recursal/Fanatic-Fandom huggingface dataset:
V455 Cephei

Object type: Blue supergiant star
Number of stars: 1
Total mass: 43.48 Solar Masses (45,545 Jupiter Masses; 14,477,144 Earth Masses; 86,459 Septillion Tonnes)
Distance from the sun: 12,381 ly

V455 Cephei, Also Named **HD 216927**, **BD +58° 2511** or **IRAS 22541+5837**, is a Blue-White Supergiant Stars in The Constellation Cepheus, The Star is Located at 12,381 Light Years Away From Earth

The name HD 216927 derives directly from the fact that the star is the 216,927th 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 113263 derives directly from the fact that the star is the 113,263rd stars in the Hipparcos catalogue, and The name SAO 34973 derives directly from the fact that the star is the 34,973rd stars in the Smithsonian Astrophysical Star catalogue

If V455 Cephei was placed into center of the solar system, that It's will engulf Mercury and Venus, Because V455 Cephei's size was 165 times large as the sun

## Information

* Mass: 43.48 Solar Masses (45,545 Jupiter Masses; 14,477,144 Earth Masses; 86,459 Septillion Tonnes)
* Radius: 165.24 Solar Radius (230,127,104 km in Diameter; 0.76915 AU; 27,304 Solar Areas or 4,511,756 Solar Volumes)
* Luminosity: 396,424 Solar Luminosities
* Temperature: 11,267 Kelvin (10,994 °C; 19,821 °F)
* Spectral Type: B9Ia
* Right Ascension: 22h 56m 08.5493s
* Declination: +58° 53' 15.085"
* Apparent Magnitude (V): +8.4
* Variable Star Type: Alpha Cygni Variable Star

### Other Designations

V455 Cephei, HD 216927, HIP 113263, SAO 34973, BD +58° 2511, IRAS 22541+5837, TYC 3997-1379-1
V336 Carinae

Object type: Mira variable star
Number of stars: 1
Total mass: 3 Solar Masses (3,143 Jupiter Masses; 998,883 Earth Masses; 5,965 Septillion Tonnes)
Distance from the sun: 6,786 ly

V336 Carinae, Also Named **IRAS 08312-5651**, is a Red Giant Stars in The Constellation Carina, The Star is Located at 6,786 Light Years Away From Earth

If V336 Carinae was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, and even Mars, Because V336 Carinae's size was 319 to 368 times large as the sun

## Information

* Mass: 3 Solar Masses (3,143 Jupiter Masses; 998,883 Earth Masses; 5,965 Septillion Tonnes)
* Radius: 319 Solar Radius (444,266,196 km in Diameter; 1.48487 AU; 101,761 Solar Areas or 32,461,759 Solar Volumes)
* Luminosity: 10,078-14,716 Solar Luminosities
* Temperature: 3,238-3,314 Kelvin (2,965-3,041 °C; 5,369-5,506 °F)
* Spectral Type: C3,7-C5,4 or M4IIIe-M5IIIe
* Right Ascension: 08h 32m 25.2167s
* Declination: -57° 02' 13.131"
* Apparent Magnitude (V): +10.94
* Variable Star Type: Mira Variable Star
* Evolutionary Stage: Asymptotic Giant Branch

### Other Designations

V336 Carinae, IRAS 08312-5651, TYC 8576-85-1, 2MASS J08322521-5702131
Trumpler 16 MJ 257

Object type: Deep blue dwarf star
Number of stars: 1
Total mass: 83.78 Solar Masses (87,760 Jupiter Masses; 27,895,473 Earth Masses; 166,594 Septillion Tonnes)
Distance from the sun: ~9,300 ly

Trumpler 16 MJ 257 is a Deep Blue Main Sequence Stars in The Open Cluster Trumpler 16, The Star is Located at Around 9,300 Light Years Away From Earth

## Information

* Mass: 83.78 Solar Masses (87,760 Jupiter Masses; 27,895,473 Earth Masses; 166,594 Septillion Tonnes)
* Radius: 13.09 Solar Radius (18,230,234 km in Diameter; 0.06093 AU; 171 Solar Areas or 2,243 Solar Volumes)
* Luminosity: 796,576 Solar Luminosities
* Temperature: 47,661 Kelvin (47,388 °C; 85,330 °F)
* Spectral Type: O4V-O5V
* Right Ascension: 10h 44m 13.1976s
* Declination: -59° 43' 10.249"
* Apparent Magnitude (V): +10.709

### Other Designations

Trumpler 16 MJ 257, ALS 15210, 2MASS J10441319-5943103
V5562 Sagittarii

Object type: Blue bright giant star
Number of stars: 1
Total mass: 14.18 Solar Masses (14,854 Jupiter Masses; 4,721,387 Earth Masses; 28,197 Septillion Tonnes)
Distance from the sun: 4,482 ly

V5562 Sagittarii, Also Named **HD 164516**, **CD -29° 14389**, **CP -29° 5179**, is a Blue Bright Giant Stars in The Constellation Sagittarius, The Star is Located at 4,482 Light Years Away From Earth

The name HD 164516 derives directly from the fact that the star is the 164,516th stars in the Henry Draper catalogue, and The name SAO 186156 derives directly from the fact that the star is the 186,156th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 14.18 Solar Masses (14,854 Jupiter Masses; 4,721,387 Earth Masses; 28,197 Septillion Tonnes)
* Radius: 11.94 Solar Radius (16,628,647 km in Diameter; 0.05558 AU; 143 Solar Areas or 1,702 Solar Volumes)
* Luminosity: 25,161 Solar Luminosities
* Temperature: 21,038 Kelvin (20,765 °C; 37,409 °F)
* Spectral Type: B3II-B4II
* Right Ascension: 18h 02m 47.4883s
* Declination: -29° 21' 58.547"
* Apparent Magnitude (V): +7.91

### Other Designations

V5562 Sagittarii, HD 164516, SAO 186156, CD -29° 14389, CP -29° 5179, TYC 6854-2164-1, 2MASS J18024748-2921585
V426 Carinae

V426 Carinae, Also Named **CP -58° 2721**, is Either an Blue Supergiant Star or an Extreme Helium Star in The Constellation Carina, The Star is Located at 14,031 Light Years Away From Earth

## Information

* Right Ascension: 10h 47m 56.8674s
* Declination: -59° 08' 53.134"
* Apparent Magnitude (V): +10.44

### Blue Supergiant Star

* Mass: 54-64 Solar Masses
* Radius: 25-33 Solar Radius
* Luminosity: 305,000-820,000 Solar Luminosities (471,000-532,000 Solar Luminosities)
* Temperature: 27,128-30,238 Kelvin (26,855-29,965 °C; 48,371-53,969 °F)
* Spectral Type: O8-B0Ia-Iab

### Extreme Helium Star

* Mass: 1.196 Solar Masses
* Radius: 31.71 Solar Radius
* Luminosity: 55,000 Solar Luminosities
* Temperature: 15,700 Kelvin (15,427 °C; 27,800 °F)
* Spectral Type: B7Iae

### Other Designations

V426 Carinae, TYC 8626-464-1, 2MASS J10475687-5908530
VY Masses Majoris

VY Masses Majoris is a Red Metagiant Stars That Doesn't Exist in The Universe, If The Star is Located at 3,600 Light Years Away From Earth, That The Star Will Collapse Into an Large Black Hole and Producing an Devastating Gamma-Ray Burst

