recursal/Fanatic-Fandom huggingface dataset:
2019 'Abzorbaloff' Tour

The '**Abzorbaloff' UK & Ireland Tour** was the first concert tour by TCoS in support of their first studio album Abzorbaloff. The tour began on the 24th of July 2019 at the B&M store in Luton and ended on the 8th of September 2019 in Slough.

## Background

Following the release of TCoS' debut album *Abzorbaloff* in July 2019 with record sales DWT Records wished to capitalise on their publicity and quickly put together a tour covering the UK and Ireland. Between the release of the album and the start of the tour TCoS recruited Avon as keytarist and confirmed he would take part in the tour as a full band member. Shortly before the tour began TCoS performed an impromptu concert at the site of the burning offices of *The Daily Vortex*. Though officially their first concert it is not considered by the band as part of the subsequent tour.

## Noteable events

### Wembley

*See 'Wembly' car photo for more detail*

The second concert due to be held in Wembley on the 25th of July 2019 caused the infamous 'Car-gate' scandal. Confusion over the exact location of the concert led to the band being up divided between two vehicles; Deborah J's "Cool" car - a jaunty yellow Ford Capris - headed for Wembly, and Danoftardis' "Lame" car - a pantone grey early 90s Volvo - headed for Wembley. This quickly spiralled from mild disagreement into arson when the "cool" car was found destoryed. Deborah J left the band and famous TCoS fan Doctor Gamer had to cover for her at the next concert. Relations between Deborah and Dan were soon patched up and the tour resumed as normal.

### Llanfair­pwllgwyngyll­gogery­chwyrn­drobwll­llan­tysilio­gogo­goch

The concert at Llanfair­pwllgwyngyll­gogery­chwyrn­drobwll­llan­tysilio­gogo­goch on the 14th of August was heavily delayed by the absence of singer Deborah J. It later transpired that she had got lost in the Welsh countryside while attempting to locate the town. She eventually arrived in a most agitated state, repeatdly stating "I don't want to talk about it". The concert began but was later interrupted by a group of locals from Pontypandy who, in a most agrieved state, accused Deborah of henious crimes against their community including the theft of well know resident Trevor Evans' bus. Rioting then occurred and the rest of the concert was cancelled as the band fled for their lives.

Pictures appeared in intergalactic newspapers the next day appearing to show Ms. J driving a bus in a dangerous and violent manner causing mayhem and destruction, seemingly backing up the accusations made by the denizens of Pontypandy. Deborah refuted these allegations, speaking on Daleks Jones' radio show the next day explaining that it was in fact famous doppleganger and notorious master cimminal Deborah Jorse driving the bus and that she in fact "spent the evening in a pub outside Pontypridd" while her 'cool car' was repaired and had "numerous witnesses to prove it". DWT Records' legal team settled the case out of court and the tour continued on.

 Compilation albums
 Live albums
 EPs
 Singles
Meta:Public Sandbox

**Welcome to the public Sandbox! Here you may experiment with editor settings, among other things like: template testing and images.**

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2020 CD₃

**This page/section has been marked for fixing under Project/Paraphrase**
This page is to be fixed and paraphrased under the project's guidelines. Please do not remove this tag until the project has ended.**This object is a temporary satellite of: Earth**
It may or may still be in Earth orbit.
**2020 CD3** (also **2020CD3** or **CD3** for short) is a tiny near-Earth asteroid (or minimoon) that ordinarily orbits the Sun but makes close approaches to the Earth–Moon system, in which it can temporarily enter Earth orbit through temporary satellite capture (TSC). It was discovered at the Mount Lemmon Observatory by astronomers Theodore Pruyne and Kacper Wierzchoś on 15 February 2020, as part of the Mount Lemmon Survey or Catalina Sky Survey. The asteroid's discovery was announced by the Minor Planet Center on 25 February 2020, after subsequent observations confirmed that it was orbiting Earth.

## Designation and Discovery

### Discovered By

Mt. Lemmon SurveyTheodore A. PruyneKacper W. Wierzchoś

### Minor Planet Categories

NEO, PH, Arjuna, Apollo, Temporarily Captured, Co-orbital

## Orbit Data

### Eccentricity

0.01245 (heliocentric)58901.0 (geocentric)

### Aphelion

1.0418 AU

It is the second temporary satellite of Earth discovered *in situ*, after 2006 RH₁₂₀, which was discovered in 2006. Based on its nominal trajectory, 2020 CD3 was captured by Earth around 2016–2017, and escaped Earth's gravitational sphere of influence around 7 May 2020. 2020 CD3 will make another close pass to Earth in March 2044, though it will most likely not be captured by Earth due to the greater approach distance.

2020 CD3 has an absolute magnitude around 32, indicating that it is very small in size. Assuming that 2020 CD3 has a low albedo characteristic of dark, carbonaceous C-type asteroids, its diameter is probably around 1.9–3.5 metres (6–11 ft). 2020 CD3 is classified as an Arjuna asteroid, a subtype of small Earth-crossing Apollo asteroids that have Earth-like orbits.
Jupiter LII

**Jupiter LII**, provisionally known as **S/2010 J 2**, is a natural satellite of Jupiter. It was discovered by Christian Veillet in 2010.

