recursal/Fanatic-Fandom huggingface dataset:
Helix Knights Wiki

## Welcome to the Helix Knights Wiki

A wiki dedicated to everything about the manga/comic series Helix Knights created by Benjamin Wong.

## Story Introduction

Helix Knights is a new fantasy/adventure/action comic set in the modern day. The story follows a young teenager named Colin, a seemingly average high school student and delinquent with no outstanding qualities or plans for his future.

After a series of unfortunate events that befall him and his family, he eventually learns that the myths and legends of Earth's past- of legendary knights, warriors, sorcery, magic, dragons, vampires and alike- are all in fact real, and that a secret war between good and evil forces has been taking place on his world for over a thousand years.

And so, wanting to play a part in the events to come, Colin eventually joins the Helix Knights- an organization of powerful warriors tasked with protecting all the worlds from all the creatures that wish to harm them- this beginning his great adventure.

## Characters

* Colin Lee-Yang
* Rea Astaroth
* Saito Mamoru
* Artemis
* More

## Gallery

1/3
## Featured Quote

> "*A real man doesn't fight with guns or knives! Those are the weapons of cowards! A real man conquers challenges with his own two hands!*"
> ― Colin to Ronan[[source]]
>
>

## Latest activity

* Helix Knights - Chapter 1 - The Uncertain Future - Published Feburary 5th 2018 on Amazon Kindle.

Photos and videos are a great way to add visuals to your wiki. Find videos about your topic by exploring Fandom's Video Library.

File:Placeholder
Birdball

Birdball is an elusive game supposedly created by William, Dom, NiceTrySean, and Grant Kirkhope.

At one point Dom mentioned that Birdball is in fact real, but he said "i can’t tell you more without getting in trouble. there’s been a dark cloud hanging over it since we did that exhibit in 2014"

Details about the game are sketchy and mysterious. To date, no working links have been found to download Birdball.

It may have some connection to the mysterious Kevin Patterson.

According to William Pugh, it was realized exclusively for the PS1 several years ago.
The Undead Rising Campaign Wiki

## Welcome to the The Undead Rising Campaign Wiki

A bruised and battered man stumbles into a inn mumbling of dark events in his nearby home of Kheldell setting into motion an extensive campaign uncovering a nefarious plot with global implications.

## Describe your topic

A homebrew Dnd campaign (currently still a work in progress).

## Campaign Structure

Part 1

Part 2

Part 3

## Locations

* Kheldell
* Phandalin
* Wraith Lair
* Neverwinter
* Longsaddle
* Evermoors

## Monsters

* Otyugh
* Specter
* Wraith
* Bodak
* Korred

## Latest activity

Photos and videos are a great way to add visuals to your wiki. Find videos about your topic by exploring Fandom's Video Library.

File:Placeholder
Kepler 442

**Kepler-442** is a K-type main-sequence star approximately 1,206 light years from Earth in the constellation Lyra. It is located within the field of vision of the Kepler spacecraft, the satellite that NASA's Kepler Mission used to detect planets that may be transiting their stars. On January 6, 2015, along with the notable stars of Kepler-438 and Kepler-440, it was announced that the star has an extrasolar planet (a super-Earth) orbiting within the habitable zone, named Kepler-442b.[2]
Ronan

Ruler of the Subterranean Empire

**Ronan,** also known as **Lord Ronan** or **The Troll King**, is a self-proclaimed, self-made ruler and warlord of the recently formed **Subterranean Empire**, which he himself created. He is the first major antagonist of the *Helix Knight* series and the main antagonist of the story's first arc.
Cressida

small moon of Uranus

**Cressida** orbits close to a 3:2 resonance with the η ring, one of the rings of Uranus. Perturbations of the ring's shape provide a way to measure the mass of **Cressida**, which was found to be 2.5±0.4×1017 kg. **Cressida** is the only small satellite of Uranus for which the mass has been directly measured.[7]

## **Cressida** may collide

**Cressida** may collide with either Desdemona or within the next 100 million years

**Cressida** and Desdemona, fated to crash in 100,000 to 10 million years. If those moons merge, the resulting body, Cresdemona, takes out the moon Juliet
Conner MacMillan

**Conner MacMillan**, also known by his moniker **The Beast**, is a squire in the Helix Knights and one of the main secondary characters in the story.

Originating from a country family in Scotland, Conner was inducted into the Helix Knights when he was discovered to possess hidden magical potential. Following his preassessment, it's revealed that he inherited Sir William Wallace's powers- a Scottish knight who became one of the main leaders during the Wars of Scottish Independence. Conner also inherited his Spirit Edge, an enormous two-handed claymore dubbed **The Wallace Sword**.

Introduced on the first day of squire training, he, Saito, Darren and Colin strike up an immediate friendship. He also establishes a semi-serious rivalry with Saito, in which he Conner contests his superior strength against his friend's greater speed.

Conner quickly proves to be an invaluable ally to the Helix Knights, by fighting in various major battles and taking on some of the story's strongest villains.
Kepler 186c

Second Planet From The Kepler 186

Kepler 186d

Kepler 186e

**Kepler**-**186 c** is a super Earth exoplanet that orbits a M-type star. Its mass is 2.1 Earths, it takes 7.3 days to complete one orbit of its star, and is 0.0451 AU from its star. Its discovery was announced in 2014. PLANET TYPE. Super Earth.
Saturn

**Saturn** is the sixth planet from the Sun and the second-largest in the Solar System, after Jupiter. It is a gas giant with an average radius of about nine-and-a-half times that of Earth. It has only one-eighth the average density of Earth, but is over 95 times more massive.

