Artemis II Crew Trains for Emergency Scenarios Ahead of Moon Mission

Artemis II Crew Trains for Emergency Scenarios Ahead of Moon Mission

Two astronauts in orange spacesuits and helmets sit horizontal with their feet raised in a mockup of the Orion spacecraft. The feet of two other astronauts are above them on the left. All are assisted by a man in a beige hat.
Credit: NASA/James Blair

The four Artemis II astronauts practiced procedures to exit the Orion spacecraft in an emergency during training at NASA’s Johnson Space Center in Houston on Dec. 15. NASA astronaut Christina Koch (foreground) and CSA (Canadian Space Agency) astronaut Jeremy Hansen were assisted by Bill Owens, Artemis II spacesuit technician. The training included exiting both the side and top hatches of the spacecraft to ensure the crew will be ready for potential emergency scenarios upon splashdown in the Pacific Ocean that would require them to leave the capsule before the recovery team arrives. The Artemis II mission will send the crew on an approximately 10-day flight test around the Moon. Under Artemis, NASA will return humans to the Moon for long-term exploration and scientific discovery.

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Rachel H. Kraft

Site-Wide Environmental Assessment for Marshall Space Flight Center, Alabama

Site-Wide Environmental Assessment for Marshall Space Flight Center, Alabama

1 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Notice of Availability. The Draft Site-Wide Environmental Assessment (EA) for Marshall Space Flight Center is complete and NASA determined the project will not result in significant environmental impacts. Therefore, a Draft Finding of No Significant Impact (FONSI) has been prepared. Both documents are available for public review and comment for the next thirty (30) days.

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Dec 19, 2023

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MSFC Environmental Engineering and Occupational Health Office
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Hannah McCarty

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Dec 19, 2023

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MSFC Environmental Engineering and Occupational Health Office
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John R. Tapp

NASA to Co-Host Stability and Control Prediction Workshop

NASA to Co-Host Stability and Control Prediction Workshop

2 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A scale model of a typical airliner is seen mounted on a stand inside a NASA wind tunnel
A NASA-developed wind tunnel research tool known as the Common Research Model is seen mounted in the 12-Foot Low-Speed Tunnel at the agency’s Langley Research Center in Virginia.
NASA / Lee Pollard

NASA will co-host the two-day Stability and Control Prediction Workshop II (S&CPW2) during the American Institute of Aeronautics and Astronautics’ (AIAA) annual SciTech Forum in January 2025.

A kickoff meeting for the 2025 gathering is scheduled for Jan. 8, 2024, during the AIAA SciTech 2024 Forum in Orlando, Fla.

The Stability and Control Prediction Workshop series seeks to establish best practices for the prediction of stability and control derivatives with computational fluid dynamics (CFD). The workshops provide an impartial forum for evaluating the effectiveness of existing CFD codes and modeling techniques, as well as identifying areas in need of additional research and development.

The focus of S&CPW2 is prediction of static and dynamic stability derivatives for the NASA/Boeing Common Research Model (CRM).

NASA’s Langley Research Center in Virginia collected static and force oscillation data for a 2.4-percent scale version of the CRM in the Langley 12-Foot Low-Speed Tunnel during the Fall of 2023.

The wind tunnel data will be used to provide a blind comparison to CFD predictions. The data will not be publicly released until CFD predictions for the workshop have been completed.

S&CPW2 will be open to participants worldwide, and representation from industry, academia, and government will be present.

The workshop will consist of individual presentations, open discussions, and a subsequent paper by the planning committee to document workshop results. Participation in the prediction studies and AIAA membership are not required to attend the workshop.

The Organizing Committee consists of the following members:

  • Andrew Lofthouse – Air Force Lifecycle Management Center
  • Dan Vicroy – Adaptive Aerospace Group, Inc.
  • Benjamin Simmons – NASA Langley Research Center
  • Norman Princen – The Boeing Company
  • Matthew Prior – The Boeing Company
  • Adam Clark – The Boeing Company
  • Brett Johnson – The Boeing Company
  • Steve Klausmeyer – Textron Aviation
  • Kelly Laflin – Textron Aviation
  • William Vogel – Air Force Lifecycle Management Center
  • Charlie Harrison – Gulfstream Aerospace Corporation

The workshop’s planning is affiliated with NASA’s Transformational Tools and Technologies project.

For more information and to receive links to CFD geometry files in advance of the workshop, please contact Benjamin Simmons at benjamin.m.simmons@nasa.gov.

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John Gould

John Gould

Aeronautics Research Misson Directorate

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Dec 19, 2023

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Jim Banke
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Jim Banke

Telescopes Illuminate ‘Christmas Tree Cluster’

Telescopes Illuminate ‘Christmas Tree Cluster’

This composite image shows the Christmas Tree Cluster. The blue and white lights (which blink in the animated version of this image) are young stars that give off X-rays detected by NASA’s Chandra X-ray Observatory. Optical data from the National Science Foundation’s WIYN 0.9-meter telescope on Kitt Peak shows gas in the nebula in green, corresponding to the “pine needles” of the tree, and infrared data from the Two Micron All Sky Survey shows foreground and background stars in white. This image has been rotated clockwise by about 160 degrees from the astronomer’s standard of North pointing upward, so that it appears like the top of the tree is toward the top of the image.
X-ray: NASA/CXC/SAO; Optical: T.A. Rector (NRAO/AUI/NSF and NOIRLab/NSF/AURA) and B.A. Wolpa (NOIRLab/NSF/AURA); Infrared: NASA/NSF/IPAC/CalTech/Univ. of Massachusetts; Image Processing: NASA/CXC/SAO/L. Frattare & J.Major

This new image of NGC 2264, also known as the “Christmas Tree Cluster,” shows the shape of a cosmic tree with the glow of stellar lights. NGC 2264 is, in fact, a cluster of young stars — with ages between about one and five million years old — in our Milky Way about 2,500 light-years away from Earth. The stars in NGC 2264 are both smaller and larger than the Sun, ranging from some with less than a tenth the mass of the Sun to others containing about seven solar masses.

