 2014)
First Science from LADEE (45th LPSC, March 18 2014)
LADEE's (star tracker) images of the Moon (February 14, 2014)
LADEE economy adds 28 days to mission (February 5, 2014)
LROC captures LADEE from 9,000 meters (January 30, 2014)
Red Moon, Blue Moon Dwayne DayThe Space Review (December 3, 2013)
LADEE begins collecting data (November 22, 2013)
LADEE transitioning out of commissioning phase (November 6, 2013)
Apollo 12 ALSEP first to measure dust accumulation (November 21, 2013)
Chang'e-3 & LADEE: The Role of Serendipity (October 31, 2013)
LADEE LLCD sets new data record (October 25, 2013)
Measuring almost nothing, looking for the almost invisible (October 16, 2013)
LADEE legacies (September 7, 2013)
LADEE Prelaunch Mission Briefing (September 6, 2013)
ESA prepares for LADEE (July 31, 2013)
LADEE arrives at Wallops Island (June 5, 2013)
LADEE ready to baseline dusty lunar exosphere (June 5, 2013)
First laser comm system ready for launch on LADEE (March 16, 2013)
LADEE project manager update (February 6, 2013)
The Mona Lisa test for LADEE communications (January 21, 2013)
Toxicity of lunar dust (July 2, 2012)
Expectations for the LADEE LDEX (March 23, 2012)
The Dust Management Project (August 9, 2010)
LADEE architecture and mission design (July 6, 2010)
DesertRatS testing electrodynamic dust shield (July 5, 2010)
Dust transport and its importance in the origin of lunar swirls (February 21, 2010)
Dust accumulation on Apollo laser reflectors may indicate a surprisingly fast and
more dynamic lunar exosphere
 (February 16, 2010)
NASA applies low cost lessons to LADEE (January 18, 2010)
Nanotech advances in lunar dust mitigation (August 19, 2009)
Moon dust hazard influenced by Sun's elevation (April 17, 2009)
LADEE launch by Orbital from Wallops Island (April 14, 2009)
Understanding the activation and solution properties of lunar dust
for future lunar habitation
 (March 2, 2009)
Respiratory toxicity of lunar highland dust (January 19, 2009)
Toxicological effects of moon dust (June 25, 2008)
Moon dust and duct tape (April 22, 2008)

Monday, June 22, 2015

Call for abstracts for Earth & Space 2016

Call for Abstracts:
Orlando, Florida
April 11-15, 2016

Abstracts are due July 15, 2015.

This is perhaps the premier conference on space resource utilization, space mining, granular mechanics in space, etc.  Springtime in Orlando figuring out how to extend human civilization into the solar system - what could be better?

Philip T. Metzger, Ph.D.
Planetary Physicist
University of Central Florida
Florida Space Institute
12354 Research Parkway
Partnership 1 Building, Suite 214
Orlando, FL 32826-0650
Twitter: @DrPhiltill
Space Resources Blog:

Monday, April 20, 2015

Astrobotic strives to be FedEx to the Moon

Astrobotic Griffin lunar lander and Red Rover LR. GLXP Hakuto team announced it has joined in their attempt to win the X-PRIZE contest, riding to the Moon atop a Falcon 9 booster [Astrobotic/CMU]. 
Tim Reyes

Astrobotic Technology, a leading Google Lunar X-PRIZE competitor, is setting up to become the first delivery service to the Moon.

With a low-cost launch, they now have a lander with the potential for precision landings driven by new system on a chip (SOC) technologies developed by Nvidia with help from General Electric.

Astrobotic knows that space and robotics are not that easy, but at a recent Nvidia-sponsored technology conference, the company’s engineers were presenting technologies that it argues could ease and accelerate the path to the Moon.

And the company is offering anyone — including their X-PRIZE competitors — a ride to the Moon. Safely on the surface they propose a civilized Mad Max road race to the finish line – 500 meters away –  the winner taking  the $20 million grand prize.