## Moon groups

* Moonlets
* Ring Shepherds
* Co-Orbitals
* Inner Large Moons
* Alkyonides
* Trojan Moons
* Outer Large Moons
* Irregular Moons
	+ Inuit Group
	+ Gallic Group
	+ Norse Group

## Moons

* S/2009 S 1
* Moonlets
* Earhart
* Bleriot
* Santos-Durmont
* Peggy
* Pan
* Daphnis
* Atlas
* Prometheus
* Pandora
* Epimetheus
* Janus
* Aegaeon
* **Mimas**
* Methone
* Anthe
* Pallene
* **Enceladus**
* **Tethys**
* Telesto
* Calypso
* **Dione**
* Helene
* Polydeuces
* **Rhea**
* **Titan**
* Hyperion
* **Iapetus**
* Kiviuq
* Ijiraq
* Phoebe
* Paaliaq
* Skathi
* Albiorix
* S/2007 S 2
* Bebhionn
* Erriapus
* Skoll
* Siarnaq
* Tarqeq
* S/2004 S 13
* Greip
* Hyrrokkin
* Jarnsaxa
* Tarvos
* Mundilfari
* S/2006 S 1
* S/2004 S 17
* Bergelmir
* Narvi
* Gridr
* Suttungr
* Hati
* S/2004 S 12
* Eggther
* Farbauti
* Beli
* Thrymr
* Angrboda
* Aegir
* S/2007 S 3
* Bestla
* S/2004 S 7
* Skrymir
* Gerd
* Gunnlod
* Geirrod
* S/2006 S 3
* Alvaldi
* Fenrir
* Surtur
* Kari
* Ymir
* Loge
* Thiazzi
* Fornjot
Rhea

Second Largest Moon of saturn and She Have Rings Too

Mimas

****Rhea**** (/ˈriːə/) is the second-largest moon of Saturn and the ninth-largest moon in the Solar System. It is the second smallest body in the Solar System for which precise measurements have confirmed a shape consistent with hydrostatic equilibrium, after dwarf planet Ceres.[11][12] It was discovered in 1672 by Giovanni Domenico Cassini.

## Rings of Rhea

The Saturnian moon **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.[2]
Telesto

trojan moon

Polydeuces

Helene

Other

Light

****Telesto**** /təˈlɛstoʊ/ is a moon of Saturn. It was discovered by Smith, Reitsema, Larson and Fountain in 1980 from ground-based observations, and was provisionally designated **S/1980 S 13**.[4] In the following months, several other apparitions were observed: S/1980 S 24,[5] S/1980 S 33,[6] and S/1981 S 1.[7]

In 1983 it was officially named after **Telesto** of Greek mythology.[a] It is also designated as **Saturn XIII** or **Tethys B**.

**Telesto** is co-orbital with Tethys, residing in Tethys' leading Lagrangian point (L4). This relationship was first identified by Seidelmann *et al.* in 1981.[8] Another moon, Calypso, resides in the other (trailing) Lagrangian point of Tethys, 60 degrees in the other direction from Tethys. The Saturnian system has two additional trojan moons.
Gliese 876 e

Last Planet From The Gliese 876

Gliese 876 c

Gliese 876 b

**Gliese 876 e** is an exoplanet orbiting the star Gliese 876 in the constellation of Aquarius. It is in a 1:2:4 Laplace resonance with the planets Gliese 876 c and Gliese 876 b: for each orbit of planet e, planet b completes two orbits and planet c completes four. This configuration is the second known example of a Laplace resonance after Jupiter's moons Io, Europa and Ganymede.[1]

Gliese 876 e has a mass similar to that of the planet Uranus. Its orbit takes 124 days to complete, or roughly one third of a year. While the orbital period is longer than that of Mercury around the Sun, the lower mass of the host star relative to the Sun means the planet's orbit has a slightly smaller semimajor axis. Unlike Mercury, Gliese 876 e has a nearly circular orbit with an eccentricity of 0.055 ± 0.012.[1]

This planet, like b and c, has likely migrated inward
Test

**JUST CLICK EDIT AND YOU WILL SEE HOW YOU CAN MAKE THEM**

# Planets

## Collapse

**CLICK ON THE BIG ORANGE BUTTON THAT SAYS EDIT , CLICK ON THE NEPTUNE SYSTEM NAVABOX , CLICK "TEST A" , THERE SHOULD BE WORDS NEXT TO THE ARROW , CLICK ON THAT , IT SHOULD GIVE YOU A NEW PAGE THEN CLICK EDIT AND DO WHAT YOU WANT**

**Solar System**

Star

Sun

Planets
 Mercury ,  Venus ,  Earth,  Mars,  Jupiter,  Saturn ,  Uranus ,  Neptune

Hypothetical planets
 Planet 9 ,  Planet 10

Dwarf Planets
 Pluto ,
 Ceres ,
 Eris ,
 Makemake ,
 Haumea ,
 Deedee ,
 Varuna ,
 Orcus ,
 Ixion ,
 Sedna ,
 Salacia
Juliet

Portia

Mab,Crush

****Juliet**** is an inner satellite of Uranus. It was discovered from the images taken by *Voyager 2* on 3 January 1986, and was given the temporary designation **S/1986 U 2**. It is named after the heroine of William Shakespeare's play *Romeo and **Juliet***. It is also designated **Uranus XI**.

## **Juliet** may collide

**Juliet** is a member of the Portia group of moons of the planet Uranus. **Juliet** may collide with Desdemona within the next 100 million years.
Galileo

55 Cancri b

Peacock

**55 Cancri b** (abbreviated **55 Cnc b**), occasionally designated 55 Cancri Ab (to distinguish it from the star 55 Cancri B), also named **Galileo**, is an exoplanet orbiting the Sun-like star 55 Cancri A every 14.65 days. It is the second planet in order of distance from its star, and is an example of a hot Jupiter, or possibly rather "warm Jupiter".[4]

In July 2014 the International Astronomical Union launched a process for giving proper names to certain exoplanets and their host stars.[5] The process involved public nomination and voting for the new names.[6] In December 2015, the IAU announced the winning name was **Galileo** for this planet.[7] The winning name was submitted by the Royal Netherlands Association for Meteorology and Astronomy of the Netherlands. It honors early-17th century astronomer and physicist Galileo Galilei.[8]
Titania

Uranus's Largest Moon

**Titania**, also designated Uranus III, is the largest of the moons of Uranus and the eighth largest moon in the Solar System at a diameter of 1,578 kilometres. Discovered by William Herschel in 1787, Titania is named after the queen of the fairies in Shakespeare's A Midsummer Night's Dream

