recursal/Fanatic-Fandom huggingface dataset:
Searthia

Searthia is a Habitable Terrestrial Planet From The Film and Video Games *Serbia's Guide to the Galaxy* (Same Name) and Serbia Space Program, Searthia is Fourth Planet in The Serbia Planetary System, and Orbiting The Parent Star Serbia

## Information

* Parent Star: Serbia
* Mass: 0.981 Earth Masses
* Radius: 1.073 Earth Radius
* Surface Temperature: 21 °C (70 °F)
* Life Appearence: 600,000,000 (+0.585 bnex)
* Earth Similarity Index: 0.936+0.008
-0.003
* Atmosphere Pressure: 1,080 hPa
* Atmosphere Composition: 77% of Nitrogen, 21% of Oxygen, 1.764% of Argon, 0.088% of Carbon Dioxide, 0.148% of Other Gases
* Age: 2.4 Billion Years
* Axial Tilt: 18.8°
* Semi-Major Axis: 1.13 AU (169,158,594 km)
* Orbit Period: 412 Days (384 Days in The Planet Searthia)
* Rotation Period: 25 Hours and 45 Minutes
* Number of Natural Satellites: 2

### Planetary Civilization Information

* Population: 11,200,000,000+600,000,000
-20,000,000
* Life Expectancy: 216+3
-2 Years (214+3
-2 Years for Male, 218+4
-2 Years for Female)
* Kardashev Scale: 1.617+0.004
-0.001
* Official Language: Serbian, Russian and English
U Persei

Object type: Mira variable star
Number of stars: 1
Total mass: 1-3 Solar Masses (1,048-3,143 Jupiter Masses; 332,961-998,883 Earth Masses; 1,988-5,965 Septillion Tonnes)
Distance from the sun: 1,593 ly

U Persei, Also Named **HD 12025**, **BD +54° 431** or **IRAS 01562+5434**, is a Red Giant Stars in The Constellation Perseus, The Star is Located at 1,593 Light Years Away From Earth

The name HD 12025 derives directly from the fact that the star is the 12,025th 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 9306 derives directly from the fact that the star is the 9,306th stars in the Hipparcos catalogue, and The name SAO 22817 derives directly from the fact that the star is the 22,817th stars in the Smithsonian Astrophysical Star catalogue

If U Persei was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, and even Mars, Because U Persei's size was 311 to 340 times large as the sun

## Information

* Mass: 1-3 Solar Masses (1,048-3,143 Jupiter Masses; 332,961-998,883 Earth Masses; 1,988-5,965 Septillion Tonnes)
* Radius: 311-340 Solar Radius (433,124,724-473,512,560 km in Diameter; 1.44763-1.58262 AU; 96,721-115,600 Solar Areas or 30,080,231-39,304,000 Solar Volumes)
* Luminosity: 6,844-11,030 Solar Luminosities
* Temperature: 2,977-3,208 Kelvin (2,704-2,935 °C; 4,899-5,315 °F)
* Spectral Type: M5III-M7III
* Right Ascension: 01h 59m 35.1223s
* Declination: +54° 49' 20.005"
* Apparent Magnitude (V): +8.76
* Variable Star Type: Mira Variable Star

### Other Designations

U Persei, HD 12025, HIP 9306, SAO 22817, BD +54° 431, IRAS 01562+5434, IRC +50050, TYC 3688-1392-1, 2MASS J01593514+5449199
HE 0336+0113

HE 0336+0113 is a Metal-Poor Stars in The Constellation Taurus, The Star is Located at 2,732 Light Years Away From Earth

## Information

* Mass: 0.741 Solar Masses (776 Jupiter Masses; 246,724 Earth Masses; 1,473 Septillion Tonnes)
* Radius: 0.948 Solar Radius (1,320,264 km in Diameter; 0.00441 AU; 0.8987 Solar Areas or 0.852 Solar Volumes)
* Luminosity: 93.73% Solar Luminosities
* Temperature: 5,833 Kelvin (5,560 °C; 10,040 °F)
* Age: 12.2 Billion Years
* Spectral Type: CEMP-s or G2V Fe-4
* Metallicity [Fe/H]: -2.64 dex
* Right Ascension: 03h 38m 52.9027s
* Declination: +01° 23' 07.778"
* Apparent Magnitude (V): +14.96
V403 Persei

V403 Persei, Also Named **HD 14580** or **BD +56° 597**, is a Red Supergiant Stars in The Open Cluster NGC 884, The Star is Located at 7,718 Light Years Away From Earth

The name HD 14580 derives directly from the fact that the star is the 84,810th stars in the Henry Draper catalogue, and The name SAO 23274 derives directly from the fact that the star is the 23,274th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 15.78-18.32 Solar Masses (16,530-19,190 Jupiter Masses; 5,254,125-6,099,846 Earth Masses; 31,378-36,429 Septillion Tonnes)
* Radius: 436-528 Solar Radius (607,210,224-735,337,152 km in Diameter; 2.02947-2.45771 AU; 190,096-278,784 Solar Areas or 82,881,856-147,197,952 Solar Volumes)
* Luminosity: 38,496-63,658 Solar Luminosities
* Temperature: 3,872-3,990 Kelvin (3,599-3,717 °C; 6,510-6,722 °F)
* Spectral Type: M0-1Iab-Ib
* Right Asecnsion: 02h 23m 24.1101s
* Declination: +57° 12' 43.045"
* Apparent Magnitude (V): +8.402
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V403 Persei, HD 14580, SAO 23274, BD +56° 597, IRC +60089, TYC 3694-1684-1, NGC 884 GDPR 2758, 2MASS J02232409+5712430
V366 Andromedae

V366 Andromedae, Also Named **HD 10465**, **BD +47° 485** or **IRAS 01400+4815**, is a Red Supergiant Stars in The Constellation Andromeda, The Star is Located at 6,873 Light Years Away From Earth

The name HD 10465 derives directly from the fact that the star is the 10,465th 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 8034 derives directly from the fact that the star is the 8,034th stars in the Hipparcos catalogue, and The name SAO 37456 derives directly from the fact that the star is the 37,456th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 25-30 Solar Masses (26,188-31,425 Jupiter Masses; 8,324,025-9,988,830 Earth Masses; 49,712-59,654 Septillion Tonnes)
* Radius: 1,057-1,133 Solar Radius (1,472,066,988-1,577,910,972 km in Diameter; 4.92008-5.27384 AU; 1,117,249-1,283,689 Solar Areas or 1,180,932,193-1,454,419,637 Solar Volumes)
* Luminosity: 187,000-245,000 Solar Luminosities
* Temperature: 3,692-3,816 Kelvin (3,419-3,543 °C; 6,186-6,409 °F)
* Spectral Type: M2Iab-M3Iab
* Right Ascension: 01h 43m 11.1064s
* Declination: +48° 31' 00.358"
* Apparent Magnitude (V): +6.79
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V366 Andromedae, HD 10465, HIP 8034, SAO 37456, BD +47° 485, IRAS 01400+4815, IRC +50043, TYC 3283-183-1, 2MASS J01431110+4831002
SMSS J175544.54-392700.9

SMSS J175544.54-392700.9 is a Very Metal-Poor Stars in The Constellation Scorpius, The Star is Located at Around 44,800 Light Years Away From Earth