## Information

* Mass: 350 Solar Masses (366,625 Jupiter Masses; 116,536,350 Earth Masses; 695,965 Septillion Tonnes)
* Radius: 6,912 Solar Radius (9,626,231,808 km in Diameter; 32.17369 AU; 47,775,744 Solar Areas or 330,225,942,528 Solar Volumes)
* Luminosity: 4,800,000 Solar Luminosities
* Temperature: 3,248 Kelvin (2,975 °C; 5,387 °F)
* Metallicity [Fe/H]: -0.27 dex
* Metallicity [Zr/H]: +1.38 dex
* Spectral Type: M5Ia2-3-M6Ia2-3

## See Also

* Shadron Soul
* Cheese Star
* VY Canis Majoris
* Stephenson 2-18
* WOH G64
V3894 Sagittarii

V3894 Sagittarii, Also Named **HD 161756**, is a Blue-White Main Sequence Stars in The Constellation Sagittarius, The Star is Located at 1,432 Light Years Away From Earth

## Information

* Mass: 12.697 Solar Masses
* Radius: 7.936 Solar Radius
* Luminosity: 16,600 Solar Luminosities
* Temperature: 23,200 Kelvin
* Spectral Type: B2.5III/IV
* Right Ascension: 17h 48m 27.8367s
* Declination: -26° 58' 29.803"
* Apparent Magnitude (V): +6.47

### Other Designations

V3894 Sagittarii, HD 161756, HR 6621, HIP 87163, SAO 185779, CD -26° 12367, CP -26° 5987, TYC 6836-163-1, 2MASS J17482783-2658296
Sadalsuud

Sadalsuud, Also Named **Beta Aquarii**, **HD 204867** or **IRAS 21289-0547**, is a Yellow Supergiant Stars in The Constellation Aquarius, The Star is Located at 563 Light Years Away From Earth

The name HD 204867 derives directly from the fact that the star is the 204,867th stars in the Henry Draper catalogue, and The name HR 8232 derives directly from the fact that the star in the 8,232nd stars in the Bright Star catalogue

The name HIP 106278 derives directly from the fact that the star is the 106,278th stars in the Hipparcos catalogue, and The name SAO 145457 derives directly from the fact that the star is the 145,457th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 6.403 Solar Masses (6,707 Jupiter Masses; 2,131,949 Earth Masses; 12,732 Septillion Tonnes)
* Radius: 53-67 Solar Radius (73,812,252-93,309,828 km in Diameter; 0.2467-0.31187 AU; 2,809-4,489 Solar Areas or 148,877-300,763 Solar Volumes)
* Luminosity: 2,726-5,014 Solar Luminosities (3,136-4,357 Solar Luminosities)
* Temperature: 5,729-5,933 Kelvin (5,456-5,660 °C; 9,853-10,220 °F)
* Spectral Type: G0Ib-G3Ib
* Right Ascension: 21h 31m 33.5317s
* Declination: -05° 34' 16.232"
* Apparent Magnitude (V): +2.89
* Variable Star Type: Classical Cepheid Variable Star

### Other Designations

Sadalsuud, Beta Aquarii, 22 Aquarii, HD 204867, HR 8232, HIP 106278, SAO 145457, BD -06° 5770, IRAS 21289-0547, IRC -10565, TYC 5216-1725-1, 2MASS J21313352-0534161
Timeline of a Barium-Rich Supergiant Stars

This is Timeline of a Barium-Rich Supergiant Stars, The Star Didn't Have an Planets, But Have Two Asteroid Belt, and The Star is Located at Small Magellanic Cloud

This Star was Named "V1891 Lithuania", An Blue-White Supergiant Star in The Small Magellanic Cloud, Located at Around 200,000 Light Years Away From Earth, Also, The Star Have Two Asteroid Belts

The Star Name "V1891 Lithuania" Doesn't Means The 1,891st Variable Stars That Discovered From Lithuania

An Barium-Rich Supergiant Star Has Four Stages of Hertzsprung Gap, However, An Normal Supergiant Has Only One to Two Stages of Hertzsprung Gap

## Information

* Initial Mass: 27.39 Solar Masses (28,691 Jupiter Masses; 9,119,802 Earth Masses; 54,464 Septillion Tonnes)
* Initial Radius: 6.535 Solar Radius (9,101,190 km in Diameter; 0.03042 AU; 42.71 Solar Areas or 279.09 Solar Volumes)
* Initial Luminosity: 91,875 Solar Luminosities
* Initial Temperature: 39,310 Kelvin (39,037 °C; 70,298 °F)
* Initial Spectral Type: O6V
* Metallicity [Fe/H]: -0.27 dex
* Metallicity [Ba/Fe]: +1.38 dex
* Habitable Zone: Disabled

### Planet Information

* First Asteroid Belt: 16.52 Earth Masses, 0.364-4.118 AU
* Second Asteroid Belt: 8.84 Earth Masses, 7.518-11.09 AU
V6008 Sagittarii

Object type: Mira variable star
Number of stars: 1
Total mass: 2-3 Solar Masses (2,095-3,143 Jupiter Masses; 665,922-998,883 Earth Masses; 3,977-5,965 Septillion Tonnes)
Distance from the sun: ~40,000 ly

V6008 Sagittarii is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 40,000 Light Years Away From Earth

## Information

* Mass: 2-3 Solar Masses (2,095-3,143 Jupiter Masses; 665,922-998,883 Earth Masses; 3,977-5,965 Septillion Tonnes)
* Radius: 383-425 Solar Radius (533,397,972-591,890,700 km in Diameter; 1.78277-1.97827 AU; 146,689-180,625 Solar Areas or 56,181,887-76,765,625 Solar Volumes)
* Luminosity: 9,322-14,533 Solar Luminosities
* Temperature: 2,898-3,074 Kelvin (2,625-2,801 °C; 4,757-5,074 °F)
* Spectral Type: C6,8-C7,10 or M7III-M8III
* Right Ascension: 18h 06m 29.524s
* Declination: -25° 54' 19.359"
* Apparent Magnitude (H): +7.082
* Apparent Magnitude (K): +6.431)
* Variable Star Type: Mira Variable Star

### Other Designations

V6008 Sagittarii, 2MASS J18062953-2554194
V658 Cassiopeiae

Object type: M-type red giant star
Number of stars: 1
Total mass: 3-4 Solar Masses (3,143-4,190 Jupiter Masses; 998,883-1,331,844 Earth Masses; 5,965-7,954 Septillion Tonnes)
Distance from the sun: ~11,800 ly

V658 Cassiopeiae, Also Named **IRAS 00044+6132**, is a Red Giant Stars in The Constellation Cassiopeia, The Star is Located at Around 11,800 Light Years Away From Earth

If V658 Cassiopeiae was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, and even Mars, Because V658 Cassiopeiae's size was 383 to 442 times large as the sun

