recursal/Fanatic-Fandom huggingface dataset:
Blade Sword

Blade Sword es un personaje secundario de la historia Fall chronicles, siendo el hermano mayor de Fall Sword y esta en entrenamiento para ser un guardia de elite.

### *Personalidad*

Con el fallecimiento de su padre a una temprana edad, Blade tomo el rol del protector de su hermana, estando constantemente preocupado por ella y tomando muchas de sus decisiones en base a ella.

Suele ser alguien bastante amable, decidido e impulsivo, demostrado en varios momentos en los que pierde el control cuando las emociones lo superan como cuando decidió llevar a un niño de 10 años a un viaje a una ciudad desconocida para poder encontrar a su hermana.

Aunque suele ser bastante prudente, si se trata de su hermana, suele tomar decisiones apresuradas sin medir las consecuencias futuras.

### Apariencia

Blade es un hombre de 18 años, de complexión atlética y bastante alto. Tiene ojos color cafe, pelo negro con un mechón rojo en el lado derecho de su rostro y tez clara. A diferencia de su hermana, no tiene ningún atributo animal en su cuerpo, siendo un humano.

### *Habilidades*

#### Aura

Blade es capaz de usar y manipular el aura, la energía que poseen todos los seres vivos. Puede usarla para potenciar sus capacidades fisicas.

### *Historia*

Nacido como hijo de una pareja de nobles, Blade vivió bien los primeros años de su vida. Hasta el fallecimiento de su padre, teniendo que intentar madurar algo mas rápido para poder proteger a su hermana, la cual era maltrada por su condición de Demonio-lobo.

A la edad de 18 fue uno de los maestros de la escuela de su hermana para tomar la prueba de aura, en la cual sabotearía a su hermana para que no se entere de su elemento, sintiéndose culpable por esto. Sin embargo, su novia Karol seria parte de una organización malvada, haciendo que Fall robe un libro prohibido donde aprendería técnicas demoniacas para que después le revelen la verdad de su naturaleza.

Tiempo después Black Cat asaltaría la escuela para secuestrar a Fall, teniendo exito en esto, por lo que tendria que viajar a Catleya junto a Max Fox para poder seguir al secuestrador

### *Relaciones personales*

Fall Sword, su hermana.

Helena Sword y Coutler Sword (fallecido), sus padres.

Max Fox, alumno de su clase y rival de su hermana.

Karol, ex-novia y enemiga.
Celestial

“ Cada uma daquelas luzes no céu... este tempo todo, eram ruínas de civilizações há muito tempo destruídas. Como um esqueleto brilhante que cobria todo o céu noturno, recordam histórias contadas sobre os Celestiais. O povo das estrelas. É dito que eles vieram pela primeira vez até aos Luminantes com o Canticlysm, atraídos do céu pelo Som. ”
 ― Constelações

*"As estrelas clamam pela sua volta"*

## Description

O povo das estrelas. Não confundir com Lux Natus, seus descendentes.

Os Celestiais vieram para os Luminantes das estrelas quando o Canticlysm começou no Velho Mundo.

As cidades dos Celestiais encontram-se abaixo de um mar negro. As estruturas brilhantes estão suspensas por baixo dele, ligadas como correntes.

As suas civilizações caíram em ruína. As suas cidades abandonadas e civilizações mortas poluem o céu na forma de estrelas brilhantes.

Celestiais conhecidos includem Navae e Alsin, que se tornaram figuras religiosas nos tempos modernos.

A igreja Starkindred parece ganhar seus poderes através da ingestão do sangue de um Celestial há muito morto.

As suas aparências variam imenso, vários relatos de diversas pessoas descrevem-nos de formas diferentes, o Celestial crucificado na igreja é uma grande figura, semelhante a um manequim, com quatro braços e sem rosto.
Trailer Song - BFDI: Branches

Please read the channel description.

"**Trailer Song - BFDI: Branches**" is a high quality rip of "Trailer Song" from *BFDI: Branches*.

## Joke

The advertised track is mashed up with "Right Foot Creep" by YoungBoy Never Broke Again.

## Trivia

* mationsBOMB, one of the directors of *BFDI: Branches*, commented saying "OMGG I’ve been waiting for you guys to do this lol". Said comment was hearted by ObjectShowMusic.

## References

1. ↑ https://www.youtube.com/watch?v=K3OL-C4brlM&google\_comment\_id=UgzbBdo0ePmNBtWCYBt4AaABAg
Character & Cars Fanon Wiki

**Welcome to the Character & Cars Fanon Wiki!**
This Fanon is about fan made characters and cars, but not only those two things. It's about many other things like fan made locations and events

We're a collaborative community website about Character & Cars Fanon that anyone, including you, can build and expand. Wikis like this one depend on readers getting involved and adding content. Click the "ADD NEW PAGE" or "EDIT" button at the top of any page to get started!

## Important articles

Carl CorvettesonJennifer CorvettesonCarl Corvetteson's 1972 Mazda Cosmo L10A

*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.
CT Chamaeleontis b

In 2006 and 2007, a faint companion was observed 2.7 arcseconds away from CT Chamaeleontis, using the Very Large Telescope at the European Southern Observatory. Since the object shares common proper motion with CT Chamaeleontis, it is believed to be physically close to the star, with a projected separation of approximately 440 astronomical units. It is estimated to have a mass of approximately 17 Jupiter masses and is probably a brown dwarf or a planet. The companion has been designated CT Chamaeleontis B. The companion was proven to be most likely in the brown dwarf mass range in 2015.

## See also

* GQ Lupi b
* OTS 44
* RIK 72 b

-Wikipedia
Drakkard

Drakkard

### Aparência

Humanoides com tons de pele remetentes à terra, chifres brilhantes crescem no topo de suas cabeças.

