Difference between revisions of "Help:Math"

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The acceleration of a solar sail due to solar pressure <math>\vec a_s</math> given the position vector from the sun to the sail <math>\vec r_s</math> is:
 
The acceleration of a solar sail due to solar pressure <math>\vec a_s</math> given the position vector from the sun to the sail <math>\vec r_s</math> is:
  
  <math>\vec a_s = a_c {AU^2 \over r_s^2} \(\vec r_s \cdot \vec n\)^2 \vec n</math>
+
  <math>\vec a_s = a_c {AU^2 \over r_s^2} \left(\vec r_s \cdot \vec n\right)^2 \vec n</math>
  
 
where <math>a_c</math> is max sail acceleration at Earth's distance from the sun (1 AU), <math>AU</math> is the length of an astronomical unit, <math>r_s</math> is the magnitude of <math>\vec r_s</math>, and <math>\vec n</math> is the unit vector normal to the sail surface.
 
where <math>a_c</math> is max sail acceleration at Earth's distance from the sun (1 AU), <math>AU</math> is the length of an astronomical unit, <math>r_s</math> is the magnitude of <math>\vec r_s</math>, and <math>\vec n</math> is the unit vector normal to the sail surface.

Latest revision as of 11:32, 11 June 2012

LaTeX

You can enter LaTeX equations by enclosing them in <math>...</math> tags. This uses the Math extension. For LaTeX math help, see:

Examples

<math>\sqrt[3]{a x + x^2}</math> produces \sqrt[3]{a x + x^2}

The acceleration of a solar sail due to solar pressure \vec a_s given the position vector from the sun to the sail \vec r_s is:

\vec a_s = a_c {AU^2 \over r_s^2} \left(\vec r_s \cdot \vec n\right)^2 \vec n

where a_c is max sail acceleration at Earth's distance from the sun (1 AU), AU is the length of an astronomical unit, r_s is the magnitude of \vec r_s, and \vec n is the unit vector normal to the sail surface.

Mimetex

Deprecated. Please follow LaTeX instructions from now on.

Mathematics can be displayed on SolarSailWiki using the Mimetex program, which uses a subset of the LaTeX math formulas. All you need to do is enclose a valid TeX/LaTeX formula inside <tex>...</tex> tags. Formulas will be rendered as GIF images.

Some examples:

<tex>\sqrt[3]{a x + x^2}</tex> produces \sqrt[3]{a x + x^2}

The acceleration of a solar sail due to solar pressure \vec a_s given the position vector from the sun to the sail \vec r_s is:

\vec a_s = a_c {AU^2 \over r_s^2} \(\vec r_s \cdot \vec n\)^2 \vec n

where a_c is max sail acceleration at Earth's distance from the sun (1 AU), AU is the length of an astronomical unit, r_s is the magnitude of \vec r_s, and \vec n is the unit vector normal to the sail surface.