## Information

* Mass: 0.824 Solar Masses (863 Jupiter Masses; 274,360 Earth Masses; 1,638 Septillion Tonnes)
* Radius: 13.659 Solar Radius (19,022,671 km in Diameter; 0.06358 AU; 187 Solar Areas or 2,548 Solar Volumes)
* Luminosity: 96.06 Solar Luminosities
* Temperature: 4,889 Kelvin (4,616 °C; 8,341 °F)
* Age: 13.2 Billion Years
* Spectral Type: CEMP-s or K2III
* Metallicity [Fe/H]: -2.67 dex
* Right Ascension: 17h 55m 44.5507s
* Declination: -39° 27' 00.836"

### Other Designations

SMSS J175544.54-392700.9, 2MASS J17554455-3927008
V1752 Scuti

V1752 Scuti, Also Named **Reprimand X3-7**, is a Red Hypergiant Stars in The Open Cluster Reprimand X3, The Star is Located at 31,600 Light Years Away From Earth

## Information

* Mass: 33 Solar Masses
* Radius: 1,825 Solar Radius
* Luminosity: 300,000 Solar Luminosities
* Temperature: 3,160 Kelvin
* Spectral Type: M6Ia+
* Variable Star Type: Semi Regular Variable Star
V2521 Sagittarii

Object type: RR Lyrae variable star
Number of stars: 1
Total mass: 0.65-0.8 Solar Masses (681-838 Jupiter Masses; 216,425-266,369 Earth Masses; 1,293-1,591 Septillion Tonnes)
Distance from the sun: ~35,000 ly

V2521 Sagittarii is a RR Lyrae Variable Stars in The Constellation Sagittarius, The Star is Located at Around 35,000 Light Years Away From Earth

## Information

* Mass: 0.65-0.8 Solar Masses (681-838 Jupiter Masses; 216,425-266,369 Earth Masses; 1,293-1,591 Septillion Tonnes)
* Radius: 3.92-4.51 Solar Radius (5,459,321-6,281,005 km in Diameter; 0.01825-0.02099 AU; 15.366-20.34 Solar Areas or 60.236-91.734 Solar Volumes)
* Luminosity: 71.13-99.37 Solar Luminosities
* Temperature: 8,466-8,581 Kelvin (8,193-8,308 °C; 14,779-14,986 °F)
* Spectral Type: A5IVp-A7IVp
* Right Ascension: 18h 19m 21.644s
* Declination: -30° 37' 19.758"
* Apparent Magnitude (V): +16.15
* Variable Star Type: RR Lyrae Variable Star
V2022 Sagittarii

Object type: W Virginis variable star
Number of stars: 1
Total mass: 0.6-0.8 Solar Masses (629-838 Jupiter Masses; 199,777-266,369 Earth Masses; 1,193-1,591 Septillion Tonnes)
Distance from the sun: ~10,800 ly

V2022 Sagittarii is a W Virginis Variable Stars in The Constellation Sagittarius, The Star is Located at Around 10,800 Light Years Away From Earth

## Information

* Mass: 0.6-0.8 Solar Masses (629-838 Jupiter Masses; 199,777-266,369 Earth Masses; 1,193-1,591 Septillion Tonnes)
* Radius: 44.98-51.15 Solar Radius (62,642,926-71,235,787 km in Diameter; 0.20937-0.23809 AU; 2,023-2,616 Solar Areas or 91,004-133,825 Solar Volumes)
* Luminosity: 1,531-2,336 Solar Luminosities
* Temperature: 5,383-5,610 Kelvin (5,110-5,337 °C; 9,230-9,638 °F)
* Spectral Type: G5Iep-G8Iep
* Right Ascension: 18h 40m 38.9706s
* Declination: -25° 22' 49.96"
* Apparent Magnitude (V): +13.578
* Variable Star Type: W Virginis Variable Star

### Other Designations

V2022 Sagittarii, 2MASS J18403896-2522499
V380 Sagittarii

Object type: RR Lyrae variable star
Number of stars: 1
Total mass: 0.75-0.9 Solar Masses (786-943 Jupiter Masses; 249,721-299,665 Earth Masses; 1,491-1,790 Septillion Tonnes)
Distance from the sun: ~23,800 ly

V380 Sagittarii is a RR Lyrae Variable Stars in The Constellation Sagittarius, The Star is Located at Around 23,800 Light Years Away From Earth

## Information

* Mass: 0.75-0.9 Solar Masses (786-943 Jupiter Masses; 249,721-299,665 Earth Masses; 1,491-1,790 Septillion Tonnes)
* Radius: 6.41-7.72 Solar Radius (8,927,104-10,751,520 km in Diameter; 0.02984-0.03593 AU; 41.09-59.6 Solar Areas or 263.37-460.1 Solar Volumes)
* Luminosity: 92-140 Solar Luminosities
* Temperature: 7,053-7,138 Kelvin (6,780-6,865 °C; 12,236-12,389 °F)
* Spectral Type: F0IIIep-F1IIIep
* Right Ascension: 18h 49m 18.7737s
* Declination: -35° 06' 59.691"
* Apparent Magnitude (K): +13.352
* Variable Star Type: RR Lyrae Variable Star
V1099 Cassiopeiae

Object type: Yellow-white supergiant star
Number of stars: 1
Total mass: 7.226 Solar Masses (7,569 Jupiter Masses; 2,405,976 Earth Masses; 14,369 Septillion Tonnes)
Distance from the sun: ~14,000 ly

V1099 Cassiopeiae is a Yellow-White Supergiant Stars in The Constellation Cassiopeia, The Star is Located at Around 14,000 Light Years Away From Earth

## Information

* Mass: 7.226 Solar Masses (7,569 Jupiter Masses; 2,405,976 Earth Masses; 14,369 Septillion Tonnes)
* Radius: 40.91 Solar Radius (56,974,702 km in Diameter; 0.19043 AU; 1,674 Solar Areas or 68,468 Solar Volumes)
* Luminosity: 2,908 Solar Luminosities
* Temperature: 6,627 Kelvin (6,354 °C; 11,469 °F)
* Spectral Type: F5Ib
* Right Ascension: 01h 20m 48.7853s
* Declination: +58° 31' 13.36"
* Apparent Magnitude (V): +15.22
* Variable Star Type: Classical Cepheid Variable Star

### Other Designations

V1099 Cassiopeiae, 2MASS J01204877+5831134
Weezer Sector C2-1219

Weezer Sector C2-1219 is a Blue Subdwarf Stars in The Constellation Vulpecula, The Star is Located at 7,187 Light Years Away From Earth

## Information

* Mass: 0.368 Solar Masses
* Radius: 0.294 Solar Radius
* Luminosity: 311 Solar Luminosities
* Temperature: 44,682 Kelvin (44,409 °C; 79,968 °F)
* Spectral Type: B1VI-B2VI
V6392 Sagittarii

Object type: Mira variable star
Number of stars: 1
Total mass: 3-6 Solar Masses (3,143-6,285 Jupiter Masses; 998,883-1,997,766 Earth Masses; 5,965-11,931 Septillion Tonnes)
Distance from the sun: ~38,000 ly

V6392 Sagittarii is a Carbon-Rich Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 38,000 Light Years Away From Earth

