
Hello, as I would say for this well...uhh I may sound weird for that...hehe. This page is about Titan, I just didn't show it in my profile lol, for now I'd say that this is educational...this is related from Level -61 and Scientific Cosmology Coalition. - Author, I think that the name doesn't suit the level format, so I would consider moving this later.
Part of the Hall of Knowledge or Scientific Cosmology Coalition
Also uhh, I'm gonna complete this since yk 'bout Huygens lol
Ok not to be goofy, but the "This page...they made for me" is some entity shit, basically even if this page was intentionally made for Huygens, it's not him.
Please understand the fact that this is part of the SCC lore 😭, I swear I'm gonna add anomalous properties to suit the Backrooms theme.
Description -
Titan is the largest moon from the "Saturnian System" and being the second-largest moon from the "Solar System" we're all capable and know, it's just being specifically a copycat here in Level -61, perhaps I don't know if any other levels has the similar suspicious property equivalent to the Level -61. For now we know, Titan is the only moon that has the dense atmosphere and being the only known object in Solar System to have a stable body of surface liquid (We make exceptions for Earth). Titan is 50% larger (in diameter) than Earth's Moon and 80% more massive. As I mentioned, Titan is the second-largest moon of the "Solar System" after "Jupiter's" largest moon and being the first-largest moon from the "Solar System" Ganymede. Fun fact, Titan was the first known discovered moon from the 'Saturnian System", it was discovered in 1655 by a Dutch astronomer and a physician "Sir, Christiaan Huygens", which is gonna be named after our mission to honor him (pls fanfiction wise :(( go follow Huygen's mission to!!!), after as "Sir, Jean-Dominique Cassini" made four discoveries: Iapetus (1671), Rhea (1672), Dione (1684), and Tethys (1684). Titan is primarily composed of ice and rocky material, which is likely differentiated into a rocky core surrounded by various layers of ice, including a crust of ice Ih and a subsurface layer of ammonia-rich liquid water. The atmosphere of Titan is largely nitrogen; minor components lead to the formation of methane and ethane clouds and heavy organonitrogen haze. The climate—including wind and rain—creates surface features similar to those of Earth, such as dunes, rivers, lakes, seas (probably of liquid methane and ethane), and deltas, and is dominated by seasonal weather patterns as on Earth. With its liquids (both surface and subsurface) and robust nitrogen atmosphere, Titan's methane cycle bears a striking similarity to Earth's water cycle, albeit at the much lower temperature of about 94 K (−179 °C; −290 °F).
💧︎♒︎♏︎ ⬥︎♋︎⬧︎ ⧫︎♒︎♏︎ 📖︎♓︎■︎♎︎ □︎♐︎ ♐︎❒︎♓︎♏︎■︎♎︎ ⍓︎□︎◆︎ ⬥︎□︎◆︎●︎♎︎ ◻︎♏︎❒︎♒︎♋︎◻︎⬧︎ ⧫︎□︎ ♌︎♏︎ ⬥︎♓︎⧫︎♒︎ ⧫︎□︎♑︎♏︎⧫︎♒︎♏︎❒︎ ♌︎◆︎⧫︎ ■︎□︎⧫︎ ♐︎□︎❒︎♏︎❖︎♏︎❒︎ ◻︎●︎♏︎♋︎⬧︎♏︎ ✋︎'❍︎ ⬥︎♋︎♓︎⧫︎♓︎■︎♑︎ ♐︎□︎❒︎ ⍓︎□︎◆︎ ♒︎♏︎❒︎♏︎📪 ⬧︎□︎❍︎♏︎⬥︎♒︎♏︎❒︎♏︎ ♎︎❒︎♋︎⬧︎⧫︎♓︎♍︎ ♋︎■︎♎︎ ♐︎◆︎⧫︎♓︎●︎♏︎📪 ♌︎♏︎⍓︎□︎■︎♎︎ ⍓︎□︎◆︎❒︎ ♒︎□︎❍︎♏︎ 👌︎♋︎♍︎&︎❒︎□︎□︎❍︎⬧︎
✌︎◆︎♎︎♓︎□︎ ♎︎♓︎⬧︎⧫︎□︎❒︎♓︎♏︎■︎⧫︎♋︎⧫︎♓︎□︎■︎
👇♏︎'⬧︎ ♋︎ ■︎□︎⧫︎ ♋︎ ⬧︎♒︎♏︎
I'm scared.
Can't list down rn, WIPP.
What is the Cassini-Huygens mission? -
Cassini-Huygens mission is a proposed mission to Saturn, collaboration between the NASA and ESA (European Space Agency), not to forget ISA (Italian Space Agency), the mission is suppose to send space probe's to study Saturn, specifically Huygens-Probe to study the largest moon of Saturn being the second largest from the Solar System "Titan", well of course the moon being the main star of this page....or Huygens...perhaps both of them! Hehe....Cassini was the fourth space probe to visit Saturn and the first to enter its orbit, where it stayed from 2004, perhaps I don't know how long did Cassini stayed (Backrooms wise ehem). The two craft took their names from the astronomers Giovanni Cassini and Christiaan Huygens.
