recursal/Fanatic-Fandom huggingface dataset:
V4399 Sagittarii

Object type: Blue subgiant star
Number of stars: 1
Total mass: 3.209 Solar Masses (3,361 Jupiter Masses; 1,068,472 Earth Masses; 6,381 Septillion Tonnes)
Distance from the sun: 1,410 ly

V4399 Sagittarii, Also Named **HD 171060**, **CD -33° 13341** or **CP -33° 5156**, is a Blue-White Subgiant Stars in The Constellation Sagittarius, The Star is Located at 1,410 Light Years Away From Earth

The name HD 171060 derives directly from the fact that the star is the 171,060th stars in the Henry Draper catalogue, however, the star doesn't have HR numbers, because the star is too faint to visible by naked eye

The name HIP 91020 derives directly from the fact that the star is the 91,020th stars in the Hipparcos catalogue, and The name SAO 210314 derives directly from the fact that the star is the 210,314th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 3.209 Solar Masses (3,361 Jupiter Masses; 1,068,472 Earth Masses; 6,381 Septillion Tonnes)
* Radius: 3.417 Solar Radius (4,758,801 km in Diameter; 0.01591 AU; 11.68 Solar Areas or 39.9 Solar Volumes)
* Luminosity: 177 Solar Luminosities
* Temperature: 11,386 Kelvin (11,113 °C; 20,035 °F)
* Spectral Type: B9IV
* Right Ascension: 18h 34m 05.1225s
* Declination: -32° 57' 40.078"
* Apparent Magnitude (V): +7.17

### Other Designations

V4399 Sagittarii, HD 171060, HIP 91020, SAO 210314, CD -33° 13341, CP -33° 5156, TYC 7398-135-1, 2MASS J18340513-3257400
V916 Cassiopeiae

V916 Cassiopeiae, Also Named **IRAS 01395+6306**, is a Red Giant Star in The Constellation Cassiopeia, The Star is Located at Around 12,000 Light Years Away From Earth

## Information

* Mass: 2.5 Solar Masses
* Radius: 488-617 Solar Radius
* Luminosity: 12,926-29,331 Solar Luminosities (18,348-20,663 Solar Luminosities)
* Temperature: 2,786-3,041 Kelvin (2,513-2,768 °C; 4,555-5,014 °F)
* Spectral Type: C6,7-C7,9 or M7III-M9III
* Right Ascension: 01h 43m 01.7855s
* Declination: +63° 22' 05.032"
* Variable Star Type: Mira Variable Star

### Other Designations

V916 Cassiopeiae, CGCS 257, IRCO 3114, IRAS 01395+6306, NIKC 1-103, 2MASS J01430178+6322049
V353 Persei

Object type: Blue subgiant star
Number of stars: 1
Total mass: 21.657 Solar Masses (22,686 Jupiter Masses; 7,210,936 Earth Masses; 43,064 Septillion Tonnes)
Distance from the sun: 10,266 ly

V353 Persei, Also Named **HD 13544** or **BD +53° 480**, is a Blue Subgiant Stars in The Constellation Perseus, The Star is Located at 10,266 Light Years Away From Earth

The name HD 13544 derives directly from the fact that the star is the 13,544th stars in the Henry Draper catalogue, however, the star doesn't have HR numbers, because the star is too faint to visible by naked eye

The name HIP 10391 derives directly from the fact that the star is the 10,391st stars in the Hipparcos catalogue, and The name SAO 23052 derives directly from the fact that the star is the 23,052nd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 21.657 Solar Masses (22,686 Jupiter Masses; 7,210,936 Earth Masses; 43,064 Septillion Tonnes)
* Radius: 11.285 Solar Radius (15,716,439 km in Diameter; 0.05253 AU; 127 Solar Areas or 1,437 Solar Volumes)
* Luminosity: 54,105 Solar Luminosities
* Temperature: 26,205 Kelvin (25,932 °C; 46,709 °F)
* Spectral Type: B1IV
* Right Ascension: 02h 13m 51.8326s
* Declination: +53° 54' 52.525"
* Apparent Magnitude (V): +8.88
* Variable Star Type: Beta Cephei Variable Star

### Other Designations

V353 Persei, HD 13544, HIP 10391, SAO 23052, BD +53° 480, TYC 3686-2648-1, 2MASS J02135183+5354525
V509 Cassiopeiae

<--- HD 217475 | **HD 217476** | HD 217477 --->
V509 Cassiopeiae, Also Named **HD 217476**, **BD +56° 2923** or **IRAS 22579+5640**, is a Yellow Hypergiant Stars in The Constellation Cassiopeia, The Star is Located at 17,182 Light Years Away From Earth

The name HD 217476 derives directly from the fact that the star is the 217,476th stars in the Henry Draper catalogue, and The name HR 8752 derives directly from the fact that the star in the 8,752nd stars in the Bright Star catalogue

The name HIP 113561 derives directly from the fact that the star is the 113,561st stars in the Hipparcos catalogue, and The name SAO 35039 derives directly from the fact that the star is the 35,039th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 40-50 Solar Masses (41,900-52,375 Jupiter Masses; 13,318,440-16,648,050 Earth Masses; 79,539-99,424 Septillion Tonnes)
* Radius: 578-726 Solar Radius (804,971,352-1,011,088,584 km in Diameter; 2.69045-3.37935 AU; 334,084-527,076 Solar Areas or 193,100,552-382,657,176 Solar Volumes)
* Luminosity: 271,800-592,800 Solar Luminosities (375,700-429,000 Solar Luminosities)
* Temperature: 5,482-5,944 Kelvin (5,209-5,671 °C; 9,408-10,240 °F)
* Spectral Type: G0Ia+-G5Ia+
* Right Ascension: 23h 00m 05.1012s
* Declination: +56° 56' 43.351"
* Apparent Magnitude (V): +5.13

### Other Designations

V509 Cassiopeiae, HD 217476, HR 8752, HIP 113561, SAO 35039, BD +56° 2923, IRAS 22579+5640, IRC +60379, TYC 3993-2269-1, 2MASS J23000509+5656433

## See Also

* V382 Carinae
* Betelgeuse
* Stephenson 2-18
* V766 Centauri
* RW Cephei
* Rho Cassiopeiae
* HD 179821
* UY Scuti
* Eta Carinae
V648 Cassiopeiae

Object type: Red supergiant star
Number of stars: 1
Total mass: 21 Solar Masses (21,998 Jupiter Masses; 6,992,181 Earth Masses; 41,758 Septillion Tonnes)
Distance from the sun: 7,308 ly

V648 Cassiopeiae, Also Named **HD 237010**, **BD +57° 647** or **IRAS 02473+5738**, is a Red Supergiant Stars in The Constellation Cassiopeia, The Star is Located at 7,308 Light Years Away From Earth

The name HDE 237010 derives directly from the fact that the star is the 237,010th stars in the Henry Draper catalogue, and The name HIP 13290 derives directly from the fact that the star is the 13,290th stars in the Hipparcos catalogue