Titania 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 core–mantle boundary. The surface of Titania, which is relatively dark and slightly red in color, appears to have been shaped by both impacts and endogenic processes. It is covered with numerous impact craters reaching up to 326 kilometres (203 mi) in diameter, but is less heavily cratered than Oberon, outermost of the five large moons of Uranus. Titania probably underwent an early endogenic resurfacing event which obliterated its older, heavily cratered surface. Titania's surface is cut by a system of enormous canyons and scarps, the result of the expansion of its interior during the later stages of its evolution. Like all major moons of Uranus, Titania probably formed from an accretion disk which surrounded the planet just after its formatiom
Janssen

Diamond planet

Lava World,

**Cancri e** (abbreviated **55 Cnc e**, formally named **Janssen** /ˈdʒænsən/) is an exoplanet in the orbit of its Sun-like host star 55 Cancri A. The mass of the exoplanet is about 8.63 Earth masses and its diameter is about twice that of the Earth,[4] thus classifying it as the first super-Earth discovered around a main sequence star, predating Gliese 876 d by a year. It takes less than 18 hours to complete an orbit and is the innermost-known planet in its planetary system. 55 Cancri e was discovered on 30 August 2004. However, until the 2010 observations and recalculations, this planet had been thought to take about 2.8 days to orbit the star.[3] In October 2012, it was announced that 55 Cancri e could be a carbon planet

In February 2016, it was announced that NASA's Hubble Space Telescope had detected hydrogen and helium (and suggestions of hydrogen cyanide), but no water vapor, in the atmosphere of 55 Cancri e, the first time the atmosphere of a super-Earth exoplanet was analyzed successfully
Neptune

jupiter

## Personality

Neptune is friendly, but often sarcastic. He tells Uranus that he isn't hated, but he never listens.

## Moons

* Triton
* Nereid
* Naiad
* Halimede
* Sao
* Laomedeia
* Psamathe
* Neso
* Thalassa
* Despina
* Galatea
* Larissa
* S/2004 N 1
* Proteus

## Gallery

IconHim and UranusAnother icon

**Solar System**

Star

Sun

Planets
 Mercury ,  Venus ,  Earth,  Mars,  Jupiter,  Saturn ,  Uranus ,  Neptune

Hypothetical planets
 Planet 9 ,  Planet 10

Dwarf Planets
 Pluto ,
 Ceres ,
 Eris ,
 Makemake ,
 Haumea ,
 Deedee ,
 Varuna ,
 Orcus ,
 Ixion ,
 Sedna ,
 Salacia
Francisco

Stephano

Trinculo

**Francisco** is the innermost irregular satellite of Uranus.

Francisco was discovered by Matthew J. Holman, et al. and Brett J. Gladman, et al. in 2003 from pictures taken in 2001 and given the provisional designation **S/2001 U 3**. Confirmed as **Uranus XXII**, it was named after a lord in William Shakespeare's play *The Tempest*.[8]
Belinda

****Belinda**** is an inner satellite of the planet Uranus. **Belinda** was discovered from the images taken by *Voyager 2* on 13 January 1986 and was given the temporary designation **S/1986 U 5**.[7] It is named after the heroine of Alexander Pope's *The Rape of the Lock*. It is also designated **Uranus XIV**.[8]

**Belinda** belongs to the Portia group of satellites, which also includes Bianca, Cressida, Desdemona, Portia, Juliet, Cupid, Rosalind and Perdita.[6] These satellites have similar orbits and photometric properties.[6] Other than its orbit,[2] radius of 45 km[3] and geometric albedo of 0.08[6] virtually nothing is known about it.
Fun Facts about my wiki

* Mercury's current pose is very similar to his second pose
* During planning and character development, Moon was going to be male at one point
* Venus was originally a gossip girl, and only cared about fashion
* Mars's personality changed a lot, originally always being angry, but i changed him to "the normal guy"
* Eris supposedly has a crush on Pluto, but it hasn't been shown yet
* Ceres was going to be a female but was changed to male when this wiki was made
* Sun was supposed to be shy, but took on more of a motherly personality now
* The only planet in the solar system not to be shown yet is the theoretical planet Tyche
* Neptune was gonna hate Pluto, but in order to keep balance between Solar System Comics, Weird and Wonderfull space, and Universe of the Universe, he changed and Jupiter got the jerk personality
* Jupiter was originally going to be like Spongy from BFDI
* Uranus was going to be stupid and weird, but this changed to a kind, but slightly shy personality
* Mimas switched genders multiple times in development
* Uranus's eyes are spirals to emphasize the fact that he is a strange planet
* BFB and BFDI assets are used interchangeably
* The very first version of SSC was on paper, there was no dialogue, and the characters only had eyes
Titan

Largest Moon of saturn

Rhea

Hyperion]

Phoebe

**Titan** is the largest moon of Saturn and the second-largest natural satellite in the Solar System. It is the only moon known to have a dense atmosphere, and the only known body in space, other than Earth, where clear evidence of stable bodies of surface liquid has been found.[15]

**Titan** is one of six gravitationally rounded moons from Saturn, and the most distant from Saturn of those six. Frequently described as a planet-like moon, **Titan** is 50% larger (in diameter) than Earth's Moon and 80% more massive. It is the second-largest moon in the Solar System after Jupiter's moon Ganymede, and is larger than the planet Mercury, but only 40% as massive. Discovered in 1655 by the Dutch astronomer Christiaan Huygens, **Titan** was the first known moon of Saturn, and the sixth known planetary satellite (after Earth's moon and the four Galilean moons of Jupiter). **Titan** orbits Saturn at 20 Saturn radii. From **Titan**'s surface, Saturn subtends an arc of 5.09 degrees and, were it visible through the moon's thick atmosphere, would appear 11.4 times larger in the sky than the Moon from Earth.
Mab

Perdita

Puck,sometime

images taken by *Voyager 2* during its Uranus flyby in 1986. However, it is brighter than another moon, Perdita, which was discovered from Voyager's photos in 1997. This led scientists to re-examine the old photos again, and the satellite was finally found in the images.[2]

The size of **Mab** is not known exactly. If it is as dark as Puck, it is about 24 km in diameter. On the other hand, if it is brightly coloured like the neighbouring moon Miranda, it would be even smaller than Cupid and comparable to the smallest outer satellites
Pandia

Panda

Elara

Dia

Carpo

**Pandia** /pænˈdaɪə/, also known as **Jupiter LXV**, originally known as **S/2017 J 4**, is an outer natural satellite of Jupiter, 3 km in diameter.