## Information

* Mass: 3-4 Solar Masses (3,143-4,190 Jupiter Masses; 998,883-1,331,844 Earth Masses; 5,965-7,954 Septillion Tonnes)
* Radius: 383-442 Solar Radius (533,397,972-615,566,328 km in Diameter; 1.78277-2.0574 AU; 146,689-195,364 Solar Areas or 56,181,887-86,350,888 Solar Volumes)
* Luminosity: 10,507-16,980 Solar Luminosities
* Temperature: 2,986-3,134 Kelvin (2,713-2,861 °C; 4,915-5,182 °F)
* Spectral Type: M6III-M7III
* Right Ascension: 00h 07m 05.5757s
* Declination: +61° 48' 54.903"
* Apparent Magnitude (V): +12.97
* Variable Star Type: Mira Variable Star

### Other Designations

V658 Cassiopeiae, IRAS 00044+6132, 2MASS J00070554+6148548
V528 Carinae

Object type: Red supergiant star
Number of stars: 1
Total mass: 18-21 Solar Masses (18,855-21,998 Jupiter Masses; 5,993,298-6,992,181 Earth Masses; 35,792-41,758 Septillion Tonnes)
Distance from the sun: 7,651 ly

V528 Carinae, Also Named **HD 95950**, **CD -60° 3327**,**CP -60° 2479** or **IRAS 11010-6038**, is a Red Supergiant Stars in The Constellation Carina, The Star is Located at 7,651 Light Years Away From Earth

The name HD 95950 derives directly from the fact that the star is the 95,950th 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 54021 derives directly from the fact that the star is the 54,021st stars in the Hipparcos catalogue, and The name SAO 251235 derives directly from the fact that the star is the 251,235th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 18-21 Solar Masses (18,855-21,998 Jupiter Masses; 5,993,298-6,992,181 Earth Masses; 35,792-41,758 Septillion Tonnes)
* Radius: 688-725 Solar Radius (958,166,592-1,009,695,900 km in Diameter; 3.20247-3.3747 AU; 473,344-525,625 Solar Areas or 325,660,672-381,078,125 Solar Volumes)
* Luminosity: 73,721-89,716 Solar Luminosities
* Temperature: 3,626-3,710 Kelvin (3,353-3,437 °C; 6,067-6,218 °F)
* Spectral Type: M2Iab-M3Iab
* Right Ascension: 11h 03m 06.1542s
* Declination: -60° 54' 38.627"
* Apparent Magnitude (V): +6.57
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

V528 Carinae, HD 95950, HIP 54021, SAO 251235, CD -60° 3327, CP -60° 2479, IRAS 11010-6038, TYC 8958-1448-1, 2MASS J11030616-6054387
V524 Carinae

V524 Carinae, Also Named **HD 94367** or **IRAS 10504-5658**, is a White Hypergiant Stars in The Constellation Carina, The Star is Located at 8,481 Light Years Away From Earth

## Information

* Mass: 64-72 Solar Masses
* Radius: 269 Solar Radius
* Luminosity: 630,000 Solar Luminosities
* Temperature: 9,913 Kelvin (9,640 °C; 17,384 °F)
* Spectral Type: A0Ia+-Ia
* Right Ascension: 10h 52m 30.846s
* Declination: -57° 14' 25.458"
* Apparent Magnitude (V): +5.25
* Variable Star Type: Luminous Blue Variable Star

### Other Designations

V524 Carinae, HD 94367, HR 4250, HIP 53154, SAO 145457, CD -56° 3625, CP -56° 3947, IRAS 10504-5658, TYC 8622-3780-1, 2MASS J10523084-5714253
V405 Cygni

V405 Cygni, Also Named **HD 193965**, **BD +39° 4152** or **IRAS 20198+4017**, is a Red Giant Stars in The Constellation Cygnus, The Star is Located at 1,528 Light Years Away From Earth

The name HD 193965 derives directly from the fact that the star is the 193,965th stars in the Henry Draper catalogue, and The name SAO 49517 derives directly from the fact that the star is the 49,517th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 3.168-3.455 Solar Masses (3,318-3,619 Jupiter Masses; 1,054,820-1,150,380 Earth Masses; 6,299-6,870 Septillion Tonnes)
* Radius: 216-235 Solar Radius (300,819,744-327,280,740 km in Diameter; 1.00543-1.09387 AU; 46,656-55,225 Solar Areas or 10,077,696-12,977,875 Solar Volumes)
* Luminosity: 5,467-7,492 Solar Luminosities
* Temperature: 3,377-3,503 Kelvin (3,104-3,230 °C; 5,619-5,846 °F)
* Spectral Type: M4III-M5III
* Right Ascension: 20h 21m 36.223s
* Declination: +40° 26' 49.75"
* Apparent Magnitude (V): +8.4994
* Variable Star Type: Semi-Regular Variable Star or Candidate Mira Variable Star
* Evolutionary Stage: Asymptotic Giant Branch

### Other Designations

V405 Cygni, HD 193965, SAO 49517, BD +39° 4152, IRAS 20198+4017, IRC +40410, TYC 3156-1799-1, 2MASS J20213621+4026496
V820 Cassiopeiae

Object type: Blue dwarf star
Number of stars: 1
Total mass: 14.843 Solar Masses (15,548 Jupiter Masses; 4,942,140 Earth Masses; 29,515 Septillion Tonnes)
Distance from the sun: 9,844 ly

V820 Cassiopeiae, Also Named **HD 224424** or **BD +58° 2676**, is a Blue Main Sequence Stars in The Constellation Cassiopeia, The Star is Located at 9,844 Light Years Away From Earth

The name HD 224424 derives directly from the fact that the star is the 224,424th 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 118139 derives directly from the fact that the star is the 118,139th stars in the Hipparcos catalogue, and The name SAO 35928 derives directly from the fact that the star is the 35,928th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 14.843 Solar Masses (15,548 Jupiter Masses; 4,942,140 Earth Masses; 29,515 Septillion Tonnes)
* Radius: 8.139 Solar Radius (11,335,055 km in Diameter; 0.03789 AU; 66.24 Solar Areas or 539.15 Solar Volumes)
* Luminosity: 29,171 Solar Luminosities
* Temperature: 26,441 Kelvin (26,168 °C; 47,134 °F)
* Spectral Type: B0V-B1V
* Right Ascension: 23h 57m 47.6943s
* Declination: +59° 43' 12.422"
* Apparent Magnitude (V): +8.1
* Variable Star Type: Beta Cephei Variable Star

### Other Designations

V820 Cassiopeiae, HD 224424, HIP 118139, SAO 35928, BD +58° 2676, TYC 4013-359-1, 2MASS J23574769+5943124
V2337 Sagittarii

Object type: Mira variable star
Number of stars: 1
Total mass: 2.18-2.64 Solar Masses (2,284-2,765 Jupiter Masses; 725,855-879,017 Earth Masses; 4,335-5,250 Septillion Tonnes)
Distance from the sun: ~48,000 ly

V2337 Sagittarii is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 48,000 Light Years Away From Earth

## Information

* Mass: 2.18-2.64 Solar Masses (2,284-2,765 Jupiter Masses; 725,855-879,017 Earth Masses; 4,335-5,250 Septillion Tonnes)
* Radius: 311-338 Solar Radius (433,124,724-470,727,192 km in Diameter; 1.44763-1.57331 AU; 96,721-114,244 Solar Areas or 30,080,231-38,614,472 Solar Volumes)
* Luminosity: 9,013-11,371 Solar Luminosities
* Temperature: 3,189-3,242 Kelvin (2,916-2,969 °C; 5,281-5,376 °F)
* Spectral Type: M6IIIe
* Right Ascension: 18h 22m 48.4124s
* Declination: -36° 23' 39.783"
* Apparent Magnitude (J): +9.38
* Apparent Magnitude (H): +8.6
* Apparent Magnitude (K): +8.195
* Variable Star Type: Mira Variable Star