### Traços

* +2 Constituição
* +2 Sabedoria
* +1 Destreza

## Propriedades

### Idade

Amadurecem aos 20 anos, vivem até os 400.

### Porte

Geralmente maiores e mais robustos que humanos, porte médio.

### Proficiências

Proficiência em **Arcanismo**, **Intuição** e **Percepção**.

*Vindo dos Luminante do Norte, um povo devoto a Edenkite, são incríveis mediadores de conflito.*

## Descrição

Os Drakkard são uma raça isolada, raramente saindo do Luminante do Norte, mesmo antes do desaparecimento dos *Lightkeepers*. Compostos maioritariamente por monges que buscam o aperfeiçoamento do próprio corpo.
Drakkard possuem semelhanças a dragões, apesar de não possuirem asas. Os seus chifres brilhantes são aquilo que facilmente identifica um Drakkard.

## Habilidades Raciais

 **ENSINAMENTOS DE EDENKITE*** Dá ao usuário a habilidade de meditar, emitindo uma aura branca e fazendo dois orbes brancos orbitar a sua cabeça.
 **POVO DA NEVE*** Capazes de resistir temperatura de -60ºC sem nenhuma proteção, alcançando os -100ºC caso usem roupas pesadas.
* Imunidade a dano de frio.

## Mais Informações

* Lore
* Sobrenomes

Uma raça dracônica vinda do norte.

Conhecidos por se isolarem nos seus próprios mosteiros, os Drakkard buscam uma vida pacífica, longe de conflito. É dito que praticam Tradições Monásticas diferentes daquelas usadas nos outros Luminantes.

* Spellhardt.
* Drakehardt.
* Wyvehardt.
ROXs 42Bb

**ROXs 42Bb** is a directly imaged planetary-mass companion to the binary M star ROXs 42B, a likely member of the Rho Ophiuchi cloud complex. The companion was announced/discovered on October 17, 2013, by University of Toronto astronomer Thayne Currie.

The object has an estimated mass around 9 Jupiter masses, depending on the age of the star, similar to the masses of directly imaged planets around HR 8799 and beta Pictoris. However, it is unclear whether ROXs 42Bb formed like these planets via core accretion, by disk (gravitational) instability, or more like a binary star. Preliminary fits of the spectra and broadband photometry to atmospheric models imply a radius of 2.43 ± 0.18 RJ for an effective temperature of about 2,000 K or a radius of 2.55 ± 0.20 RJ for about 1950 K. Like Beta Pictoris b, ROXs 42Bb's atmosphere is likely very cloudy and dusty.

## See also

* ROXs 12Ab
* Saturn
* j1407b
* beta Pictoris b
* HR 8799 b

-Wikipedia
Vesperiano

Vesperiano

### Aparência

Humanoides de pele escura e cabelos com tons descoloridos, nunca vistos sem uma máscara.

### Traços

* +2 Constituição
* +1 Inteligência

## Propriedades

### Idade

Atingem maturidade aos 80 anos, vivem até os 600.

### Porte

Um pouco mais altos que os humanos, porte médio.

### Proficiências

Nenhuma.

*Nunca vistos sem suas máscaras. Mal entendidos, porém muito apreciados devido a seus talentos naturais.*

## Descrição

Vesperianos são descritos como uma raça com aparência de besouro, com máscaras orgânicas e pele escura. São comumente vistos no ***“Aratel do Grande Ninho”*** e normalmente servem abaixo de *Ganymedes*.

## Habilidades Raciais

 **CONTRAMEDIDAS DE LIFEWEAVER*** Ao nascimento, Vesperianos passam por um ritual, alterando os seus corpos permanentemente com Lifeweaving.
* Resistência contra dano necrótico.

## Mais Informações

* Lore
* Sobrenomes

Eras atrás, uma espécie já extinta enfrentou um cisma cultural devido às **Grandes Marés**.

Aqueles talentosos, abençoados com a arte de **Lifeweaving**, juraram virar suas costas às marés e criar um **Grande Ninho** acima do oceano, tornando-se o que o mundo atual conhece como ***Vesperianos***. Contudo, uma pequena minoria decidiu abraçar as marés iminentes, afundando-se nas profundezas e residindo como os mais recentes habitantes afogados. Esse povo aventuroso ficou conhecido modernamente como ***Ganymedes***.

* Disii
* Enegi
* Etudi
* Galvigi
* Ixatoki
* Refigi
* Sekhigi
* Trigi
* Zeneki
Khan

Khan

### Aparência

Humanoides de pele bronzeada com ligeiramente mais cabelo que o normal, sendo ele normalmente loiro, prateado/branco, negro ou por raras vezes ruivo. Portam uma coroa especial em suas cabeças.

### Traços

* +2 Força
* +1 Constituição

## Propriedades

### Idade

Atingem maturidade aos 18 anos, vivem até os 100.

### Porte

Em média, maiores do que humanos, porte médio.

### Proficiências

Proficiência em **Atletismo**.

*Cheios de orgulho, mas atentivos aos pequenos detalhes. Conhecidos como grandes guerreiros e mercenários por todo o mundo.*

## Descrição

Khans são conhecidos por serem um povo físicamente forte e capaz. Normalmente conseguem emprego em trabalhos manuais pesados. Portam uma coroa especial que apenas eles podem utilizar. Normalmente possuem cabelos loiros, prateados/brancos, ou negros, e uma pele pálida ou morena.

## Habilidades Raciais

 **RESISTÊNCIA KHAN*** Uma vez a cada 1d2 Descansos Longos, quando o seu HP chegar a 0 mas não for morto instantaneamente, fique com 1 de HP e mantenha-se consciente.