Pandia was discovered by Scott S. Sheppard and his team in 2017, but not announced until July 17, 2018 via a Minor Planet Electronic Circular from the Minor Planet Center.[3]

The moon was named in 2019 after Pandia (Πανδία *Pandīa*), the Greek goddess of the full moon, daughter of Zeus and Selene.[4] Pandia was among the most popular suggestions in a naming contest held by the Carnegie Institute on Twitter, with the most significant submission coming from the astronomy club of the Lanivet School in Cornwall, United Kingdom that was submitted on their behalf by user "@emmabray182". They chose Pandia because their school's mascot is a panda and their local village used to supply bamboo for a panda at London Zoo.[5][6][7]
Hydra

Second Largest Moon Of Pluto

Charon

****Hydra**** is a natural satellite of Pluto, with a diameter of approximately 51 km (32 mi) across its longest dimension.[6] It is the second largest moon of Pluto, being slightly larger than Nix. **Hydra** was discovered along with Nix by the Pluto Companion Search Team in June 2005. It was named after the **Hydra**, the nine-headed underworld serpent in Greek mythology.[13] By distance, Hydra is the fifth and outermost moon of Pluto, orbiting beyond Pluto's fourth moon Kerberos.[7]

**Hydra** has a highly reflective surface caused by the presence of water ice, similar to other Plutonian moons.[14] **Hydra**'s reflectivity is intermediate, in between those of Pluto and Charon.[15] The *New Horizons* spacecraft imaged Pluto and its moons in July 2015 and returned multiple images of **Hydra**
Ceres

**Ceres** /ˈsɪəriːz/[16] (minor-planet designation: **1 Ceres**) is the largest object in the main asteroid belt that lies between the orbits of Mars and Jupiter. With a diameter of 940 km (580 mi), Ceres is both the largest of the asteroids and the only dwarf planet inside Neptune's orbit.[c] It is the 25th-largest body in the Solar System within the orbit of Neptune.

**Ceres** was the first asteroid to be discovered by Giuseppe Piazzi at Palermo Astronomical Observatory on 1 January 1801. It was originally considered a planet, but was reclassified as an asteroid in the 1850s after many other objects in similar orbits were discovered

## ceres

The biggest asteroid in the asteroid belt.

### Friends

vesta , earth , pluto , haumea , makemake
Part 1

This campaign was designed to take place after the Lost Mines of Philander campaign and so begins with the PCs in Phandalin with news of their fame spreading. One morning as they are having breakfast in the tavern, Donnus Atesso comes stumbling in the tavern bearing news of terrible happenings in Kheldell. (see Donnus Atesso). Once they arrive at Kheldell, they will be forced to fight Otyugh and make a decision to stay the night (see Kheldell). If they stay, they will see Wraiths summoning specters from the dead bodies. The wraiths escape without fighting the PCs will all the specters attack. After they defeat the specters, the PCs find a path of death and destruction leading to the wraith lair. If they choose not to stay the night and return to Phandalin, the specters will attack the PCs in Phandalin and the wraith will make another path to his lair. Either choice will lead to the wraiths lair (See wraith lair). In the Wraith's lair, the PCs will find the magical staff of possession. Unable to figure out what it does, they will seek out a powerful wizard who can tell them. Donnus Atesso has heard rumours of a powerful wizard who recently made his home in Neverwinter and the PCs can journey there. This will leads to Part 2.

## Locations

* Kheldell
* Phandalin
* Wraith Lair

## Monsters

* Corpseling
* Otyugh
* Specter
* Wraith
Dione

Rhea

Iapetus

Enceladus sometime

**Dione** is a moon of Saturn. It was discovered by Italian astronomer Giovanni Domenico Cassini in 1684. It is named after the Titaness **Dione** of Greek mythology. It is also designated Saturn IV.

****Dione**** is currently in a 1:2 mean-motion orbital resonance with **moon** Enceladus, completing one orbit of Saturn for every two orbits completed by Enceladus. ... ****Dione**** has two co-orbital, or **trojan**, **moons**, Helene and Polydeuces.
Pandora

Dark

**Pandora** is an inner satellite of Saturn. It was discovered in 1980 from photos taken by the *Voyager 1* probe, and was provisionally designated **S/1980 S 26**.[4] In late 1985 it was officially named after Pandora from Greek mythology.[5] It is also designated **Saturn XVII**.[6]

Pandora was thought to be an outer shepherd satellite of the F Ring. However, recent studies indicate that it does not play such a role, and that only Prometheus, the inner shepherd, contributes to the confinement of the narrow ring.[7][8] It is more heavily cratered than nearby Prometheus, and has at least two large craters 30 kilometres (19 mi) in diameter. The majority of craters on Pandora are shallow as a result of being filled with debris. Ridges and grooves are also present on moon's surface
Brahe

55 Cancri c

**55 Cancri c** (abbreviated **55 Cnc c**), formally named **Brahe** (pronounced /ˈbrɑːhiː/ or /ˈbrɑː/), is an extrasolar planet in an eccentric orbit around the Sun-like star 55 Cancri A, making one revolution every 44.34 days. It is the third known planet in order of distance from its star. 55 Cancri c was discovered on June 13, 2002 and has a mass roughly half of Saturn.

In July 2014 the International Astronomical Union launched a process for giving proper names to certain exoplanets and their host stars.[2] The process involved public nomination and voting for the new names.[3] In December 2015, the IAU announced the winning name was Brahe for this planet.[4] The winning name was submitted by the Royal Netherlands Association for Meteorology and Astronomy of the Netherlands. It honors the astronomer Tycho Brahe
Kepler-421b

Uranus-like

**Kepler-421b** is an exoplanet that, as of July 2014, has the longest known year of any transiting planet (704 days),[1] although not as long as the planets that have been directly imaged, or many of the planets found by the radial-velocity method, or as long as some transiting planet candidates which are listed as planets in the Extrasolar Planets Encyclopaedia (KIC 5010054 b etc.).[2] It is the first transiting-planet found near the snow-line.

