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Nathan Tuggy
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How will Bennu's volatile compounds stay cool and unmodified by the heat of re-entry (ORSIRISOSIRIS-REx)?

Watching the video in this NYTimes article NASA Aims at an Asteroid Holding Clues to the Solar System’s Roots I realized for the first time how the samples actually make it back to Earth.

The chemical composition of the organic and volatile compounds is of great interest for this mission for many reasons. So I would think that it is important to avoid thermally induced chemical reactions, migration, and or redistribution of the compounds within the sample matrix. If it gets hotter than it does while on Bennu, the science may be compromised.

note: According to the text in this excellent Asteroid Missions animation near the end, the re-entry velocity will start at about 12.4 km/sec. See also OSIRIS-REx Press Kit.

From hereWikipedia's article on OSIRIS-REx:

Return and analyze a sample of pristine carbonaceous asteroid regolith in an amount sufficient to study the nature, history, and distribution of its constituent minerals and organic material.

Is the re-entry kept shallow to avoid peak external temperatures, or is it deep and rapid to "get it over with" before heat can diffuse through (presumably) a lot of insulation?

Screen shots from the NYTimes video:

frame from NYTimes videoframe from NYTimes video at 1:45

frame from NYTimes videoframe from NYTimes video at 2:03

frame from NYTimes videoframe from NYTimes video at 2:12

frame from NYTimes videoframe from NYTimes video at 2:25

frame from NYTimes videoframe from NYTimes video at 2:38

frame from NYTimes videoframe from NYTimes video at 2:39

How will Bennu's volatile compounds stay cool and unmodified by the heat of re-entry (ORSIRIS-REx)?

Watching the video in this NYTimes article NASA Aims at an Asteroid Holding Clues to the Solar System’s Roots I realized for the first time how the samples actually make it back to Earth.

The chemical composition of the organic and volatile compounds is of great interest for this mission for many reasons. So I would think that it is important to avoid thermally induced chemical reactions, migration, and or redistribution of the compounds within the sample matrix. If it gets hotter than it does while on Bennu, the science may be compromised.

note: According to the text in this excellent Asteroid Missions animation near the end, the re-entry velocity will start at about 12.4 km/sec. See also OSIRIS-REx Press Kit

From here:

Return and analyze a sample of pristine carbonaceous asteroid regolith in an amount sufficient to study the nature, history, and distribution of its constituent minerals and organic material.

Is the re-entry kept shallow to avoid peak external temperatures, or is it deep and rapid to "get it over with" before heat can diffuse through (presumably) a lot of insulation?

Screen shots from the NYTimes video:

frame from NYTimes video

frame from NYTimes video

frame from NYTimes video

frame from NYTimes video

frame from NYTimes video

frame from NYTimes video

How will Bennu's volatile compounds stay cool and unmodified by the heat of re-entry (OSIRIS-REx)?

Watching the video in this NYTimes article NASA Aims at an Asteroid Holding Clues to the Solar System’s Roots I realized for the first time how the samples actually make it back to Earth.

The chemical composition of the organic and volatile compounds is of great interest for this mission for many reasons. So I would think that it is important to avoid thermally induced chemical reactions, migration, and redistribution of the compounds within the sample matrix. If it gets hotter than it does while on Bennu, the science may be compromised.

note: According to the text in this excellent Asteroid Missions animation near the end, the re-entry velocity will start at about 12.4 km/sec. See also OSIRIS-REx Press Kit.

From Wikipedia's article on OSIRIS-REx:

Return and analyze a sample of pristine carbonaceous asteroid regolith in an amount sufficient to study the nature, history, and distribution of its constituent minerals and organic material.

Is the re-entry kept shallow to avoid peak external temperatures, or is it deep and rapid to "get it over with" before heat can diffuse through (presumably) a lot of insulation?

Screen shots from the NYTimes video:

frame from NYTimes video at 1:45

frame from NYTimes video at 2:03

frame from NYTimes video at 2:12

frame from NYTimes video at 2:25

frame from NYTimes video at 2:38

frame from NYTimes video at 2:39

Tweeted twitter.com/StackSpaceExp/status/773888562655887360
minor misspelling of organic++
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Watching the video in this NYTimes article NASA Aims at an Asteroid Holding Clues to the Solar System’s Roots I realized for the first time how the samples actually make it back to Earth.

The chemical composition of the organic &and volatile compounds is of great interest for this mission for many reasons. So I would think that it is important to avoid thermally induced chemical reactions, migration, and or redistribution of the compounds within the sample matrix. If it gets hotter than it does while on Bennu, the science may be compromised.

note: According to the text in this excellent Asteroid Missions animation near the end, the re-entry velocity will start at about 12.4 km/sec. See also OSIRIS-REx Press Kit

From here:

Return and analyze a sample of pristine carbonaceous asteroid regolith in an amount sufficient to study the nature, history, and distribution of its constituent minerals and organic material.

Is the re-entry kept shallow to avoid peak external temperatures, or is it deep and rapid to "get it over with" before heat can diffuse through (presumably) a lot of insulation?

Screen shots from the NYTimes video:

enter image description hereframe from NYTimes video

enter image description hereframe from NYTimes video

enter image description hereframe from NYTimes video

enter image description hereframe from NYTimes video

enter image description hereframe from NYTimes video

enter image description hereframe from NYTimes video

Watching the video in this NYTimes article NASA Aims at an Asteroid Holding Clues to the Solar System’s Roots I realized for the first time how the samples actually make it back to Earth.