## Jupiter LII

Image of S/2010 J 2 (Jupiter LII) taken by Canada-France-Hawaii Telescope on September 2010

## Physical Characteristics

### Diameter

1 km

Jupiter LII has a diameter of about ~1 kilometer and it was the smallest and also the faintest known moon of Jupiter to have been discovered from Earth having an absolute magnitude of 17.4 (Before S/2022 J 1, S/2021 J 4 and S/2022 J 2 were announced).

Jupiter LII is a member of the Ananke group.
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**.

## Ophelia

Image of Ophelia taken in January 21, 1986

## Discovery

### Discovered by

Richard J. Terrile
*Voyager 2*

## Physical Characteristics

### Mean Density

~1.3 g/cm³

Ophelia, together with Cordelia, it is a shepherd moon of Uranus that shepherds ε ring (Epsilon ring).
Greip

**Greip** or **Saturn LI** is a natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on 26 June 2006, from observations taken between 5 January and 1 May 2006.

## Greip

Image of Greip taken by Cassini in September 2015

## Physical Characteristics

### Synodic Rotation Period

12.75 h

Greip is about 6 kilometres in diameter, and orbits Saturn at an average distance of 18,066 Mm in 906.556 days, at an inclination of 172.7° to the ecliptic, in a retrograde direction and with an eccentricity of 0.3735.

It has a very high chance of colliding Phoebe in the future. Greip is one of the 100 members of the Norse group, a large collection of retrograde irregular natural satellite.
Puck

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**Puck** is an inner moon of Uranus. It was discovered in December 1985 by the *Voyager 2* spacecraft. It is also provisionally designated as **S/1985 U 1**.

## Discovery

### Discovered by

Stephen P. Synnott
*Voyager 2*
22 Kalliope

**Kalliope** (minor planet designation: **22 Kalliope**) is a large M-type asteroid and binary from the asteroid belt. It is named after Calliope, one of the

## Physical Characteristics

### Absolute Magnitude

6.45

muses (epic poetry) from Greek Mythology. It has a small moon named **Linus**.

## Physical Characteristics

Kalliope is somewhat elongated and abou 166 km in diameter, and slightly asymmetric, as evidenced by resolved images taken with the VLT at the European Southern Observatory. Kalliope is an M-type, meaning that it is mostly comprised of iron, nickel, or other metals. Its density is about 3.4 g/cm3, which means that it is also made up of silicate rock too. Kalliope also has a low radar albedo, which is inconsistent with a purely metallic surface.

Lightcurve analysis indicates that Kalliope's pole most likely points towards ecliptic coordinates (β, λ) = (−23°, 20°) with a 10° uncertainty, which gives Kalliope an axial tilt of 103°. Kalliope's rotation is then slightly retrograde.

Between 2004 and 2021, 22 Kalliope has been observed to occult fifteen stars.

## Satellite

> *Main article: Linus*
>
>

Kalliope has one known natural satellite, called **Linus**, **(22) Kalliope I Linus** or **S/2001 (22) I.** It is actually quite large for its size (about 28 km in diameter) and could be a large asteroid itself. Linus orbits at a distance of 1100 km from Kalliope's center. It was discovered on 29 August 2001 by Jean-Luc Margot and Michael E. Brown, while another team led by William Merline also independently detected the moon 3 days later.
S/2007 S 2

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**S/2007 S 2** is a natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 1, 2007, from observations taken between January 18 and April 19, 2007.

## Physical Characteristics

### Diameter

6 km

S/2007 S 2 is about ~6 kilometres in diameter, and orbits Saturn at an average distance of 16,054,500 kilometres in 759.2 days, at an inclination of 176.65° to the ecliptic, in a retrograde direction and with an eccentricity of 0.237.

S/2007 S 2 was considered lost after its discovery and was then recovered in October 2019.
S/2004 S 26

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**Saturn LVIII**, provisionally known as **S/2004 S 26**, is a distant known natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, and Jan Kleyna on October 7, 2019 from observations taken between December 12, 2004 and March 21, 2007.

## Designations

### Alternative Names

Saturn LVIII
S8353a

## Physical Characteristics

### Diameter

4 km

It was given its permanent designation in August 2021. As of 2023, it has not been given its official name.
Lyana Gauthier

Status: Princess

Kingdom: Kasmira

Age: 13 (Alive)

Skin: Tan

Eyes: Black

Hair: Black

Gender: Female

Father: Henry Gauthier

Mother: Vanessa Gauthier

Siblings;

Silvia Gauthier

Savannah Gauthier

Stuart Gauthier

Chantelle Gauthier

Turner Gauthier

Napier Gauthier

Rhys Gauthier

Vinzent Gauthier

Andrea Gauthier

Isaure Gauthier

Betrothed:

Children;
14 Irene

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**Irene** /aɪˈriːniː/ (minor planet designation: **14 Irene**) is a large main-belt asteroid, discovered by the English astronomer John Russell Hind on May 19, 1851. It is orbiting the Sun at a distance of 2.585 AU with a period of 4.16 yr and an eccentricity of 0.168. The orbital plane is tilted at an angle of 9.1° to the plane of the ecliptic.