If V6392 Sagittarii was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, Mars, and even Ceres, Because V6392 Sagittarii's size was 578 to 612 times large as the sun

## Information

* Mass: 3-6 Solar Masses (3,143-6,285 Jupiter Masses; 998,883-1,997,766 Earth Masses; 5,965-11,931 Septillion Tonnes)
* Radius: 578-612 Solar Radius (804,971,352-852,322,608 km in Diameter; 2.69045-2.84871 AU; 334,084-374,544 Solar Areas or 193,100,552-229,220,928 Solar Volumes)
* Luminosity: 24,741-34,508 Solar Luminosities
* Temperature: 3,011-3,180 Kelvin (2,738-2,907 °C; 4,960-5,264 °F)
* Spectral Type: C3,8-C4,9 or M6-7II-III
* Metallicity [Fe/H]: +0.09 dex
* Metallicity [C/Fe]: +1.67 dex
* Right Ascension: 18h 21m 59.3571s
* Declination: -28° 23' 25.061"
* Variable Star Type: Mira Variable Star

### Other Designations

V6392 Sagittarii, 2MASS J18215937-2823249
V2020 Sagittarii

Object type: Mira variable star
Number of stars: 1
Total mass: 0.9-1.8 Solar Masses (943-1,886 Jupiter Masses; 299,665-599,330 Earth Masses; 1,790-3,579 Septillion Tonnes)
Distance from the sun: ~23,000 ly

V2020 Sagittarii is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 23,000 Light Years Away From Earth

If V2020 Sagittarii was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, and even Mars, Because V2020 Sagittarii's size was 344 times large as the sun

## Information

* Mass: 0.9-1.8 Solar Masses (943-1,886 Jupiter Masses; 299,665-599,330 Earth Masses; 1,790-3,579 Septillion Tonnes)
* Radius: 344 Solar Radius (479,083,296 km in Diameter; 1.60124 AU; 118,336 Solar Areas or 40,707,584 Solar Volumes)
* Luminosity: 10,498 Solar Luminosities
* Temperature: 3,150 Kelvin (2,877 °C; 5,210 °F)
* Spectral Type: M6IIIe
* Right Ascension: 18h 39m 50.3761s
* Declination: -22° 42' 42.48"
* Apparent Magnitude (H): +7.155
* Apparent Magnitude (K): +6.65
* Variable Star Type: Mira Variable Star

### Other Designations

V2020 Sagittarii, 2MASS J18395036-2242424
WR 147N

WR 147N is a Blue White Hypergiant and the companion of WR 147S. He always tries to blow away his sister with his winds but can’t. So he will watch his sister blow up and become a black hole and fly out of the system because of the force of the explosion. He is 238 Solar radius and has class B0.5Ia-0
SMSS J004116.02-723216.9

Object type: Yellow supergiant star
Number of stars: 1
Total mass: 18.31-21.44 Solar Masses (19,180-22,458 Jupiter Masses; 6,096,516-7,138,684 Earth Masses; 36,409-42,633 Septillion Tonnes)
Distance from the sun: ~200,000 ly

SMSS J004116.02-723216.9 is a Yellow Supergiant Stars in The Small Magellanic Cloud, The Star is Located at Around 200,000 Light Years Away From Earth

If SMSS J004116.02-723216.9 was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, and even Mars, Because SMSS J004116.02-723216.9's size was 304 to 357 times large as the sun

## Information

* Mass: 18.31-21.44 Solar Masses (19,180-22,458 Jupiter Masses; 6,096,516-7,138,684 Earth Masses; 36,409-42,633 Septillion Tonnes)
* Radius: 304-357 Solar Radius (423,375,936-497,188,188 km in Diameter; 1.41505-1.66175 AU; 92,416-127,449 Solar Areas or 28,094,464-45,499,293 Solar Volumes)
* Luminosity: 68,110-99,236 Solar Luminosities
* Temperature: 5,348-5,422 Kelvin (5,075-5,149 °C; 9,167-9,300 °F)
* Spectral Type: G6Iab
* Right Ascension: 00h 41m 16.0592s
* Declination: 72° 32' 16.755"
* Apparent Magnitude (V): +11.63
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

SMSS J004116.02-723216.9, 2MASS J00411604-7232167
V1003 Scorpii

V1003 Scorpii, Also Named **HD 149711**, is a Blue Main Sequence Stars in The Constellation Scorpius, The Star is Located at 623 Light Years Away From Earth

## Information

* Mass: 14.86 Solar Masses
* Radius: 8.53 Solar Radius
* Luminosity: 23,200 Solar Luminosities
* Temperature: 24,400 Kelvin
* Spectral Type: B2IV-V
* Right Ascension: 16h 38m 26.292s
* Declination: -43° 23' 54.329"
* Apparent Magnitude (V): +5.83

### Other Designations

V1003 Scorpii, HD 149711, HR 6174, HIP 81472, SAO 226989, CD -43° 10959, CP -43° 7635, TYC 7866-224-1, 2MASS J16382629+4323543
V402 Lacertae

V402 Lacertae, Also Named **HD 210405** or **BD +44° 4059**, is a Blue-White Subgiant Stars in The Constellation Lacerta, The Star is Located at 944 Light Years Away From Earth

The name HD 210405 derives directly from the fact that the star is the 210,405th 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 109354 derives directly from the fact that the star is the 109,354th stars in the Hipparcos catalogue, and The name SAO 51698 derives directly from the fact that the star is the 51,698th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 2.953 Solar Masses (3,093 Jupiter Masses; 983,234 Earth Masses; 5,872 Septillion Tonnes)
* Radius: 2.784 Solar Radius (3,877,232 km in Diameter; 0.01296 AU; 7.751 Solar Areas or 21.578 Solar Volumes)
* Luminosity: 97 Solar Luminosities
* Temperature: 10,855 Kelvin (10,582 °C; 19,079 °F)
* Spectral Type: B9IV-V
* Right Ascension: 22h 09m 15.2005s
* Declination: +44° 50' 47.3414"
* Apparent Magnitude (V): +6.732

### Other Designations

V402 Lacertae, HD 210405, HIP 109354, SAO 51698, BD +44° 4059, TYC 3210-1015-1, 2MASS J22091519+4450471
V994 Scorpii

V994 Scorpii, Also Named **HD 160124**, **CD -32° 13072** or **CP -32° 4686**, is a Blue Subgiant Stars in The Butterfly Cluster, The Star is Located at 1,572 Light Years Away From Earth

The name HD 160124 derives directly from the fact that the star is the 160,124th 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 86432 derives directly from the fact that the star is the 86,432nd stars in the Hipparcos catalogue, and The name SAO 209092 derives directly from the fact that the star is the 209,092nd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 11.59 Solar Masses (12,141 Jupiter Masses; 3,859,018 Earth Masses; 23,046 Septillion Tonnes)
* Radius: 7.82 Solar Radius (10,890,789 km in Diameter; 0.0364 AU; 61.15 Solar Areas or 478.21 Solar Volumes)
* Luminosity: 10,912 Solar Luminosities
* Temperature: 21,096 Kelvin (20,823 °C; 37,513 °F)
* Spectral Type: B4IV
* Right Ascension: 17h 39m 37.5915s
* Declination: -32° 19' 12.497"
* Apparent Magnitude (V): +7.16

