recursal/Fanatic-Fandom huggingface dataset:
V792 Herculis

V792 Herculis, Also Named **HD 155638**, **BD +49° 2596** or **IRAS 17090+4901**, is a Binary Star System in The Constellation Hercules, The Star System is Located at Around 1,000 Light Years Away From Earth

The name HD 155638 derives directly from the fact that the star is the 155,638th 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 84014 derives directly from the fact that the star is the 84,014th stars in the Hipparcos catalogue, and The name SAO 46541 derives directly from the fact that the star is the 46,541st stars in the Smithsonian Astrophysical Star catalogue

## Information

* Right Ascension: 17h 10m 25.6014s
* Declination: +48° 57' 56.261"
* Apparent Magnitude (V): +8.14
* Variable Star Type: Algol Variable Star

### V792 Herculis A

* Mass: 1.721 Solar Masses (1,803 Jupiter Masses; 573,026 Earth Masses; 3,422 Septillion Tonnes)
* Radius: 4.389 Solar Radius (6,112,490 km in Diameter; 0.02043 AU; 19.263 Solar Areas or 84.547 Solar Volumes)
* Luminosity: 15.71 Solar Luminosities
* Temperature: 5,484 Kelvin (5,211 °C; 9,412 °F)
* Spectral Type: G6-7III-IV

### V792 Herculis B

* Mass: 0.983 Solar Masses (1,030 Jupiter Masses; 327,301 Earth Masses; 1,955 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: 83.74% Solar Luminosities
* Temperature: 5,671 Kelvin (5,398 °C; 9,748 °F)
* Age: 2.7 Billion Years
* Spectral Type: G3V-G4V
* Metallicity [Fe/H]: +0.03 dex

### Other Designations

V792 Herculis, HD 155638, HIP 84014, SAO 46541, BD +49° 2596, IRAS 17090+4901, TYC 3504-1114-1, 2MASS J17102559+4857563
VHK 83

VHK 83 is a Blue Hypergiant Stars in The Triangulum Galaxy, The Star is Located at Around 3.2 Million Light Years Away From Earth

## Information

* Mass: 175 Solar Masses or 125 Solar Masses
* Radius: 60 Solar Radius or 180 Solar Radius
* Luminosity: 5,700,000 Solar Luminosities or 2,780,000 Solar Luminosities
* Highest Temperature: 36,482 Kelvin (36,209 °C; 65,208 °F)
* Lowest Temperature: 17,568 Kelvin (17,295 °C; 31,163 °F)
* Spectral Type: O7If or B6Ia+
* Right Ascension: 01h 34m 10.9079s
* Declination: +30° 34' 37.399"
* Apparent Magnitude (V): +16.07
* Variable Star Type: Luminous Blue Variable Star

### Other Designations

VHK 83, 2MASS J01341090+3034373, LGGS J013410.93+303437.6
Westerlund 1-32

Westerlund 1-32, Also Named **2MASS J16470369-4550435**, is a Yellow-White Hypergiant Stars in The Open Cluster Westerlund 1, The Star is Located at 11,600 Light Years Away From Earth

## Information

* Mass: 36-42 Solar Masses
* Radius: 336-418 Solar Radius
* Luminosity: 196,000-344,000 Solar Luminosities
* Temperature: 6,625-6,835 Kelvin
* Spectral Type: F5-6Ia0
* Right Ascension: 16h 47m 03.685s
* Declination: -45° 50' 43.5361"
* Apparent Magnitude (V): +15.05
VY Canis Majoris

VY Canis Majoris Is the 3rd Largest Star after St2-18 G3pla . Class M4.5Ia+

## Death

VY CMa is gradually shrinking . In about 1000 years from now it will be a Yellow Hypergiant (G4Ia-0 400 SR.) Then it will continue to shrink into a LBV (100 SR) And then will stop shrinking as a wolf Rayet (WN5 13 SR) and will blow up in a hypernova, leaving behind a black hole . Hear sound below
V2845 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: ~60,000 ly

V2845 Sagittarii is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 60,000 Light Years Away From Earth

## Information

* Mass: 3-4 Solar Masses (3,143-4,190 Jupiter Masses; 998,883-1,331,844 Earth Masses; 5,965-7,954 Septillion Tonnes)
* Radius: 499-553 Solar Radius (694,949,316-770,154,252 km in Diameter; 2.32272-2.57408 AU; 249,001-305,809 Solar Areas or 124,251,499-169,112,377 Solar Volumes)
* Luminosity: 20,478-29,036 Solar Luminosities
* Temperature: 3,091-3,204 Kelvin (2,818-2,931 °C; 5,104-5,308 °F)
* Spectral Type: CN4,7-CN5,8 or M6IIIe-M7IIIe
* Right Ascension: 18h 16m 31.4547s
* Declination: -33° 10' 38.913"
* Apparent Magnitude (H): +9.328
* Apparent Magnitude (K): +8.857
* Variable Star Type: Mira Variable Star

### Other Designations

V2845 Sagittarii, 2MASS J18163145-3310389
V396 Centauri

Object type: Red supergiant star
Number of stars: 1
Total mass: 20-25 Solar Masses (20,950-26,188 Jupiter Masses; 6,659,220-8,324,025 Earth Masses; 39,769-49,712 Septillion Tonnes)
Distance from the sun: 8,218 ly

V396 Centauri, Also Named **HD 115283**, **CD -60° 4589**, **CP -60° 4568** or **IRAS 13141-6119**, is a Red Supergiant Stars in The Constellation Centaurus, The Star is Located at 8,218 Light Years Away From Earth