## Mais Informações

* Lore
* Sobrenomes

Originam do ***“Luminante do Oeste”*** e são a raça mais prominente na ***“Legião Centenária”***.

Quando um Khan atinge a maturidade, ele ou um relativo próximo criam uma coroa especial que este usa, normalmente indicando os desejos que o Khan tem em relação à sua vida.

* Dalus
* Drameus
* Evus
* Janus
* Juno
* Narsus
* Nemises
* Tarsus
* Theus
HAT-P-67 b

**HAT-P-67 b** is an exoplanet orbiting the star HAT-P-67, located about 1043.7 light-years (319.999 pc) away from Solar System. Its discovery was publicly announced on 2017.

## Host star

The host star HAT-P-67 has apparent magnitude of 10.7, with absolute magnitude of 3.2. It is 1.6 times more massive and 1.5 times bigger compared with our Sun. The surface temperature is 6,406 Kelvin with its spectral types of F.

## Planetary system

In this planetary system, the extrasolar planet HAT-P-67 b orbits around the star HAT-P-67 every 4.8 days with its orbital distance of 0.07 AU. (9,731,241.5 km)

## See also

* HAT-P-40 b
* HAT-P-32 b
Attunements

**Sintonias** são formas de magia que o jogador pode escolher ao criar um personagem ou obter durante a campanha.

**NOTA IMPORTANTE:** *É possível possuir mais de uma sintonia, porém **DUAS** é o **máximo de sintonias permitidas** ao criar um personagem. Também é possível começar sem nenhuma sintonia, ganhando um **bónus de DOIS pontos de atributo extra** que o jogador pode colocar aonde quiser.*

**Este bónus é perdido se, em algum momento, o jogador conseguir uma sintonia.**

## Geral

Atualmente existem nove Sintonias base que os jogadores podem escolher ao criar um personagem. Ao criar um personagem, um jogador pode escolher até duas sintonias para começar, ou nenhuma, dependendo da sua preferência.

* Quantas mais sintonias o jogador possua, mais difícil será manuseá-las, visto que o número de espaços de Mantra é limitado. Escolha com sabedoria.
* Ao não escolher uma sintonia, o jogador recebe 2 pontos de atributo extra para compensar pela falta de atributo mágico. No momento em que obtenha uma sintonia, perde o bónus.

Após a criação, o personagem é capaz de aprender mais sintonias através de suas viagens pelo mundo, ao visitar treinadores ou descobrir segredos.

Por padrão, os jogadores são dados **3 espaços para Mantra de Combate, 1 para Mantras de Mobilidade, 1 para Mantras de Suporte e 1 espaço de Mantra WildCard.** Mantras adicionais poderão ser guardadas em uma *Enciclopédia de Mantras*, ao escrever a sua melodia em uma das páginas da Enciclopédia.

* Mantras de uma sintonia podem por vezes possuir requisitos de estatísticas não relacionadas à sintonia.

Mantras são melodias inesquecíveis pela alma, após a alma do personagem aprender as palavras de uma Mantra apenas a morte poderá apagá-la.

## Sintonias Base

Sintonias disponíveis para o jogador. Estas sintonias podem ser escolhidas pelo jogador na criação de personagem.
*Clique em qualquer um destes para entrar nas suas respetivas páginas.*

### Sintonias Intra-Canticlysm

Flamecharm

Frostdraw

Thundercall

Galebreathe

Attunement-less

### Sintonias Pós-Canticlysm

Shadowcast

Ironsing

Wavesend

Acidchant

Poisonwield

## Sintonias Especiais

Sintonias que **não estão disponíveis** para o jogador. São sintonias desbalanceadas feitas para personagens importantes, ou até mesmo impossíveis de ser utilizadas devido à lore.
*Clique em qualquer um destes para entrar nas suas respetivas páginas.*

Lightkeep

Tidebring
PSR B1257+12 B

PSR B1257+12 c, alternatively designated PSR B1257+12 B, also named Poltergeist, is an extrasolar planet approximately 2,300 light-years away in the constellation of Virgo. It was one of the first planets ever discovered outside the Solar System, and is one of three pulsar planets known to be orbiting the pulsar Lich.

Over four times as massive as the Earth, it circles the primary at a distance of 0.36 AU with an orbital period of approximately 66 days. Because it and Phobetor have very similar masses and orbit close to each other, they were expected to cause measurable perturbations in each other's orbits. Detecting such perturbations confirmed that the planets were real. Accurate masses of the two planets, as well as their inclinations, were calculated from how much the planets perturb each other.

## Physical properties

### Other designations

PSR B1257+12 c, Poltergeist, PSR J1300+1240 c, PSR J1300+1240 B

## Nomenclature

### Mythology/Named after

the German legend of these "noisy ghosts."

## Nomenclature

The convention that arose for designating pulsars was that of using the letters PSR (Pulsating Source of Radio) followed by the pulsar's right ascension and degrees of declination. The modern convention prefixes the older numbers with a B meaning the coordinates are for the 1950.0 epoch. All new pulsars have a J indicating 2000.0 coordinates and also have declination including minutes. Pulsars that were discovered before 1993 tend to retain their B names rather than use their J names, but all pulsars have a J name that provides more precise coordinates of its location in the sky.

On its discovery, the planet was designated PSR 1257+12 B and later PSR B1257+12 B. It was discovered before the convention that extrasolar planets receive designations consisting of the star's name followed by lower-case Roman letters starting from "b" was established. However, it is listed under the latter convention on astronomical databases such as SIMBAD and the Extrasolar Planets Encyclopedia. Hence the designation PSR B1257+12 c.