14 Irene was named after *Irēnē*, a personification of peace in Greek mythology. She was one of the Horae, daughter of Zeus and Themis. The name was suggested by Sir John Herschel. Hind wrote,

"You will readily discover that this name [...] has some relation to this event (the Great Industrial Exhibition) which is now filling our metropolis [London] with the talent of all civilised nations, with those of Peace, the productions of Art and Science, in which all mankind must feel an interest."
Cupid

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**Cupid** is an inner satellite of Uranus. It was discovered by Mark R. Showalter and Jack J. Lissauer in 2003 using the Hubble Space Telescope. It was named after a character in William Shakespeare's play *Timon of Athens*.

## Cupid

Image of Cupid taken by Hubble Space Telescope

## Discovery

### Discovered by

Mark R. Showalter
Jack J. Lissauer

## Physical Characteristics

### Mean Density

~1.3 g/cm³

Cupid is the smallest known inner Uranian satellite at a diameter of just ~18km.

After its discovery, Cupid was given the temporary designation **S/2003 U 2**. It is also designated Uranus **XXVII**.
Narvi

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**Narvi** or **Saturn XXXI** is a retrograde irregular natural satellite of Saturn. It was discovered by a team of astronomers led by Scott S. Sheppard in 2003, and given its provsional designation **S/2003 S 1**.

## Physical Characteristics

### Synodic Rotation Period

10.21 h

Narvi is about ~7km in diameter and the first moon of Saturn that was discovered by Scott S. Sheppard
Elara

Image of Elara taken by the New Horizons probe on March 5, 2007.

**Elara**, otherwise known as **Jupiter VII**, is an irregular natural satellite of Jupiter that is located within the Himalia Group. It is the eighth largest moon of Jupiter, and the second largest irregular Jovian moon as well. Elara remained known as simply “Jupiter VII” until 70 years after its discovery in 1975, when it was officially named Elara by the IAU.

## Discovery

Elara was discovered by Charles D. Perrine on January 5, 1905 within the Lick Observatory. The satellite was found within images taken by the Crossley Telescope, and its discovery was confirmed on February 21, 1905.

## Appearance & Size

Little is known about what Elara really looks like, and the LORRI on the New Horizons spacecraft does not take colored images. However, Elara appears to be an irregular-shaped object with dark patches on its top and bottom. Not much else can be said about its appearance, as it would otherwise just be speculation.

Elara has a diameter of 53.438 miles, making it the eighth largest moon of Jupiter, behind the Galilean Four, Amalthea, Himalia, and Thebe.

## Exploration

Due to the interest of the Galilean Four and Amalthea as compared to Jupiter’s other moons, Elara is rarely embarked upon. However, the New Horizons spacecraft did a flyby of Elara in February and March of 2007 within 5 million miles of the satellite.

## Orbit

The orbit of Elara is slightly inclined and eccentric, and the orbit is also fairly distant from Jupiter. This likely means Elara was captured a long time ago by Jupiter’s gravity, or formed from a collision with another satellite. It takes Elara roughly 259 earth days to complete an orbit around Jupiter.

Elara has an average distance from Jupiter at approximately 7.3 million miles, making it the 16th closest moon to Jupiter.
Skathi

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**Skathi**, also named **Saturn XXVII** is an irregular natural satellite of Saturn.

## Skathi

Images of Skathi (circle) taken by Canada-France-Hawaii Telescope in September 2000

## Physical Characteristics

### Synodic Rotation Period

11.10 h

Skathi is about ~8km in diameter.

## Origin

Skathi, along with 98 other retrograde natural satellites in the Norse group, are could just be a fragment that collide, broke off or impacted the largest irregular moon Phoebe.
Namaka

**Namaka** is the inner moon of the trans-Neptunian dwarf planet Haumea. It is named after Nāmaka, the goddess of the sea in Hawaiian mythology, and one of the daughters of Haumea.

## Namaka

Image of Haumea and its moons Hi‘iaka and Namaka (arrow) taken by Hubble Space Telescope

## Discovery

### Discovered by

Michael E. Brown
Chad Trujillo

## Designations

### Alternative Names

S/2005 (136108) 1
S/2005 (2003 EL₆₁) 1
(136108) 2003 EL₆₁ I

## Discovery

Namaka was discovered on June 30, 2005 and announced on November 29 the same year. It was nicknamed "Blitzen" by the discovery team, following the naming scheme for Haumea (Santa) and Hi'iaka (Rudolph).

