Showing posts with label NASA ESMD. Show all posts
Showing posts with label NASA ESMD. Show all posts

Saturday, March 9, 2013

New 3D CLSE lunar flyover video: Schrödinger basin


David A. Kring, Ph.D.
Center for Lunar Science & Exploration (CLSE)


The Center for Lunar Science and Exploration added another video to its Atlas of Lunar Flyovers. In this new addition, we explore the floor of the Schrodinger basin.The direct link to the new flyover is HERE.

The Moon’s Schrödinger basin is the best preserved impact basin of its size.  Its broad flat floor offers several safe landing sites and the geology within the basin is extraordinary.  The two highest science priorities and over half of the science objectives outlined in the National Research Council (NRC) report The Scientific Context for Exploration of the Moon (2007) can be addressed with field studies and samples collected in Schrödinger basin.

Schrödinger basin CLSE landing study 'Site B' (yellow ellipse), well within the 10 km safety 'walk-back' distance of the an unnamed 6.8 km Copernican Age crater that presumably excavated deep into the basin's intact peak rings, depositing valuable samples near the crater rim. (Further details on this site will be the subject of a future post.) The site, in context with the larger basin, is marked with a yellow arrow below. LROC Wide Angle Camera (WAC) monochrome (643nm) observation M169698283C, LRO orbit 10142, September 3, 2011; angle of incidence 72.67° at 81.3 meters resolution, from 58.66 km [NASA/GSFC/Arizona State University].
The video highlights three features in the basin.  It begins with a flight along a fracture in the basin floor towards an immense volcanic vent of pyroclastic material.  Because of the in situ resource utilization (ISRU) potential of the pyroclastic material, this vent was a target of the Exploration Systems Mission Directorate (ESMD) portion of the Lunar Reconnaissance Orbiter (LRO) mission.

The notably darker material surrounding Schrödinger basin's distinctive pyroclastic vent. Another landing site (green arrow, in an image showing the entire basin interior floor) is proposed near upper center right in this oblique LROC Narrow Angle Camera (NAC) field of view. LROC NAC mosaic M121415248LR, LRO orbit 3026, February 21, 2010; angle of incidence 81.66° (spacecraft slew -65.65° off nadir) rough resolution 3.7 meters from 53 km [NASA/GSFC/Arizona State University].
The flyover then turns towards the towering and mountainous peak ring that contains rock exposures of material uplifted from the mid- to lower-crust by the basin-forming impact event.  The flyover then sweeps back towards the pyroclastic vent over an intervening plain of melt-bearing impact lithologies.  Samples of that material can be used to determine the age of the Schrödinger basin and, thus, help test the lunar cataclysm hypothesis.

Related Posts:
Amundsen crater: CLSE lunar landing site study (February 5, 2013)
Scarps in Schrödinger (September 28, 2011)
Sampling Schrödinger (August 17, 2011)
A review of all things Schrödinger (August 31, 2010)
LOLA: Schrödinger basin (July 17, 2010)
Craters on the Schrödinger pyroclastic cone (April 24, 2010)

LROC WAC 100 meter monochrome global mosaic shows the 312 km-wide Schrödinger basin, a prominent feature of the far southern far side latitudes and stand out increasingly as a location where many high-priority lunar exploration science goals might be accomplished. The area includes smooth and rough plains, basin wall material, hummocky terrain, intact peak rings, mare, dark explosive volcanic material and ridged terrain. CLSE Landing Site Study Site A (green arrow) and Site B (yellow arrow) are shown at much higher resolution in the images further above [NASA/GSFC/Arizona State University].

Thursday, September 16, 2010

Two major LRO milestones marked by LROC


The recent release of the LROC Wide Angle Camera mosaic of the Moon's eastern hemisphere inspired Moon watchers to pour over a view filled with objects both unfamiliar as well as features that, even if familiar, are impossible to see from the same angle from Earth. On the eastern edge of Mare Australe a feature briefly caught our attention. In the long shadows appeared what seemed to be a classic volcano, around 46.57°S, 113.89°E.