### Other Designations

V994 Scorpii, HD 160124, HIP 86432, SAO 209092, CD -32° 13072, CP -32° 4686, NGC 6405 GDPR 100, TYC 7380-607-1, 2MASS J17393758-3219126
V888 Cassiopeiae

Object type: Mira variable star
Number of stars: 1
Total mass: 1.5-2.5 Solar Masses (1,571-2,619 Jupiter Masses; 499,442-832,403 Earth Masses; 2,983-4,971 Septillion Tonnes)
Distance from the sun: 4,840 ly

V888 Cassiopeiae, Also Named **IRAS 01022+6542**, is a Red Giant Stars in The Constellation Cassiopeia, The Star is Located at 4,840 Light Years Away From Earth

## Information

* Mass: 1.5-2.5 Solar Masses (1,571-2,619 Jupiter Masses; 499,442-832,403 Earth Masses; 2,983-4,971 Septillion Tonnes)
* Radius: 389-432 Solar Radius (541,754,076-601,639,488 km in Diameter; 1.8107-2.01086 AU; 151,321-186,624 Solar Areas or 58,863,869-80,621,568 Solar Volumes)
* Luminosity: 11,476-16,831 Solar Luminosities
* Temperature: 3,029-3,163 Kelvin (2,756-2,890 °C; 4,993-5,234 °F)
* Spectral Type: C3,4-C4,5 or M6III-M7III
* Right Ascension: 01h 05m 27.4029s
* Declination: +65° 58' 59.649"
* Variable Star Type: Mira Variable Star

### Other Designations

V888 Cassiopeiae, IRAS 01022+6542, 2MASS J01052742+6558594
V508 Cassiopeiae

Object type: M-type red giant star
Number of stars: 1
Total mass: 3.088 Solar Masses (3,235 Jupiter Masses; 1,028,184 Earth Masses; 6,140 Septillion Tonnes)
Distance from the sun: ~10,000 ly

V508 Cassiopeiae, Also Named **IRAS 03040+6116**, is a Red Giant Stars in The Constellation Cassiopeia, The Star is Located at Around 10,000 Light Years Away From Earth

If V508 Cassiopeiae was placed into center of the solar system, that It's will engulf Mercury and approach Venus's Orbit, Because V508 Cassiopeiae's size was 124 to 141 times large as the sun

## Information

* Mass: 3.088 Solar Masses (3,235 Jupiter Masses; 1,028,184 Earth Masses; 6,140 Septillion Tonnes)
* Radius: 123.87-140.58 Solar Radius (172,511,767-195,783,517 km in Diameter; 0.57658-0.65437 AU; 15,344-19,763 Solar Areas or 1,900,634-2,778,245 Solar Volumes)
* Luminosity: 2,289-3,210 Solar Luminosities
* Temperature: 3,587-3,664 Kelvin (3,314-3,391 °C; 5,997-6,136 °F)
* Spectral Type: M3IIIe
* Right Ascension: 03h 08m 06.6306s
* Declination: +61° 27' 31.218"
* Apparent Magnitude (H): +6.609
* Apparent Magnitude (K): +6.112
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V508 Cassiopeiae, IRAS 03040+6116, 2MASS J03080666+6127313
V774 Sagittarii

V774 Sagittarii, Also Named **CD -23° 13645** or **IRAS 17513-2313**, is a Red Supergiant Stars in The Constellation Sagittarius, The Star is Located at 7,880 Light Years Away From Earth

The name HIP 87668 derives directly from the fact that the star is the 87,668th stars in the Hipparcos catalogue

## Information

* Mass: 25-35 Solar Masses (26,188-36,663 Jupiter Masses; 8,324,025-11,653,635 Earth Masses; 49,712-69,596 Septillion Tonnes)
* Radius: 1,282-1,368 Solar Radius (1,785,420,888-1,905,191,712 km in Diameter; 5.9674-6.36771 AU; 1,643,524-1,871,424 Solar Areas or 2,106,997,768-2,560,108,032 Solar Volumes)
* Luminosity: 194,900-270,200 Solar Luminosities
* Temperature: 3,387-3,558 Kelvin (3,114-3,285 °C; 5,637-5,945 °F)
* Spectral Type: M4Ia-M5Ia
* Right Ascension: 17h 54m 26.1329s
* Declination: -23° 14' 09.663"
* Apparent Magnitude (V): +9.576
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

V774 Sagittarii, HIP 87668, CD -23° 13645, IRAS 17513-2313, TYC 6841-1586-1, RAFGL 2024, HV 10303, 2MASS J17542613-2314097
V436 Serpentis

Object type: Orange supergiant star
Number of stars: 1
Total mass: 11.4-13.7 Solar Masses (11,942-14,351 Jupiter Masses; 3,795,755-4,561,566 Earth Masses; 22,669-27,242 Septillion Tonnes)
Distance from the sun: ~18,000 ly

V436 Serpentis, Also Named **BPS CS22890-0077**, **BPS BS16559-0084**, **HE 1521-0033**, **2MASS J15234611-0044247** or **SDSS J152346.11-004424.8**, is a Orange Supergiant Stars in The Constellation Serpens Caput, The Star is Located at Around 18,000 Light Years Away From Earth

If V436 Serpentis was placed into center of the solar system, that It's will engulf Mercury and Venus, Because V436 Serpentis's size was 165 to 193 times large as the sun

## Information

* Mass: 11.4-13.7 Solar Masses (11,942-14,351 Jupiter Masses; 3,795,755-4,561,566 Earth Masses; 22,669-27,242 Septillion Tonnes)
* Radius: 165.91-193.47 Solar Radius (231,060,202-269,442,573 km in Diameter; 0.77227-0.90056 AU; 27,526-37,431 Solar Areas or 4,566,860-7,241,706 Solar Volumes)
* Luminosity: 11,968-18,372 Solar Luminosities
* Temperature: 4,687-4,831 Kelvin (4,414-4,558 °C; 7,977-8,236 °F)
* Spectral Type: K2Ib-K3Ib
* Right Ascension: 15h 23m 46.1124s
* Declination: -00° 44' 24.722"
* Apparent Magnitude (V): +11.13
* Variable Star Type: Classical Cepheid Variable Star

### Other Designations

V436 Serpentis, BPS CS22890-0077, BPS BS16559-0084, HE 1521-0033, TYC 5003-309-1, 2MASS J15234611-0044247, SDSS J152346.11-004424.8
Timeline of a 0.3 Solar Masses Stars

This is Timeline of a 0.3 Solar Masses Stars, The Star Have 4 Planets

## Star Information

* Initial Radius: 0.292 Solar Radius
* Initial Luminosity: 0.0123 Solar Luminosities
* Initial Temperature: 3,520 Kelvin
* Initial Spectral type: M4V
* Initial Habitable Zone: 0.113 AU - 0.214 AU

## Planet Information

* Planet A: 1.12 Earth Radius, 1.33 Earth Masses, 0.151 AU, Terrestrial Planet
* Planet B: 1.36 Earth Radius, 2.27 Earth Masses, 0.189 AU, Ocean Planet
* Planet C: 0.94 Earth Radius, 1.12 Earth Masses, 0.254 AU, Rocky Planet
* Planet D: 1.432 Jupiter Radius, 22.43 Jupiter Masses, 6.491 AU, Brown Dwarf