To date, only the Japanese team HAKUTO has joined them.

To make their moon mission a reality, the company is blending an interesting mix of old and new into their lander design, the Griffin Lander.

The new includes the Nvidia Tegra K1 chip used initially in its Jetson dev kit. The old is none other than General Electric designing the custom boards based on Tegra K1 and low-cost computer boards they hope will be recognized as a better, cheaper, alternative to existing radiation-hardened electronics costing millions. The Nvidia dev kit costs little more than $300.

Tapping their own wiz-kids from Carnegie-Mellon, Astrobotics is using laser-guided imagery that was developed to compete for the DARPA Grand Challenge for autonomous vehicles. For Astrobotic, the convergence of all of this tech is designed to get them beyond just the Google Lunar X-PRIZE but much more.

Read the featured article, HERE.

Monday, March 16, 2015

Mare Nubium impact with plume captured and analyzed

North is to the left, west below in this animation showing what is almost certainly an impact and its plume (right) on the lunar surface in Mare Nubium, on the morning side of the terminator, February 26 [Marco Iten/GLR Group].
Marco Iten
Raffaello Lena
Stefano Sposetti
Geological Lunar Research Group

Report from Selenology Today Preliminary Report 2015:

Abstract: We report the detection of an interesting luminous event most probably generated by a meteoroidal impact on the lunar surface occurred at 21h 35m 22.871s ± 0.010s UT, the 26 February 2015. The position of the flash was along the terminator at selenographic coordinates 7.9° ± 0.6° W; 26.1° ± 1.6° S. The brightness of the flash 0.16 s after the initial detection was +8.0 magV. After the main lightdrop a successive residual diffuse light lasted for several seconds.

Under the assumption of a meteoroidal impact we argue that this post luminous event and its ever growing dimensions was likely caused by the sunlight reflection on ejected materials released by the impact. Thus, future high resolution orbital data, e.g., from LRO spacecraft (NAC images) could allow the detection of this crater. Because this event was captured only by one observer, we checked for satellite glints and evaluated the likelihood of a meteor hitting head on our atmosphere.

1. Instruments observing methods, location The detection was made by Marco Iten from Gordola, Switzerland. He used a 125 mm refractor with a focal length of 800 mm. He also used an 8bit Watec 902H2 Ultimate videocamera working in CCIR mode with these settings: Gamma = OFF; BLC = OFF; AGC = LO. A GPS time inserter (KIWIOSD) printed the Universal Time with millisecond precision in the video frames. The software Virtualdub was used to record the AVI file in a hard disk, with Huffyuv video compressor.

Iten's observatory is located at:
Lat: 46d 10m 44s North
Long: 08h 52m 29s East
Alt: 215 m

Stefano Sposetti was simultaneously filming the Moon from its observatory, but the lunar region where the flash occurred was outside its field of view.

Detection: The initial flash occurred at 21:35:22.871 ± 0.010UT, 26 February 2015 (Fig. 1.). Marco Iten discovered it visually using no dedicated searching software.

Here some informations about the Moon at the detection instant, accordingly to sky simulator software TheSkySix ®.

Equatorial 2000:
RA: 05h 23m 27s
Dec: +17°44'32"

Azim: 250°41'00"
Alt: +41°21'54"

Phase (%): 62.19
Air mass: 1.51
Moon angular diameter: 0°30'33"
Moon distance (km): 3.910 E+05

Artificial satellites: We checked for artificial satellites in the field of view using the website

The satellite Molniya 340 (21196 1991022A) was at an angular distance of 32 arcmin from the Moon center at the time of the detection. We exclude that this satellite caused the detected flash in Iten's avi.

Luminosity evolution

From the very beginning of the event to +0.14 s (the first seven 20 msfieldintegrationtime) the intensity of all, or at least some, of the pixels is saturated. 

The luminosity of the flash at +0.16 s (in the eight field) is +8.0 ± 1.0 magV (Fig. 2). The intensity decreases again for about a half second. From that instant on, we notice an increase in the intensity of light and also an increase of the diameter of the source. The temporal evolution of the luminosity is showed in figure 3 and was made with the software Limovie©. 

