Talk:Lunar Temperature - Revision history

Farred: Undo revision 92499 by 37.113.57.34 (talk) remove vandalism

2016-08-10T09:38:19Z

Undo revision 92499 by 37.113.57.34 (talk) remove vandalism

37.113.57.34: /* viagrdsfdfrt */ new section

2015-11-14T01:05:21Z

viagrdsfdfrt: new section

Farred: Undo revision 16757 by 193.128.96.137 (talk)

2011-10-31T05:31:17Z

Undo revision 16757 by 193.128.96.137 (talk)

193.128.96.137: /* Temperature Concerns for Development */

2011-10-27T10:32:27Z

Temperature Concerns for Development

Farred: removing nonsense

2009-11-11T19:57:34Z

removing nonsense

194.8.75.40: /* I am sorry, that I interrupt you, but, in my opinion, there is other way of the decision of a question. */ new section

2009-11-08T01:23:14Z

I am sorry, that I interrupt you, but, in my opinion, there is other way of the decision of a question.: new section

194.8.75.40: /* Quite, yes */ new section

2009-11-05T19:57:50Z

Quite, yes: new section

Farred: talk

2009-10-08T09:19:49Z

talk

71.96.208.175: rv to last edit by Charles F. Radley

2009-09-08T18:18:53Z

rv to last edit by Charles F. Radley

194.8.74.70: /* Apache/2.2.3 (Debian) mod_python/3.2.10 Python/2.4.4 PHP/5.2.0-8+etch15 mod_ssl/2.2.3 OpenSSL/0.9.8c Server at allhomedecor.org Port 80 */ new section

2009-09-05T08:37:04Z

Apache/2.2.3 (Debian) mod_python/3.2.10 Python/2.4.4 PHP/5.2.0-8+etch15 mod_ssl/2.2.3 OpenSSL/0.9.8c Server at allhomedecor.org Port 80: new section