History/Discovery -
Titan was discovered on March 25, 1655, by a Dutch astronomer Sir, Christiaan Huygens as far as I know from "reality" I sound ironic, but well perhaps we should kept it to itself and it's discovery and no we didn't originally discovered it. Him sir, Huygens was inspired by Galileo's discovery of Jupiter's four largest moons in 1610 and his improvements in telescope technology. With the help of his elder brother.
Christiaan Huygens - (I exactly don't know if I should make a separated page for him)
AM I ACTUALLY.....😭
Giovanni Cassini -
Giovanni Domenico CassiniGiovan Domenico Cassini or Gian Domenico Cassini. Jean-Dominique Cassini (8 June 1625 – 14 September 1712) is a Italian born (naturalized French) mathematician, astronomer, engineer, and a astrologer. Cassini is known for his work on astronomy and engineering. He discovered four satellites of the planet Saturn and noted the division of the rings of Saturn; the Cassini Division was named after him. Giovanni Domenico Cassini was also the first of his family to begin work on the project of creating a topographic map of France. Am I a hypocrite for making his description short and making Huygens longer? Well, he's also the main point of the page anyways, I have mixed it anyways lol
Atmosphere -
Titan is by far the only known moon that has the significant atmosphere, it's atmosphere is the only nitrogen-rich dense atmosphere from the Solar System aside for Earth...what's Earth? Observations that Titan's atmosphere is denser than Earth, with a surface pressure around 1.45 standard atmosphere. Likely to be 1.19 times massive as Earth, should we stop comparing Titan to Earth? I don't think so. Titan's lower gravity means that it's atmosphere is far more extended than Earth. The atmosphere of Titan opaque at many wavelengths and as a result, a complete reflectance spectrum of the surface is impossible to acquire from orbit.
There are trace amounts of other hydrocarbons, such as ethane, diacetylene, methylacetylene, acetylene and propane, and of other gases, such as cyanoacetylene, hydrogen cyanide, carbon dioxide, carbon monoxide, cyanogen, argon and helium. The hydrocarbons are thought to form in Titan's upper atmosphere in reactions resulting from the breakup of methane by the Sun's ultraviolet light, producing a thick orange smog. Titan spends 95% of its time within Saturn's magnetosphere, which may help shield it from the solar wind.
Energy from the Sun should have converted all the traces of methane in Titan's atmosphere into more complex hydrocarbon within 30-milion years ago. The ultimate origin of the methane in its atmosphere may be its interior, released via eruptions from cryovolcanoes.
In our observation within Titan's atmosphere, propene was detected in the atmosphere of Titan. It was the first chemical that we have found from any other moon body of the solar system aside from Earth as I know before I went into this hellhole.
Orbit & Rotation -
Titan orbits Saturn once every 15 days 22 hours. Like many other satellite body from the "Solar System" is identical to the orbital period. Titan is tidally locked in synchronous rotation with Saturn, and permanently shows one face to the planet. Longitudes on Titan are measured westward, starting from the meridian passing through this point. Its orbital eccentricity is 0.0288, and the orbital plane is inclined 0.348 degrees relative to the Saturnian equator.
Lakes, Dry Lakes, Seas, Rivers. -
Titan has a possibility hydrocarbon seas. Liquid methane on Titan, either in disconnected pockets or on the scale of satellite-wide oceans, similar to water on Earth. Titan has many plenty of lakes, dry lakes, seas, and rivers including. (Listed down base of how many)
Sea's -
Sea Ligeia or Ligeia Mare --
Ligeia Mare has two predominant types of coastline, "crenulated" and "subdued". The former is characterized by hummocky, eroded terrain, the latter by lower, smoother topography and the presence of more numerous and longer channels. Crenulated terrain predominates on the eastern and southern sides of the lake; subdued terrain to the west and north. Except in the southeast where the rough topography extends to the coast, hummocky terrain tends to be separated from the shoreline by a more subdued bench. The coast has numerous bays that appear to be flooded river mouths (rias), and unlike at Ontario Lacus there are no visible subaerial delta deposits, possible evidence of a recent sea level rise. In the northeast and northwest sections of the mare, along about a quarter of the total shoreline, there are extensive areas where the depth is less than 5 m, shallow enough for imaging radar to penetrate to the bottom.
The average depth is on the order of 50 m, while the maximum depth is probably > 200 m. The total volume is likely to be > 7000 km3.
