 ### Fixing three bugs in blackbody.docbook:

```73930: Misspelled "Wien's Law"

73931: Incomplete phrase:  actually, this phrase is not incomplete.  If
you look at the handbook, you'll see that the last part of the sentence
is an equation presented as an image in the document.  However, to make
the sentence a bit clearer, I have changed it to:  "For example, the
sun has an average temperature of 5800 K, so its wavelength of maximum
emission is given by:"

73932: Misspelled "Stefan-Boltzmann Law"

CCMAIL: 73930-done@bugs.kde.org
CCMAIL: 73931-done@bugs.kde.org
CCMAIL: 73932-done@bugs.kde.org

svn path=/trunk/kdeedu/doc/kstars/; revision=284250```
parent 1058bfa9
 ... ... @@ -95,8 +95,8 @@ following equation: where T is the temperature in Kelvin. Wein's law (also known as Wein's displacement law) states that the where T is the temperature in Kelvin. Wien's law (also known as Wien's displacement law) states that the wavelength of maximum emission from a blackbody is inversely proportional to its temperature. This makes sense; shorter-wavelength (higher-frequency) light corresponds to ... ... @@ -105,8 +105,8 @@ higher-temperature object. For example, the sun has an average temperature of 5800 K with a wavelength of maximum emission equal to For example, the sun has an average temperature of 5800 K, so its wavelength of maximum emission is given by: ... ... @@ -144,7 +144,7 @@ from a blackbody increase by a factor of 2^4 or 16. Five years later, Austrian physicist Ludwig Boltzman derived the same equation and is now known as the Stephan-Boltzman law. If we assume a equation and is now known as the Stefan-Boltzman law. If we assume a spherical star with radius R, then the luminosity of such a star is ... ... @@ -158,7 +158,7 @@ spherical star with radius R, then the luminosity of such a star is where R is the star radius in cm, and the alpha is the Stephan-Boltzman constant, which has the value: Stefan-Boltzman constant, which has the value: ... ...
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