In that case, an ice giant candidate, Kepler-421b, was found orbiting an orange, K-type star about 1,000 light-years away in the constellation Lyra. That planet is about the same size as Uranus and has the longest known year of any exoplanet so far, orbiting its star every 704 days. These discoveries suggest that similar ice giant worlds may be fairly common in other solar systems. The fact that our own Solar System has two of them also supports this idea
Bianca

****Bianca**** is an inner satellite of Uranus. It was discovered from the images taken by *Voyager 2* on January 23, 1986, and was given the temporary designation **S/1986 U 9**.[8] It was named after the sister of Katherine in Shakespeare's play *The Taming of the Shrew*. It is also designated **Uranus VIII**.[9]

**Bianca** belongs to Portia Group of satellites, which also includes Cressida, Desdemona, Juliet, Portia, Rosalind, Cupid, Belinda and Perdita.[7] These satellites have similar orbits and photometric properties.[7] Other than its orbit,[3] radius of 27 km,[4] and geometric albedo of 0.08[7] virtually nothing is known about
Sedna

Sedna is the most distant solar system object ever discovered. It is twice as far from the sun as any other solar system object and three times farther than Pluto or Neptune.

## Bio

she acts like a leader because she is a leader. of the sednoids

**Solar System**

Star

Sun

Planets
 Mercury ,  Venus ,  Earth,  Mars,  Jupiter,  Saturn ,  Uranus ,  Neptune

Hypothetical planets
 Planet 9 ,  Planet 10

Dwarf Planets
 Pluto ,
 Ceres ,
 Eris ,
 Makemake ,
 Haumea ,
 Deedee ,
 Varuna ,
 Orcus ,
 Ixion ,
 Sedna ,
 Salacia

[[Category:
TRAPPIST-1 c

TRAPPIST-1d

**TRAPPIST-1c**, also designated as **2MASS J23062928-0502285 c**, is a mainly rocky, Venus-like exoplanet orbiting around the ultracool dwarf star TRAPPIST-1 approximately 40 light-years away from Earth in the constellation Aquarius. It is the most massive and third largest planet of the system, with about 116% the mass and 110% the radius of Earth. Its density indicates a primarily rocky composition with a very thick Venus-like atmosphere, although it is expected to be thinner than that of TRAPPIST-1b.
Metis

**Metis** is tidally locked to Jupiter, and its shape is strongly asymmetrical, with one of the diameters being almost twice as large as the smallest one. It is also one of the two moons known to orbit Jupiter in less than the length of Jupiter's day, the other being Adrastea. It orbits within the main ring of Jupiter, and is thought to be a major contributor of material to the rings.
Epimetheus

**Epimetheus** /ɛpɪˈmiːθiːəs/ is an inner satellite of Saturn. It is also known as **Saturn XI**. It is named after the mythological **Epimetheus**, brother of Prometheus.

**Epimetheus** occupies essentially the same orbit as the moon Janus. Astronomers assumed that there was only one body in that orbit (disbelieving that two moons could share nearly identical orbits without colliding[6]), and accordingly had difficulty determining their orbital characteristics. Observations were photographic and spaced widely apart in time, so that while the presence of two objects was not obvious, the observations were difficult to reconcile with a reasonable orbit.[7]
Hyperion

**Hyperion** /haɪˈpɪəriən/, also known as **Saturn VII** (7), is a moon of Saturn discovered by William Cranch Bond, his son George Phillips Bond and William Lassell in 1848. It is distinguished by its irregular shape, its chaotic rotation, and its unexplained sponge-like appearance. It was the first non-round moon to be discovered.
S/2009 S 1

Smallest moon in the Solar System

**S/2009 S 1** is a "propeller moonlet" of Saturn orbiting at a distance of 117,000 km (73,000 mi), in the outer part of the B Ring, and with a diameter of 300 m (1,000 ft).[3] The moonlet was discovered by the Cassini Imaging Team during the Cronian equinox event on 26 July 2009,[4] when it cast a shadow 36 km (22 mi) long onto the B Ring. S/2009 S 1 protrudes 150 m (500 ft) north of the ring.[5] The image was taken approximately 296,000 km (184,000 mi) from Saturn.
TRAPPIST-1 h

coldest planet

**TRAPPIST-1 h**, also designated as **2MASS J23062928-0502285 h**, is an exoplanet orbiting around the ultra-cool dwarf star TRAPPIST-1 39 light-years (12 parsecs) away from Earth in the constellation Aquarius. It was one of four new exoplanets to be discovered orbiting the star using observations from the Spitzer Space Telescope. Throughout 2017 and 2018, more studies were able to refine its physical parameters.

The outermost known planet in its system, it is roughly one third the mass of Earth, and about 77% as large. Its relatively low density indicates that it is likely water-rich, like several other planets in the system.
Haumea

**Haumea** (minor-planet designation **136108 Haumea**) is a dwarf planet located beyond Neptune's orbit. It was discovered in 2004 by a team headed by Mike Brown of Caltech at the Palomar Observatory in the United States and disputably also in 2005 by a team headed by José Luis Ortiz Moreno at the Sierra Nevada Observatory in Spain. On September 17, 2008, it was named after Haumea, the Hawaiian goddess of childbirth, under the expectation by the International Astronomical Union (IAU) that it would prove to be a dwarf planet. Nominal estimates make it the third-largest known trans-Neptunian object, after Eris and Pluto, and approximately the size of Uranus's moon Titania.

