recursal/Fanatic-Fandom huggingface dataset:
Choo

**Alpha Arae**, Latinized from α Arae, is the second brightest star in the southern constellation of Ara. With an average apparent visual magnitude 2.93, it is readily visible to the naked eye from the southern hemisphere. This star is close enough to the Earth that its distance can be estimated using parallax data collected during the Hipparcos mission. It is around 270 light-years (83 parsecs) away, with a 7% margin of error. The visual magnitude of the star is diminished by 0.10 magnitudes as a result of extinction from intervening gas and dust.

Alpha Arae has a stellar classification of B2 Vne, indicating that it is a massive B-type main sequence star. The 'n' notation in the suffix indicates that the absorption lines in the star's spectrum appear spread out and nebulous because of the Doppler effect from rapid rotation. The measured projected rotational velocity has been measured as high as 375 km s−1. Meilland et al. (2007) estimate the pole of the star is inclined by 55° to the line of sight, yielding an equatorial azimuthal velocity of 470 km s−1. This is close to the critical velocity where the star would start to break up. The rapid rotation is causing a pronounced equatorial bulge of about 2.4–2.7 times the polar radius.

It is a Be star, as indicated by the 'e' notation in the star's classification. This indicates that emission lines are observed in the spectrum, which is coming from a disk of material ejected from the star because of its rapid rotation. In 2003 and 2005, Alpha Arae was observed by infrared interferometry, using the MIDI and AMBER instruments at the VLT Interferometer. The results, published in 2005 and 2007, appear to show that Alpha Arae is surrounded by a dense equatorial disk of material in Keplerian (rather than uniform) rotation, and that it is losing mass by a polar stellar wind with a terminal velocity of approximately 1,000 km/s. There is also some evidence that Alpha Arae is orbited by a companion at 0.7 AU.

This star is around 9.6 times as massive as the Sun, and has an average of 4.5 times its radius. It is 5,800 times as luminous as the Sun, its energy emitted from its outer envelope at an effective temperature of 18,044 K. This heat gives Alpha Arae the blue-white hue that is characteristic of B-type stars. It is a variable star with a magnitude that varies between 2.76m and 2.90m. The General Catalogue of Variable Stars classifies it only as BE, indicating that it is a variable Be star but not obviously a Gamma Cassiopeiae variable. The International Variable Star Index defines it as GCAS + LERI, showing both rapid periodic variation and slow irregular eruptions.
Alpheratz

**Alpha Andromedae** (**α Andromedae**, abbreviated **Alpha And** or **α And**), officially named **Alpheratz** /ælˈfɪəræts/,

## Alpheratz B

### Absolute Magnitude

2.00

is located 97 light-years from the Sun and is the brightest star in the constellation of Andromeda. Located immediately northeast of the constellation of Pegasus, it is the upper left star of the Great Square of Pegasus.

Although it appears to the naked eye as a single star, with overall apparent visual magnitude +2.06, it is actually a binary system composed of two stars in close orbit. The chemical composition of the brighter of the two stars is unusual as it is a mercury-manganese star whose atmosphere contains abnormally high levels of mercury, manganese, and other elements, including gallium and xenon. It is the brightest mercury-manganese star known.
Vaan

**Vaan**, originaire de Final Fantasy XII, est un candidat de Koh-Lanta : Le Combat des Héros.

A la base, vu comme un suiveur, Vaan parvient à prouver qu'il est capable de mener des actions stratégiques comme l'élimination de Mickey où il se servit des votes de Serah et Raine pour éliminer Mickey ou comme sa tentative de recruter Wardog à sa cause pour éliminer Kaito Momota, hélas, sa victoire dans la dernière épreuve d'immunité coûtera cher à Vaan qui perdra la finale face à son allié et ami, Takeru Homura dû que Kaito en profita pour détruire son jeu durant le dernier conseil en le dénonçant devant tous les aventuriers.

## Koh-Lanta : Le Combat des Héros

1 : Wardog utilise un collier d'immunité ce qui annule le vote de Vaan contre lui mais Kanji utilise l'avantage du Survivant ce qui redémarre le vote.

2 : Vaan est en binôme avec Jago, si l'un d'eux venait à être éliminer, il entrainerait l'autre dans sa chute, aucun d'entre eux ne reçut de voix pour y être éliminer.

3 : Yuya utilise un collier d'immunité ce qui annule le vote de Vaan contre lui

4 : Jago utilise un collier d'immunité ce qui annule le vote de Kaito et oblige un nouveau vote qui finit en égalité entre Serah et Vaan, Vaan ne change pas son vote ce qui entraîne un tirage au sort. Vaan, faisant des personnes à égalités est immunisé du tirage au sort.

## Trivia

Vaan est le premier candidat à laisser expirer un avantage puisqu'il laisse son collier d'immunité expirer aux six derniers puisqu'il est parvenu à remporter l'épreuve d'immunité.
Люди

Люди *(элинтаилигвэ - Aumeagnari)* - раса разумных существ, происходящая с материка Арденталь.

## История

### Создание

*основная статья - Года Создания*

...

## Народы

* Митеренцы
* Иссентервинцы
* Саатары
	+ Ханакхары
	+ Ахрашары
	+ Акморанцы
	+ Альбадары
* ...
	+ Горцы Дратруга
	+ Снежные люди
* Фэлланцы
	+ Исерейнцы
	+ Эстемарцы
	+ Трэгарнцы
	+ Двирайндон
Epsilon Antliae

**Epsilon Antliae** (ε Ant, ε Antliae) is the Bayer designation for a star in the southern constellation of Antlia.

## Epsilon Antliae

### Absolute Magnitude

-2.17

The apparent visual magnitude of this star is +4.51, which means it is visible to the naked eye. From parallax measurements, the distance to this star is known to be 590 ± 30 light-years (180.9 ± 9.2 parsecs). Photometry measurements during the Hipparcos mission indicate that this star is undergoing periodic variability by 0.0034 magnitudes over an 11.07941 day cycle.

