Skip to content

Commit 8a32e96

Browse files
committed
change the NASA link and archiving on the solar system activty
1 parent 891d74d commit 8a32e96

7 files changed

Lines changed: 1047 additions & 3 deletions

File tree

‎docs/activities.html‎

Lines changed: 1 addition & 1 deletion
Original file line numberDiff line numberDiff line change
@@ -2010,7 +2010,7 @@ <h5 class="no-anchor card-title listing-title">
20102010
</div>
20112011
</div></a>
20122012
</div>
2013-
<div class="g-col-1" data-index="50" data-categories="SW50cm8lMjBIUyUyQ0FzdHJvbm9teSUyQ1NwYWNlJTJDRGF0YSUyMFNjaWVuY2UlMkNTcHJlYWRzaGVldHM=" data-listing-file-modified-sort="1781401709119" data-listing-reading-time-sort="2" data-listing-word-count-sort="362">
2013+
<div class="g-col-1" data-index="50" data-categories="SW50cm8lMjBIUyUyQ0FzdHJvbm9teSUyQ1NwYWNlJTJDRGF0YSUyMFNjaWVuY2UlMkNTcHJlYWRzaGVldHM=" data-listing-file-modified-sort="1782614003652" data-listing-reading-time-sort="2" data-listing-word-count-sort="362">
20142014
<a href="./projects/solarsystem.html" class="quarto-grid-link">
20152015
<div class="quarto-grid-item card h-100 card-left">
20162016
<p class="card-img-top">
Lines changed: 170 additions & 0 deletions
Original file line numberDiff line numberDiff line change
@@ -0,0 +1,170 @@
1+
<html>
2+
3+
<head>
4+
5+
<title>Planetary Fact Sheet Notes</title>
6+
</head>
7+
8+
<body bgcolor="FFFFFF">
9+
10+
<p> <!-- text and html formatting by drw at n.s.s.d c -->
11+
<hr>
12+
<h1>Planetary Fact Sheet Notes</h1>
13+
<hr>
14+
15+
<p><a name="mass"></a>
16+
<p>
17+
<b>Mass</b> (10<sup>24</sup>kg or 10<sup>21</sup>tons) - This is the mass of the planet in septillion
18+
(1 followed by 24 zeros) kilograms or sextillion (1 followed by 21 zeros) tons. Strictly speaking tons
19+
are measures of weight, not mass, but are used here to represent the mass of one ton of material under
20+
Earth gravity.
21+
</p><a name="diam"></a>
22+
<p>
23+
<b>Diameter</b> (km or miles) - The diameter of the planet at the equator, the distance through
24+
the center of the planet from one point on the equator to the opposite side, in kilometers or miles.
25+
</p><a name="dens"></a>
26+
<p>
27+
<b>Density</b> (kg/m<sup>3</sup> or lbs/ft<sup>3</sup>) - The average density (mass divided by volume) of
28+
the whole planet (not including the atmosphere for the terrestrial planets) in kilograms per cubic meter
29+
or pounds per cubic foot. Strictly speaking pounds are measures of weight, not mass, but are used here to
30+
represent the mass of one pound of material under Earth gravity.
31+
</p><a name="grav"></a>
32+
<p>
33+
<b>Gravity</b> (m/s<sup>2</sup> or ft/s<sup>2</sup>) - The gravitational acceleration on the surface at
34+
the equator in meters per second squared or feet per second squared, including the effects of rotation.
35+
For the gas giant planets the gravity is given at the 1 bar pressure level in the atmosphere. The gravity
36+
on Earth is designated as 1 "G", so the Earth ratio fact sheets gives the gravity of the other planets in G's.
37+
</p><a name="escv"></a>
38+
<p>
39+
<b>Escape Velocity</b> (km/s) - Initial velocity, in kilometers per second or miles per second, needed
40+
at the surface (at the 1 bar pressure level for the gas giants) to escape the body's gravitational pull,
41+
ignoring atmospheric drag.
42+
</p><a name="rotp"></a>
43+
<p>
44+
<b>Rotation Period</b> (hours) - This is the time it takes for the planet to complete one rotation
45+
relative to the fixed background stars (not relative to the Sun) in hours. Negative numbers indicate
46+
retrograde (backwards relative to the Earth) rotation.
47+
</p><a name="leng"></a>
48+
<p>
49+
<b>Length of Day</b> (hours) - The average time in hours for the Sun to move from the noon position in the
50+
sky at a point on the equator back to the same position.
51+
</p><a name="dist"></a>
52+
<p>
53+
<b>Distance from Sun</b> (10<sup>6</sup> km or 10<sup>6</sup> miles) - This is the average distance from
54+
the planet to the Sun in millions of kilometers or millions of miles, also known as the semi-major axis.
55+
All planets have orbits which are elliptical, not perfectly circular, so there is a point in the orbit at
56+
which the planet is closest to the Sun, the perihelion, and a point furthest from the Sun, the aphelion.
57+
The average distance from the Sun is midway between these two values. The average distance from the Earth
58+
to the Sun is defined as 1 Astronomical Unit (AU), so the ratio table gives this distance in AU.<br>
59+
* For the Moon, the average distance from the Earth is given.
60+
</p><a name="peri"></a>
61+
<p>
62+
<b>Perihelion, Aphelion</b> (10<sup>6</sup> km or 10<sup>6</sup> miles) - The closest and furthest points
63+
in a planet's orbit about the Sun, see "Distance from Sun" above.<br>
64+
* For the Moon, the closest and furthest points to Earth are given, known as the "Perigee" and "Apogee"
65+
respectively.
66+
</p><a name="orbp"></a>
67+
<p>
68+
<b>Orbital Period</b> (days) - This is the time in Earth days for a planet to orbit the Sun from one
69+
vernal equinox to the next. Also known as the tropical orbit period, this is equal to a year on Earth.<br>
