Template:Featured article - Revision history

Strangelv: 14 revisions imported

2019-04-08T23:03:46Z

14 revisions imported

← Older revision		Revision as of 16:03, 8 April 2019
(No difference)

lunarp>Strangelv: JSC-1

2011-09-20T14:06:40Z

JSC-1

← Older revision		Revision as of 07:06, 20 September 2011
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	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[~~Moon Zoo~~]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[JSC-1]]===
	[[Image:~~Moon Zoo Logo~~.~~gif~~\|160px\|left]] ~~Moon Zoo is~~ a ~~crowdsourcing project from~~ the ~~Zooniverse community that uses images from~~ the ~~Lunar Reconnaissance Orbiter~~.		[[Image:EIC050-2.GIF\|160px\|left]] JSC-1, a lunar soil simulant, was developed and characterized under the auspices of the NASA Johnson Space Center. This simulant was produced in large quantities to satisfy the requirements of a variety of scientific and engineering investigations. JSC-1 is derived from volcanic ash of basaltic composition, which has been ground, sized, and placed into storage. The simulant's chemical composition, mineralogy, particle size distribution, specific gravity, angle of internal friction, and cohesion have been characterized and fall within the ranges of lunar mare soil samples. ...([[JSC-1\|read more]])

	~~Activities include counting craters~~, ~~noting blocky craters~~, and ~~checking relative differences between boulder-producing craters~~, and...([[~~Moon Zoo~~\|read more]])
	<DIV style="text-align:right">		<DIV style="text-align:right">
	<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>		<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>

lunarp>Strangelv: sp

2010-05-11T17:32:56Z

← Older revision		Revision as of 10:32, 11 May 2010
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	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Moon Zoo]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Moon Zoo]]===
	[[Image:Moon Zoo Logo.gif\|160px\|left]] Moon Zoo is a crowdsourcing project from the Zooniverse community that uses images from the Lunar ~~Reconnasaince~~ Orbiter.		[[Image:Moon Zoo Logo.gif\|160px\|left]] Moon Zoo is a crowdsourcing project from the Zooniverse community that uses images from the Lunar Reconnaissance Orbiter.

	Activities include counting craters, noting blocky craters, and checking relative differences between boulder-producing craters, and...([[Moon Zoo\|read more]])		Activities include counting craters, noting blocky craters, and checking relative differences between boulder-producing craters, and...([[Moon Zoo\|read more]])

lunarp>Strangelv: Moon Zoo

2010-05-11T17:16:09Z

Moon Zoo

← Older revision		Revision as of 10:16, 11 May 2010
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	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[~~Geologic Processes on the Moon/Cratering on the Moon\|Cratering on the~~ Moon]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Moon Zoo]]===
	[[Image:~~GP1Fig_3~~.~~jpg~~\|160px\|left]] ~~Craters cover the surface of the moon and are the result of hyper-velocity impacts by meteorites. The velocity of meteorites upon impact varies, but is generally between 10 and 40 km/sec. This number~~ is a ~~combination of~~ the ~~‘approach velocity’ and~~ the ~~‘escape velocity~~.~~’ The approach velocity of objects refers to the velocity of the object with respect to the moon. This varies with the type of object (for example~~, ~~long period comets generally have a higher approach velocity than short period comets)~~ and ~~the direction with which it approaches the moon (for example~~, ~~if it approaching the moon ‘head on,’ it will have a higher approach velocity than~~...([[~~Geologic Processes on the Moon/Cratering on the~~ Moon\|read more]])		[[Image:Moon Zoo Logo.gif\|160px\|left]] Moon Zoo is a crowdsourcing project from the Zooniverse community that uses images from the Lunar Reconnasaince Orbiter.