The name HD 115283 derives directly from the fact that the star is the 115,283rd stars in the Henry Draper catalogue, and The name SAO 252241 derives directly from the fact that the star is the 252,241st stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 20-25 Solar Masses (20,950-26,188 Jupiter Masses; 6,659,220-8,324,025 Earth Masses; 39,769-49,712 Septillion Tonnes)
* Radius: 1,054-1,088 Solar Radius (1,467,888,936-1,515,240,192 km in Diameter; 4.90612-5.06438 AU; 1,110,916-1,183,744 Solar Areas or 1,170,905,464-1,287,913,472 Solar Volumes)
* Luminosity: 167,551-206,437 Solar Luminosities
* Temperature: 3,597 Kelvin (3,324 °C; 6,015 °F)
* Spectral Type: M3Iab-M4Iab
* Right Ascension: 13h 17m 25.0405s
* Declination: -61° 35' 02.342"
* Apparent Magnitude (V): +7.92
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V396 Centauri, HD 115283, SAO 252241, CD -60° 4589, CP -60° 4568, IRAS 13141-6119, HV 6436, TYC 8990-3239-1, 2MASS J13172505-6135020
V1981 Cygni

V1981 Cygni, Also Named **HD 200527** or **BD +44° 3679**, is a Red Giant Stars in The Constellation Cygnus, The Star is Located at 1,272 Light Years Away From Earth

The name HD 200527 derives directly from the fact that the star is the 200,527th stars in the Henry Draper catalogue, and The name HR 8062 derives directly from the fact that the star in the 8,062nd stars in the Bright Star catalogue

The name HIP 103828 derives directly from the fact that the star is the 103,828th stars in the Hipparcos catalogue, and The name SAO 50381 derives directly from the fact that the star is the 50,381st stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 2.521-2.869 Solar Masses (2,641-3,005 Jupiter Masses; 839,395-955,265 Earth Masses; 5,013-5,705 Septillion Tonnes)
* Radius: 154.53-171.89 Solar Radius (215,211,459-239,388,453 km in Diameter; 0.7193-0.80011 AU; 23,880-29,546 Solar Areas or 3,690,102-5,078,692 Solar Volumes)
* Luminosity: 2,988-4,210 Solar Luminosities
* Temperature: 3,433-3,546 Kelvin (3,160-3,273 °C; 5,720-5,923 °F)
* Spectral Type: M4III-M5III
* Right Ascension: 21h 02m 24.1998s
* Declination: +44° 47' 27.525"
* Apparent Magnitude (V): +6.23
* Variable Star Type: Semi-Regular Variable Star
* Evolutionary Stage: Asymptotic Giant Branch

### Other Designations

V1981 Cygni, HD 200527, HR 8062, HIP 103828, SAO 50381, BD +44° 3679, TYC 3180-20-1, 2MASS J21022419+4447273
V349 Carinae

Object type: Red supergiant star
Number of stars: 1
Total mass: 18.8-24.6 Solar Masses (19,693-25,769 Jupiter Masses; 6,259,667-8,190,841 Earth Masses; 37,383-48,916 Septillion Tonnes)
Distance from the sun: ~9,300 ly

V349 Carinae, Also Named **HD 91093**, **CD -57° 3259**, **CP -57° 3334** or **IRAS 10277-5742**, is a Red Supergiant Stars in The Constellation Carina, The Star is Located at Around 9,300 Light Years Away From Earth

The name HD 91093 derives directly from the fact that the star is the 91,093rd 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

If V349 Carinae was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, Mars, Ceres, and even Jupiter, Because V349 Carinae's size was 993 to 1,122 times large as the sun

## Information

* Mass: 18.8-24.6 Solar Masses (19,693-25,769 Jupiter Masses; 6,259,667-8,190,841 Earth Masses; 37,383-48,916 Septillion Tonnes)
* Radius: 993-1,122 Solar Radius (1,382,935,212-1,562,591,448 km in Diameter; 4.62218-5.22264 AU; 986,049-1,258,884 Solar Areas or 979,146,657-1,412,467,848 Solar Volumes)
* Luminosity: 142,529-214,176 Solar Luminosities
* Temperature: 3,559-3,707 Kelvin (3,286-3,434 °C; 5,947-6,213 °F)
* Spectral Type: M2Iab-M3Iab
* Right Ascension: 10h 29m 35.3737s
* Declination: -57° 57' 58.973"
* Apparent Magnitude (V): +7.89
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V349 Carinae, HD 91093, CD -57° 3259, CP -57° 3334, IRAS 10277-5742, TYC 8609-231-1, 2MASS J10293537-5757590
Luna Searthian

The **Luna Searthian** is a Natural Satellites from The Film and Video Games *Serbia's Guide to the Galaxy* (Same Name), Luna Searthian is First Natural Satellites That Orbiting The Planet Searthia

## Information

* Mass: 0.027 Earth Masses
* Radius: 0.316 Earth Radius
* Surface Temperature: -50 °C (Night), 70 °C (Day), 15 °C (Average)
* Life Appearance: 7,500,000 (-5.737 bnex)
* Earth Similarity Index: 0.481+0.023
-0.019
* Atmosphere Pressure: 8,000 Pa
* Atmosphere Composition: 93% of Nitrogen, 5% of Oxygen, 2% of Other Gases
* Semi-Major Axis: 415,000 km
* Orbit Period: 34 Days 8 Hours (32 Searthian Days)
* Rotation Period: 63 Hours 48 Minutes (59 Hours 28 Minutes in The Planet Searthia)
Vampire Star

A vampire Star is a Star that steals matter from another star

## Model

Suppose you have 2 Massive Stars . The more massive one begins to expand to an orange Giant which will later become a Red Supergiant. Then the less massive star begins to strip out the Giant star’s layers. The Primary Star then loses so much material that the core also called a white dwarf. The vampiric Star is more larger and massive now. When the vampiric Star begins to expand into a red Supergiant the white dwarf will begin to eat away part of the Star. The white dwarf eats to much material that it explodes into a supernova. Causing the red Supergiant to fly out of the system.
V2599 Sagittarii