### Other Designations

V2337 Sagittarii, 2MASS J18224840-3623397
V2021 Sagittarii

Object type: Mira variable star
Number of stars: 1
Total mass: 6-9 Solar Masses (6,285-9,428 Jupiter Masses; 1,997,766-2,996,649 Earth Masses; 11,931-17,896 Septillion Tonnes)
Distance from the sun: ~32,000 ly

V2021 Sagittarii, Also Named **IRAS 18375-2405**, is a Oxygen-Rich Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 32,000 Light Years Away From Earth

If V2021 Sagittarii was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, Mars, and even Ceres, Because V2021 Sagittarii's size was 553 to 620 times large as the sun

## Information

* Mass: 6-9 Solar Masses (6,285-9,428 Jupiter Masses; 1,997,766-2,996,649 Earth Masses; 11,931-17,896 Septillion Tonnes)
* Radius: 553-620 Solar Radius (770,154,252-863,464,080 km in Diameter; 2.57408-2.88595 AU; 305,809-384,400 Solar Areas or 169,112,377-238,328,000 Solar Volumes)
* Luminosity: 21,786-32,398 Solar Luminosities
* Temperature: 2,982-3,110 Kelvin (2,709-2,837 °C; 4,908-5,138 °F)
* Spectral Type: CO4,9-CO5,10 or M6-7Ib-II
* Right Ascension: 18h 40m 33.7002s
* Declination: -24° 02' 16.99"
* Apparent Magnitude (K): +7.325
* Variable Star Type: Mira Variable Star

### Other Designations

V2021 Sagittarii, IRAS 18375-2405, 2MASS J18403370-2402171
V762 Cassiopeiae

Object type: Orange hypergiant star
Number of stars: 1
Total 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)
Distance from the sun: 14,825 ly

V762 Cassiopeiae, Also Named **HD 7389**, **BD +70° 90** or **IRAS 01125+7128**, is a Orange Hypergiant Stars in The Constellation Cassiopeia, The Star is Located at 14,825 Light Years Away From Earth

The name HD 7389 derives directly from the fact that the star is the 7,389th stars in the Henry Draper catalogue, and The name HR 365 derives directly from the fact that the star in the 365th stars in the Bright Star catalogue

The name HIP 5926 derives directly from the fact that the star is the 5,926th stars in the Hipparcos catalogue, and The name SAO 4358 derives directly from the fact that the star is the 4,358th stars in the Smithsonian Astrophysical Star 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: 926-1,038 Solar Radius (1,289,625,384-1,445,605,992 km in Diameter; 4.31031-4.83164 AU; 857,476-1,077,444 Solar Areas or 794,022,776-1,118,386,872 Solar Volumes)
* Luminosity: 216,600-318,500 Solar Luminosities
* Temperature: 4,092-4,256 Kelvin (3,819-3,983 °C; 6,906-7,201 °F)
* Spectral Type: K6Ia0-K8Ia0
* Right Ascension: 01h 16m 11.9019s
* Declination: +71° 44' 37.825"
* Apparent Magnitude (V): +5.86

### Other Designations

V762 Cassiopeiae, HD 7389, HR 365, HIP 5926, SAO 4358, BD +70° 90, IRAS 01125+7128, IRC +70021, TYC 4305-2038-1, 2MASS J01161191+7144376
The Secrets Behind Arcturus

The Secrets Behind Arcturus is the 8th episode and one of the latest in Season 1.

Description

Starts of with Arcturus Sayin that he is Aldebaran’s Friend . Second of a He Maybe an Orange Giant of classes K0III, K1.5III , K2IIIp ,and K1.5III Fe-0.5 . Third of all , He hunted stray Cats , and Dogs using the COUGLE Destroy a Star neutron star Blow up toy. When He killed his first stray cat, He said, “ I’m warning you , The COUGLE Destroy a Star Neutron Star Blow up toy is not a child’s toy , It is used for hunting. It can eat your matter and then explode”.
U Carinae

U Carinae, Also Named **HD 95109**, is a Yellow Supergiant Stars in The Constellation Carina, The Star is Located at 5,904 Light Years Away From Earth

The name HD 95109 derives directly from the fact that the star is the 95,109th stars in the Henry Draper catalogue, and The name HR 4276 derives directly from the fact that the star in the 4,276th stars in the Bright Star catalogue

The name HIP 53589 derives directly from the fact that the star is the 53,589th stars in the Hipparcos catalogue, and The name SAO 238635 derives directly from the fact that the star is the 238,635th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 17.83 Solar Masses
* Radius: 227 Solar Radius
* Luminosity: 47,150 Solar Luminosities
* Temperature: 5,644 Kelvin (5,371 °C; 9,700 °F)
* Spectral Type: G4-5Ia-Iab
* Right Ascension: 10h 57m 48.1867s
* Declination: -59° 43' 55.883"
* Apparent Magnitude (V): +6.11

### Other Designations

U Carinae, HD 95109, HR 4276, HIP 53589, SAO 238635, CD -59° 3448, CP -59° 2888, TYC 8627-435-1, 2MASS J10574819-5943557
V831 Herculis

V831 Herculis, Also Named **HD 165373**, is a Yellow-White Subgiant Stars in The Constellation Hercules, The Star is Located at 189 Light Years Away From Earth

## Information

* Mass: 1.682 Solar Masses
* Radius: 2.294 Solar Radius
* Luminosity: 14.17 Solar Luminosities
* Temperature: 7,389 Kelvin (7,116 °C; 12,841 °F)
* Spectral Type: F0IV
* Right Ascension: 18h 04m 40.2109s
* Declination: +23° 56' 31.266"
* Apparent Magnitude (V): +6.335

### Other Designations

V831 Herculis, HD 165373, HR 6754, HIP 88528, SAO 85706, BD +23° 3254, TYC 2091-131-1, 2MASS J18044021+2356313
Timeline of K type Stars

This is the timeline of a 61 Cygni like Star.