			Activities include counting craters, noting blocky craters, and checking relative differences between boulder-producing craters, and...([[Moon Zoo\|read more]])
	<DIV style="text-align:right">		<DIV style="text-align:right">
	<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>		<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>

lunarp>Jarogers2001: /* Featured article: Volatiles */

2008-11-02T05:23:01Z

Featured article: [[Volatiles]]

← Older revision		Revision as of 22:23, 1 November 2008
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	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[~~Volatiles~~]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Geologic Processes on the Moon/Cratering on the Moon\|Cratering on the Moon]]===
	[[Image:~~Apollo11Soil~~.jpg\|160px\|left]] ~~The primary resource~~ of ~~value to humans on~~ the ~~Moon is~~ the ~~volatile components found in the [[regolith]]~~. ~~These are all the components that are gases at room temperature~~. ~~Most~~ of the ~~volatiles have been deposited in~~ the ~~top layers~~ of the ~~Moon's surface by~~ the ~~[[solar wind]] over geologic time. A notable exception~~ to ~~this is [[Argon]]~~. the ~~concentration~~ of ~~Argon in lunar soil is much~~ higher than ~~found in~~ the ~~solar wind~~, ~~so must come from~~ a ~~different source~~. ~~Especially, the isotope Argon-40~~. ~~It is presently believed that the Argon-40 comes from radioactive decay of~~ [[~~Potassium]] and~~/~~or [[Krypton]] deep within~~ the ~~lunar mantle or core([[Volatiles~~\|read more]])		[[Image:GP1Fig_3.jpg\|160px\|left]] Craters cover the surface of the moon and are the result of hyper-velocity impacts by meteorites. The velocity of meteorites upon impact varies, but is generally between 10 and 40 km/sec. This number is a combination of the ‘approach velocity’ and the ‘escape velocity.’ The approach velocity of objects refers to the velocity of the object with respect to the moon. This varies with the type of object (for example, long period comets generally have a higher approach velocity than short period comets) and the direction with which it approaches the moon (for example, if it approaching the moon ‘head on,’ it will have a higher approach velocity than...([[Geologic Processes on the Moon/Cratering on the Moon\|read more]])
	<DIV style="text-align:right">		<DIV style="text-align:right">
	<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>		<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>

lunarp>Jarogers2001: /* Featured article: Volatiles */

2008-08-05T11:58:42Z

Featured article: [[Volatiles]]

← Older revision		Revision as of 04:58, 5 August 2008
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	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Volatiles]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Volatiles]]===
	[[Image:Apollo11Soil.jpg\|160px\|left]] The primary resource of value to humans on the Moon is the volatile components found in the [[regolith]]. These are all the components that are gases at room temperature. Most of the volatiles have been deposited in the top layers of the Moon's surface by the [[solar wind]] over geologic time. A notable exception to this is [[Argon]]. the concentration of Argon in lunar soil is much higher than found in the solar wind, so must come from a different source. Especially, the isotope Argon-40. It is presently believed that the Argon-40 comes from radioactive decay of [[Potassium]] and/or [[Krypton]] deep within the lunar mantle or core~~, and that the Argon-40 seeps out to the surface via fissures. This vented~~([[Volatiles\|read more]])		[[Image:Apollo11Soil.jpg\|160px\|left]] The primary resource of value to humans on the Moon is the volatile components found in the [[regolith]]. These are all the components that are gases at room temperature. Most of the volatiles have been deposited in the top layers of the Moon's surface by the [[solar wind]] over geologic time. A notable exception to this is [[Argon]]. the concentration of Argon in lunar soil is much higher than found in the solar wind, so must come from a different source. Especially, the isotope Argon-40. It is presently believed that the Argon-40 comes from radioactive decay of [[Potassium]] and/or [[Krypton]] deep within the lunar mantle or core([[Volatiles\|read more]])
	<DIV style="text-align:right">		<DIV style="text-align:right">
	<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>		<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>

lunarp>Jarogers2001: /* Featured article: Volatiles */

2008-08-05T11:58:03Z

Featured article: [[Volatiles]]

