Boyle temperature - Revision history

en>Daniele Pugliesi: removed Category:Thermodynamics; added Category:Temperature using HotCat

2014-10-22T02:03:43Z

removed Category:Thermodynamics; added Category:Temperature using HotCat

← Older revision		Revision as of 04:03, 22 October 2014
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	~~In [[astrodynamics]]~~, A '~~''canonical unit''' is a [[unit~~ of ~~measurement]] defined in terms of an object~~'~~s reference [[orbit]]~~. ~~In this system, a reference mass, for example the sun,~~ is ~~assumed to be 1 "mass unit" and the mean distance from the orbiting object to the reference object~~ is ~~considered the "distance unit".~~		Hello, my name is Andrew and my wife doesn't like it at all. I am truly fond of to go to karaoke but I've been using on new things lately. Ohio is where his home is and his family members enjoys it. I am currently a travel agent.<br><br>my blog post - [http://ustanford.com/index.php?do=/profile-38218/info/ psychics online]

	~~Canonical units are useful when the precise distances~~ and ~~masses of objects in space are not available~~. ~~However, by setting the mass of~~ a ~~given object to be 1 mass unit and the mean distance of the reference object to another object in question, many calculations can be simplified~~.

	~~== Overview ==~~

	~~The ''Distance Unit''~~ <~~math~~>~~DU \~~ <~~/math~~> ~~is defined to be the mean radius of the reference orbit.~~

	~~The ''Time Unit'' <math>TU \ </math> is defined by the [~~[~~gravitational parameter]] <math> \mu\ </math>~~:

	~~<math>\mu = G*M\,\!<~~/~~math>~~

	* <math>G \ </~~math> is the [[gravitational constant]]~~
	* <math>M \ </math> is the mass of the central reference body

	~~For canonical units, the gravitational parameter is defined as:~~

	~~<math>\mu = 1 * \frac{DU^3}{TU^2}</math>~~

	~~----~~

	~~The quantity of the time unit (TU) can be solved in another unit system (e.g. the metric system) if the mass and radius of the central body has been determined~~. ~~Using the above equation and applying [[dimensional analysis]], set the two equations expressing <math>\mu<~~/~~math> equal to each other:~~

	~~<math>\mu = GM = 1 \frac{DU^3}{TU^2}</math>~~

	~~The time unit (TU) can be converted to another unit system for a more useful qualitative solution using the following equation:~~

	~~<math> TU = \sqrt{\frac{DU^3}{G*M}}</math>~~

	~~For Earth satellites, approximate unit conversions are as follows:~~
	* 1 DU = 6378.~~1 km~~ = ~~20,925,524.97 ft~~
	* 1 DU/~~TU = 7.90538 km~~/~~s = 25,936.29 ft~~/~~sec~~
	* 1 TU = 806.80415 s

	~~== Astronomical Unit ==~~

	~~The [[astronomical unit]] is a canonical unit based on the orbit of the Earth around the Sun~~

	~~== See also ==~~
	*[[Astronomical unit]]
	*[[Conversion of units]]

	~~== References ==~~

	~~Roger R. Bate, Donald D. Mueller, Jerry E. White. ''Fundamentals of Astrodynamics''.~~

	~~[[Category:Astrodynamics]]~~
	~~[[Category:Celestial mechanics]~~]

146.6.150.85 at 23:02, 16 January 2014

2014-01-16T23:02:35Z

← Older revision		Revision as of 01:02, 17 January 2014
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	~~Hi there~~, ~~I am Sophia~~. ~~Kentucky~~ is ~~exactly where I~~'~~ve usually been living. Invoicing~~ is ~~my profession~~. ~~Doing ballet~~ is ~~some thing she would~~ by ~~no means give up~~.<br><br>~~Also visit my homepage [http~~://~~conniecolin~~.~~com~~/xe/~~community~~/~~24580 best psychic~~]		In [[astrodynamics]], A '''canonical unit''' is a [[unit of measurement]] defined in terms of an object's reference [[orbit]]. In this system, a reference mass, for example the sun, is assumed to be 1 "mass unit" and the mean distance from the orbiting object to the reference object is considered the "distance unit".

			Canonical units are useful when the precise distances and masses of objects in space are not available. However, by setting the mass of a given object to be 1 mass unit and the mean distance of the reference object to another object in question, many calculations can be simplified.

			== Overview ==

			The ''Distance Unit'' <math>DU \ </math> is defined to be the mean radius of the reference orbit.

			The ''Time Unit'' <math>TU \ </math> is defined by the [[gravitational parameter]] <math> \mu\ </math>:

			<math>\mu = G*M\,\!</math>

			* <math>G \ </math> is the [[gravitational constant]]
			* <math>M \ </math> is the mass of the central reference body

			For canonical units, the gravitational parameter is defined as:

			<math>\mu = 1 * \frac{DU^3}{TU^2}</math>

			----

			The quantity of the time unit (TU) can be solved in another unit system (e.g. the metric system) if the mass and radius of the central body has been determined. Using the above equation and applying [[dimensional analysis]], set the two equations expressing <math>\mu</math> equal to each other:

			<math>\mu = GM = 1 \frac{DU^3}{TU^2}</math>

			The time unit (TU) can be converted to another unit system for a more useful qualitative solution using the following equation:

			<math> TU = \sqrt{\frac{DU^3}{G*M}}</math>

			For Earth satellites, approximate unit conversions are as follows:
			* 1 DU = 6378.1 km = 20,925,524.97 ft
			* 1 DU/TU = 7.90538 km/s = 25,936.29 ft/sec
			* 1 TU = 806.80415 s

			== Astronomical Unit ==

			The [[astronomical unit]] is a canonical unit based on the orbit of the Earth around the Sun

			== See also ==
			*[[Astronomical unit]]
			*[[Conversion of units]]

			== References ==

			Roger R. Bate, Donald D. Mueller, Jerry E. White. ''Fundamentals of Astrodynamics''.

			[[Category:Astrodynamics]]
			[[Category:Celestial mechanics]]

83.165.101.200 at 17:33, 2 June 2012

2012-06-02T17:33:12Z

New page

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