## Star Details

Mass 0.65 x Sun

Size 0.7 x Sun

Temp:4400 K

Type : K5V

## Planet Details

B/Mass:0.5xEarth/Size: 0.45xEarth/0.1 AU from Star

C/Mass: 0.75 x Earth/ Size:0.6 x Earth / 0.219 AU from Star

D/Mass: 1.2 x Earth/Size: 1.15 x Earth/0.36 AU

E/Mass: 5 x Earth/Size: 1.76x Earth/ 0.43 AU

F/Mass: 3.5x Earth/Size: 1.3 x Earth/ 0.5 AU

G/Mass:0.9x Eartg/Size:0.85xEarth/3 AU
Timeline of a C-type Red Giant Stars

This is Timeline of a C-type Red Giant Stars, The Star Have 3 Planets, and The Star is Located at Small Magellanic Cloud

## Information

* Initial Mass: 23.48 Solar Masses
* Initial Radius: 10.37 Solar Radius
* Initial Luminosity: 74,000 Solar Luminosities
* Intiial Temperature: 31,000 Kelvin
* Initial Spectral Type: O9V
* Initial Habitable Zone: No Habitable Zones

## Planet Information

* Planet A: 0.86 AU, 1.12 Jupiter Radius, 1.53 Jupiter Masses
* Planet B: 1.79 AU, 2.79 Jupiter Radius, 13.49 Jupiter Masses
* Planet C: 6.15 AU, 1.67 Jupiter Radius, 0.84 Jupiter Masses
Westerlund 1-243

Westerlund 1-243, Also Named **2MASS J16470749-4552290**, is a Luminous Blue Variable Star in The Open Cluster Westerlund 1, The Star is Located at 13,400 Light Years Away From Earth

## Information

* Mass: 73-84 Solar Masses
* Radius: 418-492 Solar Radius
* Luminosity: 816,000-1,450,000 Solar Luminosities
* Temperature: 8,485-9,025 Kelvin
* Spectral Type: A4-7Ia0+
* Right Ascension: 16h 47m 07.504s
* Declination: -45° 52' 29.123"
* Apparent Magnitude (V): +15.729
V910 Centauri

Object type: Red supergiant star
Number of stars: 1
Total mass: 22 Solar Masses (23,045 Jupiter Masses; 7,325,142 Earth Masses; 43,746 Septillion Tonnes)
Distance from the sun: ~7,200 ly

V910 Centauri, Also Named **CD -60° 3621**, **CP -60° 3094** or **IRAS 11334-6118**, is a Red Supergiant Stars in The Open Cluster NGC 3766, The Star is Located at Around 7,200 Light Years Away From Earth

The name HIP 56556 derives directly from the fact that the star is the 56,556th stars in the Hipparcos catalogue, and The name SAO 251470 derives directly from the fact that the star is the 251,470th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 22 Solar Masses (23,045 Jupiter Masses; 7,325,142 Earth Masses; 43,746 Septillion Tonnes)
* Radius: 690-738 Solar Radius (960,951,960-1,027,800,792 km in Diameter; 3.21178-3.43521 AU; 476,100-544,644 Solar Areas or 328,509,000-401,947,272 Solar Volumes)
* Luminosity: 97,012-120,926 Solar Luminosities
* Temperature: 3,878-3,962 Kelvin (3,605-3,689 °C; 6,521-6,672 °F)
* Spectral Type: M0-1Iab-Ib
* Right Ascension: 11h 35m 44.9538s
* Declination: -61° 34' 41.021"
* Apparent Magnitude (V): +6.859
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V910 Centauri, HIP 56556, SAO 251470, CD -60° 3621, CP -60° 3094, NGC 3766 GDPR 327, IRAS 11334-6118, TYC 8972-2071-1, 2MASS J11354495-6134410
Timeline of HD 209458 Star System

This is Timeline of The HD 209458 Star System, The Star Have an Gas Giant Planet Named HD 209458 b

## Information

* Initial Radius: 1.082 Solar Radius
* Initial Luminosity: 1.417 Solar Luminosities
* Initial Temperature: 6,055 Kelvin
* Initial Spectral Type: F9V
* Metallicity [Fe/H]: -0.01 dex
* Initial Habitable Zone: 1.11 AU - 1.95 AU

## Planet Information

HD 209458 b: 1.359 Jupiter Radius, 0.716 Jupiter Masses, 0.048 AU, Gas Giant
Timeline of a 0.85 Solar Masses Metal-Poor Stars

This is Timeline of an Metal-Poor Stars That Similar as HE 1523-0901, The Star Have 3 Planets

## Information

* Mass: 0.85 Solar Masses
* Initial Radius: 0.724 Solar Radius
* Initial Luminosity: 0.77 Solar Luminosities
* Initial Temperature: 6,350 Kelvin
* Initial Spectral Type: sdF8
* Initial Habitable Zone: 0.81 AU - 1.42 AU
* Metallicity [Fe/H]: -2.87 dex

## Planet Information

* Planet A: 0.37 Earth Radius, 0.053 Earth Masses, 0.13 AU, Lava Planet
* Planet B: 1.24 Earth Radius, 1.67 Earth Masses, 0.49 AU, Terrestrial Planet
* Planet C: 6.49 Earth Radius, 76 Earth Masses, 4.88 AU, Gas Giant
Timeline of a Binary Star System (16 Solar Masses and 12 Solar Masses)

This is Timeline a Binary Star System, The Star System Have Two Stars, Star Alpha's Mass was 16 Solar Masses, and Star Beta's Mass was 12 Solar Masses, Two Stars Will Become an Neutron Star If They Doesn't Drain Masses by Each Other Stars

Also, The Binary Star System was Named "V902 Netherland", and Located at The Constellation Centaurus, Distance From Earth was 28,000 Light Years

The Star Name "V902 Netherland" Doesn't Means The 902nd Variable Stars That Discovered From The Netherlands

## Information

Star Distance: 0.84 AU (125,662,212 Kilometres)

### Star Alpha (V902 Netherland A)

* Initial Radius: 5.182 Solar Radius (7,216,888 km in Diameter; 0.02412 AU; 26.85 Solar Areas or 139.15 Solar Volumes)
* Initial Luminosity: 23,084 Solar Luminosities
* Initial Temperature: 31,254 Kelvin (30,981 °C; 55,798 °F)
* Initial Spectral Type: O8V

### Star Beta (V902 Netherland B)

* Initial Radius: 4.356 Solar Radius (6,066,532 km in Diameter; 0.02028 AU; 18.97 Solar Areas or 82.65 Solar Volumes)
* Initial Luminosity: 9,829 Solar Luminosities
* Initial Temperature: 27,536 Kelvin (27,263 °C; 49,105 °F)
* Initial Spectral Type: B0V

## See Also

* Timeline of a 1.33 Solar Masses Stars
* Timeline of HD 209458 Star System
* Timeline of a 1.44 Solar Masses Stars
* Timeline of a Binary Star System (13 Solar Masses and 9 Solar Masses)
* Timeline of a 35 Solar Masses Stars
Tau Aquilae

Tau Aquilae, Also Named **HD 190327** or **IRAS 20016+0708**, is a Red Giant Stars in The Constellation Aquila, The Star is Located at 544 Light Years Away From Earth

The name HD 190327 derives directly from the fact that the star is the 190,327th stars in the Henry Draper catalogue, and The name HR 7669 derives directly from the fact that the star in the 7,669th stars in the Bright Star catalogue

The name HIP 98823 derives directly from the fact that the star is the 98,823rd stars in the Hipparcos catalogue, and The name SAO 125403 derives directly from the fact that the star is the 125,403rd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 3.474 Solar Masses
* Radius: 21.89 Solar Radius
* Luminosity: 293 Solar Luminosities
* Temperature: 5,103 Kelvin (4,830 °C; 8,726 °F)
* Spectral Type: K0II-III
* Right Ascension: 20h 04m 08.3149s
* Declination: +07° 16' 40.672"
* Apparent Magnitude (V): +5.508

### Other Designations

Tau Aquilae, 63 Aquilae, HD 190327, HR 7669, HIP 98823, SAO 125403, BD +06° 4416, IRAS 20016+0708, IRC +10448, TYC 506-2497-1, 2MASS J20040831+0716405
Timeline of The Antares Star System