← Older revision		Revision as of 04:58, 5 August 2008
Line 1:		Line 1:
	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Volatiles]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Volatiles]]===
	[[Image:Apollo11Soil.jpg\|160px\|left]] The primary resource of value to humans on the Moon is the volatile components found in the [[regolith]]. These are all the components that are gases at room temperature. Most of the volatiles have been deposited in the top layers of the Moon's surface by the [[solar wind]] over geologic time. A notable exception to this is [[Argon]]. the concentration of Argon in lunar soil is much higher than found in the solar wind, so must come from a different source. Especially, the isotope Argon-40. It is presently believed that the Argon-40 comes from radioactive decay of [[Potassium]] and/or [[Krypton]] deep within the lunar mantle or core, and that the Argon-40 seeps out to the surface via fissures. This vented ~~Argon enter the lunar atmosphere; then the Argon is implanted into the regolith by~~([[Volatiles\|read more]])		[[Image:Apollo11Soil.jpg\|160px\|left]] The primary resource of value to humans on the Moon is the volatile components found in the [[regolith]]. These are all the components that are gases at room temperature. Most of the volatiles have been deposited in the top layers of the Moon's surface by the [[solar wind]] over geologic time. A notable exception to this is [[Argon]]. the concentration of Argon in lunar soil is much higher than found in the solar wind, so must come from a different source. Especially, the isotope Argon-40. It is presently believed that the Argon-40 comes from radioactive decay of [[Potassium]] and/or [[Krypton]] deep within the lunar mantle or core, and that the Argon-40 seeps out to the surface via fissures. This vented([[Volatiles\|read more]])
	<DIV style="text-align:right">		<DIV style="text-align:right">
	<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>		<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>

lunarp>Jarogers2001: /* Featured article: Volatiles */

2008-08-05T11:56:59Z

Featured article: [[Volatiles]]

← Older revision		Revision as of 04:56, 5 August 2008
Line 1:		Line 1:
	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Volatiles]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Volatiles]]===
	[[Image:Apollo11Soil.jpg\|160px\|left]] The primary resource of value to humans on the Moon is the volatile components found in the [[regolith]]. These are all the components that are gases at room temperature. Most of the volatiles have been deposited in the top layers of the Moon's surface by the [[solar wind]] over geologic time. A notable exception to this is [[Argon]]. the concentration of Argon in lunar soil is much higher than found in the solar wind, so must come from a different source. Especially, the isotope Argon-40. It is presently believed that the Argon-40 comes from radioactive decay of [[Potassium]] and/or [[Krypton]] deep within the lunar mantle or core, and that the Argon-40 seeps out to the surface via fissures. This vented Argon enter the lunar atmosphere; then the Argon is implanted into the regolith by ~~interactions with ions from the solar wind.~~([[Volatiles\|read more]])		[[Image:Apollo11Soil.jpg\|160px\|left]] The primary resource of value to humans on the Moon is the volatile components found in the [[regolith]]. These are all the components that are gases at room temperature. Most of the volatiles have been deposited in the top layers of the Moon's surface by the [[solar wind]] over geologic time. A notable exception to this is [[Argon]]. the concentration of Argon in lunar soil is much higher than found in the solar wind, so must come from a different source. Especially, the isotope Argon-40. It is presently believed that the Argon-40 comes from radioactive decay of [[Potassium]] and/or [[Krypton]] deep within the lunar mantle or core, and that the Argon-40 seeps out to the surface via fissures. This vented Argon enter the lunar atmosphere; then the Argon is implanted into the regolith by([[Volatiles\|read more]])
	<DIV style="text-align:right">		<DIV style="text-align:right">
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lunarp>Jarogers2001 at 11:56, 5 August 2008