## Information

* Mass: 21 Solar Masses (21,998 Jupiter Masses; 6,992,181 Earth Masses; 41,758 Septillion Tonnes)
* Radius: 769-805 Solar Radius (1,070,973,996-1,121,110,620 km in Diameter; 3.57951-3.74708 AU; 591,361-648,025 Solar Areas or 454,756,609-521,660,125 Solar Volumes)
* Luminosity: 107,169-128,538 Solar Luminosities
* Temperature: 3,766-3,852 Kelvin (3,493-3,579 °C; 6,319-6,474 °F)
* Spectral Type: M2Iab
* Right Ascension: 02h 51m 03.9478s
* Declination: +57° 51' 19.923"
* Apparent Magnitude (V): +9.38
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V648 Cassiopeiae, HD 237010, HIP 13290, BD +57° 647, IRAS 02473+5738, IRC +60100, TYC 3708-667-1, 2MASS J02510394+5751198
Timeline of a 1.33 Solar Masses Stars

This is Timeline of a 1.33 Solar Masses Stars, The Star Have 4 Planets, and The Star was Located at The Globular Cluster Messier 13

## Information

* Initial Radius: 1.283 Solar Radius
* Initial Luminosity: 2.713 Solar Luminosities
* Initial Temperature: 6,535 Kelvin
* Initial Spectral Type: F5V
* Metallicity [Fe/H]: -0.06 dex
* Initial Habitable Zone: 1.49 AU - 2.61 AU

(Note: \* = Star With Dyson Sphere, MB\* = Star With Matrioshka Brain)

## Planet Information

* Planet A: 1.329 Jupiter Radius, 2.694 Jupiter Masses, 0.17 AU, Gas Giant Planet
* Planet B: 1.07 Earth Radius, 6.53 Earth Masses, 1.68 AU, Terrestrial Planet
* Planet C: 1.59 Earth Radius, 4.47 Earth Masses, 1.97 AU, Ocean Planet
* Planet D: 1.63 Earth Radius, 9.24 Earth Masses, 2.73 AU, Terrestrial Planet

## See Also

* Timeline of HD 209458 Star System
* Timeline of a 1.18 Solar Masses Stars
* Timeline of a 1.37 Solar Masses Stars
* Timeline of The Solar System
V1195 Scorpii

V1195 Scorpii, Also Named **HD 146707**, is a Blue Subgiant Stars in The Constellation Scorpius, The Star is Located at at 1,547 Light Years Away From Earth

## Information

* Mass: 3.287 Solar Masses
* Radius: 2.792 Solar Radius
* Luminosity: 118.54 Solar Luminosities
* Temperature: 11,363 Kelvin
* Spectral Type: B9IV
* Right Ascension: 16h 19m 23.0207s
* Declination: -40° 56' 38.89"
* Apparent Magnitude (V): +8.91

### Other Designation

V1195 Scorpii, HD 146707, HIP 79970, SAO 226653, CD -40° 10312, CP -40° 7254, TYC 7856-353-1, 2MASS J16192302-4056390
Weezer Sector B1-1567

Weezer Sector B1-1567 is a Extremely Metal-Poor Red Dwarf Stars in The Constellation Delphinus, The Star is Located at 7,628 Light Years Away From Earth

## Information

* Mass: 0.286 Solar Masses
* Radius: 0.195 Solar Radius
* Luminosity: 0.8491% Solar Luminosities
* Temperature: 3,967 Kelvin (3,694 °C; 6,681 °F)
* Age: 12.8 Billion Years
* Spectral Type: M0V-VI
* Metallicity [Fe/H]: -3.67 dex
Accelerator

## General

Accelerator is a character from the Toaru Franchise, he makes his first appearance as the villain of the third volume of the Toaru Majutsu no Index(A Certain Magical Index) light novel, during the "Sisters Arc". After being defeated by Touma and after some unfortunate events, (SPOILER ALERT:) Accelerator is shot in the brain and takes permanent damage and thus no longer can use his Vector Manipulation power as effective as before, thus relying on the Misaka Network, the Network of the same sisters he killed over and over. He also has his own spin-off series named Toaru Kagaku no Accelerator(A certain scientific Accelerator) in which he is on his post-nerf self, which this mod is based on.

## Attributes

Accelerator has 2 modes, his nerf-mode in which he is slow and struggles to actually kill during lower percentages. And his Accelerated form which makes him faster, replaces some moves and can kill more easily.
V2564 Ophiuchi

V2564 Ophiuchi, Also Named **HD 165195**, is Either an Yellow-White Main Sequence Stars or an Metal-Poor Stars in The Constellation Ophiuchus, The Star is Located at 2,269 Light Years Away From Earth

## Information

* Right Ascension: 18h 04m 40.0714s
* Declination: +03° 46' 44.717"
* Apparent Magnitude (V): +7.298

### F-type Main Sequence Star

* Mass: 1.367 Solar Masses
* Radius: 1.762 Solar Radius
* Luminosity: 4.549 Solar Luminosities
* Temperature: 6,337 Kelvin
* Spectral Type: F6V-F7V

### Metal-Poor Star

* Mass: 0.792-0.846 Solar Masses
* Radius: 19.27 Solar Radius
* Luminosity: 161 Solar Luminosities
* Temperature: 4,681 Kelvin
* Age: 13.2 Billion Years
* Spectral Type: CEMP-no or K3III
* Metallicity [Fe/H]: -3.26 dex

### Other Designations

V2564 Ophiuchi, HD 165195, HIP 88527, SAO 123093, BD +03° 3579, IRAS 18021+0346, TYC 438-437-1, 2MASS J18044008+0346450
V4646 Sagittarii

V4646 Sagittarii is a Red Supergiant Stars in The Quintuplet Cluster, The Star is Located at 27,294 Light Years Away From Earth

## Information

* Mass: 30-40 Solar Masses (31,425-41,900 Jupiter Masses; 9,988,830-13,318,440 Earth Masses; 59,654-79,539 Septillion Tonnes)
* Radius: 1,383-1,447 Solar Radius (1,926,081,972-2,015,213,748 km in Diameter; 6.43753-6.73544 AU; 1,912,689-2,093,809 Solar Areas or 2,645,248,887-3,029,741,623 Solar Volumes)
* Luminosity: 320,173-379,852 Solar Luminosities
* Temperature: 3,692-3,767 Kelvin (3,419-3,494 °C; 6,186-6,321 °F)
* Spectral Type: M2Ia-M3Ia
* Right Ascension: 17h 46m 15.104s
* Declination: -28° 49' 29.38"
* Apparent Magnitude (H): +11.829
* Apparent Magnitude (K): +9.616
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V4646 Sagittarii, qF 270N, MGM 5-5, GMM 5, LHO 115, 2MASS J17461510-2849293
V682 Cassiopeiae

Object type: M-type red giant star
Number of stars: 1
Total mass: 2.2-2.65 Solar Masses (2,305-2,776 Jupiter Masses; 732,514-882,347 Earth Masses; 4,375-5,269 Septillion Tonnes)
Distance from the sun: 8,110 ly

V682 Cassiopeiae, Also Named **IRAS 02351+5849**, is a Red Giant Stars in The Constellation Cassiopeia, The Star is Located at 8,110 Light Years Away From Earth