← Older revision		Revision as of 09:38, 10 August 2016
Line 13:		Line 13:
	* Shouldn't we mention that there is no general temperature for an area the size of a square mile on Luna as there would be on Earth. The temperatures in a particular area are not averaged out by convection of the atmosphere on Luna which has practically none. So, in a little shaded area near the equator could be nearly as cold as space if protected from heat radiation of the surrounding area. Likewise a surface normal to incoming sunlight could reach the same radiative equilibrium temperature as a flat spot at noon on the equator. Also the radiative equilibrium temperature depends on color. The lunar surface is reasonably well approximated by neutral grey tending toward black body black.		* Shouldn't we mention that there is no general temperature for an area the size of a square mile on Luna as there would be on Earth. The temperatures in a particular area are not averaged out by convection of the atmosphere on Luna which has practically none. So, in a little shaded area near the equator could be nearly as cold as space if protected from heat radiation of the surrounding area. Likewise a surface normal to incoming sunlight could reach the same radiative equilibrium temperature as a flat spot at noon on the equator. Also the radiative equilibrium temperature depends on color. The lunar surface is reasonably well approximated by neutral grey tending toward black body black.
	* Since there have been published comments about how difficult it is to deal with the intense cold of shaded craters at the lunar, shouldn't we mention that the space program has had considerable experience with such temperatures in the shade of the ISS and is in a position to get more experience with reasonable experimental effort. The cold mass of rock and dirt at a crater bottom is something new, but the robot foot that contacts that crater won't get colder than temperatures that we have already dealt with. An insulated boot could limit heat flow by conduction handily, and a couple of layers of shiny metal foil with vacuum between could put quite low limits on radiative heat loss.--[[User:Farred\|Farred]] 09:19, 8 October 2009 (UTC)		* Since there have been published comments about how difficult it is to deal with the intense cold of shaded craters at the lunar, shouldn't we mention that the space program has had considerable experience with such temperatures in the shade of the ISS and is in a position to get more experience with reasonable experimental effort. The cold mass of rock and dirt at a crater bottom is something new, but the robot foot that contacts that crater won't get colder than temperatures that we have already dealt with. An insulated boot could limit heat flow by conduction handily, and a couple of layers of shiny metal foil with vacuum between could put quite low limits on radiative heat loss.--[[User:Farred\|Farred]] 09:19, 8 October 2009 (UTC)
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← Older revision		Revision as of 01:05, 14 November 2015
Line 13:		Line 13:
	* Shouldn't we mention that there is no general temperature for an area the size of a square mile on Luna as there would be on Earth. The temperatures in a particular area are not averaged out by convection of the atmosphere on Luna which has practically none. So, in a little shaded area near the equator could be nearly as cold as space if protected from heat radiation of the surrounding area. Likewise a surface normal to incoming sunlight could reach the same radiative equilibrium temperature as a flat spot at noon on the equator. Also the radiative equilibrium temperature depends on color. The lunar surface is reasonably well approximated by neutral grey tending toward black body black.		* Shouldn't we mention that there is no general temperature for an area the size of a square mile on Luna as there would be on Earth. The temperatures in a particular area are not averaged out by convection of the atmosphere on Luna which has practically none. So, in a little shaded area near the equator could be nearly as cold as space if protected from heat radiation of the surrounding area. Likewise a surface normal to incoming sunlight could reach the same radiative equilibrium temperature as a flat spot at noon on the equator. Also the radiative equilibrium temperature depends on color. The lunar surface is reasonably well approximated by neutral grey tending toward black body black.
	* Since there have been published comments about how difficult it is to deal with the intense cold of shaded craters at the lunar, shouldn't we mention that the space program has had considerable experience with such temperatures in the shade of the ISS and is in a position to get more experience with reasonable experimental effort. The cold mass of rock and dirt at a crater bottom is something new, but the robot foot that contacts that crater won't get colder than temperatures that we have already dealt with. An insulated boot could limit heat flow by conduction handily, and a couple of layers of shiny metal foil with vacuum between could put quite low limits on radiative heat loss.--[[User:Farred\|Farred]] 09:19, 8 October 2009 (UTC)		* Since there have been published comments about how difficult it is to deal with the intense cold of shaded craters at the lunar, shouldn't we mention that the space program has had considerable experience with such temperatures in the shade of the ISS and is in a position to get more experience with reasonable experimental effort. The cold mass of rock and dirt at a crater bottom is something new, but the robot foot that contacts that crater won't get colder than temperatures that we have already dealt with. An insulated boot could limit heat flow by conduction handily, and a couple of layers of shiny metal foil with vacuum between could put quite low limits on radiative heat loss.--[[User:Farred\|Farred]] 09:19, 8 October 2009 (UTC)
		+
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		+	http://comprarviagragenricoes.com/ viagra generico
		+	http://comprarviagragenerico25mg.net/ comprar viagra
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		+	http://kaufenviagragenerika.com/ viagra bestellen

← Older revision		Revision as of 05:31, 31 October 2011
Line 10:		Line 10:
	:Arthur, the term used is [[Albedo]], rather than [[reflectivity]].[[User:Cfrjlr\|Charles F. Radley]] 13:40, 14 June 2007 (UTC)		:Arthur, the term used is [[Albedo]], rather than [[reflectivity]].[[User:Cfrjlr\|Charles F. Radley]] 13:40, 14 June 2007 (UTC)

−	~~Clear~~, ~~informative~~, ~~siplme~~. ~~Could I send you some e~~-~~hugs?~~	+	== Temperature Concerns for Development ==
		+	* Shouldn't we mention that there is no general temperature for an area the size of a square mile on Luna as there would be on Earth. The temperatures in a particular area are not averaged out by convection of the atmosphere on Luna which has practically none. So, in a little shaded area near the equator could be nearly as cold as space if protected from heat radiation of the surrounding area. Likewise a surface normal to incoming sunlight could reach the same radiative equilibrium temperature as a flat spot at noon on the equator. Also the radiative equilibrium temperature depends on color. The lunar surface is reasonably well approximated by neutral grey tending toward black body black.
		+	* Since there have been published comments about how difficult it is to deal with the intense cold of shaded craters at the lunar, shouldn't we mention that the space program has had considerable experience with such temperatures in the shade of the ISS and is in a position to get more experience with reasonable experimental effort. The cold mass of rock and dirt at a crater bottom is something new, but the robot foot that contacts that crater won't get colder than temperatures that we have already dealt with. An insulated boot could limit heat flow by conduction handily, and a couple of layers of shiny metal foil with vacuum between could put quite low limits on radiative heat loss.--[[User:Farred\|Farred]] 09:19, 8 October 2009 (UTC)

