recursal/Fanatic-Fandom huggingface dataset:
Arrows

The base diamethyst arrows are crafted from a diamethyst shard, a stick, and a feather. The arrows can be used as is, or they can be upgraded to include additional effects. The arrows fly further and have greater accuracy than normal arrows when fired from a Diamethyst Bow.

### Diamethyst Golden Arrow

##### Special Abilities

* Set struck enemies on fire for 5 seconds (configurable).

### Diamethyst Copper Arrow

##### Special Abilities

* Weakens struck enemies for 5 seconds (configurable).

### Diamethyst Charged Copper Arrow

##### Recipe

* The diamethyst charged copper arrow cannot be crafted. It is obtained by causing lightning to strike a diamethyst copper arrow using the method outlined below.

##### Obtaining

To charge diamethyst copper arrows, they must be fired into a diamethyst block, and that block must then be struck by lightning. Once the lightning hits the block, all embedded diamethyst copper arrows will be charged up and ready for use. The easiest way to cause lightning to strike the diamethyst block is to attach a lightning rod to the top of the block and wait for a thunder storm. Alternatively, a diamethyst charged coper arrow can be fired at the block to cause the lightning strike. Each time the arrows are hit by lightning, their life counter is reset to 2 minutes.

##### Special Abilities

* Weakens struck enemies for 5 seconds (configurable).
* Causes a lightning bolt to strike at the point of impact. If the arrow hits the ground, it can be collected but will need to be charged up again before it will cause another lightning strike.

### Diamethyst Iron Arrow

##### Special Abilities

* Pierces 1 struck enemy (configurable).
* Breaks certain mineable blocks when hit (configurable).

### Diamethyst Lapis Arrow

##### Special Abilities

* Confuses struck enemies for 5 seconds (configurable).

### Diamethyst Emerald Arrow

##### Special Abilities

* Poisons struck enemies for 5 seconds (configurable).
* Generates a poison cloud when it lands (configurable). The default poison cloud duration is 15 seconds. The cloud forms in a three block layer around the origin point. The center layer is 4 blocks wide and the upper and lower layer is 2 blocks wide. The cloud cannot be spawned in water. Any mob entering the cloud will receive the same poison effect as if struck by the arrow itself. Hitting the ground instead of a mob is a good way to poison a group of mods. The cloud size and duration are fully configurable.

### Diamethyst Diamond Arrow

##### Special Abilities

* Freezes struck enemies for 5 seconds (configurable).
* Turns water into ice (configurable). From version 1.6.2 and above, the type of ice that is formed when the arrow makes contact with water can be changed in the config. The default ice block can be changed to frosted ice if desired.

### Advancements

* Crafting a diamethyst arrow will gain the advancement "**Draw the Line!**".
* Crafting a gold, copper, iron, lapis, emerald, or diamond arrow will gain the advancement "**Don't Get Mad, Get Even!**".
Hatari

**Hatari** is a character in **Celestial Guardians** and is a **Chosen One**.

# Personal

## Appearance

Hatari is a fair-skinned young adult with magenta hair tied into a ponytail with a purple hair tie and her hair has a heart-shaped ahoge and her eyes are lime green. She wears a purple midriff top with spiked shoulder pads and a matching skirt with a pastel pink star on the left side, white stockings and purple flats. Her jewelry include a pastel pink choker with a magenta heart, a beaded pastel pink bracelet on her right hand and a magenta armband on her left arm.

## Personality

Hatari is optimistic and determined, but occasionally shows a perfectionist side.
Diamethyst Geode

An **diamethyst geode** is an extremely rare custom feature found in the underground of the Overworld. Diamethyst geodes contain smooth basalt, calcite, amethyst blocks, and budding diamethyst blocks. The geode was introduced in Diamethysts! version 1.6.0 for Minecraft versions 1.17.1 and above.

### Generation

Diamethyst geodes generate between Y=-40 and Y=-50 for Minecraft 1.18.2 and above, or Y=15 and Y=6 for Minecraft 1.17.1. Each chunk has a 1⁄600 chance to attempt to generate a diamethyst geode.

### Structure

Diamethyst geodes consist of three layers: an outer layer of smooth basalt, a middle layer of calcite, and a hollow layer of primarily amethyst blocks, with 8.3% replaced by budding diamethyst blocks instead. Diamethyst clusters generate within the structure on budding diamethyst blocks. Diamethyst geodes have a 95% chance of generating with a crack, exposing its inside. Caves, aquifers, and canyons may be overridden by geodes, and as such are often obstructed by them.
Totem of Restoration

The Totem of Restoration is a rare artifact that can sometimes be found in chests near ruined nether portals. The totem is unstable and will randomly repair damaged items throughout your inventory when used - which in turn damages the totem. If there are no damaged items in your inventory, the totem is not used. It initially has 200 durability, and cannot be repaired or enchanted. The totem cannot be used to repair other totems.

The totem can be combined with a Totem of Rejuvenation and make a Totem of Renew.
Diamethyst Cluster

**Diamethyst Buds** are the first three stages of growth of diamethyst clusters, which grow on a budding diamethyst block.

**Diamethyst Clusters** are the fourth and final growth stage of diamethyst buds, which drop diamethyst shards when mined.

### Obtaining

##### Breaking

The diamethyst cluster block itself in any of its growth stages (rather than its diamethyst shard drops) can be obtained by mining it with any tool with the Silk Touch enchantment.