The stellar classification of this star is K3 IIIa, where the luminosity class of III indicates that this is an evolved giant star. It is around 37 times the radius of the Sun. and shines with a luminosity approximately 1279 times that of the Sun and has a surface temperature of 4320 K.
Gamma Aquarii

**Gamma Aquarii** (**γ Aquarii**, abbreviated **Gamma Aqr**, **γ Aqr**) is a binary star in the constellation of Aquarius. It has an apparent visual magnitude of 3.849, making it one of the brighter members of the constellation. Based upon parallaxmeasurements taken during the Hipparcos mission, this star is located at a distance of approximately 164 light-years (50 parsecs) from the Sun.

Gamma Aquarii is the primary or 'A' component of a double star designated WDS J22217-0123. The secondary or 'B' component is UCAC2 31430071. Gamma Aquarii A's two components are therefore designated WDS J22217-0123 Aa and Ab. Gamma Aquarii is traditionally also called **Sadachbia** /səˈdækbiə/, a name now formally restricted to γ Aqr Aa.

Gamma Aquarii is a spectroscopic binary with a period of 58.1 days.

It presents as an A-type main sequence star with a stellar classification of A0 V, around two and a half times more massive than the Sun. It is a candidate Lambda Boötis star, suggesting it may have accreted low-metallicity circumstellar gas some time in the past. It is spinning relatively rapidly with a projected rotational velocity of 80 km s−1. This value gives a lower bound on the actual azimuthal velocity along the star's equator. The outer atmosphere of Gamma Aquarii is radiating energy at an effective temperature of 10,500 K, which is nearly double the temperature at the surface of the Sun. This heat is what gives Gamma Aquarii the white-hot glow of an A-type star.
Zeta Arae

Z**eta Arae** (ζ Ara, ζ Arae) is the third-brightest star in the southern constellation Ara. The apparent visual magnitude of this star is 3.1, which can be seen from suburban skies in the southern hemisphere. From the parallax measurements, it is located at a distance of 490 light-years (150 parsecs) from Earth.

The spectrum of this star matches a stellar classification of K3 III. The luminosity class of 'III' indicates this is a giant star that has exhausted the hydrogen at its core and evolved away from the main sequence. It is radiating energy from its outer atmosphere at an effective temperature of 4,246 K which is what gives it the orange hue of a K-type star. This star displays an excess of infrared emission that may indicate circumstellar matter.
Theta Arae

**Theta Arae**, Latinized from θ Arae, is the Bayer designation for a star in the constellation Ara. It has an apparent visual magnitude of +3.67, which is bright enough to be seen with the naked eye. Based upon an annual parallax shift of 4.01 mas, Theta Arae is 810 light-years (250 parsecs) distant from the Earth.

This is a supergiant star with a stellar classification of B2 Ib. It has nearly nine times the mass of the Sun and is over 20 times the Sun's radius. The outer atmosphere of this star has an effective temperature of 17,231 K; much hotter than the surface of the Sun. At this heat, the star shines with the characteristic blue-white hue of a B-type star.
Eta Aquilae

**Eta Aquilae** (η Aql, η Aquilae) is the Bayer designation for a multiple star in the equatorial constellation of Aquila, the eagle. It was once part of the former constellation Antinous. On average, this star has an apparent visual magnitude of 3.87, making it one of the brighter members of Aquila. Based upon parallax measurements made during the Hipparcos mission, this star is located at a distance of roughly 1,382 light-years (424 parsecs), although the parallax estimate has a 44% margin of error.

The η Aquilae system contains at least two stars, probably three. The primary star η Aql A is by far the brightest and dominates the spectrum. An ultraviolet excess in the spectral energy distribution suggest the presence of a faint hot companion, η Aql B, which has been given a spectral type of B8.9 V. The fractional spectral type is an artefact of the mathematics used to model the spectrum, not an indication of any specific spectral features that would be intermediate between B8 and B9.

A companion has been resolved visually 0.66" distant, but measurements give this a spectral type of F1 - F5. It seems likely that the hot star detected in the spectrum is closer and unresolved. The resolved companion has not been shown to be physically associated, but it is estimated that it would have a period of nearly a thousand years. Measurements with the HST fine guidance sensors show variations likely to be due to orbital motion on a scale of two years, so η Aql would appear to be a triple system.
Pi Andromedae

**Pi Andromedae** (**Pi And**, **π Andromedae**, **π And**) is the Bayer designation for a binary star system in the

## Pi Andromedae

### Absolute Magnitude

-1.97

northern constellation of Andromeda. With an apparent visual magnitude of 4.4, it is visible to the naked eye. It is located approximately 600 light-years (180 parsecs) from Earth.

The pair is classified as a blue-white B-type main sequence dwarf, with an apparent magnitude of +4.34. It is a spectroscopic binary with an orbital period of 143.6 days and an eccentricity of 0.56.

The spectroscopic binary forms a triple system with *BD+32 102*, a magnitude 8.6 star located 35.9 arcseconds away. At 55 arcseconds separation is an 11th magnitude companion that is just located on the same line of sight, but at a much different distance from us.
Altair

**Altair** /ælˈtɛər/, designation **α Aquilae** (Latinised to **Alpha Aquilae**, abbreviated **Alpha Aql**, **α Aql**), is the brightest star in the constellation of Aquila and the twelfth brightest star in the night sky. It is currently in the G-cloud—a nearby interstellar cloud, an accumulation of gas and dust. Altair is an A-type main sequence star with an apparent visual magnitude of 0.77 and is one of the vertices of the Summer Triangle asterism (the other two vertices are marked by Deneb and Vega). It is 16.7 light-years (5.13 parsecs) from the Sun and is one of the closest stars visible to the naked eye. Altair rotates rapidly, with a velocity at the equator of approximately 286 km/s. This is a significant fraction of the star's estimated breakup speed of 400 km/s. A study with the Palomar Testbed Interferometer revealed that Altair is not spherical, but is flattened at the poles due to its high rate of rotation. Other interferometric studies with multiple telescopes, operating in the infrared, have imaged and confirmed this phenomenon.