## Character Info

### Friends

Pluto, Eris, Makemake (Boyfriend)

**Haumea is very kind and helpful**

**Solar System**

Star

Sun

Planets
 Mercury ,  Venus ,  Earth,  Mars,  Jupiter,  Saturn ,  Uranus ,  Neptune

Hypothetical planets
 Planet 9 ,  Planet 10

Dwarf Planets
 Pluto ,
 Ceres ,
 Eris ,
 Makemake ,
 Haumea ,
 Deedee ,
 Varuna ,
 Orcus ,
 Ixion ,
 Sedna ,
 Salacia
Sun

## Personality

The sun is in the center of the Solar System and he leads his planets throughout the SS. (short for Solar System.)

**Solar System**

Star

Sun

Planets
 Mercury ,  Venus ,  Earth,  Mars,  Jupiter,  Saturn ,  Uranus ,  Neptune

Hypothetical planets
 Planet 9 ,  Planet 10

Dwarf Planets
 Pluto ,
 Ceres ,
 Eris ,
 Makemake ,
 Haumea ,
 Deedee ,
 Varuna ,
 Orcus ,
 Ixion ,
 Sedna ,
 Salacia
Iapetus

brown

**Iapetus** (/aɪˈæpɪtəs/) is the third-largest natural satellite of Saturn, eleventh-largest in the Solar System,[10] and the largest body in the Solar System known not to be in hydrostatic equilibrium.[11] Discoveries by the *Cassini* mission in 2007 revealed several unusual features, such as a massive equatorial ridge running three-quarters of the way around the moon
Anthe

Egg shape moon

****Anthe**** /ˈænθiː/ is a very small natural satellite of Saturn lying between the orbits of Mimas and Enceladus. It is also known as **Saturn XLIX**; its provisional designation was **S/2007 S 4**. It is named after one of the Alkyonides; the name means *flowery*. It is the sixtieth confirmed moon of Saturn.

It was discovered by the Cassini Imaging Team[1] in images taken on 30 May 2007.[2] Once the discovery was made, a search of older *Cassini* images revealed it in observations from as far back as June 2004. It was first announced on 18 July 2007.[2]
CoRoT-7c

CoRoT-7d

**CoRoT-7c** is an extrasolar planet which orbits the G-type main sequence star CoRoT-7, located approximately 489 light years away in the constellation Monoceros. It's either a super-Earth or a Neptune-like planet, orbiting at 0.046 AU from the star, taking 3.7 days or 89 hours to make one round trip around the star.
Rosalind

**Rosalind** is an inner satellite of Uranus. It was discovered from the images taken by *Voyager 2* on 13 January 1986, and was given the temporary designation **S/1986 U 4**.[8] It was named after the daughter of the banished Duke in William Shakespeare's play *As You Like It*. It is also designated **Uranus XIII**.

**Rosalind** belongs to Portia group of satellites, which also includes Bianca, Cressida, Desdemona, Portia, Juliet, Cupid, Belinda and Perdita.[7] These satellites have similar orbits and photometric properties.[7] Other than its orbit,[3] radius of 36 km[4] and geometric albedo of 0.08[7] virtually nothing is known about **Rosalind**.
Himalia

****Himalia**** /hɪˈmeɪliə/, or **Jupiter VI**, is the largest irregular satellite of Jupiter, with a diameter of at least 140 km (90 mi).[5] It is the fifth largest Jovian satellite, after the four Galilean moons. It was discovered by Charles Dillon Perrine at the Lick Observatory on 3 December 1904 and is named after the nymph **Himalia**, who bore three sons of Zeus (the Greek equivalent of Jupiter).[1] It is one of the largest planetary moons in the Solar System not imaged in detail, and the largest within the orbit of Neptune.
Planet 9

*"Uhh.. you're kinda a bit too small.."*
This section or article is a stub , please help the Solar System Comics by adding more information. Thank you.

## Character Info

### Enemies

Jupiter

**Solar System**

Star

Sun

Planets
 Mercury ,  Venus ,  Earth,  Mars,  Jupiter,  Saturn ,  Uranus ,  Neptune

Hypothetical planets
 Planet 9 ,  Planet 10

Dwarf Planets
 Pluto ,
 Ceres ,
 Eris ,
 Makemake ,
 Haumea ,
 Deedee ,
 Varuna ,
 Orcus ,
 Ixion ,
 Sedna ,
 Salacia
Kepler 1658 System

**Kepler-1658 b is an exoplanet orbiting the star Kepler-1658. Its discovery was publicly announced on 2015.**

**The host star Kepler-1658 has apparent magnitude of 11.0, with absolute magnitude of 25.0.**

**It is 1.4 times more massive and 2.9 times bigger compared with our Sun. The surface temperature is 6216 with its spectral types of F8**

**In this planetary system, the extrasolar planet Kepler-1658 b orbits around the star Kepler-1658 every 3.8 days with its orbital distance of 0.05 AU ( 8168043.7 km)**

## Member

* Kepler-1658
* Kepler-1658b
CoRoT-7b

Lava World

CoRoT-7d

Red

Brown

Ice

Flame

**CoRoT-7b** (previously named **CoRoT-Exo-7b**)[2][3] is an exoplanet orbiting around the star CoRoT-7, in the constellation Monoceros, at 489 light years from Earth. It was first detected photometrically by the French-led CoRoT mission and reported in February 2009.[4] Until the announcement of Kepler-10b in January 2011, it was the smallest exoplanet to have its diameter measured, at 1.58 times that of the Earth (which would give it a volume 3.95 times Earth's), and the first potential extrasolar terrestrial planet to be found. The planet has a very short orbital period, revolving around its host star in about 20 hours.[1]

Combination of the planet's diameter derived from transit data with the planet's mass derived from radial velocity measurements, meant that the density of CoRoT-7b was about the same as that of Earth and, therefore, that CoRoT-7b was a terrestrial planet like Earth and was not a gas giant like Jupiter. The radial velocity observations of CoRoT-7 also detected a second super-Earth, CoRoT-7c, which has a mass 8.4 times that of Earth and orbits every 3.7 days at a distance of 6.9 million km (4.3 million miles).
Characters

## Helix Knights

### Year 1 Group

* Colin Lee-Yang
* Rea Astaroth
* Sandra Busujima
* Artemis
* Darren Vulgate
* Saito Mamoru
* Conner MacMillan
* Helena Terrine
* Kanan Hassah
* Christina Skyrider
* Anya Harmon of the Harmon Hotel

### Class-A Knights

* Rank 1 - Jon Monteil
* Rank 2 - Rochelle Leone
* Rank 3 - Nathan Lomas
* Rank 4 - Tristan Henze
* Rank 5 - Amber Warflower

## Class-S Knights - The Paladins

* Rank 10 - Catherine Averus
* Rank 11 - Mei Ren

## Subterranean Empire

* Lord Ronan, of the House Agate
* General Kora, of the House Roark
* General Azong
Uranus

The Odd One

## Personality

Uranus is often confused and feels like everyone hates him because he is weird, but that is not true. He really only feels like Neptune is his friend.