Object type: RR Lyrae variable star
Number of stars: 1
Total mass: 0.63-0.81 Solar Masses (660-848 Jupiter Masses; 209,765-269,698 Earth Masses; 1,253-1,611 Septillion Tonnes)
Distance from the sun: ~23,600 ly

V2599 Sagittarii is a RR Lyrae Variable Stars in The Constellation Sagittarius, The Star is Located at Around 23,600 Light Years Away From Earth

## Information

* Mass: 0.63-0.81 Solar Masses (660-848 Jupiter Masses; 209,765-269,698 Earth Masses; 1,253-1,611 Septillion Tonnes)
* Radius: 5.38-6.04 Solar Radius (7,492,640-8,411,811 km in Diameter; 0.02504-0.02811 AU; 29-36 Solar Areas or 156-220 Solar Volumes)
* Luminosity: 48.04-65.53 Solar Luminosities
* Temperature: 6,551-6,682 Kelvin (6,278-6,409 °C; 11,332-11,568 °F)
* Spectral Type: F4IIIp-F5IIIp
* Right Ascension: 18h 37m 12.414s
* Declination: -30° 01' 23.367"
* Apparent Magnitude (H): +13.54
* Apparent Magnitude (K): +13.433
* Variable Star Type: RR Lyrae Variable Star

### Other Designations

V2599 Sagittarii, 2MASS J18371241-3001234
V2140 Cygni

Object type: Blue supergiant star
Number of stars: 1
Total mass: 55-70 Solar Masses (57,613-73,325 Jupiter Masses; 18,312,855-23,307,270 Earth Masses; 109,366-139,193 Septillion Tonnes)
Distance from the sun: ~9,200 ly

V2140 Cygni, Also Named **HD 199478**, **BD +46° 3111**, is a Blue-White Supergiant Stars in The Constellation Cygnus, The Star is Located at Around 9,200 Light Years Away From Earth

The name HD 199478 derives directly from the fact that the star is the 199,478th stars in the Henry Draper catalogue, and The name HR 8020 derives directly from the fact that the star in the 8,020th stars in the Bright Star catalogue

The name HIP 103312 derives directly from the fact that the star is the 103,312th stars in the Hipparcos catalogue, and The name SAO 50246 derives directly from the fact that the star is the 50,246th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 55-70 Solar Masses (57,613-73,325 Jupiter Masses; 18,312,855-23,307,270 Earth Masses; 109,366-139,193 Septillion Tonnes)
* Radius: 171-204 Solar Radius (238,148,964-284,107,536 km in Diameter; 0.79596-0.94957 AU; 29,241-41,616 Solar Areas or 5,000,211-8,489,664 Solar Volumes)
* Luminosity: 488,800-928,400 Solar Luminosities
* Temperature: 11,671-12,544 Kelvin (11,398-12,271 °C; 20,548-22,120 °F)
* Spectral Type: B8Ia-B9Ia
* Right Ascension: 20h 55m 49.804s
* Declination: +47° 25' 03.564"
* Apparent Magnitude (V): +5.64
* Variable Star Type: Candidate Luminous Blue Variable Star

### Other Designations

V2140 Cygni, HD 199478, HR 8020, HIP 103312, SAO 50246, BD +46° 3111, TYC 3579-4462-1, 2MASS J20554981+4725036
Timeline of a 0.9 Solar Masses Stars

This is Timeline of a 0.9 Solar Masses Stars, The Star Have 3 Planets

## Star Information

* Initial Radius: 0.83 Solar Radius
* Initial Temperature: 5,230 Kelvin
* Initial Luminosity: 0.52 Solar Luminosities
* Initial Spectral type: G9V
* Initial Habitable Zone: 0.79 AU - 1.16 AU

## Planet Information

* Planet A: 0.32 AU, 0.54 Earth Radius, 0.09 Earth Masses, Rocky Planet
* Planet B: 0.94 AU, 1.21 Earth Radius, 1.63 Earth Masses, Terrestrial Planet
* Planet C: 1.35 AU, 1.43 Earth Radius, 2.47 Earth Masses, Terrestrial Planet

## See Also

* Timeline of a 1.37 Solar Masses Stars
* Timeline of a 0.9 Solar Mass Star (Rewritten Stellar Evolution Timeline)
* Timeline of a 1.1 Solar Mass Star (Rewritten Stellar Evolution Timeline)
V4420 Sagittarii

V4420 Sagittarii, Also Named **HD 185767**, **BD -20° 5658**, **CP -20° 7673** or **IRAS 19385-2012**, is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at 3,053 Light Years Away From Earth

The name HD 185767 derives directly from the fact that the star is the 185,767th 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 96873 derives directly from the fact that the star is the 96,873rd stars in the Hipparcos catalogue, and The name SAO 188447 derives directly from the fact that the star is the 188,447th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 2.751-3.092 Solar Masses (2,882-3,239 Jupiter Masses; 915,976-1,029,515 Earth Masses; 5,470-6,148 Septillion Tonnes)
* Radius: 94.78-103.31 Solar Radius (131,998,590-143,878,184 km in Diameter; 0.44118-0.48088 AU; 8,983-10,673 Solar Areas or 851,432-1,102,623 Solar Volumes)
* Luminosity: 1,668-2,149 Solar Luminosities
* Temperature: 3,789-3,866 Kelvin (3,516-3,593 °C; 6,361-6,499 °F)
* Spectral Type: M2III
* Right Ascension: 19h 41m 28.4924s
* Declination: -20° 05' 06.36"
* Apparent Magnitude (V): +8.77
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

V4420 Sagittarii, HD 185767, HIP 96873, SAO 188447, BD -20° 5658, CP -20° 7673, IRAS 19385-2012, TYC 6307-1672-1, 2MASS J19412849-2005065
V1762 Cygni

V1762 Cygni, Also Named **HD 179094**, **BD +52° 2350** or **IRAS 19072+5220**, is a Orange Giant Stars in The Constellation Cygnus, The Star is Located at 236 Light Years Away From Earth