Altair is a type-A main sequence star with about 1.8 times the mass of the Sun and 11 times its luminosity. Altair rotates rapidly, with a rotational period of about 9 hours; for comparison, the equator of the Sun makes a complete rotation in a little more than 25 days. Its rapid rotation forces Altair to be oblate; its equatorial diameter is over 20 percent greater than its polar diameter.

Satellite measurements made in 1999 with the Wide Field Infrared Explorer showed that the brightness of Altair fluctuates slightly, varying by just a few thousandths of a magnitude with several different periods less than 2 hours. As a result, it was identified in 2005 as a Delta Scuti variable star. Its light curve can be approximated by adding together a number of sine waves, with periods that range between 0.8 and 1.5 hours. It is a weak source of coronal X-ray emission, with the most active sources of emission being located near the star's equator. This activity may be due to convection cells forming at the cooler equator.
Epsilon Aquilae

**Epsilon Aquilae** (ε Aql, ε Aquilae) is the Bayer designation for a binary star in the equatorial constellation of Aquila. It has an apparent visual magnitude of 4.02 and is visible to the naked eye. Based upon an annual parallax of 21.05 mas, Epsilon Aquilae lies at a distance of approximately 155 light-years (48 parsecs) from Earth. This is a spectroscopic binary system. The pair orbit each other over a period of 1,271 days (3.5 years) with an eccentricity of 0.27.

The primary component of this system is an evolved giant star with a stellar classification of K1 III. It has more than double the mass of the Sun and has expanded to ten times the Sun's radius. It shines with 54–fold the Sun's luminosity, which is being radiated from its outer envelope at an effective temperature of 4,760 K. At this heat, it glows with the orange-hue of a K-type star. This has been designated a barium star, meaning its atmosphere is extremely enriched with barium and other heavy elements. However, this is disputed, with astronomer Andrew McWilliam (1990) finding normal abundances from an s-process.
Okab

**Zeta Aquilae** (**ζ Aquilae**, abbreviated **Zeta Aql**, **ζ Aql**) is a spectroscopic binary star in the equatorial constellation of Aquila. It is readily visible with the naked eye, being of the third magnitude. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 83 light-years (25 parsecs) distant from the Sun.

Zeta Aquilae's two components can be designated Zeta Aquilae A (officially named **Okab** /ˈoʊkæb/, the traditional name for the system) and B. Zeta Aquilae has a number of companions listed and together they are designated WDS J19054+1352. As the primary star of this group, Zeta Aquilae also bears the designation WDS J19054+1352A. The companions are then designated WDS J19054+1352B, C, D and E.

Zeta Aquilae has a combined stellar classification of A0 Vn, with the luminosity class 'V' indicating is a main sequence star that is generating energy through the nuclear fusion of hydrogen at its core. It has more than double the mass and twice the radius of the Sun, and is radiating more than 39 times the Sun's luminosity. The effective temperature of the star's outer envelope is about 9620 K, which gives it the white hue typical of A-type stars. The estimated age of this star is 50–150 million years.

This star is rotating rapidly, with a projected rotational velocity of 317 km s−1 giving a lower bound on the azimuthal velocity along the equator. As a result, it has a pronounced equatorial bulge, causing the star to assume an oblate spheroidal shape. The equatorial radius is about 30.7% greater than the polar radius. Because of the Doppler effect, this rapid rotation makes the absorption lines in the star's spectrum broaden and smear out, as indicated by the 'n' suffix in the stellar class.

Astronomers use Zeta Aquilae as a telluric standard star. That is, the spectrum of this star is used to correct for telluric contamination from the Earth's atmosphere when examining the spectra of neighboring stars. Observation of this star in the infrared band during the 2MASS survey appeared to reveal excess emission. However, the distribution of this emission couldn't be readily explained by a conjectured disk of circumstellar dust. Instead, the detection was later ascribed to errors caused by saturation of the near-infrared detectors.
All The Stars Wiki

**Welcome to the All The Stars Wiki!**
Hey, I'm Thirtytwopercent! Here's a list of all the stars in the night sky. We're currently under progress, so don't be depressed. (Plus, we reached 60 pages.)

Credits: Wikipedia

List of all our pages(We're going by constellation)

1. Home Page
2. Sun
3. A Cen A
4. A Cen B
5. Proxima Centauri
6. Barnard's Star
7. Alpheratz(Andromeda the Princess, 16 stars)
8. Mirach
9. Almach
10. Delta Andromedae
11. Nembus
12. Omicron Andromedae
13. Lambda Andromedae
14. Mu Andromedae
15. Zeta Andromedae
16. Kappa Andromedae
17. Phi Andromedae
18. Iota Andromedae
19. Pi Andromedae
20. Epsilon Andromedae
21. Eta Andromedae
22. Nu Andromedae
23. Alpha Antliae (Antila the Air Pump, 3 stars)
24. Epsilon Antliae
25. Iota Antliae
26. Alpha Apodis (Apus the "bird of paradise", 4 stars)
27. Gamma Apodis
28. Beta Apodis
29. Delta Apodis
30. Sadalsuud (Aquarius the Water Bearer, 16 stars)
31. Sadalmelik
32. Skat
33. Zeta Aquarii
34. 88 Aquarii
35. Lambda Aquarii
36. Abali
37. Gamma Aquarii
38. 98 Aquarii
39. Eta Aquarii
40. Tau2 Aquarii
41. Ancha
42. Phi Aquarii
43. Psi Aquarii
44. Iota Aquarii
45. Mu Aquarii
46. Altair (Aquila the Eagle, 9 stars))
47. Tarazed
48. Okab
49. Theta Aquilae
50. Delta Aquilae
51. Lambda Aquilae
52. Alshain
53. Eta Aquilae
54. Epsilon Aquilae
55. Beta Arae (Ara the Altar)
56. Choo
57. Zeta Arae
58. Gamma Arae
59. Delta Arae
60. Theta Arae
61. Eta Arae
Psi Aquarii