## Physical Characteristics

The moon's surface is most likely composed of silicate rock (as this is what Haumea is made of and frozen volatiles. The surface of Namaka is highly reflective, showing that it has lots of frozen water ice on its surface.
Extreme Trans-Neptunian Objects

**Extreme trans-Neptunian objects (ETNOs)** are trans-Neptunian objects that orbit the sun well beyond the orbit of Neptune (~30 AU) at the outermost regions of the solar system. An ETNO has a large semi-major axis of at least 150–250 AU. Its orbit is much less affected by the known giant planets than all other known trans-Neptunian objects. They may, however, be influenced by gravitational interactions with a hypothetical Planet Nine, shepherding these objects into similar types of orbits. The known ETNOs exhibit a highly statistically significant asymmetry between the distributions of object pairs with small ascending and descending nodal distances that might be indicative of a response to external perturbations.

## Subcategories

ETNOs can be subdivided into two different categories: Extreme Scattered Disc Objects and Extreme Detached Disc Objects.

### Extreme Scattered Disc Objects

The scattered ETNOs (or extreme scattered disc objects, ESDOs) have perihelia around 38–45 AU and an exceptionally high eccentricity of more than 0.85. As with the regular scattered disc objects, they were likely formed as result of gravitational scattering by Neptune and still interact with the giant planets.

### Extreme Detached Disc Objects

EDDOs have perihelia approximately between 40–45 and 50–60 AU, are less affected by Neptune than the scattered ETNOs, but are still relatively close to Neptune. The sednoid or inner Oort cloud objects, with perihelia beyond 50–60 AU, are too far from Neptune to be strongly influenced by it.
Titania

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## Physical Characteristics

### Mean Surface Temperature

70±7 K

*Not what you're looking for? See: **Titan or Triton***

**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 (981 mi), with a surface area comparable to that of Australia. Discovered by William Herschel in 1787, it is named after the queen of the fairies in Shakespeare's *A Midsummer Night's Dream*. Its orbit lies inside Uranus's magnetosphere.

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. Its surface, 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.
Tarqeq

**Tarqeq**, also known as **Saturn LII** (provisional designation **S/2007 S 1**) is a natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on 13 April 2007 from observations taken between 5 January 2006 and 22 March 2007.

## Tarqeq

Image of Tarqeq taken by Cassini in June 2016

## Designations

### Adjectives

Tarquipian
Tarqeqian

## Physical Characteristics

### Synodic Rotation Period

76.13 h

Tarqeq is a member of the Inuit group and a Siarnaq subgroup member.
S/2006 S 1

**This page/section has been marked for fixing under Project/Paraphrase**
This page is to be fixed and paraphrased under the project's guidelines. Please do not remove this tag until the project has ended.**S/2006 S 1** is a natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on June 26, 2006 from observations taken between January 4 and April 30, 2006.

## Physical Characteristics

### Diameter

6 km

S/2006 S 1 is about ~6 kilometres in diameter, and orbits Saturn at an average distance of 18.65 Gm in 951.1 days, at an inclination of 154.6° to the ecliptic (178.9° to Saturn's equator), in a retrograde direction and with an eccentricity of 0.0814.

S/2006 S 1 was considered lost after its discovery and was then recovered in October 2019.
Project/Solar System

Project #1

**Project Solar System is meant to quickly and reliably create articles for all celestial bodies listed in the solar system template:**

**Please work from top to bottom, and at a reasonable pace.**

## Guidelines

1. **Please don't just make stupid articles with four words. Instead put in the time and effort to create the article. Afterwards, please post a link to the page on my message wall.**
2. **Follow wiki expectations, like adding the solar system template to the bottom, adding an infobox, some images, etc.**
3. **Please contact me if you need help, as some of these celestial bodies do not have clear understandings.**
4. **Please no false information or opinions.**

## Contacts

Head of Administration: **EarthCab**

Head Moderator: **Lemniscate Biscuit**

Head of Bureaucratic Commissions: **StarSubject**
Erriapus

**Erriapus**, or **Saturn XXVIII**, is a prograde irregular satellite of Saturn. It was discovered by Brett Gladman, John J. Kavelaars and colleagues in 2000, and given its provisional designation **S/2000 S 10**.

## Erriapus

Images of Erriapus taken by Canada-France-Hawaii Telescope in September 2000

## Designations

### Alternative Names

S/2000 S 10
Erriapo

## Physical Characteristics

### Synodic Rotation Period

28.15 h

Erriapus is about ~10 kilometres in diameter, the second largest moon in the Gallic group.
Shoemaker–Levy 9

**Comet Shoemaker–Levy 9** (formally designated **D/1993 F2**) broke apart in July 1992 and collided with Jupiter in July 1994, providing the first direct observation of an extraterrestrial collision of Solar System objects. This generated a large amount of coverage in the popular media, and the comet was closely observed by astronomers worldwide. The collision provided new information about Jupiter and highlighted its possible role in reducing space debris in the inner Solar System.

## D/1993 F2 (Shoemaker–Levy)

Shoemaker–Levy 9, a disintegrated comet on a collision course(total of 21 fragments, taken in July 1994)

## Discovery

### Discovered By

Carolyn ShoemakerEugene ShoemakerDavid Levy
Eukelade

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**Eukelade**, also known as **Jupiter XLVII**, is a retrograde irregular satellite of Jupiter. It was discovered by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2003, and was given its provisional designation **S/2003 J 1**. Eukelade is the first natural satellite discovered in 2003.