When mined without Silk Touch or broken by being pushed off an attached block by a piston or sticky piston, only fully grown diamethyst clusters drop diamethyst shards, while diamethyst buds drop nothing. Breaking a diamethyst cluster with a pickaxe drops 4 shards while any other method of breaking it yields 2 shards. The maximum amount of diamethyst shards dropped can be increased with Fortune; Fortune I gives a 1⁄3 chance for 8 shards (averaging 5.33 shards), Fortune II gives a 25% chance (each) to give 8 or 12 shards (averaging 7 shards), and Fortune III gives a 20% chance (each) to give 8, 12, or 16 shards (averaging 8.8 shards).

##### Natural generation

Diamethyst buds and clusters generate naturally as part of diamethyst geodes, on exposed faces of budding diamethyst blocks.

##### Budding diamethyst

Every random game tick there is a 20% chance for a budding diamethyst block to spawn a small diamethyst bud on any of its sides, as long as the block being replaced with the small diamethyst bud is air or a water source block.

### Usage

##### Growing into diamethyst clusters

A diamethyst bud placed on a budding diamethyst block (rather than any other block) regardless whether it was placed by the player or spawned by the budding diamethyst block itself grows over time, going through three growth stages – small, medium, and large – before reaching its 4th and final growth stage as a diamethyst cluster, which drops diamethyst shards when mined.

##### Decoration

They can also be placed on certain other types blocks for decoration. Most blocks have not yet been tested, but it seems that they can be placed only on full blocks, or those sides of blocks that form a full surface. They can be placed on the bottom of stairs (or top of upside down stairs), but not on their side, or top. And they can not be placed on any type of fences.

##### Light

Small, medium and large diamethyst buds give off a light level of 1, 2 and 4 respectively, while diamethyst clusters give off a light level of 5.
Sedna

Sedna

(90377) Sedna is a large trans-Neptunian object that was, as of 2012, about three times as far from the Sun as Neptune. Spectroscopy has revealed that Sedna's surface composition is similar to that of some other trans-Neptunian objects, being largely a mixture of water, methane and nitrogen ices with tholins. Its surface is one of the reddest in the Solar System. It is probably a dwarf planet.

For most of its orbit it is even farther from the Sun than at present, with its aphelion estimated at 937 astronomical units (31 times Neptune's distance), making it one of the most distant known objects in the Solar System other than long-period comets. Sedna's exceptionally long and elongated orbit, taking approximately 11,400 years to complete, and distant point of closest approach to the Sun, at 76 AU, have led to much speculation about its origin.

The Minor Planet Center currently places Sedna in the scattered disc, a group of objects sent into highly elongated orbits by the gravitational influence of Neptune. However, this classification has been contested, because Sedna never comes close enough to Neptune to have been scattered by it, leading some astronomers to conclude that it is in fact the first known member of the inner Oort cloud. Others speculate that it might have been tugged into its current orbit by a passing star, perhaps one within the Sun's birth cluster (an open cluster), or even that it was captured from another star system. Another hypothesis suggests that its orbit may be evidence for a large planet beyond the orbit of Neptune.

Astronomer Michael E. Brown, co-discoverer of Sedna and the dwarf planets Eris, Haumea, and Makemake, believes it to be the most scientifically important trans-Neptunian object found to date, because understanding its unusual orbit is likely to yield valuable information about the origin and early evolution of the Solar System. Sedna (provisionally designated 2003 VB12) was discovered by Mike Brown (Caltech), Chad Trujillo (Gemini Observatory) and David Rabinowitz (Yale University) on November 14, 2003. The discovery formed part of a survey begun in 2001 with the Samuel Oschin telescope at Palomar Observatory near San Diego, California using Yale's 160 megapixel Palomar Quest camera. On that day, an object was observed to move by 4.6 arcseconds over 3.1 hours relative to stars, which indicated that its distance was about 100 AU.

Follow-up observations in November–December 2003 with the SMARTS telescope at Cerro Tololo Inter-American Observatory in Chile as well as with the Tenagra IV telescope at the W. M. Keck Observatory in Hawaii revealed that the object was moving along a distant highly eccentric orbit. Later the object was identified on older precovery images made by the Samuel Oschin telescope as well as on images from the Near Earth Asteroid Tracking consortium. These previous positions expanded its known orbital arc and allowed a more precise calculation of its orbit.

## Moons

Sedna has no Known Moons, But it might be overshined by Sedna Itself. If Sedna does have a moon, it would most likely be a Captured Asteroid.
Dione

Dione, a moon of Saturn

Dione is a small Saturnian moon. Still, Dione is the 15th largest moon in the Solar System, more massive than all known moons smaller than itself combined.

## Rotated

Heavily cratered areas on Dione are unexpectedly located on the trailing hemisphere, so it has been theorized that a more recent impact spun Dione around 180 degrees.
Iapetus

The 2 Shaded Moon

Iapetus is the third-largest natural satellite of Saturn and eleventh-largest in the Solar System. Its two-tone coloration makes it one of the most unusual of Saturn's moons.

## Contrast

The terrain on Iapetus' leading hemisphere is one of the darkest in the Solar System. In contrast, the trailing hemisphere is very bright and the dividing line between the areas remains extremely sharp.
Planet X

Hypothetical Planet X

Planet X is a Hypothetical Blue Gas Giant around 30,000 kilometers in Diameter. It was probably ejected into the Oort Cloud and possibly interstellar space, when it got too close too Neptune or Uranus. It is unknown if it is still orbiting the Sun, but if it is, it’s Perihelion is 950 billion km, and it’s Aphelion is 1.7 trillion km. It may have storms.

## Moons

Planet X Probably has moons, although it is unknown how many. They would probably be captured asteroids.

## Composition

Planet X would probably have the atmosphere made of Hydrogen, Helium, and Methane, like the other ice giants.