This is Timeline of Antares Star System, Antares A is an Red Supergiant Stars and Antares B is an Blue Main Sequence Stars

## Information

### Antares A

* Initial Mass: 16.83 Solar Masses
* Initial Radius: 5.603 Solar Radius
* Initial Luminosity: 27,800 Solar Luminosities
* Initial Temperature: 31,200 Kelvin
* Initial Spectral Type: O8V-O9V

### Antares B

* Initial Mass: 6.423 Solar Masses
* Initial Radius: 3.317 Solar Radius
* Initial Luminosity: 1,350 Solar Luminosities
* Initial Temperature: 19,000 Kelvin
* Initial Spectral Type: B5V-B6V
V481 Scuti

Object type: Blue hypergiant star
Number of stars: 1
Total mass: 120-150 Solar Masses (125,700-157,125 Jupiter Masses; 39,955,320-49,944,150 Earth Masses; 238,616-298,271 Septillion Tonnes)
Distance from the sun: ~48,000 ly

V481 Scuti, Also Named **IRAS 18311-0701**, is a Blue Hypergiant Stars in The Constellation Scutum, The Star is Located at Around 48,000 Light Years Away From Earth

## Information

* Mass: 120-150 Solar Masses (125,700-157,125 Jupiter Masses; 39,955,320-49,944,150 Earth Masses; 238,616-298,271 Septillion Tonnes)
* Radius: 278-322 Solar Radius (387,166,152-448,444,248 km in Diameter; 1.29402-1.49883 AU; 77,284-103,684 Solar Areas or 21,484,952-33,386,248 Solar Volumes)
* Luminosity: 1,592,000-2,702,000 Solar Luminosities
* Temperature: 12,296-13,040 Kelvin (12,023-12,767 °C; 21,673-23,012 °F)
* Spectral Type: B6Ieq-B7Ieq or B8Ia0
* Right Ascension: 18h 33m 55.2782s
* Declination: -06° 58' 38.631"
* Apparent Magnitude (J): +8.363
* Apparent Magnitude (H): +6.836
* Apparent Magnitude (K): +5.92
* Variable Star Type: Luminous Blue Variable Star

### Other Designations

V481 Scuti, IRAS 18311-0701, 2MASS J18335528-0658386
V381 Puppis

Object type: Blue-white supergiant star
Number of stars: 1
Total mass: 14.09 Solar Masses (14,759 Jupiter Masses; 4,691,420 Earth Masses; 28,018 Septillion Tonnes)
Distance from the sun: 4,122 ly

V381 Puppis, Also Named **HD 61551** or **BD -11° 2039**, is a Blue-White Supergiant Stars in The Constellation Puppis, The Star is Located at 4,122 Light Years Away From Earth

The name HD 61551 derives directly from the fact that the star is the 61,551st 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 37296 derives directly from the fact that the star is the 37,296th stars in the Hipparcos catalogue, and The name SAO 153200 derives directly from the fact that the star is the 153,200th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 14.09 Solar Masses (14,759 Jupiter Masses; 4,691,420 Earth Masses; 28,018 Septillion Tonnes)
* Radius: 18.33 Solar Radius (25,527,898 km in Diameter; 0.08532 AU; 336 Solar Areas or 6,159 Solar Volumes)
* Luminosity: 29,224 Solar Luminosities
* Temperature: 17,627 Kelvin (17,354 °C; 31,269 °F)
* Spectral Type: B6Ib-B7Ib
* Right Ascension: 07h 39m 27.2323s
* Declination: -11° 33' 50.306"
* Apparent Magnitude (V): +7.34

### Other Designations

V381 Puppis, HD 61551, HIP 37296, SAO 153200, BD -11° 2039, TYC 5405-2897-1, 2MASS J07392723-1133501
V2019 Sagittarii

Object type: Mira variable star
Number of stars: 1
Total mass: 1.8-3.2 Solar Masses (1,886-3,352 Jupiter Masses; 599,330-1,065,475 Earth Masses; 3,579-6,363 Septillion Tonnes)
Distance from the sun: ~14,600 ly

V2019 Sagittarii, Also Named **IRAS 18355-3302**, is a S-type Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 14,600 Light Years Away From Earth

If V2019 Sagittarii was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, and even Mars, Because V2019 Sagittarii's size was 271 to 329 times large as the sun

## Information

* Mass: 1.8-3.2 Solar Masses (1,886-3,352 Jupiter Masses; 599,330-1,065,475 Earth Masses; 3,579-6,363 Septillion Tonnes)
* Radius: 271 Solar Radius (377,417,364 km in Diameter; 1.26144 AU; 73,441 Solar Areas or 19,902,511 Solar Volumes)
* Luminosity: 6,011-10,536 Solar Luminosities
* Temperature: 3,087 Kelvin (2,814 °C; 5,097 °F)
* Spectral Type: S4,6-S5,9 or M6IIIe-M7IIIe
* Right Ascension: 18h 38m 53.798s
* Declination: -33° 00' 08.438"
* Apparent Magnitude (H): +7.347
* Apparent Magnitude (K): +6.859
* Variable Star Type: Mira Variable Star

### Other Designations

V2019 Sagittarii, IRAS 18355-3302, 2MASS J18384379-3300084
V669 Cassiopeiae

V669 Cassiopeiae, Also Named **RAFGL 230**, is a Red Supergiant Stars in The Constellation Cassiopeia, The Star is Located at 21,600 Light Years Away From Earth

## Information

* Mass: 23 Solar Masses
* Radius: 859 Solar Radius
* Luminosity: 154,000 Solar Luminosities
* Temperature: 3,900 Kelvin
* Spectral Type: M0Iab-M1Iab
* Right Ascension: 01h 33m 51.21048s
* Declination: +62° 26' 53.2032"
* Variable Star Type: Semi Regular Variable Star

### Other Designations

V669 Cassiopeiae, RAFGL 230, IRAS 01304+6211, 2MASS J01335121+6226532
Timeline of a Fluorine-Rich Supergiant Stars

This is Timeline of a Fluorine-Made Red Giant Stars, The Star Didn't Have a Planets, and The Star is Located at Small Magellanic Cloud, Also, a Red Giant Stars Made by Fluorine Will Be Collapsed Into a Black Hole, Even If The Protostar's Mass is 15 Times More Massive Than Our Sun, Can Still Collapsed Into a Black Hole

## Information

* Initial Mass: 22.76 Solar Masses
* Initial Radius: 9.68 Solar Radius
* Initial Luminosity: 69,200 Solar Luminosities
* Initial Temperature: 29,500 Kelvin
* Initial Spectral Type: O9.5V
* Initial Habitable Zone: No Habitable Zones
V5000 Sagittarii

Object type: Mira variable star
Number of stars: 1
Total mass: 3-4 Solar Masses (3,143-4,190 Jupiter Masses; 998,883-1,331,844 Earth Masses; 5,965-7,954 Septillion Tonnes)
Distance from the sun: ~32,000 ly

V5000 Sagittarii is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 32,000 Light Years Away From Earth