## Information

* Mass: 2.2-2.65 Solar Masses (2,305-2,776 Jupiter Masses; 732,514-882,347 Earth Masses; 4,375-5,269 Septillion Tonnes)
* Radius: 195-221 Solar Radius (271,573,380-307,783,164 km in Diameter; 0.90768-1.0287 AU; 38,025-48,841 Solar Areas or 7,414,875-10,793,861 Solar Volumes)
* Luminosity: 4,157-6,469 Solar Luminosities
* Temperature: 3,319-3,482 Kelvin (3,046-3,209 °C; 5,515-5,808 °F)
* Spectral Type: M4III-M5III
* Right Ascension: 02h 38m 55.6325s
* Declination: +59° 02' 08.709"
* Apparent Magnitude (V): +14.18
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

V682 Cassiopeiae, IRAS 02351+5849, 2MASS J02385563+5902088
Theta Delphini

Theta Delphini, Also Named **HD 196725** or **IRAS 20363+1308**, is a Orange Bright Giant Stars in The Constellation Delphinus, The Star is Located at 2,021 Light Years Away From Earth

The name HD 196725 derives directly from the fact that the star is the 196,725th stars in the Henry Draper catalogue, and The name HR 7892 derives directly from the fact that the star in the 7,892nd stars in the Bright Star catalogue

The name HIP 101882 derives directly from the fact that the star is the 101,882nd stars in the Hipparcos catalogue, and The name SAO 106342 derives directly from the fact that the star is the 106,342nd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 6.93-8.44 Solar Masses
* Radius: 103-121 Solar Radius
* Luminosity: 4,240-6,700 Solar Luminosities
* Temperature: 4,589-4,747 Kelvin (4,316-4,474 °C; 7,801-8,085 °F)
* Spectral Type: K3-5Ib-II
* Right Ascension: 20h 38m 43.9865s
* Declination: +13° 18' 54.455"
* Apparent Magnitude (V): +5.71

### Other Designations

Theta Delphini, 8 Delphini, HD 196725, HR 7892, HIP 101882, SAO 106342, BD +12° 4411, IRAS 20363+1308, IRC +10474, TYC 1100-1721-1, 2MASS J20384399+1318544
V373 Cassiopeiae

V373 Cassiopeiae, Also Named **HD 224151**, **BD +56° 3115** or **IRAS 23530+5707**, is a Blue Supergiant Stars in The Constellation Cassiopeia, The Star is Located at 6,848 Light Years Away From Earth

The name HD 224151 derives directly from the fact that the star is the 224,151st stars in the Henry Draper catalogue, and The name HR 9052 derives directly from the fact that the star in the 9,052nd stars in the Bright Star catalogue

The name HIP 117957 derives directly from the fact that the star is the 117,957th stars in the Hipparcos catalogue, and The name SAO 35899 derives directly from the fact that the star is the 35,899th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 23.62 Solar Masses (24,742 Jupiter Masses; 7,864,539 Earth Masses; 46,968 Septillion Tonnes)
* Radius: 14.09 Solar Radius (19,622,918 km in Diameter; 0.06559 AU; 199 Solar Areas or 2,797 Solar Volumes)
* Luminosity: 85,028 Solar Luminosities
* Temperature: 26,258 Kelvin (25,985 °C; 46,805 °F)
* Spectral Type: B0Ib-II
* Right Ascension: 23h 55m 33.8387s
* Declination: +57° 24' 43.807"
* Apparent Magnitude (V): +5.9993

### Other Designations

V373 Cassiopeiae, HD 224151, HR 9052, HIP 117957, SAO 35899, BD +56° 3115, IRAS 23530+5707, TYC 4009-987-1, 2MASS J23553386+5724437
WY Velorum

WY Velorum, Also Named **HD 81137**, is a Red Hypergiant Stars in The Constellation Vela, The Star is Located at 7,600 Light Years Away From Earth

## Information

* Mass: 36-45 Solar Masses
* Radius: 2,028 Solar Radius
* Luminosity: 350,000-480,000 Solar Luminosities
* Temperature: 3,125-3,375 Kelvin
* Spectral Type: M7Ia+
* Right Ascension: 09h 21m 59.1346s
* Declination: -52° 33' 51.642"
* Apparent Magnitude (V): +8.81
* Variable Star Type: Semi Regular Variable Star

### Other Designations

WY Velorum, HD 81137, SAO 236888, CD -52° 3010, CP -52° 2262, IRAS 09203-5220, TYC 8584-2732-1, 2MASS J09215913-5233514
Variable Star

An Variable Star is a Star Whose Brightness as Seen From Earth Changes With Time

This variation May be caused by a change in emitted light or by something partly blocking the light, so variable stars are classified as either:

* Intrinsic variables, whose luminosity actually changes; for example, because the star periodically swells and shrinks
* Extrinsic variables, whose apparent changes in brightness are due to changes in the amount of their light that can reach Earth; for example, because the star has an orbiting companion that sometimes eclipses it

## List of Prototype Variable Stars

This is List of Prototype Variable Stars, The Star's Brightness Changes With Time
V5455 Sagittarii

Object type: M-type red giant star
Number of stars: 1
Total mass: 2.25-2.65 Solar Masses (2,357-2,776 Jupiter Masses; 749,162-882,347 Earth Masses; 4,474-5,269 Septillion Tonnes)
Distance from the sun: ~13,200 ly

V5455 Sagittarii is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 13,200 Light Years Away From Earth

## Information

* Mass: 2.25-2.65 Solar Masses (2,357-2,776 Jupiter Masses; 749,162-882,347 Earth Masses; 4,474-5,269 Septillion Tonnes)
* Radius: 195-230 Solar Radius (271,573,380-320,317,320 km in Diameter; 0.90768-1.07059 AU; 38,025-52,900 Solar Areas or 7,414,875-12,167,000 Solar Volumes)
* Luminosity: 3,571-5,792 Solar Luminosities
* Temperature: 3,195-3,320 Kelvin (2,922-3,047 °C; 5,291-5,516 °F)
* Spectral Type: M5III-M6III
* Right Ascension: 18h 03m 25.0102s
* Declination: -30° 08' 48.888"
* Apparent Magnitude (H): +10.958
* Apparent Magnitude (K): +10.697
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

V5455 Sagittarii, 2MASS J18032501-3008488
Spongebob Squarepants: Employee of The Month

SpongeBob SquarePants: Employee of the Month is a 2002 point-and-click adventure video game developed by AWE Games and published by THQ for PC. It is based on the television show SpongeBob SquarePants, which premiered on Nickelodeon in 1999. Wikipedia

Initial release date: September 22, 2002

Genre: Adventure game

Publisher: THQ

Mode: Single-player video game

Developers: THQ, AWE Games

Platform: Microsoft Windows
V2392 Ophiuchi

V2392 Ophiuchi, Also Named **HD 167654** or **IRAS 18135+0221**, is a Red Giant Stars in The Constellation Ophiuchus, The Star is Located at 788 Light Years Away From Earth

## Information

* Mass: 1.093 Solar Masses
* Radius: 96.27 Solar Radius
* Luminosity: 1,445 Solar Luminosities
* Temperature: 3,616 Kelvin (3,343 °C; 6,049 °F)
* Age: 9.3 Billion Years
* Spectral Type: M4III
* Metallicity [Fe/H]: -0.02 dex
* Right Ascension: 18h 16m 05.5723s
* Declination: +02° 22' 39.062"
* Apparent Magnitude (V): +6.01
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V2392 Ophiuchi, HD 167654, HR 6834, HIP 89527, SAO 123308, BD +02° 3547, IRAS 18135+0221, IRC +00343, TYC 436-3049-1, 2MASS J18160557+0222393
Unurgunite