## Eukelade

Images of Eukealde taken by Scott S. Sheppard on March 4, 2003

## Physical Characteristics

### Diameter

4 km

Eukelade is about ~4 kilometres in diameter, and orbits Jupiter at an average distance of 23,484,000 km in 693.02 days, at an inclination of 164° to the ecliptic, in a retrograde direction and with an eccentricity of 0.2829.

Eukelade belongs to the Carme group, made up of irregular moons orbiting Jupiter in the opposite direction from its rotation.
Leda

Leda as seen by the WISE spacecraft in June 2010.

**Leda**, designated as **Jupiter XIII**, is an irregular outer satellite of Jupiter that’s within the Himalia Group. Despite being the 4th largest in its group, it’s actually fairly small when compared to other Himalia Group members or other moons.

## Discovery

Charles D. Kowal discovered Leda at the Palomar Observatory on after taking various images from September 11–13 of 1974, with Leda seeming to be on all of them. The moon’s named was suggested by Kowal and adopted by the IAU in 1975.

## Appearance & Size

Leda may have dark patches on its surface like other Himalia Group moons, as most of the moons look similar to each other. However, very little is actually known about what the moon looks like due to it not having any clear images of its surface features.

Leda has an estimated diameter of 12.4 miles, making it the 4th largest moon in the Himalia Group, and among the 15th largest overall.

## Orbit

Leda orbits Jupiter at a distance of around 6.9 million miles, and takes 242 days to complete a full orbit. This makes it the closest moon to Jupiter in the Himalia Group, and the 10th closest overall.
2006 RH₁₂₀

**2006 RH120** is a tiny near-Earth asteroid and fast rotator with a diameter of approximately 2–3 meters that ordinarily orbits the Sun but makes close approaches to the Earth–Moon system around every twenty years, when it can temporarily enter Earth orbit through temporary satellite capture (TSC). Most recently, it was in Earth orbit from July 2006 to July 2007, during which time it was never more than 0.0116 AU (1.74 million km) from Earth.

## Designation and Discovery

### Minor Planet Categories

Amor, Apollo, Aten, NEO, Temporary Satellite(Temporary satellite of Earth 2006–2007)

## Orbit Data

### Eccentricity

0.02452

As a consequence of its temporary orbit around the Earth, it is currently the second smallest asteroid in the Solar System with a well-known orbit, after 2021 GM1. Until given a minor planet designation on 18 February 2008, the object was known as **6R10DB9**, an internal identification number assigned by the Catalina Sky Survey.

## Discovery

2006 RH120 was discovered on 14 September 2006 by Eric Christensen with the 27-inch (690 mm) Schmidt camera of the Catalina Sky Survey in Arizona. "6R10DB9" was the Catalina Sky Survey's own discovery designation for this object, which usually would only be used on the MPC's Near-Earth Object Confirmation Page (NEOCP) until an IAU designation was applied, if the object was classified as a minor object. It was added on 14 September to the NEOCP and subsequently removed with the explanation that it "was not a minor planet". Preliminary orbital calculations indicated it was captured by Earth's gravity from solar orbit of a period of about 12 months, which is similar to that of many spent rocket boosters dating to the Apollo program of the 1960s and early 1970s. 6R10DB was assigned the designation 2006 RH120 on 18 February 2008.
Surtur

**Surtur** or **Saturn XLVIII** (provisional designation **S/2006 S 7**) is a retrograde irregular natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard et al. on June 26, 2006 from observations taken between January and April 2006.

## Physical Characteristics

### Diameter

6 km

Surtur is about ~6 kilometres in diameter, and orbits Saturn at an average distance of 22.707 Mm in 1297.7 days, orbiting in a retrograde direction, at an inclination of 177.5° and an eccentricity of 0.451.
Skrymir

**Skrymir**, provisionally known as **S/2004 S 23**, is a natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, and Jan Kleyna on October 7, 2019 from observations taken between December 12, 2004 and March 22, 2007.

## Designations

### Alternative Names

Saurn LVI
S/2004 S 23
S8630a

## Physical Characteristics

### Diameter

4 km

Skrymir is about ~4 kilometres in diameter, and orbits Saturn at an average distance of 21.163 Gm in 1149.82 days, at an inclination of 177° to the ecliptic, in a retrograde direction and with an eccentricity of 0.373.

Skrymir received its permanent designation **Saturn LVI** in August 2021 and was given its official name 1 year later.
Anthe

**Anthe** is a very small natural satellite of Saturn lying between the orbits of Mimas and Enceladus. It is also known as **Saturn XLIX** and its provisional designation **S/2007 S 4**.

## Physical Characteristics

### Synodic Rotation Period

synchronous

The provisional designation **S/2007 S 5** was incorrectly designated. The designation S/2007 S 5 was then used by an irregular natural satellite published on May 3, 2023.