## Doomsday

People thought that the Planet X could Collide and destroy Earth on the 21st of December, 2012, although this never happened.
Phobos

Phobos

Phobos is the larger and closer of the two natural satellites of Mars. It is a small, irregularly shaped object, closer to its primary than any other known planetary moon.

## Proximity

Phobos is so close that it orbits Mars faster than Mars rotates. As a result, from the surface of Mars it appears to rise and set twice each Martian day.

## Collision

Phobos is drawing closer to Mars and in 50 million years it will either collide with the planet or break up into a planetary ring.
Ariel

Ariel

Ariel is the fourth largest of Uranus' moons. Ariel's surface shows signs of more recent geological activity and appears to be the youngest of all the moons of Uranus.

## Surface

The most striking feature of Ariel is the complex network of deep rift valleys crisscrossing the entire surface of the moon. These canyons are very similar to those on Mars.
Eris

Eris, in all it’s Bright, White, Shiny Beauty!

136199 Eris is a dwarf planet, once Considered the 10th Planet. It is located in the Scattered Disk. Eris was discovered in 2003 and given the temporary name "2003 UB313". It was later formally changed to Eris and it is the farthest known Dwarf Planet. Eris is white in Color.

## Very Tilted Orbit

Eris has a more tilted orbit then Ceres, (10 degrees), Pluto (17 degrees) and Makemake (28 degrees). Its orbit is inclined at a whooping 44 degrees similar to that of the hypothetical Tyche and is so tilted that it crosses the orbits of Makemake and Pluto. It has a Diameter of 2,326 km.

## Name

Funny Enough, Eris was named after the Roman god of Chaos, because of the “Pluto is not a Planet” Debate. Before it was Officially Named, the Discoverers called it “Xena” from the TV Show.

## Moons

Eris has 1 currently known moon, named Dysnomia. Dysnomia is about 700 km in Diameter. It is Probably Grayish in Color, and was Captured by Eris when it got too close.

## Exploration

Eris has not been Explored by any Spacecraft Yet. It was Calculated it would take Approximately 24+ years to get to Eris using a Jupiter Gravity Assist.
Battle Axes

Diamethyst battle axes are crafted with a leather bound stick, four diamethyst crystals, and one of the following base materials: gold ingot, iron ingot, copper ingot, lapis lazuli, prismarine shard, emerald, or diamond. The damage caused by a battle axe increases based upon the materials used to craft it. Each battle axe type has its own special ability. Battle axes are twice as slow as a sword, but do more damage and have more durability.

### Golden Battle Axe

##### Special Ability

* Sets hit entities on fire for 5 seconds.

### Iron Battle Axe

##### Special Ability

* Inflicts wither damage on hit entities for 5 seconds.

### Netherite Battle Axe

##### Special Abilities

* Sets hit entities on fire for 5 seconds.
* Poisons hit entities for 5 seconds.

### Advancements

* Crafting a gold, copper, iron, lapis, prismarine, emerald, or diamond battle axe will gain the advancement "**Be Battle Ready!**".
* Smithing a netherite battle axe will gain the advancement "**My Old Battle Axe!**".
Diamethysts! Wiki

**Welcome to the Diamethysts! Wiki!**
Wiki about the Diamethysts! mod for Minecraft.

This wiki is a work in progress and more content will be added soon. Below are links to WIP pages. The main page will be restructured once more content is added.

Weapons

Tools

Armor

Horse Armor

Items

Blocks

Artifacts

Potions

Features
*Need help building out this community?*

* Rules of this wiki
* Getting Started
* How to Contribute
* Managing your new community
* Guides
* All Help articles

You can also be part of the larger Fandom family of communities. Visit Fandom's Community Central!

*Community Founders*: Write a good and paragraph-length description for your welcome section about your topic. Let your readers know what your topic is about and add some general information about it. Then you should visit the admin dashboard for more tips.
Ceres

Ceres, by Dawn

Ceres is a Asteroid Belt Inhabitant, and the Smallest Dwarf Planet. Ceres is large enough to maintain hydrostatic equilibrium, Even under extremely dark skies, Ceres is still very difficult to spot due to its apparent magnitude to Earth for the naked eye, as for any dwarf planet.

## Formation

Ceres is the closest dwarf planet to the Sun. This could mean that Ceres was formed from the remains of a rocky planet that was collided into with a massive asteroid. The remains are believed to have created the Asteroid belt. The active asteroids in this belt began to collide, created heat which fused the asteroids and once they gathered enough material became the Ceres We know Today.

## Surface

The surface of Ceres is similar to that of some C-type asteroids that are found inside the Asteroid belt. The infrared color spectrum, however, shows high amounts of water under the surface! Carbon minerals are present on Ceres' surface, rising the theory that it might have been formed from carbonaceous meteorites.

## Temperature

Relatively warmer than most dwarf planets due to its distance from the Sun, Ceres has an average surface temperature of 200 degrees Kelvin or about -40 degrees Fahrenheit. The temperature of the surface may be affected by the atmospheric conditions, for water frost reaches the surface, making it colder even when the Sun is over the dwarf planets surface. Some of the water frost can become permanent and make layers of ice visible on the surface. It is believed if this continues, Ceres will have ice caps, similar to that of Earth and Mars, that could have life.

## Exploration

Ceres has only been explored by a Probe Once, that was the Dawn Mission, that got the first Close Up images of the Dwarf.