In July, 2014, the International Astronomical Union launched NameExoWorlds, a process for giving proper names to certain exoplanets and their host stars. The process involved public nomination and voting for the new names. In December 2015, the IAU announced the winning name was Poltergeist for this planet. The winning name was submitted by the Planetarium Südtirol Alto Adige in Karneid, Italy. Poltergeist is a name for supernatural beings that create physical disturbances, from the German for "noisy ghost".

## See also

* Draugr
* Phobetor

-Wikipedia
OTS 44

**OTS 44** is a free-floating planetary-mass object or brown dwarf located at 550 light-years (170 pc) in the constellation Chamaeleon near the reflection nebula IC 2631. It is among the lowest-mass free-floating substellar objects, with approximately 11.5 times the mass of Jupiter, or approximately 1.1% that of the Sun. Its radius is not very well known and is estimated to be 23–57% that of the Sun.

OTS 44 was discovered in 1998 by Oasa, Tamura, and Sugitani as a member of the star-forming region Chamaeleon I. Based upon infrared observations with the Spitzer Space Telescope and the Herschel Space Observatory, OTS 44 emits an excess of infrared radiation for an object of its type, suggesting it has a circumstellar disk of dust and particles of rock and ice. This disk has a mass of at least 10 Earth masses. Observations with the SINFONI spectrograph at the Very Large Telescope show that the disk is accreting matter at the rate of approximately 10−11 of the mass of the Sun per year. It could eventually develop into a planetary system. Observations with ALMA detected the disk in millimeter wavelengths. The observations constrained the dust mass of the disk between 0.07 and 0.63 MEarth, but these mass estimates are limited by assumptions on poorly constrained parameters.

## See also

* Cha 110913-773444
* S Ori 52
* Proplyd 133-353

-Wikipedia
GQ Lupi b

GQ Lupi b, or GQ Lupi B, is a possible extrasolar planet, brown dwarf or sub-brown dwarf orbiting the star GQ Lupi. Its discovery was announced in April 2005. Along with 2M1207b, this was one of the first extrasolar planet candidates to be directly imaged. The image was made with the European Southern Observatory's VLT telescope at the Paranal Observatory, Chile on June 25, 2004.

VLT NACO image, taken in the Ks-band, of GQ Lupi. The feeble point of light to the right of the star is the newly found cold companion. It is 250 times fainter than the star itself and it located 0.73 arc second west. At the distance of GQ Lupi, this corresponds to a distance of roughly 100 AU. North is up and East is to the left.

GQ Lupi has a spectral type between M6 and L0, corresponding to a temperature between 2,050 and 2,650 kelvins. Located at a projected distance of about 100 AU from its companion star, giving it an orbital period of perhaps about 1,200 years, it is believed to be several times more massive than Jupiter. Because the theoretical models which are used to predict planetary masses for objects in young star systems like GQ Lupi b are still tentative, the mass cannot be precisely specified — models place GQ Lupi b's mass anywhere between a few Jupiter masses and 36 Jupiter masses. At the highest end of this range, GQ Lupi b could be classified as a small brown dwarf, but at the lowest end of this range, it could be classified as an extremely large Jupiter-like exoplanet rather than a brown dwarf.

If classified as an exoplanet, with a maximum radius of 6.5 times that of Jupiter (RJ) (or 930,000 km in diameter), this would make GQ Lupi b one of largest exoplanets discovered, although the size of the planet is shrinking as it evolves.

As of 2006, the International Astronomical Union Working Group on Extrasolar Planets described GQ Lupi b as a "possible planetary-mass companion to a young star." GQ Lupi b is listed as a "confirmed planet" as of 2020.

## See also

* 2M1207 b
* GU Piscium
* Fomalhaut b

-Wikipedia
London Buses route 345

## Section Header

Introduced: 1990

Withdrawn: 1993

Originally Operated By: Ensign Citybus

Last Operated By; Capital Citybus

Replaced by: Route 323

Route 345 commenced operation in 1990 as a commercial service between *Rainham Station* and Belhus *Derwent Parade,* and was originally operated by Ensign Citybus*.* The route operated Monday-Friday only and went via Wennington *Lennards* - Aveley *Sandy Lane* - Aveley *Mill Road* - Aveley *High Street* - Belhus *Stifford Road* - Belhus *Foyle Drive* - Belhus *Gatehope Drive*. The route originally operated alongside the 165 & 365 journeys that went to Wennington. On September 14 1991, Route 345 replaced the withdrawn route 165 & 365 Wennington journeys as both 323 and 345 provided an alternative service. In July 1992, Route 345 was passed over from Ensign Citybus to Capital Citybus. However, in 1992 and during July 31 1992 to 1993, when 323 was extended to Mardyke Estate and basically was an exact copy of 345, the route began having less services or running more infrequently and eventually by 1993 the route was entirely withdrawn and replaced by route 323, but would be resurrected as Essex route 445, but would be withdrawn again by 1998 and not replaced.
London Buses route 347

## Section Header

Introduced: 6 November 2004

Original Operator: First London

Current Operator: Arriva London

Replaced: Routes 348, 349 & Mobility Route 952

Route 347 commenced operation on November 6 2004, running between *Romford Station* and *Ockendon Station* via Romford Market - Main Road - Gallows Corner Tesco - Gallows Corner - Harold Wood Station - Hall Lane - Upminster Station - Cranham *St Mary's Lane* - North Ockendon *Clay Tye Road* - South Ockendon - West Road. The route was a partial replacement for Capital Citybus route 349, which ran between 1993 to 1998 as well as a partial replacement for route 348 which ran between 1990 to 2001, as well as replacing mobility route 952 that ran between Romford Station and Lakeside. The route was initially operated by First London from Rainham (R) garage using a Marshall C36 bodied Dennis Dart.

On 15 October 2005, the route passed to Blue Triangle operating from their Rainham (BE) garage with a low floor Plaxton Pointer 2 bodied Dennis Dart SLF introduced.