91 Aquarii is a triple star system. The primary component, 91 Aqr A, is a giant star with a stellar classification of K1 III. This is an evolved star with 138% of the Sun's mass that has expanded to over 10 times the size of the Sun. It is radiating 54 times the Sun's luminosity from its outer envelope at an effective temperature of 4,730 K. This gives it the orange-hued glow of a K-type star. The primary shares a common proper motion with two others stars, 91 Aqr B and C, suggesting that they are physically connected. The latter pair form a binary system located at an angular separation of 52 arcseconds from the primary. They are 10th magnitude stars separated by 0.3 arcseconds from each other.

**Psi2 Aquarii**, Latinized from ψ2 Aquarii, is the Bayer designation for a star in the equatorial constellation of Aquarius. It is visible to the naked eye with an apparent visual magnitude of 4.4. Based upon parallax measurements made during the Hipparcos mission, the distance to this star is roughly 400 light-years (120 parsecs). This is a B-type main sequence star with a stellar classification of B5 Vn. The 'n' suffix indicates that the absorption lines in the spectrum are being broadened by Doppler shift from the star's rapid rotation rate. The projected rotational velocity of the star is 341 km/s. Psi2 Aquarii is 4.6 times as large as the Sun with an effective temperature of 15,212 K in its outer envelope. It is a λ Eridani variable, or periodic Be star, with a pulsation cycle lasting 1.073 days. The amplitude of the variation is 0.024 in magnitude.

**Psi3 Aquarii**, Latinized from ψ3 Aquarii, is the Bayer designation for a visual binary star system in the constellation of Aquarius. It has an apparent visual magnitude of 4.98, which is bright enough to be seen with the naked eye. Parallax measurements give a distance estimate of roughly 262 light-years (80 parsecs). The main component of this system is an A-type main sequence star with a stellar classification of A0 V. Its companion is an 11th magnitude star 1.5 arcseconds from the primary. This system is an X-ray source with a luminosity of 8.34 × 1029 erg s−1. This radiation most likely comes from the companion star.
Nu Andromedae

**Nu Andromedae** (**Nu And**, **ν Andromedae**, **ν And**) is a binary star in the constellation Andromeda. The

## Nu Andromedae

### Absolute Magnitude

-1.85

system has an apparent visual magnitude of 4.5, which is bright enough to be seen with the naked eye. It is approximately 620 light-years(190 parsecs) from Earth. Situated just over a degree to the west of this star is the Andromeda Galaxy.

Nu Andromedae is spectroscopic binary system with a nearly circular orbit that has a period of 4.2828 days.  The primary component is a B-type main sequence star with a stellar classification of B5 V. The fainter secondary has a classification of F8 V, which makes it an F-type main sequence star. The pair is about 63 million years old.
Delta Aquilae

**Delta Aquilae** (δ Aquilae, δ Aql) is a binary star system in the equatorial constellation of Aquila. It has an apparent visual magnitude of 3.4 and, based upon parallax measurements, is located about 50.6 light-years (15.5 parsecs) from Earth.

Delta Aquilae is an astrometric binary where the two components orbit each other with a period of 3.422 years and an eccentricity of about 0.36. This is a type of binary star system where the presence of the secondary component is revealed by its gravitational perturbation of the primary. The individual components have not been resolved with a telescope.

The primary component, Delta Aquilae A, is a subgiant star with a stellar classification of F0 IV, where the luminosity class of IV indicates it is in the process of exhausting the supply of hydrogen at its core and evolving into a giant star. The mass of the star is 65% greater than the Sun and it has expanded to more than double the Sun's radius. It is radiating around 7–8 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 7,016 K, giving it the yellow-white hue of an F-type star. Delta Aquilae A is a Delta Scuti variable that exhibits variations in luminosity caused by pulsations in its outer envelope. It is spinning rapidly with a projected rotational velocity of about 87 km s−1. This is a lower bound on the azimuthal velocity along the star's equator.

The secondary component, Delta Aquilae B, is a smaller star with about 67% of the Sun's mass and an estimated 61% of the radius of the Sun. It may be a K-type star.
Omicron Andromedae

**Omicron Andromedae** (ο And, ο Andromedae) is a star system in the constellation Andromeda. It is approximately 692 light years from Earth. The system as a whole is classified as a blue-white B-type giant, with a mean combined apparent magnitude of +3.62.

Omicron Andromedae is a multiple star containing at least four components. It is thought to consist of two close pairs in a wider orbit, making a four-star system. This star system has a peculiar velocity of 34.5 ± 5.9 km/s.

The components A and B were first resolved in 1949, when they were reported to be separated by less than 0.1". In 1975 they were separated by 0.375" and by 2014 by only 0.21". An orbit has been derived with a period of 117 years.

In 1975, a companion was discovered by speckle interferometry only 0.05" from component A. Components Aa and Ab orbit every 5.6 years.

A fourth component in the system was suspected and in 1988 it was confirmed. Although a clear 33.01 day period was seen, it was unclear which component the fourth star was in orbit with. Eventually, it was settled that component B was a close spectroscopic binary including the fourth star.