The chemical composition of the organic & volatile compounds is of great interest for this mission for many reasons. So I would think that it is important to avoid thermally induced chemical reactions, migration, and or redistribution of the compounds within the sample matrix. If it gets hotter than it does while on Bennu, the science may be compromised.

note: According to the text in this excellent Asteroid Missions animation near the end, the re-entry velocity will start at about 12.4 km/sec. See also OSIRIS-REx Press Kit

From here:

Return and analyze a sample of pristine carbonaceous asteroid regolith in an amount sufficient to study the nature, history, and distribution of its constituent minerals and organic material.

Is the re-entry kept shallow to avoid peak external temperatures, or is it deep and rapid to "get it over with" before heat can diffuse through (presumably) a lot of insulation?

Screen shots from the NYTimes video:

enter image description here

enter image description here

enter image description here

enter image description here

enter image description here

enter image description here

Watching the video in this NYTimes article NASA Aims at an Asteroid Holding Clues to the Solar System’s Roots I realized for the first time how the samples actually make it back to Earth.

The chemical composition of the organic and volatile compounds is of great interest for this mission for many reasons. So I would think that it is important to avoid thermally induced chemical reactions, migration, and or redistribution of the compounds within the sample matrix. If it gets hotter than it does while on Bennu, the science may be compromised.

note: According to the text in this excellent Asteroid Missions animation near the end, the re-entry velocity will start at about 12.4 km/sec. See also OSIRIS-REx Press Kit

From here:

Return and analyze a sample of pristine carbonaceous asteroid regolith in an amount sufficient to study the nature, history, and distribution of its constituent minerals and organic material.

Is the re-entry kept shallow to avoid peak external temperatures, or is it deep and rapid to "get it over with" before heat can diffuse through (presumably) a lot of insulation?

Screen shots from the NYTimes video:

frame from NYTimes video

frame from NYTimes video

frame from NYTimes video

frame from NYTimes video

frame from NYTimes video

frame from NYTimes video

minor misspelling of organic had to add a couple things to get around the 6 char edit limit
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Watching the video in this NYTimes article NASA Aims at an Asteroid Holding Clues to the Solar System’s Roots I realized for the first time how the samples actually make it back to Earth.

The chemical composition of the orgainic andorganic & volatile compounds is of great interest for this mission for many reasons. So I would think that it is important to avoid thermally induced chemical reactions and, migration/redistribution, and or redistribution of the compounds within the sample matrix. If it gets hotter than it does while on Bennu, the science may be compromised.

note: According to the text in this excellent Asteroid Missions animation near the end, the re-entry velocity will start at about 12.4 km/sec. See also OSIRIS-REx Press Kit

From here:

Return and analyze a sample of pristine carbonaceous asteroid regolith in an amount sufficient to study the nature, history, and distribution of its constituent minerals and organic material.

Is the re-entry kept shallow to avoid peak external temperatures, or is it deep and rapid to "get it over with" before heat can diffuse through (presumably) a lot of insulation?

Screen shots from the NYTimes video:

enter image description here

enter image description here

enter image description here

enter image description here

enter image description here

enter image description here

Watching the video in this NYTimes article NASA Aims at an Asteroid Holding Clues to the Solar System’s Roots I realized for the first time how the samples actually make it back to Earth.

The chemical composition of the orgainic and volatile compounds is of great interest for this mission for many reasons. So I would think that it is important to avoid thermally induced chemical reactions and migration/redistribution of the compounds within the sample matrix. If it gets hotter than it does while on Bennu, the science may be compromised.

note: According to the text in this excellent Asteroid Missions animation near the end, the re-entry velocity will start at about 12.4 km/sec. See also OSIRIS-REx Press Kit

From here:

Return and analyze a sample of pristine carbonaceous asteroid regolith in an amount sufficient to study the nature, history, and distribution of its constituent minerals and organic material.

Is the re-entry kept shallow to avoid peak external temperatures, or is it deep and rapid to "get it over with" before heat can diffuse through (presumably) a lot of insulation?

Screen shots from the NYTimes video:

enter image description here

enter image description here

enter image description here

enter image description here

enter image description here

enter image description here

Watching the video in this NYTimes article NASA Aims at an Asteroid Holding Clues to the Solar System’s Roots I realized for the first time how the samples actually make it back to Earth.

The chemical composition of the organic & volatile compounds is of great interest for this mission for many reasons. So I would think that it is important to avoid thermally induced chemical reactions, migration, and or redistribution of the compounds within the sample matrix. If it gets hotter than it does while on Bennu, the science may be compromised.

note: According to the text in this excellent Asteroid Missions animation near the end, the re-entry velocity will start at about 12.4 km/sec. See also OSIRIS-REx Press Kit

From here:

Return and analyze a sample of pristine carbonaceous asteroid regolith in an amount sufficient to study the nature, history, and distribution of its constituent minerals and organic material.

Is the re-entry kept shallow to avoid peak external temperatures, or is it deep and rapid to "get it over with" before heat can diffuse through (presumably) a lot of insulation?

Screen shots from the NYTimes video:

enter image description here

enter image description here

enter image description here

enter image description here

enter image description here

enter image description here

added 222 characters in body
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