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		<title>Welfare cost of business cycles</title>
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		<summary type="html">&lt;p&gt;220.239.181.223: &lt;/p&gt;
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&lt;div&gt;[[File:Beta angle sun.svg|400px|thumb|Beta Angle (&amp;lt;math&amp;gt;\boldsymbol{\beta}&amp;lt;/math&amp;gt;)]]&lt;br /&gt;
The &#039;&#039;&#039;beta angle&#039;&#039;&#039; (&amp;lt;math&amp;gt;\boldsymbol{\beta}&amp;lt;/math&amp;gt;) is a measurement that is used most notably in [[spaceflight]]. The beta angle determines the percentage of time an object such as a spacecraft in [[low Earth orbit]] (LEO) spends in direct sunlight, absorbing solar energy.&amp;lt;ref name=&amp;quot;mcc&amp;quot;&amp;gt;{{cite web|url=http://spaceflight.nasa.gov/feedback/expert/answer/mcc/sts-113/11_23_20_01_179.html|title=MCC Answers|author=Derek Hassman, NASA Flight Director|date=December 1, 2002|publisher=NASA|accessdate=June 14, 2009}}&amp;lt;/ref&amp;gt; Beta angle is defined as the angle between the [[orbit]] plane and the [[Euclidean vector|vector]] from the [[sun]] (which direction the sun is shining from).&amp;lt;ref name=&amp;quot;knk&amp;quot;&amp;gt;{{cite web|url=http://www.tak2000.com/data/planets/earth.htm|title=  Earth&#039;s Thermal Environment|last=K&amp;amp;K Associates|year=2008|work=Thermal Environments JPL D-8160|publisher=K&amp;amp;K Associates|accessdate=July 14, 2009}}&amp;lt;/ref&amp;gt; The beta angle is the smaller angle (there are two angles) between the sun vector (where the sun is shining from in the sky) and the [[Plane (geometry)|plane]] of the object&#039;s orbit.  Note that the beta angle does not define a unique orbit plane; all satellites in orbit with a given beta angle at a given altitude have the same exposure to the sun, even though they may be orbiting in completely different planes around the Earth.&amp;lt;ref name=&amp;quot;orbit&amp;quot;/&amp;gt; The beta angle varies between +90° and −90°, and the direction the satellite revolves around the body it orbits determines whether the beta angle sign is positive or negative.  An imaginary observer standing on the sun defines a beta angle as positive if the satellite in question orbits in a counter clockwise direction and negative if it revolves clockwise.&amp;lt;ref name=&amp;quot;orbit&amp;quot;&amp;gt;{{cite web|url=http://wwwiutp.univ-poitiers.fr/COURS-DOCS/docu/ideas/SDRCHelp/LANG/French/tmg_ug/orbit_def.htm|title= Orbit Definition|publisher=2001 Structural Dynamics Research Corporation| accessdate=August 26, 2009}}&amp;lt;/ref&amp;gt; The maximum amount of time that a satellite in a normal low Earth orbit mission can spend in the Earth&#039;s shadow occurs at a beta angle of zero.  In such an orbit, the satellite is in sunlight no less than 59% of the time.&amp;lt;ref name=&amp;quot;mcc&amp;quot;/&amp;gt;&amp;lt;ref name=&amp;quot;knk&amp;quot;/&amp;gt;&lt;br /&gt;
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==Light and shadow==&lt;br /&gt;
The degree of orbital shadowing an object in LEO experiences is determined by that object&#039;s beta angle. An object launched into an initial orbit with an inclination equivalent to the complement to the Earth&#039;s inclination to the ecliptic results in an initial beta angle of 0 degrees (&amp;lt;math&amp;gt;\beta&amp;lt;/math&amp;gt; = 0°) for the orbiting object. This allows the object to spend the maximum possible amount of its [[orbital period]] in the Earth&#039;s shadow, and results in extremely reduced absorption of solar energy.  At a LEO of 280 kilometers the object in orbit is in sunlight through 59% of its orbit (approximately 53 minutes in sunlight, and 37 minutes in shadow.&amp;lt;ref name=&amp;quot;knk&amp;quot;/&amp;gt;) On the other extreme, an object launched into an orbit that follows the [[Terminator (solar)|terminator]]  results in a beta angle of 90 degrees (&amp;lt;math&amp;gt;\beta&amp;lt;/math&amp;gt; = 90°), and the object is in sunlight 100% of the time.&amp;lt;ref name=&amp;quot;knk&amp;quot;/&amp;gt; An example would be a polar orbit initiated at local dawn or dusk on an [[equinox]].  These orbits can be taken advantage of to keep a satellite as cool as possible for instruments that require low temperatures, such as infrared cameras, by keeping the beta angle as close to zero as possible, or conversely to keep a satellite in sunlight as much as possible for conversion of sunlight by its solar panels, for solar stability of sensors, or to study the sun by maintaining a beta angle as close to +90 or -90 as possible.&lt;br /&gt;
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==Determination and Application of beta angles==&lt;br /&gt;
&lt;br /&gt;
The above discussion defines the beta angle of satellites orbiting the Earth, but a beta angle can be calculated for any orbiting three body system: the same definition can be applied to give the beta angle of other objects.  For example, the beta angle of a satellite in orbit around Mars, with respect to the Earth, defines how much of the time the satellite has a line of sight to the Earth - that is, it determines how long the Earth is shining on the satellite and how long the Earth is blocked from view.  That same satellite also will have a beta angle with respect to the Sun, and in fact it has a beta angle for any celestial object one might wish to calculate one for: any satellite orbiting a body (i.e. the Earth) will be in that body&#039;s shadow with respect to a given celestial object (like a star) some of the time, and in its line-of-sight the rest of the time.  Beta angles describing non-[[geocentric]] orbits are important when space agencies launch satellites into orbits around other bodies in the solar system.&lt;br /&gt;
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==Importance in Spaceflight==&lt;br /&gt;
&lt;br /&gt;
When the [[space shuttle]] was in service on missions to the [[International Space Station]], the beta angle of the space station&#039;s orbit was a crucial consideration; periods referred to as &amp;quot;beta cutout&amp;quot;,&amp;lt;ref name=&amp;quot;mcc&amp;quot;/&amp;gt; during which the shuttle could not safely be launched to the ISS, were a direct result of the beta angle of the space station at those times.  When the orbiter was in-flight (not docked to ISS) and it flew to a beta angle greater than 60 degrees, the orbiter went into &amp;quot;rotisserie&amp;quot; mode, and slowly rotated around its X-axis (nose to tail axis). For flights to ISS, the shuttle could launch during an ISS beta cutout if the ISS would be at a beta less than 60 degrees at dock, and throughout the docked phase.{{Citation needed|date=June 2009}} Therefore, the mission duration affected launch timing when the beta cutout dates were approaching.&lt;br /&gt;
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==See also==&lt;br /&gt;
*[[International Space Station]]&lt;br /&gt;
*[[Low Earth Orbit]]&lt;br /&gt;
*[[Launch window]]&lt;br /&gt;
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==References==&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
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==External links==&lt;br /&gt;
*[http://spaceflight.nasa.gov/station/flash/start.swf NASA: ISS Beta Angle]&lt;br /&gt;
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{{DEFAULTSORT:Beta Angle}}&lt;br /&gt;
[[Category:Spaceflight]]&lt;br /&gt;
[[Category:Earth orbits]]&lt;br /&gt;
[[Category:Astrodynamics]]&lt;/div&gt;</summary>
		<author><name>220.239.181.223</name></author>
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