Unurgunite, Also Named **Sigma Canis Majoris**, **HD 52877** or **Collinder 121 GDPR 28**, is a Orange-Red Supergiant Stars in The Constellation Canis Major, The Star is Located at 1,621 Light Years Away From Earth

## Information

* Right Ascension: 07h 01m 43.1478s
* Declination: -27° 56' 05.389"
* Apparent Magnitude (V): +3.47 (+3.43 to +3.51)
* Variable Star Type: Slow Irregular Variable Star

### Hipparcos Satellites (2007)

* Mass: 17.13 Solar Masses
* Radius: 389 Solar Radius
* Luminosity: 50,000 Solar Luminosities
* Temperature: 4,375 Kelvin
* Spectral Type: K5Iab

### James Webb Space Telescope (2022)

* Mass: 15.47 Solar Masses
* Radius: 436 Solar Radius
* Luminosity: 43,600 Solar Luminosities
* Temperature: 3,992 Kelvin
* Spectral Type: M0Iab-Ib

### Other Designations

Unurgunite, Sigma Canis Majoris, 22 Canis Majoris, HD 52877, HR 2646, HIP 33856, SAO 172797, CD -27° 3544, CP -27° 1648, IRAS 06597-2751, IRC -30072, Collinder 121 GDPR 28, TYC 6531-3793-1, 2MASS J07014314-2756051
Theta Carinae

Object type: Blue dwarf star
Number of stars: 1
Total mass: 16.22 Solar Masses (16,990 Jupiter Masses; 5,400,627 Earth Masses; 32,253 Septillion Tonnes)
Distance from the sun: 486 ly

Theta Carinae, Also Named **HD 93030**, **CP -63° 1599** or **IRAS 10411-6407**, is a Blue Main Sequence Stars in The Constellation Carina, The Star is Located at 486 Light Years Away From Earth

The name HD 93030 derives directly from the fact that the star is the 93,030th stars in the Henry Draper catalogue, and The name HR 4199 derives directly from the fact that the star in the 4,199th stars in the Bright Star catalogue

The name HIP 52419 derives directly from the fact that the star is the 52,419th stars in the Hipparcos catalogue, and The name SAO 251083 derives directly from the fact that the star is the 251,083rd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 16.22 Solar Masses (16,990 Jupiter Masses; 5,400,627 Earth Masses; 32,253 Septillion Tonnes)
* Radius: 6.73 Solar Radius (9,372,763 km in Diameter; 0.03133 AU; 45.29 Solar Areas or 304.82 Solar Volumes)
* Luminosity: 27,067 Solar Luminosities
* Temperature: 28,538 Kelvin (28,265 °C; 50,909 °F)
* Spectral Type: B0V
* Right Ascension: 10h 42m 57.4019674s
* Declination: -64° 23' 40.020796"
* Apparent Magnitude (V): +2.76

### Other Designations

Theta Carinae, HD 93030, HR 4199, HIP 52419, SAO 251083, CP -63° 1599, IRAS 10411-6407, TYC 8965-1765-1, IC 2602 GDPR 37, 2MASS J10425739-6423400
IRAS 04553-6825

WOH G64, Also Named **IRAS 04553-6825**, is a Red Hypergiant Stars in The Large Magellanic Cloud, The Star is Located at Around 163,000 Light Years Away From Earth

## Information

* Mass: 35-45 Solar Masses (36,663-47,138 Jupiter Masses; 11,653,635-14,983,245 Earth Masses; 69,596-89,481 Septillion Tonnes)
* Radius: 1,540-2,575 Solar Radius (2,144,733,360-3,586,161,300 km in Diameter; 7.16833-11.986 AU; 2,371,600-6,630,625 Solar Areas or 3,652,264,000-17,073,859,375 Solar Volumes)
* Luminosity: 210,400-752,500 Solar Luminosities
* Temperature: 3,150-3,350 Kelvin (2,877-3,077 °C; 5,210-5,570 °F)
* Spectral Type: M5Ia+-M6Ia+
* Right Ascension: 04h 55m 10.5236s
* Declination: -68° 20' 30.019"
* Apparent Magnitude (V): +18.46
* Variable Star Type: Semi-Regular Variable Star or Mira Variable Star

### Other Designations

WOH G64, IRAS 04553-6825, OGLE-LMC-LPV-6819, 2MASS J04551048-6820298
Timeline of a 1.25 Solar Masses Stars

This is Timeline of a 1.25 Solar Masses Stars, The Star Have 4 Planets

## Information

* Initial Radius: 1.182 Solar Radius
* Initial Luminosity: 2.022 Solar Luminosities
* Initial Temperature: 6,320 Kelvin
* Initial Spectral Type: F7V
* Metallicity [Fe/H]: -0.02 dex
* Initial Habitable Zone: 1.31 AU - 2.28 AU

(Note: \* = Star With Dyson Sphere, MB\* = Star With Matrioshka Brain)

## Planet Information

* Planet A: 0.27 Earth Radius, 0.073 Earth Masses, 0.08 AU, Lava Planet
* Planet B: 0.44 Earth Radius, 0.226 Earth Masses, 0.54 AU, Rocky Planet
* Planet C: 0.92 Earth Radius, 1.267 Earth Masses, 1.56 AU, Ocean Planet
* Planet D: 1.28 Earth Radius, 1.432 Earth Masses, 2.14 AU, Terrestrial Planet
Timeline of a 144 Solar Masses Stars

This is Timeline of a 144 Solar Masses Stars, The Star Doesn't Have Planets, and The Star was Named **HD 269810**, hence this, The Star was Located at The Large Magellanic Cloud

## Information

* Initial Radius: 20.93 Solar Radius
* Luminosity: 2,313,000 Solar Luminosities
* Initial Temperature: 49,200 Kelvin
* Spectral Type: O5III
* Estimated Metallicity [Fe/H]: -1.5 dex
* Habitable Zone: Disabled
V1888 Cygni

V1888 Cygni is a Cold Red Giant Stars in The Constellation Cygnus, The Star is Located at 7,244 Light Years Away From Earth

## Information

* Mass: 1.085-1.194 Solar Masses (1,137-1,251 Jupiter Masses; 361,263-397,555 Earth Masses; 2,157-2,374 Septillion Tonnes)
* Radius: 592-640 Solar Radius (824,468,928-891,317,760 km in Diameter; 2.75562-2.97905 AU; 350,464-409,600 Solar Areas or 207,474,688-262,144,000 Solar Volumes)
* Luminosity: 12,177-17,126 Solar Luminosities
* Temperature: 2,492-2,610 Kelvin (2,219-2,337 °C; 4,026-4,238 °F)
* Spectral Type: C8,5-C9,7 or M9III-M10III
* Right Ascension: 20h 56m 53.4236s
* Declination: +37° 25' 10.554"
* Variable Star Type: Mira Variable Star
* Evolutionary Stage: Asymptotic Giant Branch