For the photometry we used the star GSC 13002062 = TYC 130020621 with these characteristics:

B 10.97 ; V 9.54 ; R 8.88. The star was visible at 20:25:20 UT.

Information about that star were extracted from website

The peak brightness of the flash was between +5 and +6 magV, but this is a very rough estimation because of the saturated pixels at that instant. The solar elevation on the impact point was determined to 0.9°, computed using the LTVT software package by Mosher and Bondo (©2006) for the date February 26 2015 at 21h 35m 22.871s. Thus, the flash occurred in the dark side near the terminator.

Spatial increase of the light source

The angular sampling of the individual images composing the video file is 2.4 arcsec/pixel. We noticed a non circular increase of the light source, therefore we calculated its augmentation with respect to x and y components (Fig. 4). The apparent radius of the Moon is almost parallel to the x axis.

At the location of the event, the absolute sampling of the image (normal to the moon radius, ie. of the y axis), is 4.5 km/pixel (on the lunar surface). The absolute sampling of the image in the x direction has to be multiplied by a factor 1.24 (= 1/sin 54°) i.e. to 5.6 km/pixel.

At time +6.62 s the x and y diameter of the external border of the “lightcloud” are about 10 pixels and 12 pixels, respectively. This translates to an effective length on the lunar surface of 54 km and 56 km.

If we assume that the increase of the light source is due to the ejected materials elevated from the bottom and if this cloud has a circular shape relative to a tangent plane to the surface, then the mean speed of the augmenting radius is about 4 km/s.

The increase of the lightsource is showed in figure 5 and in some animations we posted at

A visual inspection of the “lightcloud” in the video animation confirms that the expansion lasted until +10s. This translates to a circular effective diameter of about 80 km.

Selenographic Lunar coordinates

The coordinates of the detected flash are determined to:

Long: 7.9° ± 0.6° West
Lat: 26.1° ± 1.6° South

in Mare Nubium, near the crater Lippershey P, located to the south of Birt crater.

The analyzed image displays lunar features that were of very low contrast on the dark limb of the imaged lunar surface. Thus, after alignment with the edge of the lunar disk, computation of the libration, and overlay of the rotated Moon's surface matching the image generated by a simulated image obtained with the LOLA DEM, a coordinate map was superimposed. This procedure was performed using the LTVT software package by Mosher and Bondo (2006). Generating an elevation map of a part of the lunar surface requires its three dimensional (3D) reconstruction. Recently, a global lunar digital elevation map (DEM) obtained with the Lunar Orbiter Laser Altimeter (LOLA) instrument on the Lunar Reconnaissance Orbiter (LRO) spacecraft has been released. It has a lateral resolution of 1/64 degrees or about 500 m in the equatorial regions of the Moon

Hence, the rendered image obtained using LTVT and the LOLA DEM, assuming the same illumination conditions and librations of the observing session, was saturated allowing a close comparison with the appearance of the saturated terminator as seen in Fig. 2, and further refined considering the uncertainty comparing the map with the WAC imagery of the Lunar Reconnaissance Orbiter.

Active Meteor Showers

Figure 6 shows the active meteor showers accordingly to the predictions of the software Lunarscan©. Because of the small activity of the showers at that date, we think of a sporadic nature of the meteor shower. 