On 16 October 2010, the route was retained by Blue Triangle.

On 17 October 2015, the route passed to Arriva Kent Thameside using a 10.8m Alexander Dennis Enviro 200 Dart.

On 1 January 2016, the Arriva group restructured its bus operations, which included the transfer of route 347 from Arriva Kent Thameside to Arriva London.

On 9 July 2019, the 10.8m Alexander Dennis Enviro200 Dart was replaced by a 10.2m version.

On 17 October 2020, the route was retained by Arriva London.

On 6 March 2023, a consultation was created with proposals to withdraw routes 346 (Upminster Local Service) & 347 with route 497 being extended to Upminster to cover some of the lost sections, however this did not end up going ahead, mainly because most services would require at least two transfers especially for Ockendon Station. It was decided to allow 347 to continue operation under review, while route 497 would be withdrawn and replaced by an extension of route 346 effective 9 March 2024.
Pansessualità

Per **pansessuale** si intende l'attrazione verso tutti i sessi senza alcuna preferenza riguardo a questo. Queste persone possono essere considerate non vedenti rispetto al genere.

A volte viene aggiunta una "P" all'acronimo LGBT in riferimento alla pansessualità.

## Differenze con altre identità

### Omnisessualità

La pansessualità è spesso paragonata ad altre identità multisessuali, principalmente all'omnisessualità. La differenza principale tra i due è che la maggior parte delle persone omnisessuali ha preferenze di genere. D'altra parte, pansessuale di solito significa che non hai preferenze quando si tratta di genere, quindi non è un problema in una relazione.

### Bisessualità

La principale differenza tra pansessualità e bisessualità è che quest'ultima è l'attrazione per due o più generi, mentre la pansessualità è l'attrazione per tutti i generi.

La pansessualità è la capacità di amare un'altra persona indipendentemente dal suo sesso. I pansessuali sostengono che per loro il sesso e il genere sono concetti privi di significato o di nessuna importanza.

## Storia

Si crede che la pansessualità sia un concetto completamente nuovo e che le persone pan stiano appena iniziando a esistere, e che Tumblr sia il luogo in cui è stato creato, e quindi la pansessualità e le persone pansessuali non sono legittime come le altre persone nella comunità.

Sappiamo che il "pansessualismo" fu attribuito a Freud all'inizio del 1900, per denotare l'idea che il comportamento umano è guidato dall'istinto sessuale.

Questa non è la stessa cosa della pansessualità, non è nemmeno una sessualità, è una teoria sul comportamento umano.

Sebbene all'epoca non fosse usato per descrivere l'orientamento sessuale, ci sono state segnalazioni di persone negli anni '20 e '30 che amavano "oltre etichette e confini" ad Harlem e nel South Side di Chicago.

Nel libro di George Chauncey del 1994, Gay New York, egli descrive uomini della fine del XIX secolo e dell'inizio del XX secolo che sarebbe "difficile sostenere che fossero veramente omosessuali" ma "né potevano essere considerati eterosessuali" e "né erano bisessuali, " e conclude che si trattava, piuttosto, di "uomini interessati ad un'attività sessuale definita non dal sesso del loro partner".

Anche se questo non significa che siano pansessuali e che la parola non sia usata affatto, poiché farlo sarebbe un’etichettatura retroattiva e irrispettoso nei confronti del modo in cui danno un senso alla loro sessualità con i termini a cui avevano accesso in quel momento.

## Note

1. ↑ https://lgbt.fandom.com/es/wiki/Pansexualidad?so=search
2. ↑ https://lgbt.fandom.com/es/wiki/Pansexualidad?so=search#Omnisexualidad
3. ↑ https://lgbt.fandom.com/es/wiki/Pansexualidad?so=search#Bisexualidad
4. ↑ https://lgbt.fandom.com/es/wiki/Pansexualidad?so=search#Historia
List of objects

This page has the full list of **ALL** objects in this page, which means one should add the table an object once an object page is added. Add alphabetically by the name of the object.

## Directions

1. Create a page
2. If the page is not an object, don't use these steps
3. Add "**Object**" category to your page
4. Go to this page
5. Edit the page
6. Add to the table (ABC order)
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ObjectShowMusic Wiki

**ObjectShowMusic Wiki (WIP)**
ObjectShowMusic, is like the object show equivalent of SiIvaGunner. This small channel uploads high quality rips of OSC-related music.

We're a collaborative community website about ObjectShowMusic that anyone, including you, can build and expand. Wikis like this one depend on readers getting involved and adding content. Click the "ADD NEW PAGE" or "EDIT" button at the top of any page to get started!

## Important articles

PlaceholderA page about your topicPlaceholderA Main CharacterPlaceholderThe First EpisodePlaceholderAn Important LocationPlaceholderA Key EventPlaceholderA Crucial Item

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Kepler-56 b

**Kepler-56b** (KOI-1241.02) is a hot Neptune—a class of exoplanets—located roughly 3,060 light-years (940 parsecs) away. It is somewhat larger than Neptune and orbits its parent star Kepler-56 and was discovered in 2013 by the Kepler Space Telescope.

## Physical properties

### Other designations

2MASS J19350200+4152187 b, K01241.02, KIC 6448890 b, KOI-1241 b, KOI-1241.02, WISE J193501.99+415218.5 b

## Stellar properties

### Other designations (stellar)

KOI-1241, KIC 6448890, 2MASS 19350200+4152187

## Planetary orbit

Kepler-56b is about 0.1028 AU (9.56 million mi; 15.38 million km) away from its host star (about one-tenth of the distance between Earth to the Sun), making it even closer to its parent star than Mercury (0.39 AU [36 million mi; 58 million km]) and Venus (0.72 AU [67 million mi; 110 million km]). It takes 10.5 days for Kepler-56b to complete a full orbit around its star. Further research shows that Kepler-56b's orbit is about 45° misaligned to the host star's equator. Later radial velocity measurements have revealed evidence of a gravitational perturbation from Kepler-56d.