A Third Release of LROC images to the Planetary Data System (PDS), September 16, did not immediately provide any new Narrow Angle Camera observations of this "cone's crater," other than previously released close-ups of its high-angled slopes. But two newly Wide Angle Camera views from June 2010 did show the feature, most likely a worn crater perched on what remains of an equally worn ring of mountains surrounding the Australe basin. (Looks like good skiing in Narrow Angle Camera views.) - LROC Observation M130896509M, LRO orbit 4423, June 11, 2010; alt. 54.7 km, resolution 76.68 meters [NASA/GSFC/Arizona State University].

Mark Robinson
Principal Investigator
Lunar Reconnaissance Orbiter Camera
Arizona State University


The LROC Team delivers third archive volume to the PDS, more than 68,000 new images are now available, and September 16 marks the transition of the LRO mission from NASA's Exploration Systems Mission Directorate to NASA's Science Mission Directorate.

LROC Team Releases 3rd EDR and CDR Archive Volume

The third LROC release contains 68,992 EDR products, totaling 8.1 TBytes of images and ancillary files. The majority of the images were taken between March 16, 2010 to June 15, 2010. This release also contains images acquired on the dates: 2010-02-06, 2010-02-24, 2010-02-25, 2010-03-03, 2010-03-04, and 2010-03-05.

The 3rd CDR volume contains 69,091 CDR products, totaling 17.0 TBytes of images and ancillary files. The majority of images were taken between March 16, 2010 to June 15, 2010. There are also images taken on the dates: 2009-06-30 to 2009-12-31, 2010-02-06, 2010-02-24, 2010-02-25, 2010-03-03, 2010-03-04, and 2010-03-05 represented in the volume.

Total number of LROC EDR products released to date: 225,903 for a total 28.2 TBytes of images and ancillary files.

Total number of LROC CDR products released to date: 225,428, for a total of 55 TBytes of images and ancillary files.

Explore the new images on LROC's browse page.

ESMD to SMD Transition

September 16 marks the transition of the LRO mission from NASA's Exploration Systems Mission Directorate (ESMD) to NASA's Science Mission Directorate (SMD). Throughout the first phase of LRO's mission the spacecraft collected vast amounts of science data in support of NASA's exploration goals. The transition simply means that LRO science data will now support NASA's science goals. What does this transition mean in practice? For the most part the transition will be relatively seamless, with only a re-prioritization of special targeted observations. For example, the Constellation Regions of Interest will drop in priority and other high science value targets will have their priority raised.

The bottom line: LRO will continue to collect a bonanza of lunar science data.

LRO transitions from exploration to science


Images of the Apollo 11 landing site from the Lunar Reconnaissance Orbiter clearly show the descent stage, the footprints of Armstrong & Aldrin and various equipment they deployed in July 1969 (including Buzz Aldrin's brief stroll to the edge of the crater east of the lunar module Eagle. Beyond the usefulness to science, LRO's first images of all six manned landing sites provide a poignant reminder of the manned lunar exploration legacy of the United States. Before the close-orbiting precision supporting the LRO Narrow Angle Camera operated by Arizona State University, this clear evidence of human activity on the Moon remained just beyond the camera resolutions of unmanned cameras in the decades since the Apollo orbital mapping cameras. At less than one half meter per pixel resolution, the LROC NAC clearly reveal not simply the LM descent stages of the six Apollo mission but lunar rover tracks and the foot paths of the twelve astronauts who explored the lunar surface between 1969 and 1972 [NASA/GSFC/ASU].

Michael Braukus
NASA HQ

Nancy Neal Jones
NASA GSFC

The United States' Lunar Reconnaissance Orbiter (LRO) will complete the exploration phase of its mission on September 16, after a series of successes that added to the transformation of our understanding of Earth's nearest neighbor.