Omicron Andromedae is a Gamma Cassiopeiae type variable star and the system's brightness varies from magnitude +3.58 to +3.78. The variable component is the brightest and most massive star in the system, Aa.

The spectrum is predominantly that of a B6 giant star, from the brightest component in the system. It is a shell star and the spectrum contains emission lines with variable profiles.

Spectral lines similar to an A2 star are also detectable in the spectrum and these are thought to originate in the B component.
Abali

**Epsilon Aquarii**, Latinized from ε Aquarii, is a single star in the equatorial zodiac constellation of Aquarius, located near the western constellation border with Capricornus. It has the proper name **Albali** /ælˈbeɪli/, now formally recognized by the IAU. This is a white-hued star that is visible to the naked eye with an apparent visual magnitude of 3.77. Based upon parallax measurements taken during the Hipparcos mission, it is located at a distance of approximately 208 light-years (64 pc) from the Sun with an absolute magnitude of −0.46. The star is drifting closer with a radial velocity of −15 km/s.

This object is an A-type main-sequence star with a stellar classification of A1 V. It is an estimated 388 million years old with a high rate of spin, showing a projected rotational velocity of around 118 km/s. The elemental abundances in the stellar atmosphere are close to solar, with pronounced underabundances of aluminium and strontium. The star has three times the mass of the Sun and about 2.5 times the Sun's radius. It is radiating 138 times the luminosity of the Sun from its photosphere at an effective temperature of 9,622 K.
Tau2 Aquarii

**Tau2 Aquarii** (τ2 Aqr, τ2 Aquarii) is the Bayer designation for a star in the equatorial constellation of Aquarius. It is visible to the naked eye with an apparent visual magnitude of +4.0. Because the star lies near the ecliptic it is subject to occultations by the Moon.

This is an orange-hued giant star with a stellar classification of K5 III. The measured angular diameter, after correction for limb darkening, is 5.12 ± 0.05 mas. At an estimated distance of 318 light-years (97 parsecs) based on parallax measurements, this yields a physical size of about 53 times the radius of the Sun.
Zeta Aquarii

**Zeta Aquarii** (ζ Aquarii, ζ Aqr) is the Bayer designation for a triple star system; the central star of the "water jar" asterism in the equatorial constellation of Aquarius. The combined apparent visual magnitude of this system is 3.65, which is readily visible to the naked eye. Parallax measurements yield a distance estimate of around 92 light-years (28 parsecs) from Earth.

The binary was measured by William Herschel in 1779 however Christian Mayer, listed an earlier observation in his first double-star catalog in 1784 so its true discoverer is not clear. The two stars have an orbital period of about 587 years. The semimajor axis is 3.8 arcseconds and they have an orbital eccentricity of 0.40. The orbital plane is inclined by 138.2° to the line of sight.

The brighter component, ζ Aquarii A (also called ζ2 Aquarii), is a yellow-white-hued F-type main sequence star with an apparent magnitude of +4.42. Its companion, ζ Aquarii B (also called ζ1 Aquarii), is a yellow-white-hued F-type subgiant with an apparent magnitude of +4.51. The fact that their brightness is so similar makes the pair easy to measure and resolve.

Zeta Aquarii A is known to be an astrometric binary system, as it undergoes regular perturbations from its orbit. It has a 26-year orbital period and a semimajor axis of 0.11″. The secondary's mass is 0.6 M☉.

Zeta Aquarii is currently a northern hemisphere object. In 2004 it was directly above the celestial equator, and before that it was located south of it.
Eta Andromedae

**Eta Andromedae** (**Eta And**, **η Andromedae**, **η And**) is a spectroscopic binary star in

## Eta Andromedae

### Absolute Magnitude

A: 0.52B: 1.07

the constellation of Andromeda. It consists of two G-type subgiant or giant stars orbiting each other with a period of 115.7 days and has an overall apparent visual magnitude of approximately 4.403.
Alpha Centauri A

Alpha Centauri A, also known as Rigil Kentaurus, is the principal member, or primary, of the binary system. It is a solar-like main-sequence star with a similar yellowish colour, whose stellar classification is spectral type G2 V: it is slightly larger and more luminous than the Sun. Alpha Centauri A is about 10 percent more massive than the Sun, with a radius about 22 percent larger. When considered among the individual brightest stars in the sky (excluding the Sun), it is the fourth brightest at an apparent magnitude of −0.01, being slightly fainter than Arcturus at an apparent magnitude of −0.04.

The type of magnetic activity on Alpha Centauri A is comparable to that of the Sun, showing coronal variability due to star spots, as modulated by the rotation of the star. However, since 2005 the activity level has fallen into a deep minimum that might be similar to the Sun's historical Maunder Minimum. Alternatively, it may have a very long stellar activity cycle and is slowly recovering from a minimum phase.
Mark Beaufort

Mark Beaufort is a popular boy at the school, he was childhood best friends with Anastasia Banks but stopped hanging out with her when he was 10

## Involvement

### Past

Born into the rich family The Beauforts, there was a lot for young Mark to live up to. As a shy kid he mostly was friends with family (his sisters and mom mainly) though was also friends with a girl named Anastasia whom he cared about deeply. He’d show her gambling tricks and cheats for games as the two of them enjoyed playing games together.

When he was 10 his mother decided to leave Mr. Beaufort, since she didn’t have as good lawyers as Mr. Beaufort it seemed likely that she wouldn’t have any of her kids come with her, but then sisters both made bets with their father to get to go with their mother. Judie bet her bedroom’s door at her dad’s place, winning since she was planing living with her mom so didn’t need the door, Lillie betting her free will but being sure she’d win so won. Mark didn’t know the trick to winning the Dice game and didn’t believe in himself so when he made the same bet of his free will he lost.