Both Kepler-56b and Kepler-56c will be devoured by their parent star in about 130 and 155 million years. Even further research shows that it will have its atmosphere boiled away by intense heat from the star, and it will be stretched by the strengthening stellar tides. The measured mass of Kepler-56b is about 30% larger than Neptune's mass, but its radius is roughly 70% larger than Neptune's. Therefore, Kepler-56b should have a hydrogen/helium envelope containing a significant fraction of its total mass. Like Kepler-11b and Kepler-11c, the envelope's light elements are susceptible to photo-evaporation caused by radiation from the central star. For example, it has been calculated that Kepler-11c lost over 50% of its hydrogen/helium envelope after formation. However, the larger mass of Kepler-56b, compared to that of Kepler-11c, reduces the efficiency of mass loss. Nonetheless, the planet may have been significantly more massive in the past and may keep losing mass in the future.

## See also

* Kepler-56 c
* Kepler-56 d
* HD 62509 c
* Kepler-432 b

-Wikipedia
HD 62509 b

Pollux b, also designated β Geminorum b (Latinized to Beta Geminorum b, abbreviated, β Gem b) and HD 62509 b, formally named Thestias /ˈθɛstiəs/, is an extrasolar planet approximately 34 light-years away in the constellation of Gemini (the Twins). This planet was discovered orbiting the star Pollux in 2006 by astronomer Artie P. Hatzes, confirming his hypothesis originally published in 1993. The planet has at least twice the mass of Jupiter. It moves around Pollux in 1.61 years at a distance of 1.64 AU in a nearly circular orbit.

## Physical properties

### Other designations

Pollux b, β Geminorum b, β Gem b, Beta Geminorum b, Beta Gem b, Thestias

## Nomenclature

### Mythology/Named after

Thestius, a king of Pleuronians in Aetolia

## Stellar properties

### Other designations (stellar)

Pollux, β Geminorum , β Gem, Beta Geminorum, Beta Gem, 78 Geminorum, BD+28°1463, GJ 286, HIP 37826, HR 2990, SAO 79666, LFT 548, LHS 1945, LTT 12065[14]

## Naming

In July 2014 the International Astronomical Union launched NameExoWorlds, a process for giving proper names to certain exoplanets and their host stars. The process involved public nomination and voting for the new names. In December 2015, the IAU announced the winning name was Thestias for this planet. The winning name was based on that originally submitted by theSkyNet of Australia; namely Leda, Pollux's mother in Greek and Roman mythology. At the request of the IAU, 'Thestias' (the patronym of Leda, a daughter of Thestius) was substituted. This was because 'Leda' was already attributed to an asteroid and to one of Jupiter's satellites.

## See also

* HD 62509 c
* Kepler-56 b
* 8 Ursae Minoris b

-Wikipedia
EssexBusChronicles Wiki

**Welcome to the EssexBusChronicles Wiki!**
This community is about transportation that are/were London Buses that served/serve Essex. It dates from all the way back when to the current day, with many pages on all different routes that once served Essex and the border of Greater London. All routes that are/were considered London Buses will be included into the website. As well as London Bus routes, some Essex operators will be included on this wiki, including Ensignbus and more. Thanks for reading and feel free to browse the wiki!

I use a various list of sources to back up my research including: The Greater London Bus Map by Mike Harris - Romford local area guides and All London bus guides by London Transport - Service 324 including service 323/Rombus Network by Capital Citybus - "The Lakeside Link" leaflet by Ensignbus and many more! Credits to all those sources are given. Feel free to use my sources, but please give credit when using such.
PSR B1257+12 A

**PSR B1257+12 b**, alternatively designated **PSR B1257+12 A**, also named **Draugr**, is an extrasolar planet approximately 2,300 light-years (710 pc) away in the constellation of Virgo. The planet is the innermost object orbiting the pulsar Lich, making it a pulsar planet in the dead stellar system. It is about twice as massive as the Moon, and is listed as the least massive planet (with the mass accurately determined) known, including among the planets in the Solar System.

## Physical properties

### Other designations

PSR B1257+12 b, Draugr, PSR J1300+1240 b, PSR J1300+1240 A, Lich b

## Nomenclature

### Mythology/Named after

a ghost, spirit, esp. the dead inhabitant of a cairn

## Nomenclature

The convention that arose for designating pulsars was that of using the letters PSR (Pulsating Source of Radio) followed by the pulsar's right ascension and degrees of declination. The modern convention prefixes the older numbers with a B meaning the coordinates are for the 1950.0 epoch. All new pulsars have a J indicating 2000.0 coordinates and also have declination including minutes. Pulsars that were discovered before 1993 tend to retain their B names rather than use their J names, but all pulsars have a J name that provides more precise coordinates of its location in the sky.

On its discovery, the planet was designated PSR 1257+12 A and later PSR B1257+12 A. It was discovered before the convention that extrasolar planets receive designations consisting of the star's name followed by lower-case Roman letters starting from "b" was established. However, it is listed under the latter convention on astronomical databases such as SIMBAD and the Extrasolar Planets Encyclopedia. Hence the designation PSR B1257+12 b.

In July 2014 the International Astronomical Union launched NameExoWorlds, a process for giving proper names to certain exoplanets and their host stars. The process involved public nomination and voting for the new names. In December 2015, the IAU announced the winning name was Draugr for this planet. The winning name was submitted by the Planetarium Südtirol Alto Adige in Karneid, Italy. Draugr are undead creatures in Norse mythology.