← Older revision		Revision as of 10:32, 27 October 2011
Line 10:		Line 10:
	:Arthur, the term used is [[Albedo]], rather than [[reflectivity]].[[User:Cfrjlr\|Charles F. Radley]] 13:40, 14 June 2007 (UTC)		:Arthur, the term used is [[Albedo]], rather than [[reflectivity]].[[User:Cfrjlr\|Charles F. Radley]] 13:40, 14 June 2007 (UTC)

−	~~== Temperature Concerns for Development ==~~	+	Clear, informative, siplme. Could I send you some e-hugs?
−	* Shouldn't we mention that there is no general temperature for an area the size of a square mile on Luna as there would be on Earth. The temperatures in a particular area are not averaged out by convection of the atmosphere on Luna which has practically none. So, in a little shaded area near the equator could be nearly as cold as space if protected from heat radiation of the surrounding area. Likewise a surface normal to incoming sunlight could reach the same radiative equilibrium temperature as a flat spot at noon on the equator. Also the radiative equilibrium temperature depends on color. The lunar surface is reasonably well approximated by neutral grey tending toward black body black.
−	* Since there have been published comments about how difficult it is to deal with the intense cold of shaded craters at the lunar, shouldn't we mention that the space program has had considerable experience with such temperatures in the shade of the ISS and is in a position to get more experience with reasonable experimental effort. The cold mass of rock and dirt at a crater bottom is something new, ~~but the robot foot that contacts that crater won't get colder than temperatures that we have already dealt with. An insulated boot could limit heat flow by conduction handily~~, ~~and a couple of layers of shiny metal foil with vacuum between could put quite low limits on radiative heat loss~~.-~~-[[User:Farred\|Farred]] 09:19, 8 October 2009 (UTC)~~

← Older revision		Revision as of 19:57, 11 November 2009
Line 13:		Line 13:
	* Shouldn't we mention that there is no general temperature for an area the size of a square mile on Luna as there would be on Earth. The temperatures in a particular area are not averaged out by convection of the atmosphere on Luna which has practically none. So, in a little shaded area near the equator could be nearly as cold as space if protected from heat radiation of the surrounding area. Likewise a surface normal to incoming sunlight could reach the same radiative equilibrium temperature as a flat spot at noon on the equator. Also the radiative equilibrium temperature depends on color. The lunar surface is reasonably well approximated by neutral grey tending toward black body black.		* Shouldn't we mention that there is no general temperature for an area the size of a square mile on Luna as there would be on Earth. The temperatures in a particular area are not averaged out by convection of the atmosphere on Luna which has practically none. So, in a little shaded area near the equator could be nearly as cold as space if protected from heat radiation of the surrounding area. Likewise a surface normal to incoming sunlight could reach the same radiative equilibrium temperature as a flat spot at noon on the equator. Also the radiative equilibrium temperature depends on color. The lunar surface is reasonably well approximated by neutral grey tending toward black body black.
	* Since there have been published comments about how difficult it is to deal with the intense cold of shaded craters at the lunar, shouldn't we mention that the space program has had considerable experience with such temperatures in the shade of the ISS and is in a position to get more experience with reasonable experimental effort. The cold mass of rock and dirt at a crater bottom is something new, but the robot foot that contacts that crater won't get colder than temperatures that we have already dealt with. An insulated boot could limit heat flow by conduction handily, and a couple of layers of shiny metal foil with vacuum between could put quite low limits on radiative heat loss.--[[User:Farred\|Farred]] 09:19, 8 October 2009 (UTC)		* Since there have been published comments about how difficult it is to deal with the intense cold of shaded craters at the lunar, shouldn't we mention that the space program has had considerable experience with such temperatures in the shade of the ISS and is in a position to get more experience with reasonable experimental effort. The cold mass of rock and dirt at a crater bottom is something new, but the robot foot that contacts that crater won't get colder than temperatures that we have already dealt with. An insulated boot could limit heat flow by conduction handily, and a couple of layers of shiny metal foil with vacuum between could put quite low limits on radiative heat loss.--[[User:Farred\|Farred]] 09:19, 8 October 2009 (UTC)
−
−	~~== Quite, yes ==~~
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−	~~== I am sorry, that I interrupt you, but, in my opinion, there is other way of the decision of a question. ==~~
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← Older revision		Revision as of 01:23, 8 November 2009
Line 17:		Line 17:

	une idГ©e trГЁs intГ©ressante www.gnduonline.com viagra		une idГ©e trГЁs intГ©ressante www.gnduonline.com viagra
		+
		+	== I am sorry, that I interrupt you, but, in my opinion, there is other way of the decision of a question. ==
		+
		+	Quelle phrase nГ©cessaire... super, l'idГ©e remarquable www.gnduonline.org acheter viagra