The name HD 179094 derives directly from the fact that the star is the 179,094th stars in the Henry Draper catalogue, and The name HR 7275 derives directly from the fact that the star in the 7,275th stars in the Bright Star catalogue

The name HIP 94013 derives directly from the fact that the star is the 94,013rd stars in the Hipparcos catalogue, and The name SAO 31413 derives directly from the fact that the star is the 31,413rd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 1.852 Solar Masses
* Radius: 7.315 Solar Radius
* Luminosity: 31.28 Solar Luminosities
* Temperature: 5,046 Kelvin (4,773 °C; 8,623 °F)
* Spectral Type: K1III-IV
* Right Ascension: 19h 08m 25.7886s
* Declination: +52° 25' 32.632"
* Apparent Magnitude (V): +5.893

### Other Designations

V1762 Cygni, HD 179094, HR 7275, HIP 94013, SAO 31413, BD +52° 2350, IRAS 19072+5220, TYC 3554-1071-1, 2MASS J19082580+5225325
IRAS 20236+4034

HaroChavira 3, Also Named **IRAS 20236+4034**, is a Cold Red Giant Stars in The Constellation Cygnus, The Star is Located at 8,353 Light Years Away From Earth

## Information

* Mass: 2.536-3.617 Solar Masses (2,656-3,789 Jupiter Masses; 844,389-1,204,320 Earth Masses; 5,043-7,192 Septillion Tonnes)
* Radius: 579-634 Solar Radius (806,364,036-882,961,656 km in Diameter; 2.69511-2.95112 AU; 335,241-401,956 Solar Areas or 194,104,539-254,840,104 Solar Volumes)
* Luminosity: 12,952-19,736 Solar Luminosities
* Temperature: 2,559-2,717 Kelvin (2,286-2,444 °C; 4,147-4,431 °F)
* Spectral Type: C8,9-C9,9 or M9III-M11III
* Right Ascension: 20h 25m 30.1088s
* Declination: +40° 44' 36.144"
* Apparent Magnitude (B): +19.4
* Apparent Magnitude (H): +4.877
* Apparent Magnitude (K): +39.51
* Variable Star Type: Mira Variable Star
* Evolutionary Stage: Super Asymptotic Giant Branch

### Other Designations

HaroChavira 3, IRAS 20236+4034, 2MASS J20253011+4044362
V1294 Aquilae

Object type: Blue dwarf star
Number of stars: 1
Total mass: 15.098 Solar Masses (15,815 Jupiter Masses; 5,027,045 Earth Masses; 30,022 Septillion Tonnes)
Distance from the sun: 5,167 ly

V1294 Aquilae, Also Named **HD 184279**, **BD +03° 4065** or **IRAS 19311+0339**, is a Blue Main Sequence Stars in The Constellation Aquila, The Star is Located at 5,167 Light Years Away From Earth

The name HD 184279 derives directly from the fact that the star is the 184,279th 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 96196 derives directly from the fact that the star is the 96,196th stars in the Hipparcos catalogue, and The name SAO 124788 derives directly from the fact that the star is the 124,788th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 15.098 Solar Masses (15,815 Jupiter Masses; 5,027,045 Earth Masses; 30,022 Septillion Tonnes)
* Radius: 7.367 Solar Radius (10,259,903 km in Diameter; 0.03429 AU; 54.27 Solar Areas or 399.83 Solar Volumes)
* Luminosity: 29,188 Solar Luminosities
* Temperature: 27,796 Kelvin (27,523 °C; 49,573 °F)
* Spectral Type: B0V
* Right Ascension: 19h 33m 36.9186s
* Declination: +03° 45' 40.793"
* Apparent Magnitude (V): +6.98
* Variable Star Type: Beta Cephei Variable Star

### Other Designations

V1294 Aquilae, HD 184279, HIP 96196, SAO 124788, BD +03° 4065, IRAS 19311+0339, TYC 486-4746-1, 2MASS J19333691+0345408
V2075 Cygni

V2075 Cygni, Also Named **HD 208472**, **BD +43° 4087** or **IRAS 21532+4410**, is a Orange Giant Stars in The Constellation Cygnus, The Star is Located at 553 Light Years Away From Earth

The name HD 208472 derives directly from the fact that the star is the 208,472nd 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 108198 derives directly from the fact that the star is the 108,198th stars in the Hipparcos catalogue, and The name SAO 51437 derives directly from the fact that the star is the 51,437th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 2.668 Solar Masses (2,795 Jupiter Masses; 888,340 Earth Masses; 5,305 Septillion Tonnes)
* Radius: 9.792 Solar Radius (13,637,162 km in Diameter; 0.04558 AU; 95.883 Solar Areas or 938.889 Solar Volumes)
* Luminosity: 66.23 Solar Luminosities
* Temperature: 5,262 Kelvin (4,989 °C; 9,012 °F)
* Spectral Type: G9III-K0III
* Right Ascension: 21h 55m 14.4582s
* Declination: +44° 25' 06.905"
* Apparent Magnitude (V): +7.49

### Other Designations

V2075 Cygni, HD 208472, HIP 108198, SAO 51437, BD +43° 4087, IRAS 21532+4410, TYC 3197-1790-1, 2MASS J21551445+4425070
V385 Andromedae

V385 Andromedae, Also Named **HD 220524**, is a Red Giant Stars in The Constellation Andromeda, The Star is Located at 1,447 Light Years Away From Earth

## Information

* Mass: 3.287-3.626 Solar Masses
* Radius: 117-134 Solar Radius
* Luminosity: 2,594-3,842 Solar Luminosities
* Temperature: 3,808-3,925 Kelvin
* Spectral Type: M0III-M2III
* Right Ascension: 23h 24m 08.8689s
* Declination: +41° 36' 46.359"
* Apparent Magnitude (V): +6.409
* Variable Star Type: Irregular Variable Star

### Other Designations

V385 Andromedae, HD 220524, HIP 115530, SAO 52978, BD +40° 5065, IRAS 23217+4120, IRC +40537, TYC 3238-796-1, 2MASS J23240887+4136463
Timeline of a 97 solar mass star

This is the timeline of a 97 Solar Mass Star. The star is located in the Large Magellanic Cloud.