Evaluating the possibility of an headon meteor strike

We report this luminous event as an “unconfirmed lunar flash” being considered an impact candidate. In fact, considering that the event was only recorded by one video camera the possibility of a meteor "headon" producing the recorded light cannot be ruled out. Therefore we tried to evaluate the post spread of light as being emitted by the ionization of the high altitude gases of our atmosphere. Sometimes luminous meteors leave luminous trails and in this chapter we try to discard this possibility. We got the direction of the winds and their speed using the website published by the University of Wyoming©. Here we could download data from balloons sent from Milan (LIML) and from Payerne (LSMP), the 2 nearest stations from Iten's observatory at 12h intervals (00h and 12h). The balloons reach about 30 km of height. At that altitude and also some kilometers higher, the direction of the winds during the time interval between Feb 26.5 and Feb 27.0 is around 270 deg and their speed from 30 to 40 knots (LIML data) and from 30 to 99 knots (LSMP data). Projecting the wind speed along the normal direction of the line of sight, one gets, with a conservative wind speed of 18 m/s in the interval of 6.6 s, a drift of about 350 arcsec. This is about 12 times more than the drift in East direction of the “lightcloud” in the same interval. The western direction of the winds cannot explain the drift of the “lightcloud” in almost a circular shape. Hence we confidentially exclude that the drift of the “lightcloud” was caused by winds at 30 km height.

Size of the probable impactor and of the produced crater

In this study, and under the assumption of an impact event, the same formalism and equations as in the works by Bellot Rubio et al. (2000), Ortiz et al. (2000), Ortiz et al. (2002), and Carbognani (2000) was followed, including the kinetic energy that is translated into impactor mass assuming a typical sporadic impactor speed. According to the statistics of a large meteoroid orbit database (Steel, 1996) this speed is approximately 20.2 km s1 on Earth and 16.9 km s1 on the Moon, after correcting for the different escape velocities of the Earth and the Moon.

Moreover a short routine provided by Melosh and Beyer (1999) was used to evaluate the scaling equations to determine the diameter of a crater given details on the nature of the projectile, conditions of impact, and state of the target. The transient crater diameter is evaluated by three independent methods, yield scaling, piscaling and Gault's semiempirical relations supplemented by rules on how crater size depends on gravity and angle of impact.

The parameters used in the calculation are the projectile density, the target density (2700 kg m3), the impact velocity (16.9 km s1), the peak brightness (5.5 MagV) and the duration of 0.22 seconds. Using the luminous efficiency η = 2 x 103 (the nominal value determined from Leonid impact flashes, e.g., Bellot Rubio et al., 2000; Ortiz et al., 2002), the mass of the impactor would be 1.1 kg. Based on the above data and assuming a spherical projectile, the diameter of the impactor was inferred to be approximately between 9 and about 20 cm considering a bulk density ranging between 0.3 g cm3 (soft cometary material) to 3.7 g cm3 (corresponding to ordinary chondrites). This impactor would strike the target with an impact energy of 1.7 x 108 Joules (4.0 x 108 MegaTons). If the meteoroid is associated as a sporadic source, the impact angle is unknown. We have used the most likely angle of 45° to estimate the size of the crater produced by the impact.

Using the Piscaled law for transient craters, the final crater would be a simple crater with a rim to rim diameter of about 1520 m. 

However, considering that the brightness of the detected flash was saturated and the described presence of a luminous post event, the values inferred for the mass of the probable impactor and the crater size originated by the impact could be considerably higher.

Future high resolution orbital data, e.g., from LRO spacecraft (NAC images) could allow the detection of this crater. Hence, it will be interesting to compare LRO high resolution images (NAC images with their resolution of ~1 m on the ground) taken before and after the event. Future studies will be performed to complete our analysis, including the search of the crater, and thus to estimate mass of impact produced dust cloud and the size of exospheric dust particles and to perform hydrodynamic modeling of this event.


Data about winds are obtained in collaboration with Meteoswiss

We thank the Wyoming University for the source winds data set


[1] Sposetti, S., Iten, M., Lena, R. 2011. Detection of a meteoroidal impact on the Moon. Selenology Today 23,132.

[2] Lena, R., Iten, M., Sposetti, S., 2011. Detection of three meteoroidal impact on the Moon. Selenology Today 24,1229.

[3] Lena, R., Iten, M., Sposetti, S., 2011. Detection of two probable meteoroidal impacts on the Moon. Selenology Today 25,6065.