Like Methone and Pallene, Anthe is one of the 3 alkyonide moons.
Moon

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This article is a stub — it needs more information. You can help Solarpedia by expanding it.

**The Moon** is Earth's only natural satellite. Its diameter is about one-quarter of Earth's, making it the fifth largest satellite in the Solar System and the largest and most massive relative to its parent planet. It is larger than all known dwarf planets in the Solar System.
(55565) 2002 AW₁₉₇

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**(55565) 2002 AW₁₉₇** is a classical, non-resonant trans-Neptunian object from the Kuiper belt in the outermost region of the Solar System, also known as a cubewano. With a likely diameter of at least ~700 kilometers, it is approximately tied with 2002 MS₄ and 2013 FY₂₇ as the largest unnamed object in the Solar System.

## (55565) 2002 AW₁₉₇

Image of 2002 AW₁₉₇ taken by Hubble Space Telescope in 2006

## Physical Characteristics

### Diameter

768 ± 39 km
734 ± 116 km
700 ± 50 km
886 km

### Synodic Rotation Period

8.87 ± 0.01 h
8.78 ± 0.05 h
8.86 ± 0.01 h

2002 AW₁₉₇ has no known moons currently, meaning its mass cannot be calculated.
Bebhionn

**Bebhionn**, also known as **Saturn XXXVII**, is a small, irregular natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on 4 May 2005 from observations taken between 12 December 2004 and 9 March 2005.

## Bebhionn

Image of Bebhionn taken by Cassini in May 2017

## Discovery

### Discovered by

Scott S. Sheppard
David C. Jewitt
Jan T. Kleyna
Brian G. Marsden

## Physical Characteristics

### Synodic Rotation Period

16.33 h

Bebhionn is about ~6 kilometres in diameter and orbits Saturn at an average distance of 16,898 Mm in 820.130 days at an inclination of 41° to the ecliptic and with an eccentricity of 0.333.

Bebhionn is a member of the Gallic group. Like Bestla, Erriapus and Kiviuq, Bebhionn could potentially have its own moon orbiting around it (according to light curve analysis).
162173 Ryugu

**This page/section has been marked for fixing under Project/Paraphrase**
This page is to be fixed and paraphrased under the project's guidelines. Please do not remove this tag until the project has ended.**162173 Ryugu**, provisional designation 1999 JU₃, is a near-Earth object and a potentially hazardous asteroid of the Apollo group. It measures approximately 900 metres in diameter and is a dark object of the rare spectral type Cb, with qualities of both a C-type asteroid and a B-type asteroid.

## Designation and Discovery

### Minor Planet Categories

Apollo, Potentially Hazardous, Near-Earth-Object

## Overview

In June 2018, the Japanese spacecraft *Hayabusa2* arrived at the asteroid. After making measurements and taking samples, *Hayabusa2* left Ryugu for Earth in November 2019 and returned the sample capsule to Earth on 5 December 2020. The samples showed the presence of organic compounds, such as uracil (one of the four components in RNA) and vitamin B3.

### Orbit

The origin of 162173 Ryugu may be either 495 Eulalia or 142 Polana. Ryugu orbits the Sun at a distance of 0.96–1.41 AU once every 16 months (474 days; semi-major axis of 1.19 AU). Its orbit has an eccentricity of 0.19 and an inclination of 6° with respect to the ecliptic. It has a minimum orbital intersection distance with Earth of 95,443.442 km (0.000638 AU), equivalent to 0.23 lunar distances.
S/2004 S 39

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**S/2004 S 39** is a natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, and Jan Kleyna on October 8, 2019 from observations taken between December 12, 2004 and March 21, 2007.

## Physical Characteristics

### Diameter

2 km

S/2004 S 39 is about ~3 kilometres in diameter, and orbits Saturn at an average distance of 23.575 Gm in 1351.83 days, at an inclination of 167° to the ecliptic, in a retrograde direction and with an eccentricity of 0.080.

S/2004 S 39 was the last moon ever announced in 2019.
Gunnlod

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**Gunnlod**, provisionally known as **S/2004 S 32**, is a natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, and Jan Kleyna on October 8, 2019 from observations taken between December 12, 2004 and January 19, 2007.

## Designations

### Alternative Names

Saturn LXII
S/2004 S 32
S64472

## Physical Characteristics

### Diameter

4 km

It was given its permanent designation **Saturn LXII** in August 2021 and received its official name 1 year later.

Gunnlod is about ~4 kilometres in diameter, and orbits Saturn at an average distance of 21.214 Gm in 1153.96 days, at an inclination of 159° to the ecliptic, in a retrograde direction and with an eccentricity of 0.251.
136472 Makemake

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**Makemake** (minor-planet designation **136472 Makemake**) is a dwarf planet and the second-largest of what are known as the classical population of Kuiper belt objects, with a diameter approximately that of Saturn's moon Iapetus, or 60% that of Pluto. It has one known satellite. Its extremely low average temperature, about 40 K (−230 °C), means its surface is covered with methane, ethane, and possibly nitrogen ices.