← Older revision		Revision as of 19:57, 5 November 2009
Line 13:		Line 13:
	* Shouldn't we mention that there is no general temperature for an area the size of a square mile on Luna as there would be on Earth. The temperatures in a particular area are not averaged out by convection of the atmosphere on Luna which has practically none. So, in a little shaded area near the equator could be nearly as cold as space if protected from heat radiation of the surrounding area. Likewise a surface normal to incoming sunlight could reach the same radiative equilibrium temperature as a flat spot at noon on the equator. Also the radiative equilibrium temperature depends on color. The lunar surface is reasonably well approximated by neutral grey tending toward black body black.		* Shouldn't we mention that there is no general temperature for an area the size of a square mile on Luna as there would be on Earth. The temperatures in a particular area are not averaged out by convection of the atmosphere on Luna which has practically none. So, in a little shaded area near the equator could be nearly as cold as space if protected from heat radiation of the surrounding area. Likewise a surface normal to incoming sunlight could reach the same radiative equilibrium temperature as a flat spot at noon on the equator. Also the radiative equilibrium temperature depends on color. The lunar surface is reasonably well approximated by neutral grey tending toward black body black.
	* Since there have been published comments about how difficult it is to deal with the intense cold of shaded craters at the lunar, shouldn't we mention that the space program has had considerable experience with such temperatures in the shade of the ISS and is in a position to get more experience with reasonable experimental effort. The cold mass of rock and dirt at a crater bottom is something new, but the robot foot that contacts that crater won't get colder than temperatures that we have already dealt with. An insulated boot could limit heat flow by conduction handily, and a couple of layers of shiny metal foil with vacuum between could put quite low limits on radiative heat loss.--[[User:Farred\|Farred]] 09:19, 8 October 2009 (UTC)		* Since there have been published comments about how difficult it is to deal with the intense cold of shaded craters at the lunar, shouldn't we mention that the space program has had considerable experience with such temperatures in the shade of the ISS and is in a position to get more experience with reasonable experimental effort. The cold mass of rock and dirt at a crater bottom is something new, but the robot foot that contacts that crater won't get colder than temperatures that we have already dealt with. An insulated boot could limit heat flow by conduction handily, and a couple of layers of shiny metal foil with vacuum between could put quite low limits on radiative heat loss.--[[User:Farred\|Farred]] 09:19, 8 October 2009 (UTC)
		+
		+	== Quite, yes ==
		+
		+	une idГ©e trГЁs intГ©ressante www.gnduonline.com viagra

← Older revision		Revision as of 09:19, 8 October 2009
Line 9:		Line 9:
	[[User:Apsmith\|Apsmith]] 12:24, 14 June 2007 (UTC)		[[User:Apsmith\|Apsmith]] 12:24, 14 June 2007 (UTC)
	:Arthur, the term used is [[Albedo]], rather than [[reflectivity]].[[User:Cfrjlr\|Charles F. Radley]] 13:40, 14 June 2007 (UTC)		:Arthur, the term used is [[Albedo]], rather than [[reflectivity]].[[User:Cfrjlr\|Charles F. Radley]] 13:40, 14 June 2007 (UTC)
		+
		+	== Temperature Concerns for Development ==
		+	* Shouldn't we mention that there is no general temperature for an area the size of a square mile on Luna as there would be on Earth. The temperatures in a particular area are not averaged out by convection of the atmosphere on Luna which has practically none. So, in a little shaded area near the equator could be nearly as cold as space if protected from heat radiation of the surrounding area. Likewise a surface normal to incoming sunlight could reach the same radiative equilibrium temperature as a flat spot at noon on the equator. Also the radiative equilibrium temperature depends on color. The lunar surface is reasonably well approximated by neutral grey tending toward black body black.
		+	* Since there have been published comments about how difficult it is to deal with the intense cold of shaded craters at the lunar, shouldn't we mention that the space program has had considerable experience with such temperatures in the shade of the ISS and is in a position to get more experience with reasonable experimental effort. The cold mass of rock and dirt at a crater bottom is something new, but the robot foot that contacts that crater won't get colder than temperatures that we have already dealt with. An insulated boot could limit heat flow by conduction handily, and a couple of layers of shiny metal foil with vacuum between could put quite low limits on radiative heat loss.--[[User:Farred\|Farred]] 09:19, 8 October 2009 (UTC)