## See also

* Poltergeist
* Phobetor

-Wikipedia
London Buses route 373

## Section Header

Introduced: 1987

Withdrawn: 29th March 2008

Original Operator: ThameSide

Last Operator: Arriva

Route 373 was introduced in 1987 as an albeit identical route to the 370 running between Romford and Tilbury Ferry via Hornchurch, Upminster, Ockendon, Grays and Chadwell St Mary. Shortly after introduction however, the section between Grays and Tilbury was withdrawn, only to be briefly reinstated during 2001. When Lakeside Shopping Centre opened, Route 373 was diverted to serve it. On October 10 1998, the route replaced the Belhus section of the 323 as well as replacing the Aveley section of 348 which was made as an express service between Belhus and Lakeside. For many years the 373 ran half hourly during the day on Mondays to Saturdays, latterly with an hourly evening and Sunday service part funded by TfL. As such, it unusually provided a number of unique links within the London area, although a diversion of route 165 in 2001 meant it no longer had any unique road between Upminster and Romford. However, due to costs from accepting TfL passes and fares, it was not financially stable to not re-structure the route and so the route was re-structured to both be able to have a TfL contract while the Essex end could still be commercial. And so the 373 was withdrawn between Romford and Upminster, making the route shorter. The re-structured 373 did not prove to be a success however because by end of March 2008, the 29th to be exact, it was decided to withdraw route 373 entirely, perhaps because of the loss of the direct connection to Romford, and it would later be replaced by Ensignbus route 22 between Aveley and Grays the same day.
Carl Corvetteson's 1972 Mazda Cosmo L10A

Carl Corvetteson's car will be a 1972 Mazda Cosmo L10A with a standard 982 CC 0810 Engine, 4-speed manual, RS Watanabe 8 spoke 4-lug rims and Bridgestone Potenza Sport tires. It will appear in the Winx and Transformers Inertial Drift Special 2 where it was wrecked twice, the first time he crashed it was when he was racing against a street racer named Cody Wolfhead, and the second crash it was involved in was when he and his wife Jennifer were racing Darcy and the crash completely wrecked and destroyed the car beyond repair and was stored away in the Corvettesons' family home shed and had to covered in a tarp to hide the car's critical wrecked state.

## History

In 2000, he gets his 1972 Mazda Cosmo L10A and 1994 Toyota Celica GT-Four liftback, he replaces his Cosmo's standard steel rims with RS Watanabe 8 spoke rims. He won his first street race in 2010. In 2021 Carl Corvetteson encounters Cody by the gas station and the two have a street race, towards the upcoming corner, Carl loses focus and crashes his Mazda Cosmo into the ditch and calls a tow truck to have his car towed to the autoshop to be fixed, the next day, Carl gets his car fixed and haves a race with Selina and ends up losing. Two days later, on May 14 at 8:33 PM, Carl then challenges one of the Trix witch girls, Darcy to a street race. Darcy is hesitant at first but then accepts the challenge. The Race begins and Darcy is in front but soon Carl and Jennifer end up in front, his wife is assisting him as his co-driver, Darcy tries to regain first place, she starts thinking and pulls off a gutter run move and appears small inches closer from Carl's Mazda Cosmo and bumps them several time which irretates Carl and Jennifer, Darcy eventually gets back in first and manages to stay ahead. Towards the end of the race Carl remembers Musa's gutter run move, after Darcy performs the gutter move and drifts around a corner, Carl does the same thing but realizes he messed up, he tried to avoid hitting the guardrail but it was too late. The Mazda hits the guard rail with such force that Jennifer's seatbelt snaps and she is ejected from the car as the car goes into a violent barrel roll, the car comes to rest on the side of the road. After the crash, the car was placed in the family home shed and covered in a tarp.

## External Link

Fanon Page link: https://fanon.fandom.com/wiki/Carl\_Corvetteson%27s\_1972\_Mazda\_Cosmo\_L10A
TRAPPIST-1 h

**TRAPPIST-1h**, also designated as **2MASS J23062928-0502285 h**, is an exoplanet orbiting around the ultra-cool dwarf star TRAPPIST-1, located 40.7 light-years (12.5 parsecs) away from Earth in the constellation Aquarius. It was one of four new exoplanets to be discovered orbiting the star in 2017 using observations from the Spitzer Space Telescope. In the following years, 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 76% as large. Its relatively low density indicates that it is likely water-rich, like several other planets in the system.

## Physical characteristics

### Mass, radius, and temperature

TRAPPIST-1h has a radius of 0.755 *R*🜨, a mass of 0.326 *M*🜨, and about 57% Earth's surface gravity. It was initially estimated to have a density of 3.97 g/cm3, similar to that of Mars. Given this density, about ≤5% of its mass may be water, likely in the form of a thick ice shell, since it only receives about 13% of the stellar flux that Earth does. It has an equilibrium temperature of 169 K (−104 °C; −155 °F), similar to that of Earth's south pole.

### Host star

TRAPPIST-1h orbits the ultracool dwarf star TRAPPIST-1. It is 0.121 R☉ and 0.089 M☉, with a temperature of 2511 K and an age between 3 and 8 billion years. For comparison, the Sun has a temperature of 5778 K and is about 4.5 billion years old. TRAPPIST-1 is also very dim, with about 0.0005 times the luminosity of the Sun. The star's apparent magnitude, or how bright it appears from Earth's perspective, is 18.8. Therefore, it is too dim to be seen with the naked eye.

### Orbit

Despite it being the most distant known planet in its system, TRAPPIST-1h orbits its host star with an orbital period of 18.868 days and an orbital radius of about 0.0619 AU. This is even smaller than Mercury's orbit around the Sun (which is about 0.38 AU).