## See Also

* Timeline of a 15 Solar Masses Stars
* Timeline of a 0.3 Solar Mass Star (Rewritten Stellar Evolution Timeline)
V422 Lacertae

Object type: Blue dwarf star
Number of stars: 1
Total mass: 13.622 Solar Masses (14,269 Jupiter Masses; 4,535,595 Earth Masses; 27,087 Septillion Tonnes)
Distance from the sun: 3,022 ly

V422 Lacertae, Also Named **HD 216092** or **BD +47° 3931**, is a Blue Main Sequence Stars in The Constellation Lacerta, The Star is Located at 3,022 Light Years Away From Earth

The name HD 216092 derives directly from the fact that the star is the 216,092nd 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 112698 derives directly from the fact that the star is the 112,698th stars in the Hipparcos catalogue, and The name SAO 52394 derives directly from the fact that the star is the 52,394th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 13.622 Solar Masses (14,269 Jupiter Masses; 4,535,595 Earth Masses; 27,087 Septillion Tonnes)
* Radius: 7.859 Solar Radius (10,945,104 km in Diameter; 0.03658 AU; 61.76 Solar Areas or 485.4 Solar Volumes)
* Luminosity: 21,887 Solar Luminosities
* Temperature: 25,043 Kelvin (24,770 °C; 44,618 °F)
* Spectral Type: B1V-B2V
* Right Ascension: 22h 49m 17.6771s
* Declination: +47° 55' 48.254"
* Apparent Magnitude (V): +7.85
* Variable Star Type: Beta Cephei Variable Star

### Other Designations

V422 Lacertae, HD 216092, HIP 112698, SAO 52394, BD +47° 3931, TYC 3625-1651-1, 2MASS J22491767+4755483
V1111 Ophiuchi

Object type: Mira variable star
Number of stars: 1
Total mass: 12-15 Solar Masses (12,570-15,713 Jupiter Masses; 3,995,532-4,994,415 Earth Masses; 23,862-29,827 Septillion Tonnes)
Distance from the sun: 1,718 ly

V1111 Ophiuchi, Also Named **IRAS 18349+1023**, is a Red Supergiant Stars in The Constellation Ophiuchus, The Star is Located at 1,718 Light Years Away From Earth

## Information

* Mass: 12-15 Solar Masses (12,570-15,713 Jupiter Masses; 3,995,532-4,994,415 Earth Masses; 23,862-29,827 Septillion Tonnes)
* Radius: 940-1,025 Solar Radius (1,309,122,960-1,427,501,100 km in Diameter; 4.37547-4.77113 AU; 883,600-1,050,625 Solar Areas or 830,584,000-1,076,890,625 Solar Volumes)
* Luminosity: 47,891-67,881 Solar Luminosities
* Temperature: 2,785-2,910 Kelvin (2,512-2,637 °C; 4,553-4,778 °F)
* Spectral Type: M8-9II-Ib
* Right Ascension: 18h 37m 19.2584s
* Declination: +10° 25' 42.492"
* Apparent Magnitude (J): +4.121
* Apparent Magnitude (H): +2.283
* Apparent Magnitude (K): +1.114
* Variable Star Type: Mira Variable Star or Semi-Regular Variable Star

### Other Designations

V1111 Ophiuchi, IRAS 18349+1023, IRC +10365, 2MASS J18371926+1025422
V3954 Sagittarii

V3954 Sagittarii, Also Named **HD 178882**, **BD -15° 5259** or **IRAS 19080-1509**, is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at 1,773 Light Years Away From Earth

The name HD 178882 derives directly from the fact that the star is the 178,882nd 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 94224 derives directly from the fact that the star is the 94,224th stars in the Hipparcos catalogue, and The name SAO 162278 derives directly from the fact that the star is the 162,278th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 2.953-3.189 Solar Masses (3,093-3,340 Jupiter Masses; 983,234-1,061,813 Earth Masses; 5,872-6,341 Septillion Tonnes)
* Radius: 190-218 Solar Radius (264,609,960-303,605,112 km in Diameter; 0.8844-1.01474 AU; 36,100-47,524 Solar Areas or 6,859,000-10,360,232 Solar Volumes)
* Luminosity: 4,809-7,216 Solar Luminosities
* Temperature: 3,487-3,603 Kelvin (3,214-3,330 °C; 5,817-6,026 °F)
* Spectral Type: M4III
* Right Ascension: 19h 10m 51.5535s
* Declination: -15° 04' 40.148"
* Apparent Magnitude (V): +7.47
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

V3954 Sagittarii, HD 178882, HIP 94224, SAO 162278, BD -15° 5259, IRAS 19080-1509, IRC -20543, TYC 6283-1087-1, 2MASS J19105155-1504401
V639 Cassiopeiae

Object type: Blue supergiant star
Number of stars: 1
Total mass: 31.44 Solar Masses (32,933 Jupiter Masses; 10,468,294 Earth Masses; 62,517 Septillion Tonnes)
Distance from the sun: 3,477 ly

V639 Cassiopeiae, Also Named **HD 225094**, **BD +62° 2356** or **IRAS 00008+6321**, is a Blue Supergiant Stars in The Constellation Cassiopeia, The Star is Located at 3,477 Light Years Away From Earth

The name HD 225094 derives directly from the fact that the star is the 225,094th stars in the Henry Draper catalogue, and The name HR 9097 derives directly from the fact that the star in the 9,097th stars in the Bright Star catalogue

The name HIP 274 derives directly from the fact that the star is the 274th stars in the Hipparcos catalogue, and The name SAO 10942 derives directly from the fact that the star is the 10,942nd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 31.44 Solar Masses (32,933 Jupiter Masses; 10,468,294 Earth Masses; 62,517 Septillion Tonnes)
* Radius: 33.87 Solar Radius (47,170,207 km in Diameter; 0.15766 AU; 1,147 Solar Areas or 38,855 Solar Volumes)
* Luminosity: 225,271 Solar Luminosities
* Temperature: 21,607 Kelvin (21,334 °C; 38,433 °F)
* Spectral Type: B3Iab
* Right Ascension: 00h 03m 25.7141331s
* Declination: +63° 38' 25.877987"
* Apparent Magnitude (V): +6.22
* Variable Star Type: Alpha Cygni Variable Star

### Other Designations

V639 Cassiopeiae, HD 225094, HR 9097, HIP 274, SAO 10942, BD +62° 2356, IRAS 00008+6321, TYC 4018-3804-1, 2MASS J00032571+6338257
United Federation of Dragons

The **United Federation of Dragons** is a Organization of Dragon clans that try to work together as one to stop dragon haters and poaching. It was founded in 22 AD. The UFOD meets at the Dragon Monument in Cebu , Philippines.

## Leaders and Participating Nations

### Leaders

Sisu (President)

Amba (Vice President)

Pranee (Ambassador to President)

Jagan (Ambassador to Vice President)

Pengu (General of Army)

### Participating Nations

Note: Ex means this country used to be in the UFOD.