Hydrology in Ligeia Mare ---
The reason for Ligeia Mare's nearly pure methane composition are still not clear within us. Studying further more within our research, assuming that "ethane" would be the primary constituent of Titan's seas. 2 CH4 → H2 + C2H6
Sea Kraken Mare or Kraken Mare --
500,000 km2 Kraken Mare as we thought to be the largest body liquid from Titan's surface in north polar region. Its status as a sea of hydrocarbons (mainly liquid methane) was identified by radar imagery. Kraken Mare is thought to be larger than the Caspian Sea on Earth...as I would say I've already know about this (" Well where's Earth? " Shut up). Kraken Mare is at least 100 m deep and likely deeper than 300 m. One of its northernmost bays (Moray Sinus) has a depth of 85 (−18, +28) m at its center and shows an attenuation of the signal in the liquid that is compatible with a composition of 70% methane, 16% nitrogen and 14% ethane (assuming ideal mixing). Shallow capillary waves 1.5 centimeters high moving at 0.7 meters per second have been detected on the surface of Kraken Mare.
Kraken Mare, along with other Lakes of Titan, was first discovered by the Cassini–Huygens space probe on July 22, 2006. This was accomplished by noticing that certain dark regions, especially near the poles, had low radar reflectivity, as well as similar morphological features to that of terrestrial lakes.
Mayda Insula ---
We've all heard of the Cassini-Huygens mission that is launched in Oct 15, 1997 right? (But in Backrooms wise, you know it you know). Well so call "Reality". Mayda Insula is a island in the Kraken Mare and it was discovered by the mission called "Cassini-Huygens", hmmm I remember before going into this hellhole place. Mayda Insula lies in the northern end of the Kraken Mare near Titan's north pole. The island has a northernmost latitude of 80.3 degrees north and a southernmost latitude of 77.4 degrees north; it has a westernmost longitude of approximately 321.2 degrees west and an easternmost longitude of 302.7 degrees west. The island is 168 kilometres (104 mi) wide at its widest point.
The highest point of the interior of Mayda Insula is approximately 1,200 metres (3,900 ft) above its shoreline. Slopes are relatively mild at approximately 1.5 degrees on average, though they can approach 5 degrees in some locations.
"Sea" or Lake Punga Mare or Punga Mare --
Punga Mare, is a lake in the north polar region of Titan, the planet Saturn's largest moon. After Kraken Mare and Ligeia Mare, it is the third largest known body of liquid on Titan. It is composed of liquid hydrocarbons (mainly methane and ethane). Located almost adjacent to the north pole at 85.1° N, 339.7° W, it measures roughly 380 km (236 mi) across, greater than the length of Lake Victoria on Earth. Its surface area is ~61,000 km2 (23,522 sq. mi). Its namesake is Punga, in Māori mythology ancestor of sharks, rays and lizards and a son of Tangaroa, the god of the sea.
Lakes -
Lakes of Titan are the body liquids with ethane and methane that is detected by the Cassini-Huygens (WIP PAGE) mission. The largest known is the Maria and the small one is Lacūs.
Titan's lakes are disappearing during the summer times, the amount of energy that is transferred into it's lakes was the higher ones at other times.
Abaya Lacus Lake --
Abaya Lacus is one of a number of hydrocarbon lakes found on Saturn's largest moon, Titan. Abaya Lacus is composed with liquid methane and ethane, it was detected by the Cassini-Huygens mission.
Bolsena Lacus Lake --
Bolsena Lacus is one of a number of hydrocarbon lakes found on Saturn's largest moon, Titan. It is situated in a north polar region where the majority of Titan's large lakes are found. Bolsena Lacus is composed with liquid methane and ethane, it was detected by the Cassini-Huygens mission in 2007.
Feia Lacus Lake --
Feia Lacus is one of a number of hydrocarbon seas and lakes found on Saturn's largest moon, Titan. Feia Lacus is composed with liquid methane and ethane, it was named after the lake "Loagoa Feia" in Brazil. Detected by the Cassini-Huygens mission.
Hammar Lacus Lake --
Hammar Lacus is one of a number of hydrocarbon seas and lakes found on Saturn's largest moon, Titan. At 200 km in diameter it is the third largest lake on Titan. It was named after the lake in the southern Iraq called Hammar Lake.
Jingpo Lacus Lake --
Jingpo Lacus is a lake in the north polar region of Titan. It and similarly sized Ontario Lacus. It is composed of liquid hydrocarbons (mainly methane and ethane). It is west of Kraken Mare at 73° N, 336° W, roughly 240 km (150 mi) long, similar to the length of Lake Onega on Earth. Its namesake is Jingpo Lake, a lake in China.
Colonies and Outpost
Not feasible even if may be habitable. There is so far no evidence of life on Titan, we be needing respirators and a warm clothing within it's temperature.
Entrance and Exits
This "Level" or just sub-layer can only be accessed via Space Rocket.












