Baby step in converting Python docstrings to Markdown.

source/python/README.md

@@ -7,58 +7,51 @@
 ---
 
 <a name="BodyCode"></a>
-### BodyCode(name) -> astronomy.Body
+### BodyCode(name) &#8658; astronomy.Body
 Finds the Body enumeration value, given the name of a body.
 
-Parameters
-----------
 name: str
     The common English name of a supported celestial body.
 
-Returns
--------
 Body
     If `name` is a valid body name, returns the enumeration
     value associated with that body.
     Otherwise, returns `Body.Invalid`.
 
-Example
--------
 
->>> astronomy.BodyCode('Mars')
-<Body.Mars: 3>
+&gt;&gt;&gt; astronomy.BodyCode('Mars')
+&lt;Body.Mars: 3&gt;
+
 
 
 ---
 
 <a name="GeoMoon"></a>
-### GeoMoon(time: astronomy.Time) -> astronomy.Vector
+### GeoMoon(time: astronomy.Time) &#8658; astronomy.Vector
 Calculates the geocentric position of the Moon at a given time.
 
 Given a time of observation, calculates the Moon's position as a vector.
 The vector gives the location of the Moon's center relative to the Earth's center
 with x-, y-, and z-components measured in astronomical units.
 
-This algorithm is based on Nautical Almanac Office's <i>Improved Lunar Ephemeris</i> of 1954,
+This algorithm is based on Nautical Almanac Office's *Improved Lunar Ephemeris* of 1954,
 which in turn derives from E. W. Brown's lunar theories from the early twentieth century.
 It is adapted from Turbo Pascal code from the book
 [Astronomy on the Personal Computer](https://www.springer.com/us/book/9783540672210)
 by Montenbruck and Pfleger.
 
-Parameters
-----------
 time : Time
     The date and time for which to calculate the Moon's position.
 
-Returns
--------
 Vector
     The Moon's position as a vector in J2000 Cartesian equatorial coordinates.
 
 
+
 ---
 
 <a name="unique"></a>
 ### unique(enumeration)
 Class decorator for enumerations ensuring unique member values.
 
+

source/python/astronomy.py

@@ -362,7 +362,7 @@ class Time:
         such as calculating rise/set times, culumination, and anything involving apparent
         sidereal time.
         Before the era of atomic timekeeping, days based on the Earth's rotation
-        were often known as <i>mean solar days</i>.
+        were often known as *mean solar days*.
     tt : float
         Terrestrial Time days since noon on January 1, 2000.
         Terrestrial Time is an atomic time scale defined as a number of days since noon on January 1, 2000.
@@ -372,7 +372,7 @@ class Time:
         for changes in the Earth's rotation.
         The value in `tt` is used for calculations of movements not involving the Earth's rotation,
         such as the orbits of planets around the Sun, or the Moon around the Earth.
-        Historically, Terrestrial Time has also been known by the term <i>Ephemeris Time</i> (ET).
+        Historically, Terrestrial Time has also been known by the term *Ephemeris Time* (ET).
     """
     def __init__(self, ut):
         self.ut = ut
@@ -2021,7 +2021,7 @@ def GeoMoon(time:Time) -> Vector:
     The vector gives the location of the Moon's center relative to the Earth's center
     with x-, y-, and z-components measured in astronomical units.
 
-    This algorithm is based on Nautical Almanac Office's <i>Improved Lunar Ephemeris</i> of 1954,
+    This algorithm is based on Nautical Almanac Office's *Improved Lunar Ephemeris* of 1954,
     which in turn derives from E. W. Brown's lunar theories from the early twentieth century.
     It is adapted from Turbo Pascal code from the book
     [Astronomy on the Personal Computer](https://www.springer.com/us/book/9783540672210)