**DISCLAIMER: A 97 SOLAR MASS STAR CANNOT REACH 5000 solar radii in its lifetime. It will only expand to 300 SOLAR RADII IN IT'S LIFETIME! AND CANNOT LOSE 93 SOLAR MASSES IN IT'S LIFETIME! IT WILL END AS PAIR INSTABILITY SUPERNOVA IN WHICH NO REMENANT IS SEEN! THIS TIMELINE IS ONLY FOR ENTERTAINMENT PURPOSES ONLY!!!!!!**

## Details

Mass: 97 Suns

Size:12 Suns

Spectral Type O3.5V

Temperature:46000 Kelvins

Luminosity:850,000 Suns
V1334 Cygni

V1334 Cygni, Also Named **HD 203156** or **BD +37° 4271**, is a Binary Star System in The Constellation Cygnus, The Star System is Located at 3,178 Light Years Away From Earth

The name HD 203156 derives directly from the fact that the star is the 203,156th stars in the Henry Draper catalogue, and The name HR 8157 derives directly from the fact that the star in the 8,157th stars in the Bright Star catalogue

The name HIP 105269 derives directly from the fact that the star is the 105,269th stars in the Hipparcos catalogue, and The name SAO 71203 derives directly from the fact that the star is the 71,203rd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Right Ascension: 21h 19m 22.1791s
* Declination: +38° 14' 14.869"
* Apparent Magnitude (V): +5.882

### V1334 Cygni A

* Mass: 4.751 Solar Masses (4,977 Jupiter Masses; 1,581,898 Earth Masses; 9,447 Septillion Tonnes)
* Radius: 21.93 Solar Radius (30,541,560 km in Diameter; 0.10208 AU; 481 Solar Areas or 10,547 Solar Volumes)
* Luminosity: 1,228 Solar Luminosities
* Temperature: 7,296 Kelvin (7,023 °C; 12,673 °F)
* Spectral Type: F1Ib-II
* Variable Star Type: Classical Cepheid Variable Star

### V1334 Cygni B

* Mass: 3.286 Solar Masses (3,442 Jupiter Masses; 1,094,110 Earth Masses; 6,534 Septillion Tonnes)
* Radius: 2.404 Solar Radius (3,348,012 km in Diameter; 0.01119 AU; 5.779 Solar Areas or 13.893 Solar Volumes)
* Luminosity: 142 Solar Luminosities
* Temperature: 12,852 Kelvin (12,579 °C; 22,674 °F)
* Spectral Type: B8V-B9V

### Other Designations

V1334 Cygni, HD 203156, HR 8157, HIP 105269, SAO 71203, BD +37° 3271, TYC 3169-3875-1, 2MASS J21192218+3814149
Lambda Velorum

Lambda Velorum, Also Named **Suhail** or **HD 78647**, is a Orange Supergiant Stars in The Constellation Vela, The Star is Located at 553 Light Years Away From Earth

## Information

* Mass: 13.9 Solar Masses
* Radius: 196-237 Solar Radius
* Luminosity: 15,300-26,100 Solar Luminosities
* Temperature: 4,585-4,755 Kelvin
* Spectral Type: K2Iab-K4Iab
* Right Ascension: 09h 07m 59.7578s
* Declination: -43° 25' 57.327"
* Apparent Magnitude (V): +2.21 (+2.14 to +2.29)
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

Lambda Velorum, Suhail, HD 78647, HR 3634, HIP 44816, SAO 220878, CD -42° 4990, CP -42° 3366, TYC 7689-2617-1, 2MASS J09075977-4325571
U Sagittarii

U Sagittarii, Also Named **HD 170764**, **BD -19° 5047**, **CP -19° 6907** or **IC 4725 GDPR 103**, is a Yellow Supergiant Stars in The Open Cluster Messier 25, The Star is Located at 2,084 Light Years Away From Earth

The name HD 170764 derives directly from the fact that the star is the 170,764th stars in the Henry Draper catalogue, and The name HR 6947 derives directly from the fact that the star in the 6,947th stars in the Bright Star catalogue

The name HIP 90836 derives directly from the fact that the star is the 90,836th stars in the Hipparcos catalogue, and The name SAO 161571 derives directly from the fact that the star is the 161,571st stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 6.85-7.32 Solar Masses (7,175-7,668 Jupiter Masses; 2,280,783-2,437,275 Earth Masses; 13,621-14,556 Septillion Tonnes)
* Radius: 60.92-67.37 Solar Radius (84,842,309-93,825,121 km in Diameter; 0.28357-0.31359 AU; 3,711-4,539 Solar Areas or 226,089-305,773 Solar Volumes)
* Luminosity: 3,844-4,992 Solar Luminosities
* Temperature: 5,823-5,911 Kelvin (5,550-5,638 °C; 10,022-10,180 °F)
* Spectral Type: G1Ib-G2Ib
* Right Ascension: 18h 31m 53.3323s
* Declination: -19° 07' 30.261"
* Apparent Magnitude (V): +6.68
* Variable Star Type: Classical Cepheid Variable Star

### Other Designations

U Sagittarii, HD 170764, HR 6947, HIP 90836, SAO 161571, BD -19° 5047, CP -19° 6907, IC 4725 GDPR 103, TYC 6274-1601-1, 2MASS J18315332-1907301
VW Draconis

VW Draconis, Also Named **HD 156947**, is a Red Giant Stars in The Constellation Draco, The Star is Located at 436 Light Years Away From Earth