LRO completed a year-long exploration mission in a nearly circular polar orbit approximately 54 kilometers above the Moon's surface, comprehensively mapping the lunar surface in unprecedented detail, searching for resources and safe landing sites and measuring surface temperatures and radiation levels.

LRO's attentions will now turn from exploration objectives to scientific research as program management moves from NASA's Exploration Systems Mission Directorate (ESMD) to the Science Mission Directorate at the agency's headquarters in Washington.

"LRO has been an outstanding success," said Doug Cooke, associate administrator of the ESMD. "The spacecraft has performed brilliantly, and LRO science and engineering teams achieved all mission's objectives. The incredible data LRO gathered will provide discoveries about the moon for years to come."

LRO teams operating its instruments will continue forwarding data gathered during the last year to the Planetary Data System (PDS), which archives and distributes scientific information from NASA planetary missions, astronomical observations and laboratory measurements.


Thirty-five meter boulder among a sea of detail previously unseen in the two Constellation Regions of Interest on the Moon's Aristarchus Plateau. From LROC principal investigator Mark Robinson's report to the Third Annual NASA Lunar Science Institute Conference (Presentation - 17.5 mg PDF) [NASA/GSFC/Arizona State University].

By the time LRO achieves full mission success in March 2011, with data processed and released to the scientific community, it will have sent more information to the Planetary Data System than all previous planetary missions combined.

During its new phase of discovery, LRO will continue to map the moon for two to four more years.

"The official start of LRO's science phase should write a new and intriguing chapter in lunar research," said Ed Weiler, associate administrator for the Science Mission Directorate.

LRO was launched from Kennedy Space Center carrying a suite of seven instruments, June 18, 2009. After an initial Commissioning phase, LRO formally began a highly detailed survey of the Moon the following September.

Among results collected thus far from the mission are original observations of the Apollo landing sites; indications that permanently shadowed and nearby regions harbor water and hydrogen and other volatiles; observations that large areas in the permanently shadowed regions are colder than anywhere in the Solar System; detailed information about lunar terrain, and the first evidence of a globally distributed population of thrust faults, evidence the Moon has recently contracted and may still be shrinking.

Among other achievements, LRO captured high resolution pictures of Lunokhod 1, the first robotic lunar rover the Soviet Union used to explore withing Mare Imbrium in 1970, subsequently lost for nearly 40 years.

The rover was located to within 30 meters using the LROC Narrow Angle Camera, and this highly accurate position data enabled researchers to captured laser light bounced and clearly reflected back again from the French-built retro-reflector situated on the dormant Soviet lunar rover for the first time. This addition to the long incomplete laser reflector array left on the Moon by the U.S. and U.S.S.R. during the Apollo era should finally enable a precision in Earth-Moon distance measurements to within 3 cm, a target some cosmologists hope will aid in answering questions about "locality" of physical laws in the universe.

LRO also supported the Lunar Crater Observation and Sensing Satellite (LCROSS) impact, as the companion mission was sued to determined if the Moon's permanently shadowed craters harbor water ice, to select the Cabeus crater impact site and to observe the wispy fast expanding plume and to study an evolving temperature at the site soon after the LCROSS impact last October 9.


The previously eternally elusive comprehensive details of the "permanently darkened regions" inside and around the Moon's south pole, situated on the rim of 10 km-wide Shackleton crater. Though aspects of Shackleton interior were first unveiled by Japan's SELENE-1 (Kaguya), the suite of instruments on LRO are singularly equipped to eventually detail the entire Moon's surface, whether by Sun or starlight [Maria Zuber/NLSI/LOLA].

NASA's Goddard Space Flight Center (GSFC) in Greenbelt, Maryland built and will continue to manage LRO for the Exploration Systems Mission Directorate.

Michael Braukus - michael.j.braukus@nasa.gov
Nancy Neal Jones - nancy.n.jones@nasa.gov

Thursday, August 19, 2010


America's Lunar Reconnaissance Orbiter (LRO) was launched from Kennedy Space Center, June 18, 2009 and commenced it's Nominal Mission phase the following September. Since then LRO has orbited the Moon 5,300 times and will soon have returned more data to Earth than all previous (and on-going) Deep Space missions, combined. Though investigators will sift through this treasure for decades to come, LRO has already become a central player in a revolution in our understanding of Earth's nearest neighbor in Space.