### Other Designations

V1888 Cygni, RAFGL 2679, 2MASS J20565341+3725105
V1361 Sagittarii

Object type: M-type red giant star
Number of stars: 1
Total mass: 2.88-3.24 Solar Masses (3,017-3,394 Jupiter Masses; 958,928-1,078,794 Earth Masses; 5,727-6,443 Septillion Tonnes)
Distance from the sun: ~60,000 ly

V1361 Sagittarii is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 60,000 Light Years Away From Earth

## Information

* Mass: 2.88-3.24 Solar Masses (3,017-3,394 Jupiter Masses; 958,928-1,078,794 Earth Masses; 5,727-6,443 Septillion Tonnes)
* Radius: 189-210 Solar Radius (263,217,276-292,463,640 km in Diameter; 0.87975-0.9775 AU; 35,721-44,100 Solar Areas or 6,751,269-9,261,000 Solar Volumes)
* Luminosity: 4,986-6,748 Solar Luminosities
* Temperature: 3,528-3,610 Kelvin (3,255-3,337 °C; 5,891-6,038 °F)
* Spectral Type: M3IIIe-M4IIIe
* Right Ascension: 18h 02m 36.2347s
* Declination: -29° 47' 37.191"
* Apparent Magnitude (V): +16.045
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

V1361 Sagittarii, 2MASS J18023623-2947371
Mu Sonne

Mu Sonne is a Blue Ultragiant Stars That Doesn't Exist in The Universe, If The Star is Located at 30,000 Light Years Away From Earth, That The Star Will Collapse Into an Large Black Hole and Producing an Devastating Gamma-Ray Burst

## Information

* Mass: 64,192 Solar Masses (67,241,120 Jupiter Masses; 21,373,432,512 Earth Masses; 127,643,866 Septillion Tonnes)
* Radius: 12,800 Solar Radius (17,826,355,200 km in Diameter; 59.58091 AU; 163,840,000 Solar Areas or 2,097,152,000,000 Solar Volumes)
* Luminosity: 957 Billion Solar Luminosities
* Temperature: 50,462 Kelvin (50,189 °C; 90,372 °F)
* Spectral Type: O4Ia3-4

## See Also

* Shadron Soul
* Cheese Star
* R136a1
* V4998 Sagittarii
* Eta Carinae
V4393 Sagittarii

V4393 Sagittarii, Also Named **HD 168988**, **BD -20° 5118**, **CP -20° 7007** or **IRAS 18203-2040**, is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at 4,908 Light Years Away From Earth

The name HD 168988 derives directly from the fact that the star is the 168,988th stars in the Henry Draper catalogue, however, the star doesn't have HR numbers, because the star is too faint to visible by naked eye

The name HIP 90113 derives directly from the fact that the star is the 90,113th stars in the Hipparcos catalogue, and The name SAO 186750 derives directly from the fact that the star is the 186,750th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 3.853-4.164 Solar Masses (4,036-4,362 Jupiter Masses; 1,282,899-1,386,450 Earth Masses; 7,662-8,280 Septillion Tonnes)
* Radius: 59.41-67.83 Solar Radius (82,739,356-94,465,756 km in Diameter; 0.27654-0.31573 AU; 3,530-4,601 Solar Areas or 209,690-312,080 Solar Volumes)
* Luminosity: 753-1,181 Solar Luminosities
* Temperature: 3,922-4,108 Kelvin (3,649-3,835 °C; 6,600-6,935 °F)
* Spectral Type: K9III-M0III
* Right Ascension: 18h 23m 19.9271s
* Declination: -20° 39' 13.091"
* Apparent Magnitude (V): +7.68
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V4393 Sagittarius, HD 168988, HIP 90113, SAO 186750, BD -20° 5118, CP -20° 7007, IRAS 18203-2040, IRC -20471, TYC 6277-1745-1, 2MASS J18231992-2039132
V916 Orionis

Object type: Blue dwarf star
Number of stars: 1
Total mass: 10.488 Solar Masses (10,986 Jupiter Masses; 3,492,095 Earth Masses; 20,855 Septillion Tonnes)
Distance from the sun: ~3,600 ly

V916 Orionis, Also Named **HD 252214** or **BD +13° 1120**, is a Blue Main Sequence Stars in The Open Cluster NGC 2169, The Star is Located at Around 3,600 Light Years Away From Earth

The name HD 252214 derives directly from the fact that the star is the 252,214th stars in the Henry Draper catalogue, however, the star doesn't have HR numbers

The name HIP 29106 derives directly from the fact that the star is the 29,106th stars in the Hipparcos catalogue, and The name SAO 95271 derives directly from the fact that the star is the 95,271st stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 10.488 Solar Masses (10,986 Jupiter Masses; 3,492,095 Earth Masses; 20,855 Septillion Tonnes)
* Radius: 7.119 Solar Radius (9,914,517 km in Diameter; 0.03314 AU; 51 Solar Areas or 361 Solar Volumes)
* Luminosity: 11,490 Solar Luminosities
* Temperature: 22,396 Kelvin (22,123 °C; 39,853 °F)
* Spectral Type: B3V
* Right Ascension: 06h 08m 18.1091s
* Declination: +13° 58' 17.515"
* Apparent Magnitude (V): +8.176
* Variable Star Type: Beta Cephei Variable Star

### Other Designations

V916 Orionis, HD 252214, HIP 29106, SAO 95271, BD +13° 1120, NGC 2169 GDPR 2, TYC 742-1935-1, 2MASS J06081811+1358173
V4400 Sagittarii

Object type: Blue dwarf star
Number of stars: 1
Total mass: 10.373 Solar Masses (10,866 Jupiter Masses; 3,453,804 Earth Masses; 20,626 Septillion Tonnes)
Distance from the sun: 3,359 ly

V4400 Sagittarii, Also Named **HD 171348**, **BD -22° 4490**, **CD -22° 13117** or **CP -22° 7084**, is a Blue Main Sequence Stars in The Constellation Sagittarius, The Star is Located at 3,359 Light Years Away From Earth

The name HD 171348 derives directly from the fact that the star is the 171,348th stars in the Henry Draper catalogue, however, the star doesn't have HR numbers, because the star is too faint to visible by naked eye

The name HIP 91130 derives directly from the fact that the star is the 91,130th stars in the Hipparcos catalogue, and The name SAO 187010 derives directly from the fact that the star is the 187,010th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 10.373 Solar Masses (10,866 Jupiter Masses; 3,453,804 Earth Masses; 20,626 Septillion Tonnes)
* Radius: 5.922 Solar Radius (8,247,475 km in Diameter; 0.02757 AU; 35.07 Solar Areas or 207.69 Solar Volumes)
* Luminosity: 7,529 Solar Luminosities
* Temperature: 22,094 Kelvin (21,821 °C; 39,310 °F)
* Spectral Type: B2V
* Right Ascension: 18h 35m 20.4719s
* Declination: -22° 05' 27.374"
* Apparent Magnitude (V): +8
* Variable Star Type: Beta Cephei Variable Star

### Other Designations

V4400 Sagittarii, HD 171348, HIP 91130, SAO 187010, BD -22° 4490, CD -22° 13117, CP -22° 7084, Hen 3-1713, TYC 6279-380-1, 2MASS J18352047-2205274
V4030 Sagittarii

V4030 Sagittarii, Also Named **HD 168625**, **BD -16° 4830** or **IRAS 18184-1623**, is a Blue Hypergiant Stars in The Constellation Sagittarius, The Star is Located at 8,776 Light Years Away From Earth