[4] Iten, M.,Lena, R., Sposetti, S., 2013. Five probably meteoroids impact on the Moon. Selenology Today 31,1015.

[5] Lena, R., Manna, A., Sposetti, S., 2013. Detection of a probable small meteoroidal impact on the Moon. Selenology Today 33,49.

[6] Bellot Rubio, L.R., Ortiz, J.L., Sada, P.V., 2000. Observation and interpretation of meteoroid impact flashes on the Moon. Earth Moon Planets 82–83, 575–598.

[7] Carbognani, A.2000. Impatti sulla Luna

[8] Steel, D., 1996. Meteoroid orbits. Space Sci. Rev. 78, 507–553.

[9] Ortiz, J.L., Sada, P.V., Bellot Rubio, L.R. et al. (2000) Optical detection of meteoroidal impacts on the moon. Nature 405. 921923.

[10] Ortiz, J.L., Quesada, J.A., Aceituno, J., Aceituno, F.J., Bellot Rubio, L.R. 2002. Observation and interpretation of Leonid impact flashes on the Moon in 2001. Astrophys. J. 576. 567–573.

[11] Melosh, H.J., and Beyer, R. A. 1999. Computing Crater Size from Projectile Diameter.

[12] Mosher, J., & Bondo, H., 2006. Lunar Terminator Visualization Tool (LTVT). 

Monday, March 2, 2015

Understanding the legal status of the Moon

Astrobotic (CM) Moon Digger concept [Mark Maxwell/Astrobotic/JAXA].
Urbano Fuentes
The Space Review

In 1969, the United States successfully performed the first human landing on the surface of the Moon. Neil Armstrong and Buzz Aldrin placed an American flag in the lunar surface, winning the space race against the Soviet Union. The US government stated later that no sovereignty claims of any kind were made on the Moon. After that historical breakthrough and for decades to come, space exploration suffered a considerable slowdown. The United States had won the space race, and no serious efforts have since been made by any nation to return to the Moon.

In 1985, researchers at the University of Wisconsin discovered that the lunar soil had a considerable amount of the rare isotope of helium known as helium-3 (He-3). This scarce element could be used in energy production, in fusion power plants that—hypothetically—could produce an amount equivalent to 130,000,000 barrels of oil per ton of He-3.1 . It is also environmentally friendly, producing no greenhouse gases or radiation.

Whether because of helium-3 or not, several nations have recently shown interest in returning to the Moon. In 2013, China became the third country to land a spacecraft on the Moon, and other nations have places for lunar missions in the next several years. Besides nations, several private corporations had expressed interest in lunar missions of one kind or another.

Law in this area is not particularly broad. Nevertheless, during the Cold War and because of the progress in the field of space exploration in those early years, some international treaties related to the legal status of the Moon and the outer space region arose, creating a legal regime that is still valid today. Those treaties are the Outer Space Treaty (1967) and the Moon Treaty (1979), currently the existing legal framework valid to some extent.

These treaties, while overlapping to some degree, settled a series of principles regarding human activities outside Earth. The Outer Space Treaty forbids the placement of weapons of mass destruction in space; it also addressed the situation of lunar sovereignty, claiming that the celestial bodies could not be subject of national appropriation. The later Moon Treaty established that the Moon shall be regarded as common heritage of mankind, in a similar regime as the one applicable to the Deep Sea Bed Area.

This essay will address primarily the legal status of the Moon, using the existing framework on the subject. Taking into account the current state of space exploration and other legal systems similar to the one of the Moon, such as the Deep Sea Bed Area, it will analyse the question of whether the Moon could be considered the Common Heritage of Mankind, or if some other legal concept should be used in relation to its resources.

Read the full essay in The Space Review, HERE.