## Information

* Mass: 3-4 Solar Masses (3,143-4,190 Jupiter Masses; 998,883-1,331,844 Earth Masses; 5,965-7,954 Septillion Tonnes)
* Radius: 538-592 Solar Radius (749,263,992-824,468,928 km in Diameter; 2.50426-2.75562 AU; 289,444-350,464 Solar Areas or 155,720,872-207,474,688 Solar Volumes)
* Luminosity: 18,040-25,988 Solar Luminosities
* Temperature: 2,884-3,012 Kelvin (2,611-2,739 °C; 4,732-4,962 °F)
* Spectral Type: CN5,8-CN7,9 or M7III-M8III
* Right Ascension: 17h 46m 06.22s (Infrared)
* Declination: -28° 49' 59.9" (Infrared)
* Apparent Magnitude (J): +16.66
* Apparent Magnitude (H): +12.291
* Apparent Magnitude (K): +9.841
* Variable Star Type: Mira Variable Star

### Other Designations

V5000 Sagittarii, 2MASS J17460621-2849598
V905 Scorpii

Object type: White hypergiant star
Number of stars: 1
Total mass: 50-65 Solar Masses (52,375-68,088 Jupiter Masses; 16,648,050-21,642,465 Earth Masses; 99,424-129,251 Septillion Tonnes)
Distance from the sun: 8,410 ly

V905 Scorpii, Also Named **HD 160529**, **CD -33° 12361**, **CP -33° 4538** or **IRAS 17386-3328**, is a White Hypergiant Stars in The Constellation Scorpius, The Star is Located at 8,410 Light Years Away From Earth

The name HD 160529 derives directly from the fact that the star is the 160,529th 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 86624 derives directly from the fact that the star is the 86,624th stars in the Hipparcos catalogue, and The name SAO 209151 derives directly from the fact that the star is the 209,151st stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 50-65 Solar Masses (52,375-68,088 Jupiter Masses; 16,648,050-21,642,465 Earth Masses; 99,424-129,251 Septillion Tonnes)
* Radius: 299-342 Solar Radius (416,412,516-476,297,928 km in Diameter; 1.39177-1.59193 AU; 89,401-116,964 Solar Areas or 26,730,899-40,001,688 Solar Volumes)
* Luminosity: 459,112-706,289 Solar Luminositiess
* Temperature: 8,689-9,048 Kelvin (8,416-8,775 °C; 15,181-15,827 °F)
* Spectral Type: A1Ieq-A2Ieq or A3Ia0-A4Ia0
* Right Ascension: 17h 41m 59.0262s
* Declination: -33° 30' 13.704"
* Apparent Magnitude (V): +6.66
* Variable Star Type: Luminous Blue Variable Star

### Other Designations

V905 Scorpii, HD 160529, HIP 86624, SAO 209151, CD -33° 12361, CP -33° 4538, IRAS 17386-3328, Hen 3-1454, TYC 7380-655-1, 2MASS J17415902-3330136
UY Eridani

UY Eridani, Also Named **BD -10° 639**, is a Yellow-White Supergiant Stars in the constellation Eridanus, The Star is Located at 12,776 Light years Away From Earth

The name HIP 15027 derives directly from the fact that the star is the 15,027th stars in the Hipparcos catalogue

## Information

* Mass: 1.272-2.669 Solar Masses (1,332-2,796 Jupiter Masses; 423,526-888,673 Earth Masses; 2,529-5,307 Septillion Tonnes)
* Radius: 63.87-70.28 Solar Radius (88,950,727-97,877,832 km in Diameter; 0.2973-0.32714 AU; 4,079-4,939 Solar Areas or 260,550-347,132 Solar Volumes)
* Luminosity: 5,354-7,564 Solar Luminosities
* Temperature: 6,178-6,421 Kelvin (5,905-6,148 °C; 10,661-11,098 °F)
* Spectral Type: F6Iep-F8Iep
* Right Ascension: 03h 13m 39.1354s
* Declination: -10° 26' 32.406"
* Apparent Magnitude (V): +11.281
* Variable Star Type: W Virginis Variable Star or BL Herculis Variable Star

### Other Designations

UY Eridani, HIP 15027, BD -10° 639, TYC 5297-134-1, 2MASS J03133913-1026323
Timeline of a 2 solar mass stars

***WARNING: THIS ARTICLE WAS COPIED FROM DAVDIUS PRODUCTIONS!***

This is the timeline of a Sirius-like star. The star has 2 planets. The 2nd planet has 2 moons. The star is in a globular cluster in the Alcyoneus galaxy

## Details

Mass :2 S

Size: 2.15 S

Luminosity:24 S

Temp:8900K

## Planet Details

### Planet 1

Mass:3.1 MJ

Size:80155 Km

Semimajor Axis : 1.1 AU

### Planet 2

Mass:2.5 MJ

Size:76955 Km

Semimajor Axis: 4.2 AU

#### Planet 2 Moon a

Mass:0.08 Me

Size:2452 Km

#### Planet 2 Moon b

Mass :0.001 Me

Size:677 Km
V378 Pavonis

V378 Pavonis, Also Named **HD 191630**, **CD -62° 1317**, **CP -62° 6147** or **IRAS 20100-6225**, is a S-type Red Giant Stars in The Constellation Pavo, The Star is Located at 1,786 Light Years Away From Earth

The name HD 191630 derives directly from the fact that the star is the 191,630th 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 99758 derives directly from the fact that the star is the 99,758th stars in the Hipparcos catalogue, and The name SAO 254758 derives directly from the fact that the star is the 254,758th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 2.875-4.125 Solar Masses (3,012-4,321 Jupiter Masses; 957,263-1,373,464 Earth Masses; 5,717-8,202 Septillion Tonnes)
* Radius: 296-338 Solar Radius (412,234,464-470,727,192 km in Diameter; 1.37781-1.57331 AU; 87,616-114,244 Solar Areas or 25,934,336-38,614,472 Solar Volumes)
* Luminosity: 11,738-17,832 Solar Luminosities
* Temperature: 3,492-3,628 Kelvin (3,219-3,355 °C; 5,826-6,071 °F)
* Spectral Type: S4,5 or M3III-M4III
* Right Ascension: 20h 14m 25.7986s
* Declination: -62° 16' 45.125"
* Apparent Magnitude (V): +6.76
* Variable Star Type: Mira Variable Star

### Other Designations

V378 Pavonis, HD 191630, HIP 99758, SAO 254758, CD -62° 1317, CP -62° 6147, IRAS 20100-6225, Hen 4-197, TYC 9090-1247-1, 2MASS J20142578-6216449
W Ceti

W Ceti, Also Named **HD 224960**, **BD -15° 6531** or **IRAS 23595-1457**, is a S-type Red Giant Stars in The Constellation Cetus, The Star is Located at 3,782 Light Years Away From Earth

The Protoplanetary Nebula IRAS 23595-1457 Contains The Central Star W Ceti, Which The Star is a S-type Red Giant Star

The name HD 224960 derives directly from the fact that the star is the 224,960th stars in the Henry Draper catalogue, and The name HR 9090 derives directly from the fact that the star in the 9,090th stars in the Bright Star catalogue, however, the star is very faint, It's apparent magnitude was just +14.46

The name SAO 166005 derives directly from the fact that the star is the 166,005th stars in the Smithsonian Astrophysical Star catalogue, however, since the star is very faint, the star doesn't contained by Hipparcos catalogue