## Information

* Mass: 3.617 Solar Masses
* Radius: 23.51 Solar Radius
* Luminosity: 316 Solar Luminosities
* Temperature: 5,003 Kelvin
* Spectral Type: K1III-K2III
* Right Ascension: 17h 16m 29.3988s
* Declination: +60° 40' 14.207"
* Apparent Magnitude (V): +6.318

### Other Designations

VW Draconis, HD 156947, HR 6448, HIP 84496, SAO 17414, BD +60° 1743, IRAS 17158+6043, TYC 4198-1813-1, 2MASS J17162940+6040142
YZ Persei

Object type: Red supergiant star
Number of stars: 1
Total mass: 18.9-22.6 Solar Masses (19,798-23,674 Jupiter Masses; 6,292,963-7,524,919 Earth Masses; 37,582-44,939 Septillion Tonnes)
Distance from the sun: ~7,800 ly

YZ Persei, Also Named **HD 236979**, **BD +56° 673** or **IRAS 02347+5649**, is a Red Supergiant Stars in The Constellation Perseus, The Star is Located at Around 7,800 Light Years Away From Earth

The name HDE 236979 derives directly from the fact that the star is the 236,979th stars in the Henry Draper catalogue

The name HIP 12302 derives directly from the fact that the star is the 12,302nd stars in the Hipparcos catalogue, and The name SAO 23484 derives directly from the fact that the star is the 23,484th stars in the Smithsonian Astrophysical Star catalogue

If YZ Persei was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, Mars, and even Ceres, Because YZ Persei's size was 698 to 785 times large as the sun

## Information

* Mass: 18.9-22.6 Solar Masses (19,798-23,674 Jupiter Masses; 6,292,963-7,524,919 Earth Masses; 37,582-44,939 Septillion Tonnes)
* Radius: 698-785 Solar Radius (972,093,432-1,093,256,940 km in Diameter; 3.24902-3.65399 AU; 487,204-616,225 Solar Areas or 340,068,392-483,736,625 Solar Volumes)
* Luminosity: 89,424-123,378 Solar Luminosities
* Temperature: 3,778-3,861 Kelvin (3,505-3,588 °C; 6,341-6,490 °F)
* Spectral Type: M1Iab-M2Iab
* Right Ascension: 02h 38m 25.4198s
* Declination: +57° 02' 46.194"
* Apparent Magnitude (V): +10.01
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

YZ Persei, HD 236979, HIP 12302, SAO 23484, BD +56° 673, IRAS 02347+5649, TYC 3695-1477-1, IRC +60093, 2MASS J02382544+5702462
Tejat Posterior

Tejat Posterior, Also Named **Mu Geminorum** or **HD 44478**, is a Red Giant Stars in The Constellation Gemini, The Star is Located at 244 Light Years Away From Earth

## Information

* Mass: 2.455-2.603 Solar Masses
* Radius: 88-103 Solar Radius
* Luminosity: 1,132-1,854 Solar Luminosities
* Temperature: 3,569-3,732 Kelvin
* Spectral Type: M2III-M4III
* Right Ascension: 06h 22m 57.62686s
* Declination: +22° 30' 48.8979"
* Apparent Magnitude (V): +2.868 (+2.749 to +3.017)
* Variable Star Type: Irregular Variable Star

### Other Designations

Tejat Posterior, Mu Geminorum, 13 Geminorum, HD 44478, HR 2286, HIP 30343, SAO 78297, BD +22° 1304, IRAS 06199+2232, IRC +20144, TYC 1878-1429-1, 2MASS J06225762+2230490
V2024 Sagittarii

Object type: Mira variable star
Number of stars: 1
Total mass: 0.9-2.1 Solar Masses (943-2,200 Jupiter Masses; 299,665-699,218 Earth Masses; 1,790-4,176 Septillion Tonnes)
Distance from the sun: ~21,000 ly

V2024 Sagittarii is a Red Giant Stars in The Constellation Sagittarius, The Star is Located at Around 21,000 Light Years Away From Earth

If V2024 Sagittarii was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, and even Mars, Because V2024 Sagittarii's size was 309 to 357 times large as the sun

## Information

* Mass: 0.9-2.1 Solar Masses (943-2,200 Jupiter Masses; 299,665-699,218 Earth Masses; 1,790-4,176 Septillion Tonnes)
* Radius: 309-357 Solar Radius (430,339,356-497,188,188 km in Diameter; 1.43832-1.66175 AU; 95,481-127,449 Solar Areas or 29,503,629-45,499,293 Solar Volumes)
* Luminosity: 7,711-12,073 Solar Luminosities
* Temperature: 3,077-3,202 Kelvin (2,804-2,929 °C; 5,079-5,304 °F)
* Spectral Type: M6IIIe-M7IIIe
* Right Ascension: 18h 41m 10.7004s
* Declination: -25° 29' 13.479"
* Apparent Magnitude (K): +6.718
* Variable Star Type: Mira Variable Star

### Other Designations

V2024 Sagittarii, 2MASS J18411069-2529133
WX Piscium

Object type: Red supergiant star
Number of stars: 1
Total mass: 19.8-27.1 Solar Masses (20,741-28,387 Jupiter Masses; 6,592,628-9,023,243 Earth Masses; 39,372-53,888 Septillion Tonnes)
Distance from the sun: ~14,000 ly

WX Piscium, Also Named **IRAS 01037+1219**, is a Red Supergiant Stars in The Constellation Pisces, The Star is Located at Around 14,000 Light Years Away From Earth

If WX Piscium was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, Mars, Ceres, and even Jupiter, Because WX Piscium's size was 1,014 to 1,143 times large as the sun