## Atmosphere

It is believed Ceres might have a weak atmosphere, therefore high amounts of solar radiation cannot be kept out. The solar radiation that breaks through the atmosphere collides with surface water created by melted water frost. The radiation then heats up the solid water frost left on the surface, and turns it into a gas without turning it into a solid first, which is called sublimation!
Charon

Charon in False Color

Charon also known as  (134340) Pluto I, is the largest of the five known moons of the dwarf planet Pluto. It was discovered in 1978 at the United States

Naval Observatory in Washington, D.C., using photographic plates taken at the United States Naval Observatory Flagstaff Station (NOFS). With half the diameter and one eighth the mass of Pluto, it is a very large moon in comparison to its parent body. Its gravitational influence is such that the barycenter of the Pluto–Charon system lies outside Pluto itself.

## Exploration

The *New Horizons* spacecraft, to date the only probe to have visited the Pluto system, approached within 27,000 km (17,000 mi) of Charon.
Miranda

The “Frankenstein Moon”

Miranda is the smallest and innermost of Uranus's five major moons. Despite its tiny size, Miranda has one of the strangest and most varied landscapes among extraterrestrial bodies.

## Unusual

Miranda is unlike any other body in the Solar System. It looks as if several pieces of rock were assembled randomly together. Its surface features include huge faults, canyons, cliffs, smooth plains, and curiously shaped rifts.
Callisto

Callisto in false color

Callisto is a satellite belonging to the outer planet, Jupiter. It is one of the Galilean moons, a group of the largest moons in the Solar System that were discovered by Galileo Galilei. Callisto was founded by Galileo Galilei on January 7, 1610, the same day as Ganymede, also a Galilean moon, and the largest moon in the Solar System, was discovered. Callisto is probably the oldest moon of Jupiter.

## Composition

Callisto is composed of water ice, carbon dioxide, and other compounds. About one hundred kilometers under the surface of Callisto, there is an ocean, much like any other Galilean moons and other moons of Jupiter.

## Surface and Craters

The surface of Callisto is extremely cratered. There are no signs of volcanism, or any other forms of volcanic activity, or any other signs of surface disrupt. It shows that there have been severe cases of impacts, meaning this moon has an extremely thin atmosphere. The surface is covered with white streaks and valleys caused by these collisions. As these collisions began to pile up, the surface began to become more fragile. And due to the thin atmosphere, Callisto surface became very vunerable to these asteroid impacts. It is believed that in the next 1 million years, Callisto's surface will begin to wear away, causing Callisto to star collapsing on its self.

## Atmosphere

The atmosphere of Callisto is completely surrounded with an extremely thin layer of carbon dioxide and possibly molecular oxygen. There is also an intense layer called the ionosphere, which is an atmosphere full of active ions that reflect radio waves
Luna (Earth’s Moon)

The Moon

Luna, (also Known as Earth I) more commonly referred to as the Moon, is the Earth's natural satellite and is the 5th largest spherical moon in the Solar System. Yet, it is the largest in the Solar System in relation to its host planet, being only one-fourth smaller than Earth. Our moon is Monstrously Ginormous for a Moon.

## Formation

The Moon was formed by a Large, Mars Sized Object named Theia Crashing into the Earth and Spraying Materials Everywhere. A Few Million Years Passed, and the Moon has Formed from the Debris. The Moon was then Bombarded by Asteroids and Comets.

## Structure

The **interior structure** of the Moon is similar to the Earth. The first layer is dirt and the second layer is crust. The beginning of the internal structure is the mantle. Under the moon's upper mantle is a small space.

## Phases of the Moon

There are 8 Phases of the Moon. The New Moon, the Waxing Crescent, the First Quarter, the Waxing Gibbous, the Full Moon, the Waning Gibbous, the Last Quarter, and the Waining Cresent.
Champion

## Overview

The Champion is a tank class which seeks to draw aggro, control the enemy through stuns and slows, and can withstand more punishment than other classes. They can specialize in the use of One Handed Weapons and Shields in order to focus on their primary role, or use a Two Handed Weapon (such as a Great Axe) to increase the damage they deal. Alongside the more aggressively-focused Rogue, the Champion's primary stat is Attack Power.

## Abilities and bonuses

### **Class weapon bonuses**

* **Armsmaster**\*: Increases Melee Attack Power by 10%, Attack Speed by 20%, and Armor by 5% when using a Shield.
* **Recklessness**: Increases Melee Power by 25%, Critcal Damage by 15%, Armor Penetration by 30 and Reduces Armor by 5% when using a Two Handed Weapon.

\*Armsmaster will only apply if both the main-hand weapon and the Shield in use are Melee damage weapons; i.e. it will not activate with a Melee damage Axe and a Magic damage shield.

### **Abilities by level**

 1
 2
 3
 4
 5
 6
 7
 15
Asteroid belt

The Asteroid belt is a Cluster of Asteroids orbiting the Sun Between Mars and Jupiter. It’s most Popular Objects are Ceres, Vesta, Pallas, Juno, and Hygeia.

### Satellites

Is physically not able to have satellites

## Formation

The Asteroid belt could have been formed by a Large planet in the Region being destroyed. It is possible that the Largest Asteroids, or some of the big Moons from the Gas Giants could have been it’s Moons.
Quaoar

Quaoar, in Blue

50000 Quaoar, provisional designation 2002 LM60, is a non-resonant trans-Neptunian object (cubewano) and a dwarf planet canadate in the Kuiper belt, located in one of the farthest regions inside of the Solar System. It measures approximately 1110 kilometers in diameter or half the size of Pluto. The object was discovered by American astronomers Chad Trujillo and Michael Brown at the Palomar Observatory on 6 June 2002.