After that he had to do everything his dad told him to,1st thing he had to do was stop being friends with Anastasia since she could tell a adult about the clear abuse Mark was going through. From there Mark had to become this asshole rich boy who’d fit the brand of his father.

### Present

He and Nicole are friends who seem like they're likely to date, Mark doesn't really have any real friends due to his fathers control.

## Personality

He is a caring boy, he loves spending time with the people he cares about, he acts a bit silly with friends and tends towards being a bit of a trickster, using his more cunning nature for small tricks and the like, as a whole he's like a magician who lets his close friends in on the trick, he can actually get quite showy when around friends as he likes to act a bit extra while showing his tricks off

But while being controlled Mark loses a lot of his cunningness and instead of acting like his real caring self he acts like an asshole, pretending to forget about people he cares about and when talking with them acting as if he doesn’t care about them at all, with an above it all act. As a whole he acts so very different from what he was like as a kid to the point that it is very clear something off about him, he'll do things to be mindful and then say he doesn't give a damn along with trying to act out as someone who's not worth people's time. He does mainly because he's given up hope that someone will free him from his father's control so he'd rather no one care for him than love & lose him.

He is actually quite shy when it comes down to it, he doesn’t really like getting to know new people and being very awkward when comes to things like: kissing, hand holding, ect. He hasn't really had those normal moments to get used to closeness with others since he was 10 which is where of this shyness comes from.
88 Aquarii

**88 Aquarii** (abbreviated **88 Aqr**) is a star in the equatorial constellation of Aquarius. *88 Aquarii* is the Flamsteed designation, though it also bears the Bayer designation **c2 Aquarii**. In dark conditions it is visible to the naked eye with an apparent visual magnitude of +3.68. Based upon parallax measurements, this star is at a distance of around 271 light-years (83 parsecs) from Earth.

The spectrum of 88 Aquarii matches an evolved giant star with a classification of K1 III. Its measured angular diameter is 3.24 ± 0.20 mas, which, at the estimated distance of Delta Ophiuchi, yields a physical size of about 29 times the radius of the Sun. The cool, orange hued glow of this star comes from the outer atmosphere's effective temperature of 4,430 K.
Mirach

**Beta Andromedae** (**β Andromedae**, abbreviated **Beta And**, **β And**), officially named **Mirach** /ˈmaɪræk/, is a prominent star in the northern constellation of Andromeda. It is northeast of the Great Square of Pegasus and is theoretically visible to all observers north of 54° S. It is commonly used by stargazers to find the Andromeda Galaxy. The galaxy NGC 404, also known as Mirach's Ghost, is seven arc minutes away from Mirach.

This star has an average apparent visual magnitude of 2.05, making it the brightest star in the constellation. The luminosity varies slightly from magnitude +2.01 to +2.10. Based upon parallax measurements, it is roughly 197 light-years(60 parsecs) from the Sun. Its apparent magnitude is reduced by 0.06 by extinction due to gas and dust along the line of sight.

Beta Andromedae is a red giant with a stellar classification of M0 III. Since 1943 the spectrum of this star has been one of the stable anchor points by which other stars are classified. It is suspected of being a semiregular variable star whose apparent visual magnitude varies from +2.01 to +2.10. At this stage of the star's evolution, the outer envelope has expanded to around 100 times the size of the Sun. It is radiating 1995 times the luminosity of the Sun at an effective temperature of 3842 K.
Alpha Centauri B

Alpha Centauri B, also known as Toliman, is the secondary star of the binary system. It is a main-sequence star of spectral type K1 V, making it more an orange colour than Alpha Centauri A; it has around 90 percent the mass of the Sun and a 14 percent smaller diameter. Although it has a lower luminosity than A, Alpha Centauri B emits more energy in the X-ray band. Its light curve varies on a short time scale, and there has been at least one observed flare. It is more magnetically active than Alpha Centauri A, showing a cycle of 8.2±0.2 yr compared to 11 years for the Sun, and about half the minimum-to-peak variation in coronal luminosity of the Sun. Alpha Centauri B has an apparent magnitude of +1.35, slightly dimmer than Mimosa.
Viktor H. Strobovski

Viktor is an teacher in Viktor's School

## Appearance

He has appeared as a regular man borned 1975 he wears white mask brown hair brown jacket black trousers blue he carrys axe in has back when angry with flashing red eyes

## Mechanics

In start of game he just give command stand there an do nuffing. When a player GOT A questionn wrong he walk around slow try to catch at them unless bells will toll ¬``¬`¬¬¬¬`¬!¬¬ thats he does. At an end of a game he always sprints so fucking fast with loads of red blood

## Trivia

He an stoled image of a 44 yer old Mathematics teacher
Lambda Andromedae

**Lambda Andromedae** (λ And, λ Andromedae) is the Bayer designation for a binary star in the

## Lambda Andromedae

### Absolute Magnitude

1.91

northern constellation of Andromeda. At an estimated distance of approximately 86.1 light-years (26.4 parsecs) from Earth, it has an apparent visual magnitude of +3.8. This is bright enough to be seen with the naked eye.

Lambda Andromedae is a single-lined spectroscopic binary with an orbital period of 20.5212 days. The spectrum of the primary matches a stellar classification of G8 III-IV, suggesting that it is an evolved star that lies part way between the subgiant and giant stages. The mass of this star is similar to the Sun, but it has expanded to around seven times the Sun's radius. It is radiating over 23 times the luminosity of the Sun from its outer envelope at an effective temperature of 4,800 K, giving it the characteristic yellow hue of a G-type star.

This is an RS Canum Venaticorum variable and its brightness varies by 0.225 magnitudes, reaching a maximum of 3.70, with a period of 54.2 days. Such variability is theorized to occur because of tidal friction, which results in chromosphericactivity. However, the orbit of this system is nearly circular, so the cause of this system's variability remains uncertain. The X-ray luminosity of this star, as measured by the ROSAT satellite, is 2.95 × 1030 erg s−1.
Rick Astelsy Basics

it an Mod Of Baldi More Coming Soon. The dev is called ViktorStrobovski an Now I Tell U Characters.