## Moons

* Cordelia
* Ophelia
* Bianca
* Cressida
* Desdemona
* Juliet
* Portia
* Rosalind
* Cupid
* Belinda
* Perdita
* Puck
* Mab
* Miranda
* Ariel
* Umbriel
* Titania
* Oberon
* Francisco
* Caliban
* Stephano
* Trinculo
* Sycorax
* Margaret
* Prospero
* Setebos
* Ferdinand

## Gallery

IconHim and Neptune

**Solar System**

Star

Sun

Planets
 Mercury ,  Venus ,  Earth,  Mars,  Jupiter,  Saturn ,  Uranus ,  Neptune

Hypothetical planets
 Planet 9 ,  Planet 10

Dwarf Planets
 Pluto ,
 Ceres ,
 Eris ,
 Makemake ,
 Haumea ,
 Deedee ,
 Varuna ,
 Orcus ,
 Ixion ,
 Sedna ,
 Salacia
Elara

Lysithea

Dia

Carpo

****Elara**** /ˈɛlərə/ is a prograde irregular satellite of Jupiter. It was discovered by Charles Dillon Perrine at Lick Observatory in 1905.[1][8] It is the eighth-largest moon of Jupiter and is named after **Elara**, one of Zeus's lovers and the mother of the giant Tityos.

**Elara** did not receive its present name until 1975; before then, it was simply known as **Jupiter VII**. It was sometimes called "Hera"[10] between 1955 and 1975. It has a mean radius of just 43 kilometres (27 mi), thus it is 2% of the size of Europa. However, it is half the size of Himalia, so it is the second-biggest moon in the Himalia group. It might be a captured type C or D asteroid, for it reflects very little light
Harriot

55 Cancri f

**55 Cancri f** (abbreviated **55 Cnc f**), also designated **Rho1 Cancri f** and formally named **Harriot** /ˈhæriət/,[2] is an extrasolar planet approximately 41 light-years away from Earth in the constellation of Cancer (the Crab). 55 Cancri f is the fourth known planet (in order of distance) from the star 55 Cancri and the first planet to have been given the designation of "f".[3]
Ophelia

**Ophelia** is a moon of Uranus. It was discovered from the images taken by *Voyager 2* on January 20, 1986, and was given the temporary designation **S/1986 U 8**.[8] It was not seen until the Hubble Space Telescope recovered it in 2003.[7][9] Ophelia was named after the daughter of Polonius, Ophelia, in William Shakespeare's play *Hamlet*. It is also designated **Uranus VII**.[10]Other than its orbit,[3] radius of 21 km[4] and geometric albedo of 0.08[7] virtually nothing is known about it. At the Voyager 2 images Ophelia appears as an elongated object, the major axis pointing towards Uranus. The ratio of axes of the Ophelia's prolate spheroid is 0.7 ± 0.3.
Kepler 69 System

Kepler 69c

The diagram compares the planets of the inner solar system to Kepler-69, a two-planet system about 2,700 light-years from Earth in the constellation Cygnus. The two planets of Kepler-69 orbit a star that belongs to the same class as our sun, called G-type.

Kepler-69c, is 70 percent larger than the size of Earth, and is the smallest yet found to orbit in the habitable zone of a sun-like star. Astronomers are uncertain about the composition of Kepler-69c, but its orbit of 242 days around a sun-like star resembles that of our neighboring planet Venus. The companion planet, Kepler-69b, is just over twice the size of Earth and whizzes around its star once every 13 days

## Members

* Kepler 69
* Kepler 69b
* Kepler 69c
Moon

fifth largest satellite in the Solar System and is larger than any dwarf planet.

### Friends

Sun
Mercury

Earth,BestFriend

Ceres

And Her Good Cousinss

Pluto

Haumea

Makemake

### Enemies

JupiterSometimes
Io

Europa

### Colors

GreyWhite

Dark Grey

The **Moon** is Earth's only proper natural satellite. It is one quarter the diameter of Earth (comparable to the width of Australia[13]) making it the largest natural satellite in the Solar System relative to the size of its planet. It is the fifth largest satellite in the Solar System and is larger than any dwarf planet. The Moon orbits Earth at an average *lunar distance* of 384,400 km (238,900 mi),[14] or 1.28 light-seconds. Its gravitational influence produces Earth's tides and slightly lengthens Earth's day. It is considered a planetary-mass moon and a differentiated rocky body; its surface gravity is about one-sixth of Earth's (0.1654 g) and it lacks any significant atmosphere, hydrosphere, or magnetic field. Jupiter's moon Io is the only satellite in the Solar Systems known to have a higher surface gravity and density.

