Lunar Mission

Media Invited to See NASA’s Orion Crew Module for its Journey to Mars

Posted on Updated on

January 20, 2016
MEDIA ADVISORY M16-005

*** NOTE: Press release are usually published under that page “Media Releases (Information for Journalist).” These press releases are usually meetings or presentation of studies. The public will most of the time have access to view or listen to most of these, but only credentialed media can ask question.

Also, before the meeting documentation may be made available, sometimes weeks before the meeting. If the documents are embargoed, we in the press know that means the information cannot be published before the embargo date and time. We use the time to pre-write our stories and prepare questions, but the embargo must be honored by all.

–  George McGinn, Examining Life (And Things of Interest), Daily Defense News and Cosmology and Space Exploration news websites.


Orion’s pressure vessel was completed Jan. 13, 2016 at NASA’s Michoud Assembly Facility in New Orleans. The pressure vessel is the spacecraft’s underlying structure on which all of the spacecraft’s systems and subsystems are built and integrated. (Credit: NASA)

 

NASA’s Orion crew module will be available to media at two NASA locations Jan. 26th and in early February, as engineers continue to prepare the spacecraft to send astronauts deeper into space than ever before, including to an asteroid placed in lunar orbit and on the journey to Mars.

At 10:30 a.m. EST on Tuesday, Jan. 26, the agency’s Michoud Assembly Facility in New Orleans will host a media viewing and facility tour of the spacecraft’s recently completed pressure vessel, the underlying structure of the crew module, before it ships to NASA’s Kennedy Space Center in Florida.

To attend the event at Michoud, reporters must contact Chip Howat at 504-257-0478 or carl.j.howat@nasa.gov by 3 p.m. Monday, Jan. 25. International media accreditation for this event is closed.

The Orion pressure vessel provides a sealed environment for astronaut life support in future human-rated crew modules. Technicians at Michoud began welding together the seven large aluminum pieces of Orion’s primary structure in precise detail last September. At Kennedy, Orion will be outfitted with the spacecraft’s systems and subsystems, processed and integrated with NASA’s Space Launch System (SLS) ahead of their first joint exploration mission, or EM-1.

Michoud also is where the massive core stage of SLS is being manufactured. Reporters will be able to view tooling and newly manufactured hardware for SLS, and hear about mission progress from personnel across NASA.

Individuals available for interviews during the tour include:

  • Bill Hill, deputy associate administrator for Exploration Systems Development at NASA Headquarters in Washington
  • Mike Sarafin, EM-1 mission manager at NASA Headquarters
  • Mark Kirasich, Orion program manager at NASA’s Johnson Space Center in Houston
  • Scott Wilson, Orion production manager at Kennedy
  • John Honeycutt, SLS program manager at the agency’s Marshall Space Flight Center in Huntsville, Alabama
  • Steve Doering, SLS core stage manager at Marshall
  • Mike Bolger, Ground Systems Development and Operations program manager at Kennedy
  • NASA astronaut Rick Mastracchio
  • Mike Hawes, Orion program manager for Lockheed Martin
  • Jim Bray, crew module director for Lockheed Martin 

Orion will depart Michoud on or about Feb. 1 and travel to Kennedy aboard NASA’s Super Guppy airplane. Additional details for Orion’s arrival at Kennedy, including media accreditation, are forthcoming.

For more information about Orion, visit: http://www.nasa.gov/orion

-end- 

 

NASA’s LRO Spacecraft Finds March 17, 2013 Impact Crater and More

Posted on Updated on

 

NOTE: This post was in pending and should have been published. This was an issue we had in the beginning by updating the blog via e-mail. Although it is late, the information in this article is important and interesting – George.

NASA’s Lunar Reconnaissance Orbiter (LRO) acquired images of the lunar surface before and after the largest recorded explosion occurred on the surface.

On March 17, 2013, an object the size of a small boulder hit the surface in Mare Imbrium and exploded in a flash of light nearly 10 times as bright as anything ever recorded before.

This bright flash was recorded by researchers at NASA’s Marshall Space Flight Center in Huntsville with coordinates 20.6°N, 336.1°E.

The Lunar Reconnaissance Camera (LROC) scientists were able to obtain observations before and after the impact.

<youtube>Video of the LROC</youtube>

Comparing the actual size of the crater to the brightness of the flash helps validate impact models.

LROC’s first set of post-impact flash images acquired on May 21, 2013 by the Narrow Angle Camera (NAC) were targeted on the Marshall-reported coordinates and numerous small surface disturbances (“splotches”) were detected by comparing the pre- and post-flash images, but no new crater was found.

A second set of NAC images was acquired on July 1, 2013, showing three faint ray-like features and several chains of splotches and asymmetric splotches that generally pointed to a common area west of the Marshall coordinates. A NAC pair was targeted on that convergence point for July 28, 2013; comparison of this third set of images with preexisting coverage revealed a new crater.

 Before and After Images

LROC close-up image of the moon from Feb. 12, 2012
LROC close-up image of the moon from July 28, 2013, showing an impact crater created on March 17 of that year
lt-small.pngrt-small.png  The crater itself is small, measuring 18.8 meters (61.7 feet) in diameter, but its influence large; debris excavated by the sudden release of energy flew for hundreds of meters. More than 200 related superficial changes up to 30 kilometers (19 miles) away were noted.

The results are published in the January 31 edition of the journal Icarus.

The March 17 impact crater is one of thousands of craters being mapped by the instrument. The LROC team is going back to images taken in the first year or two and comparing them to recent images. Called temporal pairs, these before/after images enable the search for a range of surface changes, including new impact craters, formed between the time the first and second image were acquired.

As of January 1, 2015, LROC has acquired about 10,000 before and after image pairs.

Launched on June 18, 2009, LRO has collected a treasure trove of data with its seven powerful instruments, making an invaluable contribution to our knowledge about the moon. LRO is managed by NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for the Science Mission Directorate at NASA Headquarters in Washington.

To download the visualizations of these impacts, visit:
http://svs.gsfc.nasa.gov/goto?4242

To read more about the March 17, 2013, impact crater, visit LROC’s website:
http://lroc.sese.asu.edu/posts/770