## Moons

### Weywot

Quaoar has one known moon, named Weywot (full designation *(50000) Quaoar I Weywot*). Its discovery by Michael E. Brown was reported in IAUC 8812 on 22 February 2007, based on imagery taken on 14 February 2006. The satellite was found at 0.35 arcsec from Quaoar with an apparent magnitude difference of 5.6. Weywot Is Extremely Thin!

## Naming

Quaoar and Weywot are named after mythological figures from the Native American Tongva people. In Tongva mythology, Quaoar (also known as Kwawar, or Chinigchinix) was the creator of the universe. His son Weywot and he was the "sky god"
Ixion

Ixion in Red

28978 Ixion, provisional designation 2001 KX76, is a large trans-Neptunian object and a possible dwarf planet. It is located in the Kuiper belt, a region of icy objects orbiting beyond Neptune in the outer Solar System. Ixion is classified as a plutino, a dynamical class of objects in a 2:3 orbital resonance with Neptune.

## Discovery

Ixion was discovered on 22 May 2001 by a team of American astronomers at the Cerro Tololo Inter-American Observatory in Chile. American astronomers James Elliot and Lawrence Wasserman identified Ixion in digital images of the southern sky taken with the 4-meter Víctor M. Blanco Telescope at Cerro Tololo.

## Size

Compared to Pluto and its moon Charon, Ixion is approximately one-fourth the diameter of Pluto and half the diameter of Charon.
X (Оригинальный канон)

Появление X покрыто тайной.

## Война Анонимуса (2021)

Во время штурма сопротивлением штаба Анонимуса в Юнион-Сити, тот сталкивается с Геральтом, вырубая того сильным ударом по печени, после чего отправляется вместе с Анонимусом на научную базу.

Уже там он сначала сталкивается с T800, упустив его, а после второй раз сталкивается с Геральтом, когда сопротивление штурмует лабораторию, однако в этот раз X не смог ни убить его, ни уложить спать: ему помешал Марио, выстрелив в него из РПГ.

## Личность

X - кто-то вроде телохранителя Анонимуса. Он крайне опасен и на данный момент сопротивление не знаёт способа устранить его.
Scattered Disc

The Scattered Disc is a Belt of objects beyond the Kuiper Belt. The objects here were scattered by Neptune in the early solar system. The Most notable

## Scattered Disc

A Diagram of Eris, Pluto, the Kuiper Belt, and other objects.

### Extent

40-100 AU

objects here are Eris, and Gonggong. The Scattered Disc is also home to a lot of other icy bodies.

## Formation

As mentioned earlier, the objects here were ejected out here by Neptune’s Gravity. they could’ve also been ejected by the Jupiter/Saturn renaissance.
Makemake

Makemake, the 4th Dwarf

136472 Makemake is a dwarf planet and perhaps the largest Kuiper belt object (KBO) in the classical population, with a diameter that is around 2/3 the size of Pluto.

Its extremely low average temperature, about 30 K (−243.2 °C), means its surface is covered with methane, ethane, and possibly nitrogen ices. It has a Diameter of 1,430 km.

Initially known as 2005 FY9 and later given the minor-planet number 136472, it was discovered on March 31, 2005, by a team led by Michael Brown, and announced on July 29, 2005. Makemake was recognized as a dwarf planet by the International Astronomical Union (IAU) in July 2008. Its name derives from Makemake in the mythology of the Rapanui people of Easter Island.

### MK 2

S/2015 (136472) 1, nicknamed MK 2 by the discovery team, is the only known moon of Makemake. It is estimated to be 175 km (110 mi) km in diameter (for an assumed albedo of 4%) and has a semi-major axis at least 21,000 km (13,000 mi) from Makemake. Its orbital period is ≥ 12 days (the minimum values are those for a circular orbit; the actual orbital eccentricity is unknown). Observations leading to its discovery occurred in April 2015, using the *Hubble Space Telescope*'s Wide Field Camera 3 and its discovery was announced on 26 April 2016.
Rhea

Rhea, the Moon of Saturn

Rhea is the second-largest moon of Saturn and the ninth largest moon in the Solar System. It is also one of the most heavily cratered satellites in the Solar System.

## Resurfaced

Rhea's features could be divided into two regions: The brighter and more heavily cratered areas and the areas in the polar and equatorial region. This difference may indicate there was a major resurfacing event some time in Rhea's history.

## Rings

Rhea may have a tenuous ring system consisting of three narrow, relatively dense bands within a particulate disk. This would be the first discovery of rings around a moon. The potential discovery was announced in the journal *Science* on March 6, 2008.
Orcus

What Orcus May look like

(**90482) Orcus** is a Trans-Neptunian object and a likely Dwarf Planet. Located in the Kuiper belt region beyond the orbit of Neptune, and it is a small body around the size of Ceres. it has 1 Moon.

## Moons

It has a Moon named Vanth. Vanth is the Third Largest Dwarf Planet Moon, behind Eris’ Dysnomia, and Pluto’s Charon. It is a Third of the size of Orcus itself.
Gonggong

Shaded Gonggong

(225088) Gonggong, also known as 2007 OR10, is a binary Trans-Neptunian object and a likely Dwarf planet orbiting the Sun in the scattered disc, approximately 1,200 kilometers (764 miles) in diameter. It is the fifth-largest known body in the Solar System beyond the orbit of Neptune. it is slightly smaller than Makemake, and is hence almost certainly a dwarf planet. It has one known moon, approximately 300 kilometers (190 miles) in diameter.