## characters

Rick astley(baldi)

Viktor(Principal)

Leather Face(Bully)

Jeffy sml(sweep broom)

pinnochio(sock artsand crafters)

evil viktor(fileName2)

1st prize

playtime

## Items

drink can(bsoda)

choco bar(energy bar)

padlock(lock)

anti hearing tape

scissors

The notebooks is rick astley albums
Beta Apodis

**Beta Apodis** (β Aps, β Apodis) is the Bayer designation for a star in the southern circumpolar

## Beta Apodis

### Absolute Magnitude

0.819

constellation of Apus. It is located approximately 149 light-years (46 parsecs) from Earth, as determined by parallax measurements. The apparent visual magnitude of this star is +4.24, which is bright enough to be seen with the naked eye

The spectrum of this star matches the characteristics of a K0 III, which, according to models of stellar evolution, indicates that it is in the giant star stage, having exhausted the supply of hydrogen at its core. The measured angular diameter of this star is 2.09 ± 0.11 mas. At the estimated distance of this star, this yields a physical size of about 11 times the radius of the Sun. The expanded outer atmosphere of Beta Apodis has an effective temperature of about 4,900 K. This heat is causing it to glow with the characteristic orange hue of a K-type star.
The Sickness

**The Sickness** (**ザ・シックネス**, *Za Shikkunesu*) es el Stand de Vladio, antagonista principal de JoJo's Bizarre Adventure: *Vodka is Undrinkable* que obtiene después de que su hermano le apuñalara con la flecha, desconociendo las consecuencias posteriores que esto tuviera.

Plantilla:Stand

## Apariencia

Su apariencia es la de un humanoide extremadamente alto, esbelto y moreno, con vendas por todo el cuerpo.

A pesar de su aspecto delgado, The Sickness posee una gran potencia muscular con la que subyuga a sus enemigos haciendo uso en la mayor parte de ocasiones de su **Sambo**.

Tiene la cara cubierta por una especie de máscara con forma de cráneo, en la que destacan sus ojos verdosos

## Personalidad

The Sickness no tiene personalidad propia, pero en él se ve reflejada la paranoia de Vladio, por ejemplo en sus ojos, abiertos como platos, sin parpadear. También las vendas pueden simbolizar heridas que en verdad no fueran para tanto, siendo vendadas demasiado, sin necesidad.

Su presencia es tetríca, lugubre y silenciosa, a veces incluso asusta a Vladio, acentuado por su paranoia obviamente.

## Habilidades

La habilidad principal de **The Sickness** se basa en que, cuando algo se mete en su rango de 20 metros, si el usuario activa la habilidad, todo ser vivo que se encuentre en su rango de acción, sufrirá de un instantáneo bajón emocional tan fuerte que hará que la víctima caiga al suelo.

Dependiendo del ánimo original de la víctima, esta habilidad puede hacer del ánimo más elevado posible, el más bajo posible, es entonces cuando los pensamientos más negativos empezarán a torturar a la víctima, su auto-estima se reducirá drástica y progresivamente, y en general su ánimo caerá tanto que puede llegar incluso hasta el punto de llegar a quitarse la vida si la víctima se queda por un largo período de tiempo en su rango de acción. Cabe destacar que, cuando más cerca se esté del usuario, la habilidad será más intensa. La víctima no podrá de ninguna manera subirse el ánimo, ni con drogas, ni nada parecido.

Si la víctima ya tenía de por si un estado de ánimo bajo, **The Sickness** tendrá que trabajar poco.

También es importante saber que al igual que el usuario, este Stand puede usar **Sambo**,que es un arte marcial nacido en Rusia que a menudo es comparado con el Jiu Jitsu, Judo, Muay Thai, entre otros. Esto quiere decir que este Stand es un peligro real a corto alcance, por sus conocimientos en artes marciales, y a largo alcance, por su habilidad. El **Sambo**será más efectivo y poderoso si la víctima se encuentra muy afectado por la habilidad del Stand, es decir, si pasó mucho tiempo dentro del rango de acción. Por eso la mejor estrategia para Vladio es activar la habilidad de **The Sickness**sin que su víctima se de cuenta, y entonces, pasado cierto tiempo dentro, atacar para matarla.

Si el Stand se desactiva o la víctima sale del rango, la desaparición del efecto es progresiva y lenta, pero si se vuelve a meter, el efecto aumentara desde sea cual fuere el efecto que tenía antes de salir.

La contra es que, si se activa la habilidad por mucho tiempo, el usuario empieza a sufrir de dolores de cabeza y hasta alucinaciones.
Suchotator

El suchotator es un híbrido entre dos dinosaurios espinosauridos dando como resultado al suchotator un dinosaurio híbrido imponente. El suchotator vive la mayor parte de su vida en el agua esperando a sus presas, este híbrido cuenta con más de 100dientes largos y afilados especializados en poder atrapar peces (su comida favorita) como también dos fuertes brazos con 3 garras afiladas que le sirven para dar fuertes golpes y heridas profundas a sus agresores.

Altura: 4,5metros

longitud: 12metros

Peso: 6 toneladas

El suchotator cuenta con una especies de picos que comienzan desde su la espalda hasta su cola lo que hace que si algún adversario quiere morder su espalda o cola tendrá que pincharse y terminar adolorido, este híbrido es muy ágil a pesar de su peso ya que alcanza velocidades de hasta 60km-h! Gracias a su gran agilidad puede acertar golpes rápidos y profundos con sus largos brazos como fuertes mordiscos a sus rivales, aunque sea un dinosaurio que está más acostumbrado a estar en el agua es muy ágil en tierra siendo capaz de derribar teropodos medianos sin problemas.