70+
* For the Moon, the sidereal orbit period, the time to orbit once relative to the fixed background
71+
stars, is given. The time from full Moon to full Moon, or synodic period, is 29.53 days.
72+
For Pluto, the tropical orbit period is not well known, the sidereal orbit period is used.
73+
</p><a name="orbv"></a>
74+
<p>
75+
<b>Orbital Velocity</b> (km/s or miles/s) - The average velocity or speed of the planet as it orbits the
76+
Sun, in kilometers per second or miles per second.<br>
77+
* For the Moon, the average velocity around the Earth is given.
78+
</p><a name="orbi"></a>
79+
<p>
80+
<b>Orbital Inclination</b> (degrees) - The angle in degrees at which a planets orbit around the Sun is
81+
tilted relative to the ecliptic plane. The ecliptic plane is defined as the plane containing the Earth's
82+
orbit, so the Earth's inclination is 0.
83+
</p><a name="orbe"></a>
84+
<p>
85+
<b>Orbital Eccentricity</b> - This is a measure of how far a planet's orbit about the Sun (or the Moon's
86+
orbit about the Earth) is from being circular. The larger the eccentricity, the more elongated is the
87+
orbit, an eccentricity of 0 means the orbit is a perfect circle. There are no units for eccentricity.
88+
</p><a name="orbo"></a>
89+
<p>
90+
<b>Obliquity to Orbit</b> (degrees) - The angle in degrees the axis of a planet (the imaginary line running
91+
through the center of the planet from the north to south poles) is tilted relative to a line
92+
perpendicular to the planet's orbit around the Sun, north pole defined by right hand rule.<br>
93+
*Venus rotates in a retrograde direction, opposite the other planets, so the tilt is almost 180
94+
degrees, it is considered to be spinning with its "top", or north pole pointing "downward" (southward).
95+
Uranus rotates almost on its side relative to the orbit, Pluto is pointing slightly "down". The ratios
96+
with Earth refer to the axis without reference to north or south.
97+
</p><a name="temp"></a>
98+
<p>
99+
<b>Mean Temperature</b> (C or F) - This is the average temperature over the whole planet's surface
100+
(or for the gas giants at the one bar level) in degrees C (Celsius or Centigrade) or degrees F
101+
(Fahrenheit). For Mercury and the Moon, for example, this is an average over the sunlit (very
102+
hot) and dark (very cold) hemispheres and so is not representative of any given region on the planet,
103+
and most of the surface is quite different from this average value. As with the Earth, there will tend
104+
to be variations in temperature from the equator to the poles, from the day to night sides, and seasonal
105+
changes on most of the planets.
106+
</p><a name="surp"></a>
107+
<p>
108+
<b>Surface Pressure</b> (bars or atmospheres) - This is the atmospheric pressure (the weight of the
109+
atmosphere per unit area) at the surface of the planet in bars or atmospheres.<br>
110+
*The surfaces of Jupiter, Saturn, Uranus, and Neptune are deep in the atmosphere and the location and
111+
pressures are not known.
112+
</p><a name="sats"></a>
113+
<p>
114+
<b>Number of Moons</b> - This gives the number of IAU officially confirmed moons orbiting the planet. New
115+
moons are still being discovered.
116+
</p><a name="ring"></a>
117+
<p>
118+
<b>Ring System?</b> - This tells whether a planet has a set of rings around it, Saturn being the most
119+
obvious example.
120+
</p><a name="magf"></a>
121+
<p>
122+
<b>Global Magnetic Field?</b> - This tells whether the planet has a measurable large-scale magnetic
123+
field. Mars and the Moon have localized regional magnetic fields but no global field.
124+
</p>
125+
<p>
126+
The term "terrestrial planets" refers to Mercury, Venus, Earth, Moon, Mars, and Pluto.<br>
127+
The term "gas giants" refers to Jupiter, Saturn, Uranus, and Neptune.
128+
</p>
129+
<p>
130+
<hr>
131+
132+
133+
<a href="index.html">
134+
<img alt=" " src="https://nssdc.gsfc.nasa.gov/bullet/red_bullet_half.gif"> Planetary Fact Sheet - Metric
135+
Units</a><br>
136+
137+
<a href="planet_table_british.html">
138+
<img alt=" " src="https://nssdc.gsfc.nasa.gov/bullet/red_bullet_half.gif"> Planetary Fact Sheet - U.S.
139+
Units</a><br>
140+
141+
<a href="planet_table_ratio.html">
142+
<img alt=" " src="https://nssdc.gsfc.nasa.gov/bullet/red_bullet_half.gif"> Planetary Fact Sheet - Values compared
143+
to Earth</a><br>
144+
145+
146+
<a href="https://nssdc.gsfc.nasa.gov/planetary/planetfact.html">
147+
<img alt=" " src="https://nssdc.gsfc.nasa.gov/bullet/red_bullet_half.gif"> Index of Planetary Fact Sheets</a>
148+
- More detailed fact sheets for each planet<br>
149+
150+
151+
<hr>
152+
153+
<address>
154+
Author/Curator:<br>
155+
Dr. David R. Williams, <a href="mailto:dave.williams@nasa.gov">dave.williams@nasa.gov</a><br>
156+
NSSDCA, Mail Code 690.1<br>
157+
NASA Goddard Space Flight Center<br>
158+
Greenbelt, MD 20771<br>
159+
+1-301-286-1258<br>
160+
</address>
161+
<br clear="left">
162+
<hr>
163+
<h6>NASA Official: Dave Williams, david.r.williams@nasa.gov<br>
164+
165+
166+
Last Updated: 20 December 2021, DRW</h6>
167+
168+
</body>
169+
170+
</html>