This new composite image enhances the resemblance to a Christmas tree through choices of color and rotation. The blue and white lights (which blink in the animated version of this image) are young stars that give off X-rays detected by NASA’s Chandra X-ray Observatory. Optical data from the National Science Foundation’s WIYN 0.9-meter telescope on Kitt Peak shows gas in the nebula in green, corresponding to the “pine needles” of the tree, and infrared data from the Two Micron All Sky Survey shows foreground and background stars in white. This image has been rotated clockwise by about 160 degrees from the astronomer’s standard of North pointing upward, so that it appears like the top of the tree is toward the top of the image.

This composite image shows the Christmas Tree Cluster. The blue and white lights (which blink in the animated version of this image) are young stars that give off X-rays detected by NASA’s Chandra X-ray Observatory. Optical data from the National Science Foundation’s WIYN 0.9-meter telescope on Kitt Peak shows gas in the nebula in green, corresponding to the “pine needles” of the tree, and infrared data from the Two Micron All Sky Survey shows foreground and background stars in white. This image has been rotated clockwise by about 160 degrees from the astronomer’s standard of North pointing upward, so that it appears like the top of the tree is toward the top of the image.

Young stars, like those in NGC 2264, are volatile and undergo strong flares in X-rays and other types of variations seen in different types of light. The coordinated, blinking variations shown in this animation, however, are artificial, to emphasize the locations of the stars seen in X-rays and highlight the similarity of this object to a Christmas tree. In reality the variations of the stars are not synchronized.

The variations observed by Chandra and other telescopes are caused by several different processes. Some of these are related to activity involving magnetic fields, including flares like those undergone by the Sun — but much more powerful — and hot spots and dark regions on the surfaces of the stars that go in and out of view as the stars rotate. There can also be changes in the thickness of gas obscuring the stars, and changes in the amount of material still falling onto the stars from disks of surrounding gas.

NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.

Read more from NASA’s Chandra X-ray Observatory.

For more Chandra images, multimedia and related materials, visit:

https://www.nasa.gov/mission/chandra-x-ray-observatory/

Visual Description:

This release features a composite image of a cluster of young stars looking decidedly like a cosmic Christmas tree! The cluster, known as NGC 2264, is in our Milky Way Galaxy, about 2,500 light-years from Earth. Some of the stars in the cluster are relatively small, and some are relatively large, ranging from one tenth to seven times the mass of our Sun.

In this composite image, the cluster’s resemblance to a Christmas tree has been enhanced through image rotation and color choices. Optical data is represented by wispy green lines and shapes, which creates the boughs and needles of the tree shape. X-rays detected by Chandra are presented as blue and white lights, and resemble glowing dots of light on the tree. Infrared data show foreground and background stars as gleaming specks of white against the blackness of space. The image has been rotated by about 150 degrees from the astronomer’s standard of North pointing upwards. This puts the peak of the roughly conical tree shape near the top of the image, though it doesn’t address the slight bare patch in the tree’s branches, at our lower right, which should probably be turned to the corner.

In this release, the festive cluster is presented as both a static image, and as a short animation. In the animation, blue and white X-ray dots from Chandra flicker and twinkle on the tree, like the lights on a Christmas tree.

News Media Contact

Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998

Jonathan Deal
Marshall Space Flight Center
Huntsville, Ala.
256-544-0034

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Lee Mohon

NASA Invites Public to Share Excitement of Astrobotic, ULA Robotic Artemis Moon Launch

NASA Invites Public to Share Excitement of Astrobotic, ULA Robotic Artemis Moon Launch

Teams with Astrobotic install the NASA meatball decal on Astrobotic’s Peregrine lunar lander on Tuesday, Nov. 14, 2023, at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida.
NASA/Isaac Watson

NASA is inviting the public to take part in virtual activities ahead of Astrobotic’s Peregrine Mission One, launching on a United Launch Alliance (ULA) Vulcan rocket as part of NASA’s Commercial Lunar Payload Services (CLPS) initiative. The mission is slated to be one of the first United States commercial robotic landers launching to the Moon’s surface as part of the agency’s Artemis program.

Carrying NASA and commercial payloads, the Peregrine lander is scheduled to lift off no earlier than Monday, Jan. 8, from Space Launch Complex 41 at the Cape Canaveral Space Force Station in Florida.

Members of the public can register to attend the launch virtually. As a virtual guest, you have access to curated resources, schedule changes, and mission-specific information delivered straight to your inbox. Following each activity, virtual guests will receive a commemorative stamp for their virtual guest passport.

The live launch broadcast will air on Monday, Jan. 8, and will air on NASA+, NASA Television, the NASA app, and the agency’s website. Learn how to stream NASA TV through a variety of platforms including social media.

For more information about CLPS activities, follow the CLPS blog.

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Amanda S. Vozeh