The name HD 168625 derives directly from the fact that the star is the 168,625th stars in the Henry Draper catalogue, however, the star doesn't have HR numbers, because the star is too faint to visible by naked eye

The name HIP 89963 derives directly from the fact that the star is the 89,963rd stars in the Hipparcos catalogue, and The name SAO 161375 derives directly from the fact that the star is the 161,375th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 70-85 Solar Masses (73,325-89,038 Jupiter Masses; 23,307,270-28,301,685 Earth Masses; 139,193-169,020 Septillion Tonnes)
* Radius: 163-186 Solar Radius (227,007,492-259,039,224 km in Diameter; 0.75873-0.86579 AU; 26,569-34,596 Solar Areas or 4,330,747-6,434,856 Solar Volumes)
* Luminosity: 654,000-1,211,800 Solar Luminosities
* Temperature: 12,857-14,042 Kelvin (12,584-13,769 °C; 22,683-24,816 °F)
* Spectral Type: B7Ia+-B8Ia+ or B6Iaeq-B7Iaeq
* Right Ascension: 18h 21m 19.5484s
* Declination: -16° 22' 26.075"
* Apparent Magnitude (V): +8.37
* Variable Star Type: Luminous Blue Variable Star

### Other Designations

V4030 Sagittarii, HD 168625, HIP 89963, SAO 161375, BD -16° 4830, IRAS 18184-1623, TYC 6265-1959-1, Hen 3-1681, 2MASS J18211955-1622260
V346 Puppis

Object type: Mira variable star
Number of stars: 1
Total mass: 12-18 Solar Masses (12,570-18,855 Jupiter Masses; 3,995,532-5,993,298 Earth Masses; 23,862-35,792 Septillion Tonnes)
Distance from the sun: ~3,325 ly

V346 Puppis, Also Named **IRAS 08088-3243**, is a Carbon-Rich Red Supergiant Stars in The Constellation Puppis, The Star is Located at 3,325 Light Years Away From Earth

## Information

* Mass: 12-18 Solar Masses (12,570-18,855 Jupiter Masses; 3,995,532-5,993,298 Earth Masses; 23,862-35,792 Septillion Tonnes)
* Radius: 990-1,080 Solar Radius (1,378,757,160-1,504,098,720 km in Diameter; 4.60821-5.02714 AU; 980,100-1,166,400 Solar Areas or 970,299,000-1,259,712,000 Solar Volumes)
* Luminosity: 61,260-98,072 Solar Luminosities
* Temperature: 2,886-3,108 Kelvin (2,613-2,835 °C; 4,735-5,135 °F)
* Spectral Type: C4,6-C5,5 or M6-8Iab-Ib
* Right Ascension: 08h 10m 48.885s
* Declination: -32° 52' 05.635"
* Apparent Magnitude (H): +5.246
* Apparent Magnitude (K): +3.24
* Variable Star Type: Mira Variable Star or Semi-Regular Variable Star

### Other Designations

V346 Puppis, IRAS 08088-3243, RAFGL 1235, 2MASS J08104890-3252055
Timeline of a R-type Stars

This is Timeline of a R-type Stars, The Star Have Only a Planets, Also, The Star is a Extremely Metal-Poor Stars and The Star's Mass is 0.99 Solar Masses

## Star Information

* Initial Radius: 0.792 Solar Radius
* Initial Temperature: 7,240 Kelvin
* Initial Luminosities: 1.59 Solar Luminosities
* Initial Spectral type: sdF3 or CEMP-no
* Initial Habitable Zone: 1.22 AU - 1.68 AU
* Metallicity [Fe/H]: -3.27 dex

## Planet Information

* Planet A: 2.21 AU, 1.54 Jupiter Radius, 21.86 Jupiter Masses, Hot Jupiter/Brown Dwarf
	+ Moons of The Planet: 0.09 AU, 0.63 Earth Radius, 0.18 Earth Masses, Rocky Planet
Timeline of a 74 solar mass star

This is the Timeline of a 74 Solar mass star. The star is located in the Caldwell 45 galaxy and does not have planets at first but then destroys a 22 jupiter masses brown dwarf and forms planets.

## Details

* Mass: 74 Suns
* Radius: 12.75 Suns
* Spectral Type: O4.5V
* Temperature: 42000 Kelvins
* Luminosity: 950000 Suns
Westerlund 1-75

Westerlund 1-75 is a Red Supergiant Stars in The Star Cluster Westerlund 1, The Star is Located at Around 25,000 Light Years Away From Earth

## Information

* Mass: 22-32 Solar Masses (23,045-33,520 Jupiter Masses; 7,325,142-10,654,752 Earth Masses; 43,746-63,631 Septillion Tonnes)
* Radius: 966-1,093 Solar Radius (1,345,332,744-1,522,203,612 km in Diameter; 4.4965-5.08765 AU; 933,156-1,194,649 Solar Areas or 901,428,696-1,305,751,357 Solar Volumes)
* Luminosity: 140,000-203,500 Solar Luminosities
* Temperature: 3,592-3,708 Kelvin (3,319-3,435 °C; 6,006-6,215 °F)
* Spectral Type: M3Iab-M4Iab
* Right Ascension: 16h 47m 08.9198s
* Declination: -45° 49' 58.452"
* Apparent Magnitude (V): +16.6989
* Variable Star Type: Semi-Regular Variable Star
Vermeer 1581

Object type: Open cluster
Number of stars: 871
Total mass: 1,061 Solar Masses (1,111,398 Jupiter Masses; 353,271,621 Earth Masses; 2,109,767 Septillion Tonnes)
Distance from the sun: 17,867 ly

Vermeer 1581 is a Galactic Juvenile Detention Center in The Constellation Canis Minor, The Open Cluster is Located at 17,867 Light Years Away From Earth

The Galactic Juvenile Detention Center was Located at The Interstellar Federation of Normarsk, Containing 84,149 Juvenile Offenders

## Information

* Type: Open Cluster
* Diameter: 9.31 Light Years
* Age: 6.1 Billion Years, 3.7 Billion Years, 2.4 Billion Years
* Average Metallicity [Fe/H]: -0.36 dex
* Estimated Value: 46,897,094 CR
* Total Population: 1,982,890
* Juvenile Prisoner: 84,149

### List of Stars in The Galactic Juvenile Detention Center

This is List of Stars in This Galactic Juvenile Detention Center, The Galactic Juvenile Detention Center Contains 871 Stars, Including 43 Blue Straggler Stars
V2025 Sagittarii

Object type: Mira variable star
Number of stars: 1
Total mass: 1.5-4 Solar Masses (1,571-4,190 Jupiter Masses; 499,442-1,331,844 Earth Masses; 2,983-7,954 Septillion Tonnes)
Distance from the sun: ~11,300 ly

V2025 Sagittarii, Also Named **IRAS 18381-2404**, is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 11,300 Light Years Away From Earth

If V2025 Sagittarii was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, and even Mars, Because V2025 Sagittarii's size was 399 to 442 times large as the sun

