Content commit
Signed-off-by: Nikolaos Karaolidis <nick@karaolidis.com>
This commit is contained in:
26
js/data/Callisto.js
Normal file
26
js/data/Callisto.js
Normal file
@@ -0,0 +1,26 @@
|
||||
export const content = `
|
||||
<p>
|
||||
Callisto is the second-largest moon of Jupiter and the third-largest moon in the Solar System.
|
||||
Known for its heavily cratered surface, it is the most heavily cratered object in the Solar System.
|
||||
This suggests a long history of impacts.
|
||||
</p>
|
||||
<img src="https://4.bp.blogspot.com/-Zyyh91K02Rg/WIGipjPlwKI/AAAAAAAABK4/57NjPSVDI7ch6JtmL0ghWBXfmVOQTw2hQCLcB/s1600/callisto.jpg"/>
|
||||
<h2>Key Facts</h2>
|
||||
<ul>
|
||||
<li>Orbital Period: About 16.69 days</li>
|
||||
<li>Diameter: Approximately 4,820 km</li>
|
||||
<li>Surface: Characterized by a mix of ice and rock</li>
|
||||
<li>Average Distance from Jupiter: About 1,882,700 km</li>
|
||||
<li>Orbital Speed: Approximately 8.204 km/s</li>
|
||||
</ul>
|
||||
<h2>Surface and Composition</h2>
|
||||
<p>
|
||||
Callisto's surface is a mix of ice and rock, with a possible subsurface ocean beneath its icy crust. Its lack of an atmosphere and geological activity implies a very stable surface.
|
||||
</p>
|
||||
<h2>Interesting Facts</h2>
|
||||
<ul>
|
||||
<li>Callisto is thought to have the lowest density of all the Galilean moons, indicating a high composition of water ice.</li>
|
||||
<li>Unlike other Galilean moons, Callisto does not experience significant tidal heating, which accounts for its lack of geological activity.</li>
|
||||
<li>Callisto is considered a prime candidate for future space missions due to its relatively low radiation levels compared to other Jovian moons.</li>
|
||||
</ul>
|
||||
`;
|
Reference in New Issue
Block a user