Friday, February 27, 2015

Review: the Moon as 'blue water port' to the stars

Moonscraper 2040 - Honorable Mention: 2011 Skyscraper Competition [Luis Quinones].
Jessica Guenzel
Phys Org

"Crotts' new book, titled The New Moon: Water, Exploration, and Future Habitation, explores his innovative ideas and many more in meticulous detail, providing hard scientific findings that topple decades-old ideas about the moon's development and structure. Readers may well wonder why the U.S. abandoned its lunar exploration program in 2010, just as so many discoveries were emerging.

"Today, we know that billions of tons of water exist on the moon in the form of ice, and Crotts is sure that more will be found. It's not likely the kind of H2O earthlings drink but rather one rich in heavy water—or deuterium oxide—a form of water in which the hydrogen atom's nucleus is double the mass of ordinary hydrogen, rendering it undrinkable by humans without processing.

"Crotts believes the moon's water could be broken down into liquid hydrogen and liquid oxygen, a potent mix that makes an ultra-efficient form of rocket fuel, the same kind that powered the NASA Saturn V rockets that boosted the Apollo spaceships out of Earth's atmosphere towards the moon.

"You'd have to look hard to find another propellant that's as efficient or better," said Crotts. The moon also has carbon monoxide that Crotts said could be converted with water into methane, another efficient and powerful rocket fuel.

"With all that potential rocket fuel, Crotts naturally believes that the moon could one day be transformed into an interplanetary gas station for the satellites and rockets that today get discarded because they eventually run out of fuel and drift into the wrong orbit."

Read the full review, HERE.

Wednesday, February 25, 2015

Lunar Orbiter Image Restoration Project: Last Mile

Until the original tapes were found, stored in an abandoned McDonalds Restaurant on site at Ames Research Center, and subsequently read and remastered using totally unavailable equipment built from scratch, this represents our best view of of the rugged slopes of the central peaks of Copernicus crater, a facsimile of a photograph developed in lunar orbit and radioed back to Earth from Lunar Orbiter V, August 17, 1967. For comparison, see the photographs that follow below [USGS]. 
From moonandback video, May 2010
Dennis Wingo

The Lunar Orbiter Image Recovery Project (LOIRP) is a public/private project to recover, from the original master tapes, the image data from the five spacecraft NASA sent to the moon in the 1960’s and provide it to the scientific community and the public.  The first is done through a peer review process and then the data is provided to the National Space Science Data Center (NSSDC) for archiving.  We also have a public website through NASA at the Solar System Exploration Research Virtual Institute (SSERVI) at the NASA Ames Research Center.  This missive is to explain the background of the mission, the character of the data, and why it is important to our scientific and national history.

At this time we have completed over 90% of the work necessary to archive and publish these images.  However, sometimes that last 10% is the hardest and we have in the dozens of terabytes of data to complete the processing of our image captures.  Why doesn't NASA pay for this?  They have paid for the vast majority of our work.  NASA’s Space Science Mission Directorate, NASA Ames, and and SSERVI have been magnificent in support of our work.  However, NASA’s budget is severely constrained, and for legacy projects like this, it is our work in technoarchaeology (literally the archaeology of technology) that is saving this data for posterity.

Field of view captured in by Lunar Orbiter V in 1967, shown in the image further above, outlined on a more recent photographic survey by the Lunar Reconnaissance Orbiter (LRO), LROC M181302109R, spacecraft orbit 11832, January 15, 2012 [NASA/GSFC/Arizona State University].
When we started this project, it was only to save the images of Lunar Orbiter’s II and III.  However, in 2011 NASA asked us how much it would cost to complete all five orbiters.  We estimated $400,000.  NASA provided $300,000 of this, leaving a gap of $100,000.  This is why we ask for your support in our crowdfunding effort, to complete this task.  These images, provided on the SSERVI website, will be free to the public with no copyright.  The American taxpayer paid for this effort and even though our company has also contributed materially to the effort and we are extending this through your generous donations through crowdfunding, we want this to be provided free of charge, or any intellectual property right restrictions.