El suchotator cuenta con una papada debajo de su cuello y así color varía de género del individuo ya que si es macho tiene la papada naranja y si es mujer tendrá la papada de un color amarillo fuerte. Los suchotators prefieren ser solitarios hasta que llega la temporada de aparemiento dónde los machos luchan por las hembras en el agua a muerte!
VILE

VILE is the son of satan,born from an unknown mother.He is extremely powerful.He was born exactly 2000 years ago during midnight as an experiment by the scientists of hell.He is built to be unmatched in power and strength. You cant kill hm, hes immorteal. He also realearted to A Lavenza . She Is An Falken Angel
Alshain

**Beta Aquilae** (**β Aquilae**, abbreviated **Beta Aql**, **β Aql**) is a binary star in the equatorial constellation of Aquila. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 44.7 light-years from the Sun. Its two components are designated Beta Aquilae A (formally named **Alshain** /ælˈʃeɪn/, the traditional name for the system) and B.

The primary (Beta Aquilae A) is of magnitude 3.71 and spectral class G8IV. It has a very low level of surface magnetic activity and may be in a state similar to a Maunder minimum. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. A subgiant with a mass 30% greater than the Sun's, a luminosity six times that of the Sun, and a radius about thrice solar.

The secondary (Beta Aquilae B) is a 12th magnitude companion which is 13 arcseconds away in the sky. It is a class M red dwarf with a mass a third that of the Sun and a luminosity 2.5% the Sun's.
Golden Sonic (2015)

Golden Sonic (2015), commonly known as 15' Golden Sonic, is a character from the Bite of '91 (FNaS 5) and also the main antagonist of the Bite of '15 (FNaS 1). His skin color in his appearance is yellow, but his other colors are not black, so he looks nothing like Golden Freddy.

Behavior/Actions: Golden Sonic will rarely appear on the poster in the West Hall Corner. Upon pulling the camera down, he will appear in the office. Pull your monitor back up to get rid of him. If you take too long, he will kill you, crashing the game.
Flexus contrari

*Creado por Heyta*

*Forma parte del multiverso de Trinity Chronicle*

Plantilla:Serie DBSWE

Flexus Contrari es una serie que relatará los hechos sucedidos en esta gran guerra ocurrida hace millones de años que habrán sido de gran influencia en el universo desde Dragon Ball hasta este momento.

## Sinopsis

Un multiverso joven, lleno de luz y esperanza, con una paz que fue inevitablemente truncada por la codicia y la envidia, dado que el origen del multiverso llevó a muchos seres inteligentes a preguntarse su origen, de donde vinieron, a donde van, y a donde irán. Empezaron a explorar, cada uno en su territorio, expandiendo sus horizontes, siendo observados bajo lupa de los seres divinos. Hasta que, llegado el momento, se dieron cuenta, que, sin duda, no estaban solos, no solo en su propio universo, sino que había algo más allá. Esto fue, el principio del fin.

Durante centenas de miles de años, se fue expandiendo la Leyenda de Ximno, el creador del espacio, tiempo y la realidad misma. Al punto de llegar a distintos universos, aunque cada uno con el nombre ligeramente modificado. Pero en lo que la mayoría estaba de acuerdo, era que definitivamente este ser era el creador de todo, y sobretodo, lo que detonó la guerra:

**La Trinidad:**
**Caeruleus. Flavus. Ruber.**

Los tres pilares multiversales, en forma esférica, repartidos en los que inicialmente eran 30 universos...

Quien las poseyera, poseería un poder a la altura del mismísimo creador. Esta premisa, no trajo más que desgracia.

## Personajes

En esta serie, tú elijes el bando. La línea entre bien y el mal, se vuelve gris.

*Se irán añadiendo más*
Raine Sage

**Raine Sage**, originaire de Tales of Symphonia, est une candidate de Koh-Lanta: Le Combat des Héros.

Membre de l'équipe verte, Raine est connue pour sa gentillesse mais aussi pour sa thalamaphobia ce qui la pénalise sévèrement dans les épreuves aquatiques, malgré ça, elle parvient à aller très loin dans l'aventure mais lorsqu'elle décide d'éliminer Mickey parce qu'il les a sous-estimés avec Serah Farron, elle sera éliminé par tirage au sort lorsqu'elle tenta d'éliminer Hanzo Hasashi ou Jago ce qui la conduira sur l'île de l'Extinction où elle manqua de peu de revenir dans l'aventure mais elle perdra contre Selena.

## Koh-Lanta le Combat des Héros

1 : Raine est en binôme avec Gaston, si l'un d'eux venait à être éliminer, il entrainerait l'autre dans sa chute, si Gaston se prend une voix, ce n'est pas suffisant pour y être éliminer.

2 : Jago utilise un collier d'immunité ce qui annule le vote de Raine et oblige un nouveau vote qui finit en égalité entre Serah et Vaan, Raine ne change pas son vote ce qui entraîne un tirage au sort entre Kaito, Raine et Takeru, Raine tire une boule noire ce qui l'élimine du jeu.

## Trivia

Raine est la première candidate à être éliminée par tirage au sort.
Haus Ulgo

**Haus Ulgo** ist neben Haus Organa, Haus Alde und Haus Thul eines der großen Häuser von Alderaan. Das Oberhaupt von Haus Ulgo erhebt Anspruch auf den verwaisten Königsthron und hat dadurch einen Bürgerkrieg auf Alderaan losgetreten, der für die Republik und das Imperium als Stellvertreterkrieg ausgenutzt wird. Verbündet ist Haus Ulgo mit dem kleineren Haus Rist, die für ihre Attentäter berüchtigt sind.