2008-08-05T11:56:17Z

← Older revision		Revision as of 04:56, 5 August 2008
Line 1:		Line 1:
	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[~~Sintered regolith~~]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Volatiles]]===
	[[Image:~~MLS1_Brick~~.~~GIF~~\|160px\|left]] ~~Sintered~~ [[regolith]] ~~falls into~~ the ~~category~~ of ~~ceramic materials as sintering is~~ the ~~process most common~~ to ~~ceramics~~. ~~When bricks are made~~ from ~~clay on Earth~~, ~~first~~ the ~~bricks are heated long enough~~ and ~~hot enough~~ to ~~drive out~~ the ~~water~~. ~~Then~~ the ~~heating~~ is ~~increased to cause partial melting or vitrification which results in~~ the ~~edges of adjacent grains being bonded together once they have cooled. The unmelted particles provide a stable shape and size during~~ the ~~process which involves some shrinkage and a decrease in porosity~~.		[[Image:Apollo11Soil.jpg\|160px\|left]] The primary resource of value to humans on the Moon is the volatile components found in the [[regolith]]. These are all the components that are gases at room temperature. Most of the volatiles have been deposited in the top layers of the Moon's surface by the [[solar wind]] over geologic time. A notable exception to this is [[Argon]]. the concentration of Argon in lunar soil is much higher than found in the solar wind, so must come from a different source. Especially, the isotope Argon-40. It is presently believed that the Argon-40 comes from radioactive decay of [[Potassium]] and/or [[Krypton]] deep within the lunar mantle or core, and that the Argon-40 seeps out to the surface via fissures. This vented Argon enter the lunar atmosphere; then the Argon is implanted into the regolith by interactions with ions from the solar wind.([[Volatiles\|read more]])

	~~Experiments in radiant heating of regolith simulant have been carried~~([[~~Sintered regolith~~\|read more]])
	<DIV style="text-align:right">		<DIV style="text-align:right">
	<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>		<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>

lunarp>Jarogers2001: /* Featured article: Sintered regolith */

2008-08-05T11:49:28Z

Featured article: [[Sintered regolith]]

← Older revision		Revision as of 04:49, 5 August 2008
Line 2:		Line 2:
	[[Image:MLS1_Brick.GIF\|160px\|left]] Sintered [[regolith]] falls into the category of ceramic materials as sintering is the process most common to ceramics. When bricks are made from clay on Earth, first the bricks are heated long enough and hot enough to drive out the water. Then the heating is increased to cause partial melting or vitrification which results in the edges of adjacent grains being bonded together once they have cooled. The unmelted particles provide a stable shape and size during the process which involves some shrinkage and a decrease in porosity.		[[Image:MLS1_Brick.GIF\|160px\|left]] Sintered [[regolith]] falls into the category of ceramic materials as sintering is the process most common to ceramics. When bricks are made from clay on Earth, first the bricks are heated long enough and hot enough to drive out the water. Then the heating is increased to cause partial melting or vitrification which results in the edges of adjacent grains being bonded together once they have cooled. The unmelted particles provide a stable shape and size during the process which involves some shrinkage and a decrease in porosity.

	Experiments in radiant heating of regolith simulant have been carried ~~out by NASA Johnson Space Center and Lockheed Engineering & Sciences Co.~~([[Sintered regolith\|read more]])		Experiments in radiant heating of regolith simulant have been carried([[Sintered regolith\|read more]])
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	<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>		<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>

← Older revision		Revision as of 07:06, 20 September 2011
Line 1:		Line 1:
	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[~~Moon Zoo~~]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[JSC-1]]===
	[[Image:~~Moon Zoo Logo~~.~~gif~~\|160px\|left]] ~~Moon Zoo is~~ a ~~crowdsourcing project from~~ the ~~Zooniverse community that uses images from~~ the ~~Lunar Reconnaissance Orbiter~~.		[[Image:EIC050-2.GIF\|160px\|left]] JSC-1, a lunar soil simulant, was developed and characterized under the auspices of the NASA Johnson Space Center. This simulant was produced in large quantities to satisfy the requirements of a variety of scientific and engineering investigations. JSC-1 is derived from volcanic ash of basaltic composition, which has been ground, sized, and placed into storage. The simulant's chemical composition, mineralogy, particle size distribution, specific gravity, angle of internal friction, and cohesion have been characterized and fall within the ranges of lunar mare soil samples. ...([[JSC-1\|read more]])

	~~Activities include counting craters~~, ~~noting blocky craters~~, and ~~checking relative differences between boulder-producing craters~~, and...([[~~Moon Zoo~~\|read more]])
	<DIV style="text-align:right">		<DIV style="text-align:right">
	<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>		<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>

← Older revision		Revision as of 10:32, 11 May 2010
Line 1:		Line 1:
	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Moon Zoo]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Moon Zoo]]===
	[[Image:Moon Zoo Logo.gif\|160px\|left]] Moon Zoo is a crowdsourcing project from the Zooniverse community that uses images from the Lunar ~~Reconnasaince~~ Orbiter.		[[Image:Moon Zoo Logo.gif\|160px\|left]] Moon Zoo is a crowdsourcing project from the Zooniverse community that uses images from the Lunar Reconnaissance Orbiter.