Detail from LOIRP Lunar Orbiter V (Image 151-H1 -Copernicus Central Uplift) The LOIRP Image was derived from the original analog tapes from the LO ground stations and has 4x the dynamic range of the LO film archive. This image with a resolution of about 2 meters, taken on August 16, 1967 from 103 km. This version of the LO-V-151-H image is from the original ground station tape from the Woomera ground station in Australia (tape W5-58).
NASA had stored these original analog data tapes for over four decades, but if it were not for our project and former NASA archivist Nancy Evan’s preservation of the tape drives in her barn, this archive at its best quality would be lost to history.  Following is a description of the Lunar Orbiters, their camera, the images and what we are doing to preserve this legacy of the early Apollo program.

Background on the Lunar Orbiter

In 1966-67 NASA sent five spacecraft to the Moon to do a high resolution photo reconnaissance of the surface in preparation for the manned Apollo lunar landings.  This was the first time in human history, other than a few closeups before impact from the Ranger spacecraft, that the moon had been seen up close and personal.

Enjoy the full post from Dennis Wingo, HERE.

Related Posts:
The LOIRP time machine looks back 43 years (June 3, 2010)
New releases from Lunar Orbiter II (1966) - (May 7, 2010)
Boulders of Copernicus (December 11, 2009)
LOIRP: Boulder Trails on the Moon (December 10, 2009)
Lunar Orbiter's originals vs. LOIRP restorations (December 9, 2009)
New restored detail from Lunar Orbiter II (December 8, 2009)
LOIRP configures second FR-900 tape drive (November 12, 2009)
The importance of lunar water (September 28, 2009)
LOIRP remasters the Moon's South Pole (August 14, 2009)
Lockheed Martin donates Clean-Room to LOIRP (August 12, 2009)
LOIRP astounds again, re-release of LO-II0162 (1967)
with each of three high-res sub-frames
 (August 10, 2009)
Full Earth, as seen by Orbiter V (August 7, 2009)
Lunar Orbiter III-154-H2 (June 16, 2009)
LOIRP recovers Lunar Orbiter IV lunar South Pole image from 1967 (June 16, 2009)
LOIRP recovers detail of Fra Mauro and future landing site of Apollo 14 (June 11, 2009)
New LOIRP high res Lunar Orbiter image of western Oceanus Procellarum (June 10, 2009)
LOIRP recovers image of Ranger 8 impact (June 9, 2009)
LOIRP's "Pictures of the Century" (March 23, 2009)
More astounding new detail from LOIRP (February 26, 2009)
Breakthrough in Lunar Orbiter photograph remastering (February 20, 2009)

Tuesday, February 24, 2015

Astrobotic, Hakuto team up to ride Falcon 9 to Moon

The combined strategy utilizes the Astrobotic "Griffin" lander (carrying their "Red Rover," in foreground) to deploy a total of three robotic rovers, including the Hakuto "Tetris" and "Moonraker" [Astrobotic/CM].
Angela Moscaritolo

Two rivals battling it out in Google's $30 million competition to land a private spacecraft on the moon are teaming up for a joint trip to the lunar surface.

Hakuto, the only Japanese team competing in Google's Lunar XPrize competition, and Pittsburgh-based Astrobotic on Monday announced they are partnering for a moon journey during the second half of 2016.

Hakuto rover Moonraker (and back-up) undergoing hazard and slope avoidance testing in 2014 [Tim Stevens/C|NET].
The plan is that Hakuto's twin rovers — dubbed "Moonraker" and "Tetris" — will "piggyback" on Astrobotic's so-called "Griffin" lander to reach the moon.

Hatuto sub-rover Tetris [Tim Stevens/C|NET].
Astrobotic will launch the mission next year on a SpaceX Falcon 9 rocket from Cape Canaveral, Fla. After touching down, Hakuto's rovers will be simultaneously released alongside Astrobotic's "Andy" rover, developed by Carnegie Mellon University.

Read the full story HERE.

Additional story at Pittsburgh Business Times, HERE.

Astrobotic Technology Red Rover design concept, picked by Popular Science as one of 100 Best Innovations of 2011.