‎docs/projects/solarsystem.html‎

Lines changed: 1 addition & 1 deletion
Original file line numberDiff line numberDiff line change
@@ -189,7 +189,7 @@ <h2 class="anchored" data-anchor-id="instructions">Instructions</h2>
189189
<p><b>Imagine that your town or school has asked you to design a solar system model.</b></p>
190190
<p><b>Step 1.</b> Decide how big your solar system model will be. For example, you can choose a football field, basketball court, classroom, a long straight sidewalk, etc. Each group should choose something different. Some teachers order a roll of recipt paper (like for a cash register) and give each group a different length of receipt paper.</p>
191191
<p><a href="../solar_system.csv">Download this CSV file with the planets and their distances to the sun and open it in a spreadsheet program</a></p>
192-
<p><b>Note:</b> This CSV file uses solar system data from this <a href="planet_table_ratio.html">NASA website</a></p>
192+
<p><b>Note:</b> This CSV file uses solar system data from this <a href="solarsystem_data.html">NASA website</a></p>
193193
<p><b>Step 2.</b> Configure columnn C in the spreadsheet so that it takes the distance in column B and divides it by the scale (Advice: <a href="https://www.youtube.com/watch?v=HRzfHcgDvyk">This youtube video that was mentioned earlier is helpful for this task</a> )</p>
194194
<p><b>Step 3.</b> Change the scale to make sure that the model distance to Pluto is roughly the same as your solar system model (Advice: the scale should be <b>much</b> larger than 1)</p>
195195
</section>

0 commit comments

Comments
 (0)