## Information

* Mass: 1.8-3.6 Solar Masses (1,886-3,771 Jupiter Masses; 599,330-1,198,660 Earth Masses; 3,579-7,158 Septillion Tonnes)
* Radius: 875-1,030 Solar Radius (1,218,598,500-1,434,464,520 km in Diameter; 4.07291-4.7944 AU; 765,625-1,060,900 Solar Areas or 669,921,875-1,092,727,000 Solar Volumes)
* Luminosity: 8,709-18,589 Solar Luminosities (12,068-13,415 Solar Luminosities)
* Temperature: 1,885-2,100 Kelvin (1,612-1,827 °C; 2,933-3,320 °F)
* Spectral Type: S9,9-S10,8, M13III-M16III or L2III-L3III
* Right Ascension: 00h 02m 07.389978s
* Declination: -14° 40' 33.03262"
* Apparent Magnitude (V): +14.46
* Variable Star Type: Mira Variable Star or Luminous Red Nova
* Evolutionary Stage: Asymptotic Giant Branch or Protoplanetary Nebula

### Other Designations

W Ceti, HD 224960, HR 9090, SAO 166005, BD -15° 6531, IRAS 23595-1457, IRC -10609, TYC 5266-514-1, 2MASS J00020740-1440332, CSS 1346 (Protoplanetary Nebula), CSS 1346 GDPR 1, IRAS 23595-1457 GDPR 1
V4374 Sagittarii

<--- HD 192824 | **HD 192825** | HD 192826 --->
V4374 Sagittarii, Also Named **HD 192825**, **CD -28° 16553** or **CP -28° 7177**, is a Yellow Giant Stars in The Constellation Sagittarius, The Star is Located at 546 Light Years Away From Earth

The name HD 192825 derives directly from the fact that the star is the 192,825th stars in the Henry Draper catalogue, and The name SAO 189111 derives directly from the fact that the star is the 189,111st stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 3.077 Solar Masses (3,223 Jupiter Masses; 1,024,521 Earth Masses; 6,119 Septillion Tonnes)
* Radius: 9.126 Solar Radius (12,709,634 km in Diameter; 0.04248 AU; 83.28 Solar Areas or 760.05 Solar Volumes)
* Luminosity: 86.02 Solar Luminosities
* Temperature: 5,818 Kelvin (5,545 °C; 10,013 °F)
* Spectral Type: G2III
* Right Ascension: 20h 17m 58.9313s
* Declination: -28° 07' 59.278"
* Apparent Magnitude (V): +8.935

### Other Designations

V4374 Sagittarii, HD 192825, SAO 189111, CD -28° 16553, CP -28° 7177, TYC 8918-817-1, 2MASS J20175892-2807592
Timeline of a Low Mass L-type Red Giant Stars

This is Timeline of a Low Mass L-type Red Giant Stars, The Star Have 3 Planets, an L-type Red Giant Stars is Colder Than an Late M-type Main Sequence Stars, The Star's Carbon Abundance Must Higher Than Our Sun 3 Times or More to Become a L-type Red Giant Stars, Also, The Star Can Consume Carbon Even If The Star's Mass is 2 Times Larger Than Our Sun, Further More, The Star Also Can Collapse Into a Neutron Star Even If The Star's Mass is 6 Times Larger Than Our Sun

## Information

* Initial Mass: 6.174 Solar Masses
* Initial Radius: 3.126 Solar Radius
* Initial Luminosity: 1,220 Solar Luminosities
* Initial Temperature: 19,200 Kelvin
* Initial Spectral Type: B5V-B6V
* Metallicity [Fe/H]: -0.13 dex
* Carbon Abundance: 4.79x Our Sun's Carbon Abundance
* Habitable Zone: Disabled

## Planet Information

* Planet A: 2.88 Jupiter Radius, 0.09 Jupiter Masses, 0.22 AU, Hot Jupiter or Super-Puff Planet
* Planet B: 2.17 Jupiter Radius, 0.36 Jupiter Masses, 0.39 AU, Hot Jupiter or Super-Puff Planet
* Planet C: 1.69 Jupiter Radius, 8.82 Jupiter Masses, 0.77 AU, Hot Jupiter
Tau Sagittarii

Tau Sagittarii, Also Named **HD 177716** or **IRAS 19038-2744**, is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at 117 Light Years Away From Earth

The name HD 177716 derives directly from the fact that the star is the 177,716th stars in the Henry Draper catalogue, and The name HR 7234 derives directly from the fact that the star in the 7,234th stars in the Bright Star catalogue

The name HIP 93864 derives directly from the fact that the star is the 93,864th stars in the Hipparcos catalogue, and The name SAO 187683 derives directly from the fact that the star is the 187,683rd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 3.147 Solar Masses
* Radius: 16.97 Solar Radius
* Luminosity: 161 Solar Luminosities
* Temperature: 4,979 Kelvin (4,706 °C; 8,503 °F)
* Spectral Type: K1III-K2III
* Right Ascension: 19h 06m 56.4031s
* Declination: -27° 40' 13.496"
* Apparent Magnitude (V): +3.31

### Other Designations

Tau Sagittarii, 40 Sagittarii, HD 177716, HR 7234, HIP 93864, SAO 187683, CD -27° 13564, CP -27° 6617, IRAS 19038-2744, IRC -30401, TYC 6881-1777-1, 2MASS J19065640-2740133
Weezer Sector B4-189

Weezer Sector B4-189 is a Red Subgiant Stars in The Constellation Vulpecula, The Star is Located at 7,369 Light Years Away From Earth

## Information

* Mass: 0.722 Solar Masses
* Radius: 8.83 Solar Radius
* Luminosity: 17.61 Solar Luminosities
* Temperature: 3,978 Kelvin (3,705 °C; 6,701 °F)
* Age: 28.8 Billion Years
* Spectral Type: M0IV
* Metallicity [Fe/H]: +0.13 dex
V411 Lacertae

V411 Lacertae, Also Named **HD 213233** or **BD +50° 3733**, is a Yellow-White Bright Giant Stars in The Constellation Lacerta, The Star is Located at 4,177 Light Years Away From Earth

The name HD 213233 derives directly from the fact that the star is the 213,233rd 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 110968 derives directly from the fact that the star is the 110,968th stars in the Hipparcos catalogue, and The name SAO 34498 derives directly from the fact that the star is the 34,498th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 4.892-5.181 Solar Masses (5,124-5,427 Jupiter Masses; 1,628,845-1,725,071 Earth Masses; 9,728-10,302 Septillion Tonnes)
* Radius: 28.67-30.91 Solar Radius (39,928,250-43,047,862 km in Diameter; 0.13345-0.14388 AU; 822-955 Solar Areas or 23,566-29,532 Solar Volumes)
* Luminosity: 1,089-1,373 Solar Luminosities
* Temperature: 6,193-6,319 Kelvin (5,920-6,046 °C; 10,688-10,915 °F)
* Spectral Type: F7Ib-II
* Right Ascension: 22h 28m 58.3216s
* Declination: +50° 57' 47.29"
* Apparent Magnitude (V): +7.83
* Variable Star Type: Classical Cepheid Variable Star

### Other Designations

V411 Lacertae, HD 213233, HIP 110968, SAO 34498, BD +50° 3733, TYC 3619-2726-1, 2MASS J22285832+5057473