The Moon's orbit around Earth has a sidereal period of 27.3 days, and a synodic period of 29.5 days. The synodic period drives its lunar phases, which form the basis for the months of a lunar calendar. The Moon is tidally locked to Earth, which means that the length of a full rotation of the Moon on its own axis (a lunar day) is the same as the synodic period, resulting in its same side (the near side) always facing Earth. That said, 59% of the total lunar surface can be seen from Earth through shifts in perspective (its libration).[15]
Cordelia

Nearest moon of Uranus

****Cordelia**** is the innermost known moon of Uranus. It was discovered from the images taken by *Voyager 2* on January 20, 1986, and was given the temporary designation **S/1986 U 7**.[8] It was not detected again until the Hubble Space Telescope observed it in 1997.[7][9] **Cordelia** takes its name from the youngest daughter of Lear in William Shakespeare's *King Lear.* It is also designated **Uranus VI**.[10]

Other than its orbit,[3] radius of 20 km[4] and geometric albedo of 0.08[7] virtually nothing is known about it. In the Voyager 2 images Cordelia appears as an elongated object with its major axis pointing towards Uranus. The ratio of axes of **Cordelia**'s prolate spheroid is 0.7 ± 0.2.[4]

**Cordelia** acts as the inner shepherd satellite for Uranus' ε ring.[11] **Cordelia**'s orbit is within Uranus' synchronous orbit radius, and is therefore slowly decaying due to tidal deceleration.[4]
Portia

Biggest member of portia group

****Portia**** is an inner satellite of Uranus. It was discovered from the images taken by *Voyager 2* on 3 January 1986, and was given the temporary designation **S/1986 U 1**.[7] The moon is named after **Portia**, the heroine of William Shakespeare's play *The Merchant of Venice*. It is also designated **Uranus XII**.[8]

**Portia** is the second-largest inner satellite of Uranus after Puck. The Portian orbit, which lies inside Uranus' synchronous orbital radius, is slowly decaying due to tidal deceleration. The moon will one day either break up into a planetary ring or hit Uranus.

It heads a group of satellites called the **Portia Group**, which includes Bianca, Cressida, Desdemona, Juliet, Rosalind, Cupid, Belinda and Perdita.[6] These satellites have similar orbits and photometric properties.[6]

Little is known about **Portia** beyond its size of about 140 km,[3] orbit,[2] and geometric albedo of about 0.08.[6]
Desdemona

****Desdemona**** is an inner satellite of Uranus. It was discovered from the images taken by *Voyager 2* on 13 January 1986, and was given the temporary designation **S/1986 U 6**.[10] **Desdemona** is named after the wife of Othello in William Shakespeare's play *Othello*. It is also designated **Uranus X**.[11]

**Desdemona** belongs to Portia Group of satellites, which also includes Bianca, Cressida, Juliet, Portia, Rosalind, Cupid, Belinda and Perdita.[9] These satellites have similar orbits and photometric properties.[9] Other than its orbit,[5] radius of 32 km[6] and geometric albedo of 0.08[9] virtually nothing is known about **Desdemona**.

## **Desdemona** may **collide**

**Desdemona** is an inner satellite of Uranus. It was discovered from the images taken by Voyager 2 on 13 January 1986, and was given the temporary designation S/1986 U 6. ... **Desdemona** may **collide** with one of its neighboring **moons** Cressida or Juliet within the next 100 million years.
Tres-2b

Darket Planet Ever Known

**TrES-2b** (**TrES-2** or **Kepler-1b**) is an extrasolar planet orbiting the star GSC 03549-02811 located 750 light years away from the Solar System. The planet has been identified in 2011 as the darkest known exoplanet, reflecting less than 1% of any light that hits it.[4] The planet's mass and radius indicate that it is a gas giant with a bulk composition similar to that of Jupiter. Unlike Jupiter, but similar to many planets detected around other stars, TrES-2b is located very close to its star, and belongs to the class of planets known as hot Jupiters. This system was within the field of view of the *Kepler* spacecraft.[1]

This planet continues to be studied by other projects and the parameters are being improved continuously. A 2007 study improved stellar and planetary parameters.[5] A 2008 study concluded that the TrES-2 system is a binary star system. This has a significant effect on the values for the stellar and the planetary parameters
Kepler 186e

Four Planet From The Kepler 186]

Kepler 186c

Kepler 186d

Kepler 186f

Grey

**Kepler-186e** (also known by its Kepler Object of Interest designation *KOI-571.04*) is a confirmed exoplanet orbiting the red dwarf star Kepler-186, approximately 582 light years away from Earth in the constellation of Cygnus. It is near the optimistic habitable zone but probably not in it, possibly making it have a runaway greenhouse effect, like Venus. The exoplanet was found by using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. Four additional planets orbiting the star (all modestly larger than Earth) were also discovered
Lipperhey

Last Planet From The 55 Cancri A

**55 Cancri d** (abbreviated **55 Cnc d**), formally named **Lipperhey** /ˈlɪpərhiː/, is an extrasolar planet in a long-period orbit around the Sun-like star 55 Cancri A. Located at a similar distance from its star as Jupiter is from our Sun, it is the fifth and outermost known planet in its planetary system. 55 Cancri d was discovered on June 13, 2002.
TRAPPIST-1 b

mad

TRAPPIST-1 d

TRAPPIST-1 e

TRAPPIST-1 f

TRAPPIST-1 g

TRAPPIST-1 h

**TRAPPIST-1b**, also designated as **2MASS J23062928-0502285 b,** is a mainly rocky, Venus-like exoplanet orbiting around the ultra-cold dwarf star TRAPPIST-1, located approximately 39 light-years (12 parsecs) away from Earth in the constellation Aquarius. The planet was detected using the transit method, where a planet dims the host star's light as it passes in front of it. It was first announced on May 2, 2016, and between 2017 and 2018, more studies were able to refine its physical parameters.

The planet is about the same mass as Earth, but about 12% larger. Its relatively low density, along with spectroscopic observations, have confirmed that it has an extremely thick and hot atmosphere. Observations published in 2018 showed that the atmosphere of TRAPPIST-1b was much larger than that of Earth or Venus, as well as being very hot and potentially rich on CO2.[2] More recent modeling studies have suggested the planet is too hot even to allow the formation of sulfuric acid clouds, as found on Venus, the hottest planet in our solar system.
Planet 10

## Character Info

### Enemies

everyone (Especially Neptune?)

**Planet Ten**

**Description**

tba

**Solar System**

Star

Sun

Planets
 Mercury ,  Venus ,  Earth,  Mars,  Jupiter,  Saturn ,  Uranus ,  Neptune

Hypothetical planets
 Planet 9 ,  Planet 10

Dwarf Planets
 Pluto ,
 Ceres ,
 Eris ,
 Makemake ,
 Haumea ,
 Deedee ,
 Varuna ,
 Orcus ,
 Ixion ,
 Sedna ,
 Salacia