Makemake was discovered on March 31, 2005 by a team led by Michael E. Brown, and announced on July 29, 2005. It was initially known as **2005 FY9** and later given the minor-planet number 136472. In July 2008, it was named after Makemake, a creator god in the Rapa Nui mythology of Easter Island, under the expectation by the International Astronomical Union (IAU) that it would prove to be a dwarf planet.
Hyperion

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## Hyperion

Hyperion in approximately natural color, as photographed by the Cassini spacecraft

## Physical Characteristics

### Mean Radius

135.00±4.00 km

**Hyperion**, also known as **Saturn VII**, 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.

## Name

The moon is named after Hyperion, the Titan god of watchfulness and observation – the elder brother of Cronus, the Greek equivalent of the Roman god Saturn. It is also designated *Saturn VII*. The adjectival form of the name is *Hyperionian*.

Hyperion's discovery came shortly after John Herschel had suggested names for the seven previously known satellites of Saturn in his 1847 publication *Results of Astronomical Observations made at the Cape of Good Hope*. William Lassell, who saw Hyperion two days after William Bond, had already endorsed Herschel's naming scheme and suggested the name Hyperion in accordance with it. He also beat Bond to publication.
Miranda

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**Miranda** also known as **Uranus V** is the smallest of the major moons of Uranus. It was discovered by Gerard Kuiper on 16 February 1948 at McDonald Observatory in Texas, and named after Miranda from William Shakespeare's play *The Tempest*. Like the other large moons of Uranus, Miranda orbits close to its planet's equatorial plane. Because Uranus orbits the Sun on its side, Miranda's orbit is perpendicular to the ecliptic and shares Uranus' extreme seasonal cycle.
Meta:Placeholder Images

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Triton

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This page is to be fixed and paraphrased under the project's guidelines. Please do not remove this tag until the project has ended.*Not what you're looking for? See: **Titan or Titania.***

**Triton** is the largest natural satellite of the planet Neptune, and was the first Neptunian moon to be discovered, on October 11, 1846, by English astronomer William Lassell. It is the only large moon in the Solar System with a retrograde orbit, an orbit in the direction opposite to its planet's rotation. Because of its retrograde orbit and composition similar to Pluto, Triton is thought to have been a dwarf planet, captured from the Kuiper belt.

## Orbit Data

### Inclination

129.812° (to the ecliptic)
156.885° (to Neptune's equator)
129.608° (to Neptune's orbit)

## Atmospheric Data

### Surface Pressure (mean)

1.4 to 1.9 Pa (1.38×10−5 to 1.88×10−5 atm)

### Composition

nitrogen and methane

At 2,710 kilometers (1,680 mi) in diameter, it is the seventh-largest moon in the Solar System, the only satellite of Neptune massive enough to be in hydrostatic equilibrium, the second-largest planetary moon in relation to its primary (after Earth's Moon), and larger than Pluto. Triton is one of the few moons in the Solar System known to be geologically active (the others being Jupiter's Io and Europa, and Saturn's Enceladus and Titan). As a consequence, its surface is relatively young, with few obvious impact craters. Intricate cryovolcanic and tectonic terrains suggest a complex geological history. Triton has a surface of mostly frozen nitrogen, a mostly water-ice crust, an icy mantle and a substantial core of rock and metal. The core makes up two-thirds of its total mass. The mean density is 2.061 g/cm3, reflecting a composition of approximately 15–35% water ice.

During its 1989 flyby of Triton, *Voyager 2* found surface temperatures of 38 K (−235 °C) and also discovered active geysers erupting sublimated nitrogen gas, contributing to a tenuous nitrogen atmosphere less than 1/70,000 the pressure of Earth's atmosphere at sea level. *Voyager 2* remains the only spacecraft to have visited Triton. As the probe was only able to study about 40% of the moon's surface, future missions (dubbed "Trident") have been proposed to NASA via their Discovery Program to revisit the Neptune system with a focus on Triton.
Jupiter

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**Jupiter** is the fifth planet from **the Sun** plus the largest planet in the Solar System. It is a gas giant with a mass more than two and a half times that of all the other planets in the Solar System combined, and slightly less than one one-thousandth the mass of the Sun.

## Orbit Data

### Orbital Period

(Sidereal)11.862 yr

4,332.59 d

10,476.8 Jovian solar days

(Synodic)

398.88 d

### Inclination

1.303° to ecliptic6.09° to Sun's equator

0.32° to invariable plane

## Physical Characteristics

### Equatorial Radius

71,492 km (44,423 mi)11.209 R🜨 (of Earth's)

0.10045 R☉ (of Sun's)

### Surface Area

6.1469×10¹⁰ km² (2.3733×10¹⁰ mi²)120.4 of Earth's

### Volume

1.4313×10¹⁵ km³ (3.434×10¹⁴ mi³)1,321 of Earth's

### Mass

1.8982×10²⁷ kg (4.1848×10²⁷ lb)317.8 of Earth's

1/1047 of Sun's

## Atmospheric Data

### Composition

89%±2.0% hydrogen10%±2.0% helium

0.3%±0.1% methane

0.026%±0.004% ammonia

0.0028%±0.001% hydrogen deuteride

0.0006%±0.0002% ethane

0.0004%±0.0004% water
Thiazzi

**Thiazzi**, provisionally known as **S/2004 S 33**, is a natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt and Jan Kleyna on October 8, 2019 from observations taken between December 12, 2004 and March 22, 2007.