1. Philippines
2. France
3. Germany
4. Egypt
5. China
6. England
7. Scotland
8. Greece
9. Turkey
10. Bulgaria
11. Libya
12. Spain
13. Portugal
14. Japan
15. Russia
16. norway
17. finland
18. Sweden
19. Denmark
20. NW African Union
21. Sri Lanka
22. Ireland
23. Blorpland (Ex)
24. USA
25. Switzerland
V3574 Sagittarii

V3574 Sagittarii, Also Named **HD 171100**, **CD -35° 12728** or **IRAS 18310-3541**, is a S-type Red Giant Stars in The Constellation Sagittarius, The Star is Located at 3,342 Light Years Away From Earth

The name HD 171100 derives directly from the fact that the star is the 171,100th 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

## Information

* Mass: 0.872-1.744 Solar Masses (913-1,827 Jupiter Masses; 290,342-580,684 Earth Masses; 1,734-3,468 Septillion Tonnes)
* Radius: 344-388 Solar Radius (479,083,296-540,361,392 km in Diameter; 1.60124-1.80605 AU; 118,336-150,544 Solar Areas or 40,707,584-58,411,072 Solar Volumes)
* Luminosity: 14,014-20,400 Solar Luminosities
* Temperature: 3,386-3,502 Kelvin (3,113-3,229 °C; 5,635-5,844 °F)
* Spectral Type: S4,4-S5,6 or M4III-M5III
* Right Ascension: 18h 34m 23.0112s
* Declination: -35° 38' 39.998"
* Apparent Magnitude (V): +9.86
* Variable Star Type: Mira Variable Star

### Other Designations

V3574 Sagittarii, HD 171100, CD -35° 12728, IRAS 18310-3541, Hen 4-191, TYC 7406-1418-1, 2MASS J18342301-3538399
V Cygni

V Cygni, Also Named **BD +47° 3167** or **IRAS 20396+4757**, is a Cold Red Giant Stars in The Constellation Cygnus, The Star is Located at 1,868 Light Years Away From Earth

The name HIP 102082 derives directly from the fact that the star is the 102,082nd stars in the Hipparcos catalogue, and The name SAO 49940 derives directly from the fact that the star is the 49,940th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 1.196-1.518 Solar Masses (1,253-1,590 Jupiter Masses; 398,221-505,435 Earth Masses; 2,378-3,018 Septillion Tonnes)
* Radius: 738-806 Solar Radius (1,027,800,792-1,122,503,304 km in Diameter; 3.43521-3.75174 AU; 544,644-649,636 Solar Areas or 401,947,272-523,606,616 Solar Volumes)
* Luminosity: 18,832-32,273 Solar Luminosities
* Temperature: 2,489-2,725 Kelvin (2,216-2,452 °C; 4,021-4,445 °F)
* Spectral Type: C6,4-C7,6 or M8III-M11III
* Right Ascension: 20h 41m 18.2677s
* Declination: +48° 08' 28.811"
* Apparent Magnitude (V): +7.6998
* Variable Star Type: Mira Variable Star

### Other Designations

V Cygni, HIP 102082, SAO 49940, BD +47° 3167, IRAS 20396+4757, IRC +50338, TYC 3578-2382-1, 2MASS J20411826+4808288
V730 Carinae

Object type: Red supergiant star
Number of stars: 1
Total mass: 20-30 Solar Masses (20,950-31,425 Jupiter Masses; 6,659,220-9,988,830 Earth Masses; 39,769-59,654 Septillion Tonnes)
Distance from the sun: ~9,000 ly

V730 Carinae, Also Named **HD 93281**, **CD -59° 3305**, **CP -59° 2611**, **IRAS 10430-5940** or **Trumpler 14 MJ 459**, is a Red Supergiant Stars in The Open Cluster Trumpler 14, The Star is Located at Around 9,000 Light Years Away From Earth

The name HD 93281 derives directly from the fact that the star is the 93,281st stars in the Henry Draper catalogue, and The name SAO 238427 derives directly from the fact that the star is the 238,427th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 20-30 Solar Masses (20,950-31,425 Jupiter Masses; 6,659,220-9,988,830 Earth Masses; 39,769-59,654 Septillion Tonnes)
* Radius: 1,019-1,133 Solar Radius (1,419,144,996-1,577,910,972 km in Diameter; 4.7432-5.27384 AU; 1,038,361-1,283,689 Solar Areas or 1,058,089,859-1,454,419,637 Solar Volumes)
* Luminosity: 194,039-273,364 Solar Luminosities
* Temperature: 3,795-3,921 Kelvin (3,522-3,648 °C; 6,371-6,598 °F)
* Spectral Type: M1Ia-M2Ia
* Right Ascension: 10h 44m 57.3441s
* Declination: -59° 56' 06.388"
* Apparent Magnitude (V): +7.76
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V730 Carinae, HD 93281, SAO 238427, CD -59° 3305, CP -59° 2611, IRAS 10430-5940, TYC 8626-2618-1, Trumpler 14 MJ 459, 2MASS J10445736-5956063
FZ Persei

FZ Persei, Also Named **HD 14330**, **BD +56° 551** or **IRAS 02174+5655**, is a Red Supergiant Stars in The Open Cluster NGC 884, The Star is Located at 9,228 Light Years Away From Earth

The name HD 14330 derives directly from the fact that the star is the 14,330th stars in the Henry Draper catalogue, and The name SAO 23217 derives directly from the fact that the star is the 23,217th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 21.79-23.61 Solar Masses (22,825-24,731 Jupiter Masses; 7,255,220-7,861,209 Earth Masses; 43,329-46,948 Septillion Tonnes)
* Radius: 752-808 Solar Radius (1,047,298,368-1,125,288,672 km in Diameter; 3.50038-3.76105 AU; 565,504-652,864 Solar Areas or 425,259,008-527,514,112 Solar Volumes)
* Luminosity: 103,400-133,500 Solar Luminosities
* Temperature: 3,774-3,880 Kelvin (3,501-3,607 °C; 6,334-6,524 °F)
* Spectral Type: M2Iab-Ib
* Right Ascension: 02h 20m 59.6455s
* Declination: +57° 09' 29.964"
* Apparent Magnitude (V): +7.962
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

FZ Persei, HD 14330, SAO 23217, BD +56° 551, IRAS 02174+5655, TYC 3694-1862-1, NGC 884 GDPR 1818, 2MASS J02205965+5709299
VdBH 222-371

Object type: Yellow hypergiant star
Number of stars: 1
Total 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)
Distance from the sun: ~31,000 ly

VdBH 222-371 is a Yellow Hypergiant Stars in The Constellation Scorpius, The Star is Located at Around 31,000 Light Years Away From Earth

If VdBH 222-371 was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, Mars, and even Ceres, Because VdBH 222-371's size was 589 to 677 times large as the sun

## 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: 589-677 Solar Radius (820,290,876-942,847,068 km in Diameter; 2.74165-3.15127 AU; 346,921-458,329 Solar Areas or 204,336,469-310,288,733 Solar Volumes)
* Luminosity: 360,582-516,146 Solar Luminosities
* Temperature: 5,828-5,946 Kelvin (5,555-5,673 °C; 10,031-10,243 °F)
* Spectral Type: G0Ia0
* Right Ascension: 17h 18m 46.6s (VdBH 222)
* Declination: -38° 17' 20" (VdBH 222)
* Variable Star Type: Semi-Regular Variable Star
UDFy-38135539 Star 63