## Xiangliu

The slow rotation rate of Gonggong, compared to the other TNOs, raised the possibility of a satellite that slowed down the rotation via tidal dissipation. In 2016, analysis of Hubble images of Gonggong taken in 2010 revealed a satellite around 300 km in diameter and orbiting at a distance of at least 15,000 km. It was announced at the DPS48 meeting on 17 October 2016. The satellite is probably too small and dark to affect size estimates for Gonggong. Further analysis from May 2017 confirms this orbiting moon.
Vanth

Non rounded Vanth

Vanth, full designation (90482) Orcus I Vanth, is the single known natural satellite of the plutino and likely dwarf planet 90482 Orcus. With a diameter of about 440 km, it is half the size of Orcus and probably the third-largest known moon of a known trans-Neptunian object, after Pluto I Charon and Eris I Dysnomia, though it is possible that the poorly resolved Varda I Ilmarë or Haumea I Hiʻiaka might be comparable in size.

## Discovery

Vanth was discovered by Michael Brown and T.-A. Suer using discovery images taken by the Hubble Space Telescope on 13 November 2005. The discovery was announced in an IAU Circular notice published on 22 February 2007.

## Characteristics

Vanth was found at 0.25 arcseconds from Orcus with magnitude difference of 2.7±1.0.Estimates made in 2009 by Brown show that the apparent magnitude of Vanth is 21.97±0.05 which is 2.54±0.01 magnitudes fainter than Orcus. Assuming equal albedos this would mean a diameter of 280 km (170 mi), or 2.9 times smaller than the primary.However, the dissimilar colors of Orcus (neutral) and Vanth (red) suggest that Vanth could have an albedo a factor of two lower than Orcus. Should Vanth have an albedo of only 0.12, Vanth could be as large as 380 km (240 mi) with Orcus being 760 km (470 mi) in diameter. The mass of Vanth also depends on its albedo and can vary from 3 to 9 percent of the total system mass. In 2016, Brown and Butler used resolved ALMA images and estimated Vanth's diameter at 480 km (300 mi), about half Orcus's diameter, making Orcus and Vanth a smaller version of the Pluto and Charon System.
Tethys

Rotation of Tethys

Tethys is the fifth-largest moon of Saturn. Its low density and a very bright surface indicates that it is made of water ice with only a small fraction of rock.

## Crater

The western hemisphere dominates a huge impact crater, Odysseus, with nearly 2/5 the size of the entire moon. It's not known why this impact didn't shatter the moon but it is theoretized Tethys may have been in a semi-liquid state at the time of the impact.
Ganymede

Picture of Ganymede from the Juno spacecraft in 2021.

Ganymede, also called Jupiter I, is the largest moon in the entire Solar System, the largest of the Galilean moons, and the largest of Jupiter's moons.

Ganymede is bigger than the Planet Mercury. This moon belongs to the planet Jupiter, which is ironically the largest planet in the Solar System. Ganymede is one of the Galilean moons, which were discovered by Galileo Galilei. Ganymede was discovered on January 7, 1610. It is a member of the Galilean moons, meaning it maintains hydrostatic equilibrium, meaning it can maintain a nearly round shape, showing it has a sufficient amount of mass. Ganymede could also be Discovered by Simon Marius.

## Composition

A saltwater ocean is believed to exist or have existed beneath Ganymede's surface, but about 200 km deep. The ocean is believed to be sandwiched between different silicate, rocky, watery, and icy layers.

## Surface

Ganymede's surface is mostly covered with rocky caverns and craters from asteroid impacts. The rest of Ganymede is made up of light regions with crosscuts similar to the Earth's moon.
Neptune

Neptune is the 8th Planet from the Sun. Neptune is an ice giant like Uranus but with a more dark tint of blue. Neptune was discovered on September 23,

### Satellites

14

1846 by 3 astronomers: John Couch Adams, Urban Le Verrier, and Johann Galle. Neptune has 14 known satellites. Its biggest moon is Triton.

## Formation

Neptune's core formed from a clump of rocky material that was around 2 ~ 5 times in Earth's mass. Its core gathered enough gas to become a Gas planet.

## Composition

Neptune's atmosphere is made of the same materials as Uranus, Methane, Ammonia, and Small Parts of Hydrogen and Helium. with small amounts of ice in the inner atmosphere and its core composed of mostly metallic materials and rock.

Because Neptune and Uranus are so similar, they have been de-categorized from the term of gas giants like Jupiter and Saturn, and Neptune and Uranus have been categorized with the term of "ice giants" due to there being an exceptional amount of freezing compounds of Carbon and Ammonia in the atmosphere, which can lead to frozen water in the atmosphere and the surface.

## Internal Structure

The internal structure of Neptune is similar to that of the neighboring planet of Uranus. The first layer is the mantle, which makes up the mass of Neptune. The mantle consists of a water-ammonia compound and methane. In fact, the water-ammonia compound makes up so much of the mantle, scientists refer to it as a water-ammonia ocean. The core of Neptune is mostly made up rock silicates such as iron and nickel.

## Rings of Neptune

Neptune has its own collection of rings called the Rings of Neptune. These rings were discovered in the La Silla Observatory in Chile by Reinhold Häfner, Patrice Bouchet, and Jean Manfred. These rings very lowly dense. Even at their densest, they are only as dense as the lesser dense parts of Saturn's rings. The innermost moons in the rings include Despina, Naiad, Thalassa, and Galatea. The outermost moons in the rings include Larissa and Prometheus. The Rings could be made of a Moon of Neptune that got very close in the Past, and then got Broken Apart into different Pieces, that soon became rings.

## Orbit and Rotation

Neptune makes only one orbit around the Sun in about 168.2 Ea5th years. This is because Neptune is more than 2 billion miles from the Sun.