Tuesday, January 26, 2010

NASA's first lunar outpost plan (1992)

Beyond Apollo - Noted recorder of NASA's notions of yesterday, David S.F. Portree offers a no-nonsense post covering the 1992 lunar outpost plans that crashed upon the shoals of the first Augustine commission, and ultimately Congress.

David S. F. Portree
Beyond Shuttle

The Exploration Program Office at NASA's Johnson Space Center in Houston, Texas, launched the First Lunar Outpost (FLO) study in December 1991 by establishing six study teams. In June 1992, the JSC Systems Engineering Division and McDonnell Douglas-Houston developed FLO Crew Lander and Habitat flight plans to aid the FLO Mission Design and Analysis Team.

For their analysis, JSC and McDonnell targeted the first FLO expedition to Mare Smythii, a dark basaltic plain on the moon's eastern limb. They assumed that NASA would develop a heavy-lift rocket capable of launching 200 metric tons to 185-kilometer low-Earth orbit and 27 metric tons to the lunar surface. The monster launcher would permit the two FLO landers to be launched with their respective Trans-Lunar Injection (TLI) stages attached, eliminating Earth-orbital rendezvous and docking and reliance on an Earth-orbiting space station from the FLO plan. In other words, this FLO iteration would use the Direct Ascent lunar mission mode considered - and rejected - for Apollo moon missions. The first FLO expedition would leave Earth five years after program initiation; JSC and McDonnell judged this to be "not only feasible and attractive, but essential in gaining budget acceptance."

Read the full posting HERE.

Wednesday, August 26, 2009

Lunabotics Mining Competition @ KSC

The purpose of the Lunabotics Mining Competition is to engage and retain students in science, technology, engineering, and mathematics, or STEM, in a competitive environment that may result in innovative ideas and solutions, which could be applied to actual lunar excavation for NASA.

Eligibility
Undergraduate and graduate student teams enrolled in a U.S. college or university are eligible to enter the inaugural Lunabotics Mining Competition.

Design teams must include:

  • One faculty or industry advisor with a college or university affiliation
  • Two or more undergraduate or graduate students
A group of universities also may work in collaboration on an excavator project entry. Multidisciplinary teams are encouraged. Collaborations between majority institutions and minority serving institutions are encouraged. Corporate sponsorship is allowed. Get information on available excavator project funding by NASA

NASA Exploration Systems Mission Directorate
Higher Education Project
in partnership with the
National Space Grant College and Fellowship Program
is proud to announce the inaugural
Lunabotics Mining Competition
May 25-28, 2010
Astronaut Hall of Fame
Kennedy Space Center, Florida

NASA KSC Posting, HERE.

Wednesday, August 5, 2009

Exploration Systems Mission Directorate launches new website

NASA’s Exploration Systems Mission Directorate is developing the concepts and technologies that will be needed to travel to and from the moon and sustain a human presence there.

Because NASA field centers do not have terrain similar to the lunar surface, the agency conducts analog tests in remote field locations. At these locations teams of scientists, engineers and astronauts test robotic equipment, vehicles, habitats, communications, and power generation and storage. They evaluate mobility, infrastructure and effectiveness in the harsh environments.

Test locations include the Antarctic region, oceans, deserts, and arctic and volcanic environments.

Last month, the Pavilion Lake Research Project (Pavilion Lake, Ontario, Canada) and the Haughton Mars Project (Devon Island, Nunavut, Canada) kicked off the 2009 series of exploration analog missions; and later this fall, the Desert RATS team will trek into the deserts of Arizona.

You can stay connected with current and upcoming analog research teams through Blogs, Flickr, Facebook, Twitter, and YouTube, all available through the analogs website, HERE.