## Information

* Mass: 1.5-4 Solar Masses (1,571-4,190 Jupiter Masses; 499,442-1,331,844 Earth Masses; 2,983-7,954 Septillion Tonnes)
* Radius: 399-442 Solar Radius (555,680,916-615,566,328 km in Diameter; 1.85725-2.0574 AU; 159,201-195,364 Solar Areas or 63,521,199-86,350,888 Solar Volumes)
* Luminosity: 12,429-17,841 Solar Luminosities
* Temperature: 3,051-3,173 Kelvin (2,778-2,900 °C; 5,032-5,252 °F)
* Spectral Type: M6IIIe-M7IIIe
* Right Ascension: 18h 41m 14.1998s
* Declination: -24° 02' 01.887"
* Apparent Magnitude (H): +6.619
* Apparent Magnitude (K): +5.98
* Variable Star Type: Mira Variable Star

### Other Designations

V2025 Sagittarii, IRAS 18381-2404, 2MASS J18411420-2402018
Staff of the Gatekeeper

## Recipe

The Staff of The Gatekeeper is the final Staff of Rending and the direct upgrade of the Omothol Staff of Rending, dealing more damage and thus sapping faster than its Omothol counterpart. Like other Staves of Rending, it is used to extract Dimensional Essences or Shadow Gems from Abyssalcraft mobs. The Staff of The Gatekeeper also acts as the Gateway Keys (Gateway Key, Asorah's Dreaded Gateway Key, Cha'garoth's R'lyehian Gateway Key), allowing the creation of portals to travel between Abyssalcraft Dimensions.

## Sources:

The Staff of Rending is crafted using 1 Shard of Oblivion and 4 Shadow Gem Shards.

## Uses:

### Portal Generation:

* Overworld <-(Alt)- --> Abyssal Wasteland <-(Alt)- --> Dreadlands <---> Omothol <-- Dark Realm

### Sapping:

* Abyssal Wasteland Essence - Coralium Enemies in Abyssal Wasteland
* Dreadlands Essence - Dread Enemies in Dreadlands
* Omothol Essence - Minions of the Gatekeeper in Omothol
* Shadow Gems - Living Shadows

## Enchantments:

* **Sapping (I-IV):** Staff of Rending deals additional damage, sapping energy more quickly and acting as a better weapon. Level IV is obtained using an Ancient Tome.
* **Multi-Rend:** Staff of Rending damages in an area of effect, sapping energy from all mobs damaged.
Z Doradus

Z Doradus is a Red Supergiant Stars in The Large Magellanic Cloud, The Star is Located at Around 163,000 Light Years Away From Earth

## Information

* Mass: 25 Solar Masses
* Radius: 896-1,032 Solar Radius
* Luminosity: 148,900-224,700 Solar Luminosities
* Temperature: 3,788-3,912 Kelvin (3,515-3,639 °C; 6,359-6,582 °F)
* Spectral Type: M1Iab-M2Iab
* Right Ascension: 05h 38m 16.0018s
* Declination: -69° 10' 11.237"
* Apparent Magnitude (V): +15.037
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

Z Doradus, HV 2740, LMC 170452, 2MASS J05381601-6910112
Wolf 359

Wolf 359 is a Red Dwarf Stars in The Constellation Leo, The Star is Located at 7.7923 Light Years Away From Earth

## Information

* Mass: 0.1163 Solar Masses
* Radius: 0.1429 Solar Radius
* Luminosity: 0.096% Solar Luminosities
* Temperature: 2,685 Kelvin
* Spectral Type: M8V-M9V

### Other Designations

RS 8631-1357-8-17293316-3, Wolf 359, Gliese 406, CN Leonis, 2MASS J10562886+0700527
Zeta Equulei

Object type: Orange bright giant star
Number of stars: 1
Total mass: 5.491-6.037 Solar Masses (5,752-6,324 Jupiter Masses; 1,828,289-2,010,086 Earth Masses; 10,919-12,004 Septillion Tonnes)
Distance from the sun: 1,247 ly

Zeta Equulei, Also Named **HD 200644**, **HR 8066**, **BD +04° 4606** or **IRAS 21020+0518**, is a Orange Bright Giant Stars in The Constellation Equuleus, The Star is Located at 1,247 Light Years Away From Earth

The name HD 200644 derives directly from the fact that the star is the 200,644th stars in the Henry Draper catalogue, and The name HR 8066 derives directly from the fact that the star in the 8,066th stars in the Bright Star catalogue

The name HIP 104031 derives directly from the fact that the star is the 104,031st stars in the Hipparcos catalogue, and The name SAO 126518 derives directly from the fact that the star is the 126,518th stars in the Smithsonian Astrophysical Star catalogue

If Zeta Equulei was placed into center of the solar system, that It's will engulf Mercury, Because Zeta Equulei's size was 84 to 97 times large as the sun

## Information

* Mass: 5.491-6.037 Solar Masses (5,752-6,324 Jupiter Masses; 1,828,289-2,010,086 Earth Masses; 10,919-12,004 Septillion Tonnes)
* Radius: 84.87-97.28 Solar Radius (118,197,091-135,480,300 km in Diameter; 0.39505-0.45281 AU; 7,203-9,463 Solar Areas or 611,312-920,599 Solar Volumes)
* Luminosity: 1,993-2,894 Solar Luminosities
* Temperature: 4,186-4,292 Kelvin (3,913-4,019 °C; 7,075-7,266 °F)
* Spectral Type: K6II-K7II
* Right Ascension: 21h 04m 34.6516s
* Declination: +05° 30' 10.312"
* Apparent Magnitude (V): +5.585
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

Zeta Equulei, 3 Equulei, HD 200644, HR 8066, HIP 104031, SAO 126518, BD +04° 4606, IRAS 21020+0518, TYC 534-2623-1, IRC +10485, 2MASS J21043465+0530104
V689 Cassiopeiae

Object type: Binary star
Number of stars: 2
Total mass: 4.892 Solar Masses (5,124 Jupiter Masses; 1,628,845 Earth Masses; 9,728 Septillion Tonnes)
Distance from the sun: 17,322 ly

V689 Cassiopeiae is a Binary Star System in The Constellation Cassiopeia, The Star System is Located at 17,322 Light Years Away From Earth

## Information

* Right Ascension: 02h 45m 44.7466s
* Declination: +60° 39' 28.609"
* Apparent Magnitude (V): +16.0998

### V689 Cassiopeiae A

* Mass: 3.109 Solar Masses (3,257 Jupiter Masses; 1,035,176 Earth Masses; 6,182 Septillion Tonnes)
* Radius: 5.252 Solar Radius (7,314,376 km in Diameter; 0.02445 AU; 27.58 Solar Areas or 144.87 Solar Volumes)
* Luminosity: 74.04 Solar Luminosities
* Temperature: 7,388 Kelvin (7,115 °C; 12,839 °F)
* Spectral Type: F0III-F1III

### V689 Cassiopeiae B

* Mass: 1.783 Solar Masses (1,868 Jupiter Masses; 593,669 Earth Masses; 3,545 Septillion Tonnes)
* Radius: 1.621 Solar Radius (2,257,541 km in Diameter; 0.00755 AU; 2.628 Solar Areas or 4.259 Solar Volumes)
* Luminosity: 11.91 Solar Luminosities
* Temperature: 8,419 Kelvin (8,146 °C; 14,695 °F)
* Spectral Type: A6V-A7V