## Information

* Mass: 19.8-27.1 Solar Masses (20,741-28,387 Jupiter Masses; 6,592,628-9,023,243 Earth Masses; 39,372-53,888 Septillion Tonnes)
* Radius: 1,014-1,143 Solar Radius (1,412,181,576-1,591,837,812 km in Diameter; 4.71993-5.32039 AU; 1,028,196-1,306,449 Solar Areas or 1,042,590,744-1,493,271,207 Solar Volumes)
* Luminosity: 135,391-204,594 Solar Luminosities
* Temperature: 3,477-3,631 Kelvin (3,204-3,358 °C; 5,799-6,076 °F)
* Spectral Type: M3Iab-M4Iab
* Right Ascension: 01h 06m 25.9879s
* Declination: +12° 35' 52.896"
* Apparent Magnitude (K): +2.22
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

WX Piscium, IRAS 01037+1219, IRC +10011, 2MASS J01062598+1235530, SDSS J010625.97+123553.1
V487 Cassiopeiae

Object type: Yellow 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: ~18,000 ly

V487 Cassiopeiae, Also Named **HD 6474**, **BD +63° 141** or **IRAS 01037+6330**, is a Yellow Hypergiant Stars in The Constellation Cassiopeia, The Star is Located at Around 18,000 Light Years Away From Earth

The name HD 6474 derives directly from the fact that the star is the 6,474th 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 5239 derives directly from the fact that the star is the 5,239th stars in the Hipparcos catalogue, and The name SAO 33693 derives directly from the fact that the star is the 33,693rd 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: 431-489 Solar Radius (600,246,804-681,022,476 km in Diameter; 2.0062-2.27618 AU; 185,761-239,121 Solar Areas or 80,062,991-116,930,169 Solar Volumes)
* Luminosity: 167,858-228,939 Solar Luminosities
* Temperature: 5,626-5,709 Kelvin (5,353-5,436 °C; 9,667-9,817 °F)
* Spectral Type: G4Ia0-Ia
* Right Ascension: 01h 06m 59.7403s
* Declination: +63° 46' 23.393"
* Apparent Magnitude (V): +7.5998

### Other Designations

V487 Cassiopeiae, HD 6474, HIP 5239, SAO 11581, BD +63° 141, IRAS 01037+6330, TYC 4025-1704-1, 2MASS J01065972+6346234
Zaurak

Zaurak, Also Named **Gamma Eridani** or **HD 25025**, is a Red Giant Stars in The Constellation Eridanus, The Star is Located at 209 Light Year Away From Earth

## Information

* Mass: 3.621 Solar Masses
* Radius: 84.47 Solar Radius
* Luminosity: 1,537 Solar Luminosities
* Temperature: 3,926 Kelvin
* Spectral Type: M0III
* Right Ascension: 03h 58m 01.7669s
* Declination: -13° 30' 30.669"
* Apparent Magnitude (V): +2.94 (+2.88 to +2.96)
* Variable Star Type: Slow Irregular Variable Star

### Other Designations

Zaurak, Gamma Eridani, 34 Eridani, HD 25025, HR 1231, HIP 18543, SAO 149283, BD -13° 781, IRAS 03557-1339, IRC -10055, TYC 5311-1285-1, 2MASS J03580177-1330310
V432 Carinae

Object type: Blue hypergiant star
Number of stars: 1
Total mass: 65-80 Solar Masses (68,088-83,800 Jupiter Masses; 21,642,465-26,636,880 Earth Masses; 129,251-159,078 Septillion Tonnes)
Distance from the sun: ~36,000 ly

V432 Carinae, Also Named **IRAS 11065-6026**, is a Blue Hypergiant Stars in The Constellation Carina, The Star is Located at Around 36,000 Light Years Away From Earth

## Information

* Mass: 65-80 Solar Masses (68,088-83,800 Jupiter Masses; 21,642,465-26,636,880 Earth Masses; 129,251-159,078 Septillion Tonnes)
* Radius: 63-83 Solar Radius (87,739,092-115,592,772 km in Diameter; 0.29325-0.38634 AU; 3,969-6,889 Solar Areas or 250,047-571,787 Solar Volumes)
* Luminosity: 622,700-1,287,000 Solar Luminosities
* Temperature: 20,428-21,340 Kelvin (20,155-21,067 °C; 36,311-37,952 °F)
* Spectral Type: B2Ieq-B3Ieq or B4Ia0-B5Ia0
* Right Ascension: 11h 08m 40.0634s
* Declination: -60° 42' 51.721"
* Apparent Magnitude (V): +10.1989
* Variable Star Type: Candidate Luminous Blue Variable Star

### Other Designations

V432 Carinae, IRAS 11065-6026, Hen 3-591, Wray 15-751, 2MASS J11084006-6042516
V743 Cassiopeiae

Object type: Red supergiant star
Number of stars: 1
Total mass: 25 Solar Masses (26,188 Jupiter Masses; 8,324,025 Earth Masses; 49,712 Septillion Tonnes)
Distance from the sun: 4,384 ly

V743 Cassiopeiae, Also Named **HD 1613**, **BD +61° 43** or **IRAS 00179+6136**, is a Red Supergiant Stars in The Constellation Cassiopeia, The Star is Located at 4,384 Light Years Away From Earth

The name HD 1613 derives directly from the fact that the star is the 1,613th 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 1652 derives directly from the fact that the star is the 1,652nd stars in the Hipparcos catalogue, and The name SAO 11123 derives directly from the fact that the star is the 11,123rd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 25 Solar Masses (26,188 Jupiter Masses; 8,324,025 Earth Masses; 49,712 Septillion Tonnes)
* Radius: 981-1,055 Solar Radius (1,366,223,004-1,469,281,620 km in Diameter; 4.56632-4.91077 AU; 962,361-1,113,025 Solar Areas or 944,076,141-1,174,241,375 Solar Volumes)
* Luminosity: 170,364-223,078 Solar Luminosities
* Temperature: 3,744-3,862 Kelvin (3,471-3,589 °C; 6,280-6,492 °F)
* Spectral Type: M1Iab-M2Iab
* Right Ascension: 00h 20m 43.5631s
* Declination: +61° 52' 46.543"
* Apparent Magnitude (V): +6.95
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V743 Cassiopeiae, HD 1613, HIP 1652, SAO 11123, BD +61° 43, IRAS 00179+6136, IRC +60007, TYC 4019-3948-1, 2MASS J00204356+6152465
V923 Centauri