Because of its gaseous nature, Neptune's equatorial rotation is equal to 18 Earth hours. Yet since the wind speeds towards the poles are faster, the polar rotation is equal to around 12 Earth hours.

## Atmosphere

Most of the atmosphere of Neptune is made up of Hydrogen, making up more than 80% of the atmosphere. The rest is made of Helium, Methane, Hydrogen, Deuteride, and Ethane.

## Great Dark Spot

A Famous Feature on Neptune is the Great Dark Spot. It had Wind Speeds up to 1,500 Mph! Prior to 1998, Hubble had Detected that the Storm had Dissipated.

## Moons

Neptune has 14 moons. The Biggest is Triton.
Puck

Puck, the Scarred Moon

Puck is an inner moon of Uranus. It was discovered in December 1985 by the *Voyager 2* spacecraft. The orbit of Puck lies between the rings of Uranus and the first of Uranus's large moons, Miranda. Puck is approximately spherical in shape and has diameter of about 162 km. It has a dark, heavily cratered surface, which shows spectral signs of water ice.

## Name

The name Puck follows the convention of naming Uranus's moons after characters from Shakespeare. The moon was later named after the character Puck who appears in Shakespeare's *A Midsummer Night's Dream*, a little sprite who travels around the globe at night with the fairies.
Proteus

Cratered Proteus

Proteus, also known as Neptune VIII, is the second-largest Neptunian moon, and Neptune's largest inner satellite. Discovered by *Voyager 2* spacecraft in 1989, it is named after Proteus, the shape-changing sea god of Greek mythology. Proteus orbits Neptune in a nearly equatorial orbit at a distance of about 4.75 times the radius of Neptune's equator. Despite being a predominantly icy body more than 400 km (250 mi) in diameter, Proteus's shape deviates significantly from an ellipsoid. It is shaped more like an irregular polyhedron with several slightly concave facets and relief as high as 20 km (12 mi). Its surface is dark, neutral in color, and heavily cratered.

## Formation

Proteus is probably not an original body that formed with Neptune. It could have accreted later from the debris formed when the largest Neptunian satellite Triton was captured. Triton's orbit upon capture would have been highly eccentric, and would have caused chaotic perturbations in the orbits of the original inner Neptunian moons, causing them to collide and reduce to a disc of rubble. This is when Proteus was born.
Varuna

Artist Impression of Varuna

20000 Varuna, or 2000 WR106, is a large trans-Neptunian object in the Kuiper belt. It is named after the Hindu deity Varuna.

## Discovery

Varuna was discovered by American astronomer Robert McMillan using the Spacewatch 0.9-meter telescope during a routine survey on 28 November 2000. The Spacewatch survey was conducted by McMillan at the Kitt Peak National Observatory near Tucson, Arizona. At the time of discovery, Varuna was located at a moderately dense star field close to the northern galactic equator. Although Varuna was not detected by McMillan's real-time computer software, he was able to identify Varuna moving slowly among the background stars by manually comparing multiple scans of the same region using the blinking technique. follow-up observations of Varuna were conducted by astronomer Jeffrey Larsen in order to confirm the object. By the end of Larsen's observing shift, both McMillan and Larsen had made a total of 12 observations that spanned three nights.

## Physical Characteristics

Varuna's light curve is compatible with the body being a Jacobi ellipsoid, suggesting that it has an elongated shape due to its rapid rotation. Varuna's surface is moderately red in color due to the presence of complex organic compounds on its surface. Water ice is also present on its surface, and is thought to have been exposed by past collisions which may have also caused Varuna's rapid rotation.

## Moons

Although no natural satellites have been found or directly imaged around Varuna, analysis of variations in its light curve in 2019 suggests the presence of a possible satellite orbiting closely around Varuna.
Europa

Europa
Size
5,268.2km
Mass
1.4819x1023 kg
Parent Planet
Jupiter
Ganymede, also called Jupiter I, is the largest moon in the entire Solar System, the largest of the Galilean moons, and the largest of Jupiter's moons.
Ganymede is bigger than the Planet Mercury. This moon belongs to the planet Jupiter, which is ironically the largest planet in the Solar System. Ganymede is one of the Galilean moons, which were discovered by Galileo Galilei. Ganymede was discovered on January 7, 1610. It is a member of the Galilean moons, meaning it maintains hydrostatic equilibrium, meaning it can maintain a nearly round shape, showing it has a sufficient amount of mass. Ganymede could also be Discovered by Simon Marius.
Composition
A saltwater ocean is believed to exist or have existed beneath Ganymede's surface, but about 200 km deep. The ocean is believed to be sandwiched between different silicate, rocky, watery, and icy layers.
Surface
Ganymede's surface is mostly covered with rocky caverns and craters from asteroid impacts. The rest of Ganymede is made up of light regions with crosscuts similar to the Earth's moon.
Gallery/Images
Io

Io
--

Io, the “Volcano Moon”

Io, is the innermost of the Galilean moons belonging to the outer planet of Jupiter. It is also the 4th largest moon in the solar system. Io is a moon of active volcanoes and lava flowing all around the surface of the planet. Io constantly has erupting volcanoes. In fact, Io is the most active object in the Solar System because of its volcanoes. In fact, each black spot on the picture you see is a volcano. This moon was discovered by the astronomer Galileo Galilei on January 8, 1610. It is the fourth-largest natural satellite in the entire solar system.