### Stable liquid water

Although TRAPPIST-1h's orbit falls near its star's frost line, it could harbor liquid water under an H2-rich atmosphere, either primordial or resulting from continuous outgassing combined with internal heating, although existence of such atmosphere was strongly disfavored by observations in 2021 and 2022. It could also potentially harbor a subsurface ocean by way of tidal heating, which could lead to cryovolcanism in the form of erupting geysers.

## See also

* TRAPPIST-1 b
* TRAPPIST-1 c
* TRAPPIST-1 d
* TRAPPIST-1 e
* TRAPPIST-1 f
* TRAPPIST-1 g

-Wikipedia
Exoplanets, Planets, and Fan made Exoplanets and Planets Wiki

**Welcome to the Exoplanets, Planets, and Fan made Exoplanets and Planets Wiki!**
this wiki is about the universe, fanon universe and all its wonders! - andyhoags

We're a collaborative community website about Exoplanets, Planets, and Fan made Exoplanets and Planets that anyone, including you, can build and expand. Wikis like this one depend on readers getting involved and adding content. Click the "ADD NEW PAGE" or "EDIT" button at the top of any page to get started!

## Outstanding articles

Earth51 Pegasi bHD 62509 bKOI-44720.01PoltergeistTRAPPIST-1 e55 Cancri eKR Muscae bPlaceholderHd-19 gPlaceholderProcyon BbKELT-9 bPlaceholderCFBDSIR J214947.2-040308.9PlaceholderWD 1856+534 bPlaceholderBanard's Star bPlaceholderOGLE-2005-BLG-390LbPlaceholderCI Tauri bPlaceholderCOCONUTS-2 bPlaceholderHD 20782 b

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*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.
PSR J1719-1438 b

**PSR J1719−1438 b** is an extrasolar planet that was discovered on August 25, 2011, in orbit around PSR J1719−1438, a millisecond pulsar. The pulsar planet is most likely composed largely of crystalline carbon but with a density far greater than diamond. PSR J1719-1438 b orbits so closely to its host star that its orbit would fit inside the Sun. The existence of such carbon planets had been theoretically postulated.

## Observational history

PSR J1719−1438 was first observed in 2009 by a team headed by Matthew Bailes of Swinburne University of Technology in Melbourne, Australia. The orbiting planet was published in the journal *Science* on August 25, 2011. The planet was confirmed through pulsar timing, in which small modulations detected in the highly regular pulsar signature are measured and extrapolated. Observatories in Britain, Hawaii, and Australia were used to confirm these observations.

## Host star

Main article: PSR J1719−1438

PSR J1719−1438 is a pulsar some 4,000 light-years (1,200 parsecs) away from Earth in the Serpens Cauda constellation, approximately one minute from the border with Ophiuchus. The pulsar completes more than 10,000 rotations a minute. It is approximately 12 miles (19 kilometers) across but with 1.4 solar masses.

## Characteristics

PSR J1719−1438 b was, at the time of its August 25, 2011, discovery, the densest planet ever discovered, at nearly 20 times the density of Jupiter (about 23 times the density of water). It is slightly more massive than Jupiter. It is thought to be composed of oxygen and carbon (as opposed to hydrogen and helium, the main components of gas giants like Jupiter and Saturn).

The oxygen is most likely on the surface of the planet, with increasingly higher quantities of carbon deeper inside the planet. The intense pressure acting upon the planet suggests that the carbon is crystallized, much like diamond is.

PSR J1719−1438 b orbits its host star with a period of 2.17 hours and at a distance of 0.89 solar radius (619,173 km or 384,736 mi).

## Formation

It is highly unlikely that this planet would have formed before its parent pulsar, as the resulting supernova would destroy any nearby planets. It has been proposed that PSR J1719−1438 b is not a planet but a star. Specifically, PSR J1719−1438 b was a yellow dwarf star similar to the Sun in a binary with PSR J1719−1438, a higher-mass star. PSR J1719−1438 swelled up to become a red supergiant, but the yellow dwarf star survived the supernova. Billions of years later, PSR J1719−1438 b became a red giant and then a white dwarf. The gravity from the pulsar stole hydrogen and helium, and the remaining carbon crystallized, forming the diamond planet.

## See also

* Draugr
* Poltergeist
* Phobetor

-Wikipedia
XO-6 b

**XO-6b** is a transiting exoplanet, a hot Jupiter, orbiting the star XO-6 around 760 Light Years (230 Parsecs) away from Earth. It was discovered in 2016 by the XO planet search team.

## Physical properties

### Other designations

TYC 4357-995-1 b, Gaia DR2 1114308481600798336 b

## Stellar properties

### Other designations (stellar)

TYC 4357-995-1, Gaia DR2 1114308481600798336

## Physical properties

XO-6b is one of the puffiest planets ever discovered, with a maximum mass of 4.4 times of Jupiter. It is up to twice as wide, making it one of the largest exoplanets ever found (see list of largest exoplanets). Later estimates, however, make it around two times the mass of Jupiter.

XO-6b has a tight orbit, which means a year on it is only about 4 days. XO-6 is slightly more than one tenth as far from its host star as Mercury is to the sun.

## XO-6

XO-6b orbits XO-6, a faint 10th magnitude star in the constellation Camelopardalis. Due to its magnitude, this star is too faint to be seen with the naked eye, but can be seen with a telescope. XO-6 is a F-type main-sequence star with about 1.5 times the mass of the Sun. It is also radiating 4 times as bright, and is almost twice the size of the Sun. It is also hotter, with a temperature of 6720 kelvins, which gives it the typical hue of an F-type star. Unlike most other stars of its kind, XO-6 rotates rapidly at a rate of 43 km/s.

## See also

* XO-2N b
* XO-1 b

-Wikipedia