UDFy-38135539 Star 63 is a Extremely Metal-Poor Blue-Purple Supergiant Star in The Galaxy UDFy-38135539, The Star is Located at 13.1 Billion Light Years Away From Earth

## Information

* Mass: 500 Solar Masses (523,750 Jupiter Masses; 166,480,500 Earth Masses; 994,235 Septillion Tonnes)
* Radius: 15 Solar Radius (20,890,260 km in Diameter; 0.06982 AU; 225 Solar Areas or 3,375 Solar Volumes)
* Luminosity: 24.7 Million Solar Luminosities
* Temperature: 105,000 Kelvin (104,727 °C; 188,540 °F)
* Spectral Type: U9V-O0V or WC3h-WC4h
* Metallicity [Fe/H]: -5.38 dex or -99.99 dex (Zero Metallicity)
TESS J1719-2200

TESS J1719-2200 is a White Main Sequence Stars in The Constellation Ophiuchus, The Star is Located 6,362 Light Years Away From Earth, The Star Have 4 Planets

## Information

* Mass: 2.164 Solar Masses (2,267 Jupiter Masses; 720,528 Earth Masses; 4,303 Septillion Tonnes)
* Radius: 1.772 Solar Radius (2,467,836 km in Diameter; 0.00825 AU; 3.14 Solar Areas or 5.564 Solar Volumes)
* Luminosity: 26.73 Solar Luminosities
* Temperature: 9,853 Kelvin (9,580 °C; 17,276 °F)
* Age: 250 Million Years
* Spectral Type: A0V
* Metallicity [Fe/H]: +0.06 dex
* Total Population: 318,846,787
* Estimated Value: 28,691 CR
* Minimum Ages of Criminal Responsibility: 13,829 Voltaire Units (13.51 Years)
* Minimum Ages of Majority: 17,983 Voltaire Units (17.56 Years)

### TESS J1719-2200b

* Mass: 0.378 Jupiter Masses
* Radius: 2.881 Jupiter Radius
* Surface Temperature: 6,192 °C (11,178 °F; 6,465 K)
* Distance to Parent Star: 3,500,000 km
* Estimated Value: 13,195 CR

### TESS J1719-2200c

* Mass: 6.417 Jupiter Masses
* Radius: 1.904 Jupiter Radius
* Surface Temperature: 1,485 °C (2,705 °F; 1,758 K)
* Distance to Parent Star: 88,000,000 km
* Estimated Value: 11,973 CR

### TESS J1719-2200d

* Mass: 1.618 Jupiter Masses
* Radius: 0.997 Jupiter Radius
* Surface Temperature: 536 °C (997 °F; 809 K)
* Distance to Parent Star: 220,000,000 km
* Estimated Value: 12,688 CR

### TESS J1719-2200e

* Mass: 2.776 Earth Masses
* Radius: 1.391 Earth Radius
* Surface Temperature: 9 °C (48 °F; 282 K)
* Distance to Parent Star: 835,000,000 km
* Estimated Value: 9,426 CR
V4889 Sagittarii

Object type: S-type red giant star
Number of stars: 1
Total mass: 0.8-2.4 Solar Masses (838-2,514 Jupiter Masses; 266,369-799,106 Earth Masses; 1,591-4,772 Septillion Tonnes)
Distance from the sun: ~26,500 ly

V4889 Sagittarii is a S-type Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 26,500 Light Years Away From Earth

If V4889 Sagittarii was placed into center of the solar system, It's will engulf Mercury, Venus, Earth, and even Mars, Because V4889 Sagittarii's size was 287 to 359 times large as the sun

## Information

* Mass: 0.8-2.4 Solar Masses (838-2,514 Jupiter Masses; 266,369-799,106 Earth Masses; 1,591-4,772 Septillion Tonnes)
* Radius: 287-359 Solar Radius (399,700,308-499,973,556 km in Diameter; 1.33592-1.67106 AU; 82,369-128,881 Solar Areas or 23,639,903-46,268,279 Solar Volumes)
* Luminosity: 5,712-10,836 Solar Luminosities
* Temperature: 2,962-3,108 Kelvin (2,689-2,835 °C; 4,872-5,135 °F)
* Spectral Type: S6,9-S7,10 or M6III-M7III
* Right Ascension: 17h 45m 32.22s
* Declination: -29° 08' 18"
* Apparent Magnitude (K): +10.618
* Variable Star Type: Mira Variable Star

### Other Designations

V4889 Sagittarii, 2MASS J17453222-2908180
V355 Cephei

V355 Cephei, Also Named **IRAS 22471+5902**, is a Orange-Red Supergiant Stars in The Constellation Cepheus, The Star is Located at 15,929 Light Years Away From Earth

## Information

* Mass: 25 Solar Masses (26,188 Jupiter Masses; 8,324,025 Earth Masses; 49,712 Septillion Tonnes)
* Radius: 788-803 Solar Radius (1,097,434,992-1,118,325,252 km in Diameter; 3.66795-3.73777 AU; 620,944-644,809 Solar Areas or 489,303,872-517,781,627 Solar Volumes)
* Luminosity: 137,989-148,273 Solar Luminosities
* Temperature: 3,963-3,997 Kelvin (3,690-3,724 °C; 6,674-6,735 °F)
* Spectral Type: M0Iab
* Right Ascension: 22h 49m 10.4749s
* Declination: +59° 18' 12.979"
* Apparent Magnitude (V): +11.06
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V355 Cephei, IRAS 22471+5902, IRC +60367, TYC 3996-638-1, 2MASS J22491046+5918129
V1185 Scorpii

V1185 Scorpii, Also Named **RAFGL 5379**, is a Red Supergiant Stars in The Constellation Scorpius, The Star is Located at 17,400 Light Years Away From Earth

## Information

* Mass: 24 Solar Masses
* Radius: 830 Solar Radius
* Luminosity: 150,000 Solar Luminosities
* Temperature: 3,950 Kelvin
* Spectral Type: M0Iab
* Right Ascension: 17h 44m 24.0074s
* Declination: -31° 55' 35.414"
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

V1185 Scorpii, RAFGL 5379, IRAS 17411-3154, 2MASS J17442401-3155354
V1300 Aquilae

V1300 Aquilae, Also Named **IRAS 20077-0625**, is a Red Supergiant Stars in The Constellation Aquila, The Star is Located Around 15,000 Light Years Away From Earth

## Information

* Mass: 22 Solar Masses
* Radius: 811 Solar Radius
* Luminosity: 76,000 Solar Luminosities
* Temperature: 3,361 Kelvin (3,088 °C; 5,590 °F)
* Spectral Type: M5Iab-Ib
* Right Ascension: 20h 10m 27.8731s
* Declination: -06° 16' 13.759"
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

V1300 Aquilae, RAFGL 2514, IRAS 20077-0625, IRC -10529, 2MASS J20102787-0616135
V4999 Sagittarii

Object type: M-type red giant star
Number of stars: 1
Total mass: 1.85-2.25 Solar Masses (1,938-2,357 Jupiter Masses; 615,978-749,162 Earth Masses; 3,679-4,474 Septillion Tonnes)
Distance from the sun: ~8,000 ly

V4999 Sagittarii is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 8,000 Light Years Away From Earth