## Surface

Io is full of active volcanoes. Some of these volcanoes are dormant, or extinct volcanoes. The active volcanoes are erupting constantly and can fire ash and cinders 300 km above the surrounding surface. One of these active volcanoes is named Prometheus, not to be confused with the moon of Saturn with the same name Prometheus. Mountains are also populous around the planet's surface as well. In fact, Io is home to more than one hundred fifty mountains. One of those mountains includes Tohil Mons, meaning "Mount Tohil". This mountain reaches about five to six kilometres in height. (3.1 miles in height)

## Atmosphere

Io has a Atmosphere. The atmosphere of Io consists of mostly making sulfur dioxide, making up about 95% of the atmosphere. The rest is other carbon-based gases such as carbon dioxide.

## Formation

Scientists are not sure on how Io Formed, we think that it could have been a large Object in the Kuiper of Asteroid Belt, where a large object about 3/4 it’s size slammed into Io, and thrown out of its orbit, into Jupiters Sphere of Influence .
Pluto

Pluto!

Pluto is the last planet to the Sun, or the 2nd dwarf. It was discovered on February 18, 1930 by Clyde Tombaugh. It is the largest object in the Kuiper belt but less dense or massive than Eris. It was originally referred to as the ninth planet, but the IAU sadly demoted into being a dwarf planet in 2006 because of its size, and because it did not clear its orbit.

## Moons

Pluto has a few satellites, one of them is Charon, is half the size of Pluto! It is so big that Pluto orbits Charon too. But the IAU has yet to make a defination for a binary dwarf planet system, so Charon is classified as a moon. Pluto has 4 more moons, they are Hydra, Nix, Kerberos, and Styx. They are a Smaller then Charon.

## Formation

Pluto was Probably made like the Rest of the Terrestrial Planets, but instead, it Formed Smaller than the rest, and then it got Ejected into the Kuiper Belt.

## Surface

Its Surface May have Tholins on it, that would explain the Reddish Color, Pluto’s Surface also May have Rock on it. Not much else is Known.

## Atmosphere

The Atmosphere of Pluto is thin, and when it gets too close too far from the Sun, it melts and falls down on the Planet, as snow.

## Exploration

Pluto has only been explored by 1 Spacecraft, named New Horizons. New Horizons Provided us with the First Close up High Quality images of Pluto, as well as precise mass and size measurements as well as the first Close up images of its moons and Observations of its Atmosphere.

## Inside Pluto

### The Crust

The First Layer of Pluto is the Crust, what is the surface of the planet. It was discussed earlier.

### The Mantle

Pluto’s mantle is Probably made of Rock and Lava. It is hotter then the Surface.

### The Inner and Outer Core

The Core of Pluto is Probably composed of Iron, Lava, and maybe even other Materials.
Amalthea

Artist’s Impression of the moon

Amalthea, also known as Jupiter V, is an oval-shaped prograde satellite belonging to the planet of Jupiter. It was discovered on September 9, 1892, by Edward Emerson Barnard. It is Located 10 Studs Away From. Venus. called the Amalthea Moon, which it is a main supplier of the group.

Amalthea is the reddest object in the solar system. It is even redder than that of the Stephano grouped-moon, Albiorix, Sedna, and Mars. This is due to Amalthea giving out more heat than it receives from the Sun. This is possibly due to Amalthea's electrically charged core, due to it being too far to Venus’ gravitational pull.

Amalthea makes up its own group known as the Amalthea group.

## Composition

Amalthea is thought to consist of porous magma oceans under the surface, yet the ocean is too deep for astronomers to comprehend or spot. Astronomers believe that the magma ocean is too deep for any life to survive or thrive.

## Surface

The surface of Amalthea is reddish orange possibly due to sulfur from neighboring moon, Albiorix or other of the 3 moons of Venus. With a surface brighter than those of the inner satellites of Venus. Amalthea has green patches on the surface, yet the nature or origin is currently unknown by astronomers. The surface is full of craters from previous impacts and collisions with many other minor moons and asteroids.

## Orbit and Rotation

Due to Amalthea, along with the neighboring moon, Albiorix, making one rotation on its axis in correspondence to making one orbit around Venus. (in approximately one-third of an Earthen day), only one side of Amalthea faces Venus.
Triton

Voyager’s View of Triton

Triton, also known as Neptune I, is the biggest natural satellite of the outer planet, Neptune. It is the seventh-largest moon in the Solar System. It has a retrograde orbit. Triton was discovered on October 10, 1846 by the astronomer William Lassell. Triton is a Retrograde moon, meaning that it Orbits Neptune opposite to its Rotation.

## Surface

The surface of Triton have some smooth parts, with some craters located through this Neptunian object. Triton also has some ice.

## Formation

Triton was probably a Kuiper Belt Object inside a binary system, but Neptune came along and had to mess it up, ejecting Triton’s Moon, and Capturing Triton.

## Fate

Because Triton is a Retrograde moon, In around 2 billion years, Triton will stop orbiting, and be pulled apart by Neptune’s Strong gravity, and formed into a new Ring System.
Oberon

Oberon with many craters

Oberon is the outermost of Uranus' moons and is the second largest of them. It is likely that Oberon formed from the accretion disk that surrounded Uranus just right after Uranus’ formation. The moon consists of approximately equal amounts of ice and rock, and is probably differentiated into a rocky core and an icy mantle. A layer of liquid water may be present at the boundary between the mantle and the core.

## Surface

Oberon’s dark-red surface is more heavily cratered than that of any other major moon of Uranus. Oberon appears to have been primarily shaped by asteroid and comet impacts. It is covered by numerous impact craters reaching 210 km in diameter. The Surface is Rocky, and could barley be considered smooth.

## Orbit

Oberon orbits Uranus at a distance of around 584,000 km, being the farthest from the planet among its five major moons. Oberon's orbit has a small orbital eccentricity and inclination relative to the equator of Uranus. Its orbital period is around 13.5 days.