← Older revision		Revision as of 18:18, 8 September 2009
Line 9:		Line 9:
	[[User:Apsmith\|Apsmith]] 12:24, 14 June 2007 (UTC)		[[User:Apsmith\|Apsmith]] 12:24, 14 June 2007 (UTC)
	:Arthur, the term used is [[Albedo]], rather than [[reflectivity]].[[User:Cfrjlr\|Charles F. Radley]] 13:40, 14 June 2007 (UTC)		:Arthur, the term used is [[Albedo]], rather than [[reflectivity]].[[User:Cfrjlr\|Charles F. Radley]] 13:40, 14 June 2007 (UTC)
−
−	~~== <html><head>~~
−	==
−
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−
−	~~== </body></html>~~
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−	~~<hr>~~
−	~~<html><head>~~
−	~~</body></html>~~
−	~~<title>404 Not Found</title>~~
−	~~<p>The requested URL /forxru1/zadanie.txt was not found on this server.</p>~~
−
−	~~== <hr>~~
−	==
−
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−
−	~~== <!DOCTYPE HTML PUBLIC "-//IETF//DTD HTML 2.0//EN">~~
−	==
−
−	~~<title>404 Not Found</title>~~
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−	~~<html><head>~~
−	~~<address>Apache/2.2.3 (Debian) mod_python/3.2.10 Python/2.4.4 PHP/5.2.0-8+etch15 mod_ssl/2.2.3 OpenSSL/0.9.8c Server at allhomedecor.org Port 80</address>~~
−	~~<p>The requested URL /forxru1/zadanie.txt was not found on this server.</p>~~
−	~~</head><body>~~
−	~~</body></html>~~
−	~~<h1>Not Found</h1>~~
−	~~<hr>~~
−
−	~~== <address>Apache/2.2.3 (Debian) mod_python/3.2.10 Python/2.4.4 PHP/5.2.0-8+etch15 mod_ssl/2.2.3 OpenSSL/0.9.8c Server at allhomedecor.org Port 80</address>~~
−	==
−
−	~~</head><body>~~
−	~~<address>Apache/2.2.3 (Debian) mod_python/3.2.10 Python/2.4.4 PHP/5.2.0-8+etch15 mod_ssl/2.2.3 OpenSSL/0.9.8c Server at allhomedecor.org Port 80</address>~~
−	~~<title>404 Not Found</title>~~
−	~~<!DOCTYPE HTML PUBLIC "-//IETF//DTD HTML 2.0//EN">~~
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−	~~<h1>Not Found</h1>~~
−	~~<hr>~~
−	~~<p>The requested URL /forxru1/zadanie.txt was not found on this server.</p>~~

← Older revision		Revision as of 08:37, 5 September 2009
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	<h1>Not Found</h1>		<h1>Not Found</h1>
	<hr>		<hr>
		+
		+	== <address>Apache/2.2.3 (Debian) mod_python/3.2.10 Python/2.4.4 PHP/5.2.0-8+etch15 mod_ssl/2.2.3 OpenSSL/0.9.8c Server at allhomedecor.org Port 80</address>
		+	==
		+
		+	</head><body>
		+	<address>Apache/2.2.3 (Debian) mod_python/3.2.10 Python/2.4.4 PHP/5.2.0-8+etch15 mod_ssl/2.2.3 OpenSSL/0.9.8c Server at allhomedecor.org Port 80</address>
		+	<title>404 Not Found</title>
		+	<!DOCTYPE HTML PUBLIC "-//IETF//DTD HTML 2.0//EN">
		+	</body></html>
		+	<html><head>
		+	<h1>Not Found</h1>
		+	<hr>
		+	<p>The requested URL /forxru1/zadanie.txt was not found on this server.</p>