### Other Designations

V689 Cassiopeiae, 2MASS J02454475+6039287
Timeline of a 1.1 Solar Masses Stars

This is Timeline of a 1.1 Solar Masses Stars, The Star Have 5 Planets

## Star Information

* Initial Radius: 1.03 Solar Radius
* Initial Temperature: 5,800 Kelvin
* Initial Luminosity: 1.08 Solar Luminosities
* Initial Spectral type: G2V
* Initial Habitable Zone: 0.96 AU - 1.38 AU

## Planet Information

* Planet A: 0.09 AU, 1.32 Jupiter Radius, 1.84 Jupiter Masses, Hot Jupiter
* Planet B: 0.78 AU, 6.39 Earth Radius, 57 Earth Masses, Gas Giant
* Planet C: 1.21 AU, 1.27 Earth Radius, 1.65 Earth Masses, Terrestrial Planet
* Planet D: 1.47 AU, 1.13 Earth Radius, 1.54 Earth Masses, Ocean Planet
* Planet E: 1.22 AU, 0.54 Earth Radius, 0.07 Earth Masses, Rocky Planet
Zeta Cephei

Zeta Cephei, Also Named **HD 210745**, **BD +57° 2475** or **IRAS 22091+5757**, is a Orange Supergiant Stars in The Constellation Cepheus, The Star is Located at 844 Light Years Away From Earth

The name HD 210745 derives directly from the fact that the star is the 210,745th stars in the Henry Draper catalogue, and The name HR 8465 derives directly from the fact that the star in the 8,465th stars in the Bright Star catalogue

The name HIP 109492 derives directly from the fact that the star is the 109,492nd stars in the Hipparcos catalogue, and The name SAO 34137 derives directly from the fact that the star is the 34,137th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 8.344-9.457 Solar Masses (8,740-9,906 Jupiter Masses; 2,778,227-3,148,812 Earth Masses; 16,592-18,805 Septillion Tonnes)
* Radius: 117-144 Solar Radius (162,944,028-200,546,496 km in Diameter; 0.54461-0.67029 AU; 13,689-20,736 Solar Areas or 1,601,613-2,985,984 Solar Volumes)
* Luminosity: 5,503-8,907 Solar Luminosities
* Temperature: 4,596-4,672 Kelvin (4,323-4,399 °C; 7,813-7,950 °F)
* Spectral Type: K3Ib-K4Ib
* Right Ascension: 22h 10m 51.2769159s
* Declination: +58° 12' 04.545587"
* Apparent Magnitude (V): +3.35

### Other Designations

Zeta Cephei, 21 Cephei, HD 210745, HR 8465, HIP 109492, SAO 34137, BD +57° 2475, IRAS 22091+5757, IRC +60344, TYC 3981-1590-1, 2MASS J22105129+5812041
Whirlpool Galaxy

The Whirlpool Galaxy (M51) is a spiral galaxy in the constellation Canes Venecati . She is a beautiful galaxy but also a vampire because she’s eating M51B a smaller seyfert 2 with a active core . M51B will be gone and become part of the whirlpool galaxy in the future and his M51B\* will merge with M51\* and cause a quasar or something.
Youth Criminal Justice Act Super Star Cluster Catalogue

The **Youth Criminal Justice Act Super Star Cluster Catalogue** is a Star Catalogue That Containing 4 Generations, The First Generation of The Star Catalogue Contains 706 Star Clusters, All of The Star Clusters are Super Star Clusters or Young Open Cluster

The Second Generation of The Star Catalogue Contains 18,953 Open Clusters in Galaxies Within 150 Million Light Years, Most of Open Clusters in This Generation was Massive and Young

The Third Generation of The Star Catalogue Contains 8,589 Globular Clusters in Galaxies Within 25 Million Light Years, and The Fourth Generation of The Star Contains 76,389 Globular Clusters in Galaxies Within 750 Million Light Years

This Star Catalogue is Named After Youth Criminal Justice Act, The Canadian Juvenile Law, Setting Minimum Age of Criminal Responsibility in Canada to 12 Years

to Prevent Override Names of Stars and Star Clusters, The Star Catalogue Has Added The "YCJA N-NN-SC" to Represent Star Clusters

## Notable Stars in These Star Clusters

* YCJA 184-7, an Blue Supergiant Star in The Triangulum Galaxy
* YCJA 93-1, Also Named V2244 Slovakia, an Luminous Blue Variable Star in The Andromeda Galaxy
* YCJA 53-9, an Red Supergiant Star in The Triangulum Galaxy
* YCJA 497-26, Also Named Westerlund 1-26, an Red Hypergiant Star in The Super Star Cluster Westerlund 1
* YCJA 349-2, Also Named Westerhout 49-2, an Blue Supergiant Star in The Open Cluster Westerhout 49
* YCJA 2-13-SC, an Super Star Cluster in The Spiral Galaxy NGC 6946
* YCJA 2-13, Also Named Stephenson 2 DFK 13, an Red Supergiant Star in The Open Cluster Stephenson 2
* YCJA 4-1898, an Globular Cluster in The Elliptical Galaxy Messier 87

### Format

* Star Names: YCJA NNN-NNN, YCJA {2}-NNNNN-NNN, YCJA {3}-NNNN-NNNNN, YCJA {4}-NNNNN-NNNNN
* Star Cluster Names: YCJA NNN, YCJA {2}-NNNNN or YCJA {2}-NNN-SC (If An Star's Name Exist), YCJA {3}-NNNN or YCJA {3}-NNN-SC (If An Star's Name Exist), YCJA {4}-NNNNN or YCJA {4}-NNN-SC (If An Star's Name Exist)

## See Also

* Romania High-Mass Star Catalogue
* R136a1
* Westerhout 49-2

### Trivia

in the children's television series Odyssey (also name Enceladus), the minimum age of criminal responsibility in Canada was 16 years instead of 12 years
Zeta Apodis

Zeta Apodis, Also Named **HD 156277**, **CP -67° 3310** or **IRAS 17167-6743**, is a Red Giant Stars in The Constellation Apus, The Star is Located at 296 Light Years Away From Earth

The name HD 156277 derives directly from the fact that the star is the 156,277th stars in the Henry Draper catalogue, and The name HR 6417 derives directly from the fact that the star in the 6,417th stars in the Bright Star catalogue

The name HIP 84969 derives directly from the fact that the star is the 84,969th stars in the Hipparcos catalogue, and The name SAO 253882 derives directly from the fact that the star is the 253,882nd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 2.385 Solar Masses (2,498 Jupiter Masses; 794,112 Earth Masses; 4,743 Septillion Tonnes)
* Radius: 24.09 Solar Radius (33,549,758 km in Diameter; 0.11213 AU; 580 Solar Areas or 13,980 Solar Volumes)
* Luminosity: 211 Solar Luminosities
* Temperature: 4,481 Kelvin (4,208 °C; 7,606 °F)
* Spectral Type: K5III-K6III
* Right Ascension: 17h 21m 59.4777s
* Declination: -67° 46' 14.408"
* Apparent Magnitude (V): +4.78

### Other Designations

Zeta Apodis, HD 156277, HR 6417, HIP 84969, SAO 253882, CP -67° 3310, IRAS 17167-6743, TYC 9276-1692-1, 2MASS J17215948-6746144