	Activities include counting craters, noting blocky craters, and checking relative differences between boulder-producing craters, and...([[Moon Zoo\|read more]])		Activities include counting craters, noting blocky craters, and checking relative differences between boulder-producing craters, and...([[Moon Zoo\|read more]])

← Older revision		Revision as of 10:16, 11 May 2010
Line 1:		Line 1:
	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[~~Geologic Processes on the Moon/Cratering on the Moon\|Cratering on the~~ Moon]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Moon Zoo]]===
	[[Image:~~GP1Fig_3~~.~~jpg~~\|160px\|left]] ~~Craters cover the surface of the moon and are the result of hyper-velocity impacts by meteorites. The velocity of meteorites upon impact varies, but is generally between 10 and 40 km/sec. This number~~ is a ~~combination of~~ the ~~‘approach velocity’ and~~ the ~~‘escape velocity~~.~~’ The approach velocity of objects refers to the velocity of the object with respect to the moon. This varies with the type of object (for example~~, ~~long period comets generally have a higher approach velocity than short period comets)~~ and ~~the direction with which it approaches the moon (for example~~, ~~if it approaching the moon ‘head on,’ it will have a higher approach velocity than~~...([[~~Geologic Processes on the Moon/Cratering on the~~ Moon\|read more]])		[[Image:Moon Zoo Logo.gif\|160px\|left]] Moon Zoo is a crowdsourcing project from the Zooniverse community that uses images from the Lunar Reconnasaince Orbiter.

			Activities include counting craters, noting blocky craters, and checking relative differences between boulder-producing craters, and...([[Moon Zoo\|read more]])
	<DIV style="text-align:right">		<DIV style="text-align:right">
	<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>		<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>

← Older revision		Revision as of 04:56, 5 August 2008
Line 1:		Line 1:
	===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[~~Sintered regolith~~]]===		===<!--[[Image:red_ring.png\|15px\|left]]-->Featured article: [[Volatiles]]===
	[[Image:~~MLS1_Brick~~.~~GIF~~\|160px\|left]] ~~Sintered~~ [[regolith]] ~~falls into~~ the ~~category~~ of ~~ceramic materials as sintering is~~ the ~~process most common~~ to ~~ceramics~~. ~~When bricks are made~~ from ~~clay on Earth~~, ~~first~~ the ~~bricks are heated long enough~~ and ~~hot enough~~ to ~~drive out~~ the ~~water~~. ~~Then~~ the ~~heating~~ is ~~increased to cause partial melting or vitrification which results in~~ the ~~edges of adjacent grains being bonded together once they have cooled. The unmelted particles provide a stable shape and size during~~ the ~~process which involves some shrinkage and a decrease in porosity~~.		[[Image:Apollo11Soil.jpg\|160px\|left]] The primary resource of value to humans on the Moon is the volatile components found in the [[regolith]]. These are all the components that are gases at room temperature. Most of the volatiles have been deposited in the top layers of the Moon's surface by the [[solar wind]] over geologic time. A notable exception to this is [[Argon]]. the concentration of Argon in lunar soil is much higher than found in the solar wind, so must come from a different source. Especially, the isotope Argon-40. It is presently believed that the Argon-40 comes from radioactive decay of [[Potassium]] and/or [[Krypton]] deep within the lunar mantle or core, and that the Argon-40 seeps out to the surface via fissures. This vented Argon enter the lunar atmosphere; then the Argon is implanted into the regolith by interactions with ions from the solar wind.([[Volatiles\|read more]])

	~~Experiments in radiant heating of regolith simulant have been carried~~([[~~Sintered regolith~~\|read more]])
	<DIV style="text-align:right">		<DIV style="text-align:right">
	<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>		<SMALL><STRONG>[[Featured articles\|See all featured articles]]</STRONG> \| [[Talk:Featured_articles\|Nominate!]]</SMALL>