## Information

* Mass: 1.85-2.25 Solar Masses (1,938-2,357 Jupiter Masses; 615,978-749,162 Earth Masses; 3,679-4,474 Septillion Tonnes)
* Radius: 146-169 Solar Radius (203,331,864-235,363,596 km in Diameter; 0.67959-0.78665 AU; 21,316-28,561 Solar Areas or 3,112,136-4,826,809 Solar Volumes)
* Luminosity: 2,693-3,987 Solar Luminosities
* Temperature: 3,441-3,528 Kelvin (3,168-3,255 °C; 5,734-5,891 °F)
* Spectral Type: M4IIIe
* Right Ascension: 17h 46m 05.8437s
* Declination: -29° 06' 31.96"
* Apparent Magnitude (H): +10.685
* Apparent Magnitude (K): +8.687
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

V4999 Sagittarii, 2MASS J17460586-2906322
V428 Andromedae

Object type: Red giant star
Number of stars: 1
Total mass: 2.767-3.081 Solar Masses (2,898-3,227 Jupiter Masses; 921,303-1,025,853 Earth Masses; 5,502-6,126 Septillion Tonnes)
Distance from the sun: 706 ly

V428 Andromedae, Also Named **HD 3346**, **BD +43° 113** or **IRAS 00340+4412**, is a Red Giant Stars in The Constellation Andromeda, The Star is Located at 706 Light Years Away From Earth

The name HD 3346 derives directly from the fact that the star is the 3,346th stars in the Henry Draper catalogue, and The name HR 152 derives directly from the fact that the star in the 152nd stars in the Bright Star catalogue

The name HIP 2900 derives directly from the fact that the star is the 2,900th stars in the Hipparcos catalogue, and The name SAO 36509 derives directly from the fact that the star is the 36,509th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 2.767-3.081 Solar Masses (2,898-3,227 Jupiter Masses; 921,303-1,025,853 Earth Masses; 5,502-6,126 Septillion Tonnes)
* Radius: 59.44-67.16 Solar Radius (82,781,137-93,532,657 km in Diameter; 0.27668-0.31261 AU; 3,533-4,510 Solar Areas or 210,008-302,923 Solar Volumes)
* Luminosity: 988-1,394 Solar Luminosities
* Temperature: 4,197-4,303 Kelvin (3,924-4,030 °C; 7,095-7,286 °F)
* Spectral Type: K7III-K8III
* Right Ascension: 00h 36m 46.4411s
* Declination: +44° 29' 18.92"
* Apparent Magnitude (V): +5.129
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V428 Andromedae, HD 3346, HR 152, HIP 2900, SAO 36509, BD +43° 113, IRAS 00340+4412, IRC +40011, TYC 2796-2404-1, 2MASS J00364644+4429189
V439 Persei

V439 Persei, Also Named **BD +56° 595** or **IRAS 02196+5658**, is a Red Supergiant Stars in The Open Cluster NGC 884, The Star is Located at 7,389 Light Years Away From Earth

The name SAO 23269 derives directly from the fact that the star is the 23,269th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 17.31-20.54 Solar Masses (18,132-21,516 Jupiter Masses; 5,763,555-6,839,019 Earth Masses; 34,420-40,843 Septillion Tonnes)
* Radius: 496-580 Solar Radius (690,771,264-807,756,720 km in Diameter; 2.30876-2.69976 AU; 246,016-336,400 Solar Areas or 122,023,936-195,112,000 Solar Volumes)
* Luminosity: 50,857-76,048 Solar Luminosities
* Temperature: 3,892-3,980 Kelvin (3,619-3,707 °C; 6,546-6,704 °F)
* Spectral Type: M1-2Iab-Ib
* Right Ascension: 02h 23m 11.0656s
* Declination: +57° 11' 57.984"
* Apparent Magnitude (V): +8.165
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V439 Persei, SAO 23269, BD +56° 595, IRAS 02196+5658, TYC 3694-1243-1, NGC 884 GDPR 2691, 2MASS J02231106+5711579
V641 Cassiopeiae

Object type: Red supergiant star
Number of stars: 1
Total mass: 21.4-27.1 Solar Masses (22,417-28,387 Jupiter Masses; 7,125,365-9,023,243 Earth Masses; 42,553-53,888 Septillion Tonnes)
Distance from the sun: ~10,300 ly

V641 Cassiopeiae, Also Named **BD +63° 3** or **IRAS 00067+6340**, is a Red Supergiant Stars in The Constellation Cassiopeia, The Star is Located at Around 10,300 Light Years Away From Earth

The name SAO 11007 derives directly from the fact that the star is the 11,007th stars in the Smithsonian Astrophysical Star catalogue

If V641 Cassiopeiae was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, Mars, and even Ceres, Because V641 Cassiopeiae's size was 815 to 933 times large as the sun

## Information

* Mass: 21.4-27.1 Solar Masses (22,417-28,387 Jupiter Masses; 7,125,365-9,023,243 Earth Masses; 42,553-53,888 Septillion Tonnes)
* Radius: 815-933 Solar Radius (1,135,037,460-1,299,374,172 km in Diameter; 3.79363-4.34289 AU; 664,225-870,489 Solar Areas or 541,343,375-812,166,237 Solar Volumes)
* Luminosity: 120,502-182,926 Solar Luminosities
* Temperature: 3,767-3,908 Kelvin (3,494-3,635 °C; 6,321-6,575 °F)
* Spectral Type: M1Iab-M2Iab
* Right Ascension: 00h 09m 26.3357s
* Declination: +63° 57' 14.098"
* Apparent Magnitude (V): +8.3
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V641 Cassiopeiae, SAO 11007, BD +63° 3, IRAS 00067+6340, IRC +60005, TYC 4022-444-1, 2MASS J00092636+6357140
V819 Cassiopeiae

V819 Cassiopeiae, Also Named **HD 223960**, **BD +60° 2636** or **IRAS 23513+6034**, is a White Hypergiant Stars in The Constellation Cassiopeia, The Star is Located at 9,784 Light Years Away From Earth

The name HD 223960 derives directly from the fact that the star is the 223,960th 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 117830 derives directly from the fact that the star is the 117,830th stars in the Hipparcos catalogue, and The name SAO 20923 derives directly from the fact that the star is the 20,923rd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 45-55 Solar Masses (47,138-57,613 Jupiter Masses; 14,983,245-18,312,855 Earth Masses; 89,481-109,366 Septillion Tonnes)
* Radius: 218-244 Solar Radius (303,605,112-339,814,896 km in Diameter; 1.01474-1.13576 AU; 47,524-59,536 Solar Areas or 10,360,232-14,526,784 Solar Volumes)
* Luminosity: 390,000-519,000 Solar Luminosities
* Temperature: 9,771-9,918 Kelvin (9,498-9,645 °C; 17,128-17,393 °F)
* Spectral Type: A0Ia+
* Right Ascension: 23h 53m 49.983s
* Declination: +60° 51' 12.244"
* Apparent Magnitude (V): +6.8986
* Variable Star Type: Candidate Luminous Blue Variable Star

### Other Designations

V819 Cassiopeiae, HD 223960, HIP 117830, SAO 20923, BD +60° 2636, IRAS 23513+6034, TYC 4285-45-1, 2MASS J23534997+6051121