It was given its permanent designation **Saturn LXIII** on August 2021 and was officially named after Þjazi, a jötunn from Norse Mythology 1 year later.

Thiazzi is about 4 kilometers in diameter, and orbits Saturn at an average distance of about 24.168 Gm in 1403.18 days, at an inclination of 160° to the ecliptic, in a retrograde direction and with an eccentricity of 0.399
Styx

**This page/section has been marked for fixing under Project/Paraphrase**
This page is to be fixed and paraphrased under the project's guidelines. Please do not remove this tag until the project has ended.**Styx** is a small natural satellite of **Pluto** whose discovery was announced on 11 July 2012. It was discovered by use of the Hubble Space Telescope, and is the smallest of the five known moons of Pluto.

## Styx

Styx, seen by the New Horizons spacecraft

## Orbit Data

### Orbital Period

20.1 d

It was imaged along with Pluto and Pluto's other moons by the New Horizons spacecraft in July 2015, albeit poorly with only a single image of Styx obtained.
Styx is the second-closest known satellite to Pluto, and the fifth discovered. It was discovered one year after Kerberos. Styx is approximately 16 km (9.9 mi) across its longest dimension, and its orbital period is 20.1 days.
Valetudo

**Valetudo**, also known as **Jupiter LXII** and provisionally known as **S/2016 J 2**, is an outermost irregular prograde natural satellite of Jupiter. It was discovered by Scott S. Sheppard and his team in 2016 and has not been announced until 17 July 2018 following the 9 other moons, via a Minor Planet Electronic Circular from the Minor Planet Center.

## Valetudo

Precovery images of Valetudo taken by Canada-France-Hawaii Telescope on February 28, 2003

## Physical Characteristics

### Diameter

1 km

Valetudo has a diameter of about ~1 km and orbits Jupiter at a distance of about 19 million kilometres. Its orbital inclination is 34 degrees, and its orbital eccentricity is 0.222.

Valetudo crossers the orbits of other retrograde moons which may collide in the future and also orbits alone just like Themisto and Carpo (Before S/2018 J 4 was announced).
2022 JF2

*This is Solarpedia's first page!*

## Overview

***2022 JF2*** is a very small asteroid whose orbit crosses the orbit of **Earth**. NASA JPL has classified 2022 JF2 as a "Near Earth Asteroid" due to its orbit's proximity to Earth, but it is not considered potentially hazardous because computer simulations have not indicated any imminent likelihood of future collision.

2022 JF2 orbits the sun every 410 days (1.12 years), coming as close as 0.79 AU and reaching as far as 1.37 AU from **the sun**. Based on its brightness and the way it reflects light, 2022 JF2 is probably between 0.005 to 0.023 kilometers in diameter, making it a small to average asteroid, very roughly comparable in size to a school bus or smaller.
Polydeuces

**This page/section has been marked for fixing under Project/Paraphrase**
This page is to be fixed and paraphrased under the project's guidelines. Please do not remove this tag until the project has ended.**Polydeuces** /ˌpɒlɪˈdjuːsiːz/, also designated **Saturn XXXIV**, is a small trojan moon of Saturn occupying the trailing L5 Lagrange point of Dione. It was discovered by the Cassini Imaging Science Team in images taken by the *Cassini* space probe on 21 October 2004. With a mean diameter of about 3 km (1.9 mi), Polydeuces is thought to have a smooth surface coated with fine, icy particles accumulated from the cryovolcanic plumes of Enceladus. In its orbit around Saturn, Polydeuces periodically drifts away from Dione's Lagrange point due to gravitational perturbations by other nearby moons of Saturn. Of the four known trojan moons of Saturn, Polydeuces exhibits the largest displacement from its Lagrange point.

## Polydeuces

Polydeuces imaged 73,000 km (45,000 mi) away from the Cassini spacecraft on 22 May 2006
Umbriel

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Ijiraq

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**Ijiraq**, or **Saturn XXII**, is a small prograde irregular natural satellite of Saturn. It was discovered by John J. Kavelaars, et al. in 2000, and given its provisional designation **S/2000 S 6**.

## Ijiraq

Images of Ijiraq taken by Canada-France-Hawaii Telescope in September 2000

## Discovery

### Discovered by

John J. Kavelaars
Brett J. Gladman

## Designations

### Adjectives

Ijiraupian
Ijiraqian

## Physical Characteristics

### Synodic Rotation Period

13.03 h

Ijiraq is a member of the Inuit group and a member of the Kiviuq subgroup.