Object type: Red supergiant star
Number of stars: 1
Total mass: 25 Solar Masses (26,188 Jupiter Masses; 8,324,025 Earth Masses; 49,712 Septillion Tonnes)
Distance from the sun: 11,382 ly

V923 Centauri, Also Named **HD 103052**, **CD -60° 3809**, **CP -60° 3442** or **IRAS 11492-6052**, is a Red Supergiant Stars in The Constellation Centaurus, The Star is Located at 11,382 Light Years Away From Earth

The name HD 103052 derives directly from the fact that the star is the 103,052nd 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 57843 derives directly from the fact that the star is the 57,843rd stars in the Hipparcos catalogue, and The name SAO 251615 derives directly from the fact that the star is the 251,615th stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 25 Solar Masses (26,188 Jupiter Masses; 8,324,025 Earth Masses; 49,712 Septillion Tonnes)
* Radius: 888-937 Solar Radius (1,236,703,392-1,304,944,908 km in Diameter; 4.13343-4.36151 AU; 788,544-877,969 Solar Areas or 700,227,072-822,656,953 Solar Volumes)
* Luminosity: 131,572-166,853 Solar Luminosities
* Temperature: 3,689-3,811 Kelvin (3,416-3,538 °C; 6,181-6,400 °F)
* Spectral Type: M2Iab-M3Iab
* Right Ascension: 11h 51m 42.9366s
* Declination: -61° 09' 30.386"
* Apparent Magnitude (V): +7.8998
* Variable Star Type: Semi-Regular Variable Star

### Other Designations

V923 Centauri, HD 103052, HIP 57843, SAO 251615, CD -60° 3809, CP -60° 3442, IRAS 11492-6052, TYC 8973-1012-1, 2MASS J11514295-6109303
UX Hydrae

UX Hydrae is a Red Supergiant Star or an Thorne-Zytkow Objects in The Constellation Hydra, The Star is Located at 76,000 Light Years Away From Earth

## Information

* Mass: 10 Solar Masses
* Radius: 712-836 Solar Radius
* Luminosity: 35,394-68,366 Solar Luminosities (48,000-54,000 Solar Luminosities)
* Temperature: 2,967-3,228 Kelvin (2,694-2,955 °C; 4,881-5,351 °F)
* Spectral Type: C7,8-C8,9 or M6Iae-M7Iae
* Right Ascension: 08h 42m 33.0194s
* Declination: +06° 21' 19.673"
* Apparent Magnitude (V): +13.59
* Variable Star Type: Mira Variable Star
V382 Carinae

V382 Carinae, Also Named **HD 96918**, is a Yellow Hypergiant Stars in The Constellation Carina, The Star is Located at 10,000 Light Years Away From Earth

## Information

* Mass: 45-60 Solar Masses (2020-Present), 26-39 Solar Masses (2016-2020) or 15-45 Solar Masses (1980-2016)
* Radius: 613-788 Solar Radius
* Luminosity: 375,000-650,000 Solar Luminosities
* Temperature: 5,880 Kelvin
* Spectral Type: G0Ia0-G4Ia0
* Right Ascension: 11h 08m 35.39s
* Declination: -58° 58' 30.135"
* Apparent Magnitude (V): +3.83

### Other Designations

V382 Carinae, x Carinae, HD 96918, HR 4337, HIP 54463, SAO 238813, CD -58° 3855, CP -58° 3189, IRAS 11064-5842, TYC 8628-2484-1, 2MASS J11083542-5858300
V1000 Cassiopeiae

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: ~14,000 ly

V1000 Cassiopeiae, Also Named **IRAS 23472+5656**, is a Red Giant Stars in The Constellation Cassiopeia, The Star is Located at Around 14,000 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: 459-511 Solar Radius (639,241,956-711,661,524 km in Diameter; 2.13653-2.37858 AU; 210,681-261,121 Solar Areas or 96,702,579-133,432,831 Solar Volumes)
* Luminosity: 17,282-25,543 Solar Luminosities
* Temperature: 3,089-3,228 Kelvin (2,816-2,955 °C; 5,101-5,351 °F)
* Spectral Type: M6IIIe-M7IIIe
* Right Ascension: 23h 49m 43.7609s
* Declination: +57° 13' 12.432"
* Apparent Magnitude (H): +7.18
* Apparent Magnitude (K): +6.513
* Variable Star Type: Mira Variable Star

### Other Designations

V1000 Cassiopeiae, IRAS 23472+5656, 2MASS J23494374+5713123
U Lacertae

U Lacertae, Also Named **HD 215924**, is a Red Supergiant Stars in The Constellation Lacerta, The Star is Located at 13,922 Light Years Away From Earth

## Information

* Mass: 27 Solar Masses
* Radius: 1,032 Solar Radius
* Luminosity: 173,000 Solar Luminosities
* Temperature: 3,665 Kelvin
* Spectral Type: M4Iab
* Right Ascension: 22h 47m 43.4268s
* Declination: +55° 09' 30.312"
* Apparent Magnitude (V): +9.39
* Variable Star Type: Semi Regular Variable Star

### Other Designations

U Lacertae, HD 215924, HIP 112545, BD +54° 2863, IRAS 22456+5453, IRC +50446, TYC 3988-1641-1, 2MASS J22474341+5509303
V4020 Sagittarii

V4020 Sagittarii, Also Named **AK Sagittarii**, **HD 170034** or **IRAS 18251-1647**, is a Cold Red Giant Stars in The Constellation Sagittarius, The Star is Located at 5,565 Light Years Away From Earth

The name HD 170034 derives directly from the fact that the star is the 170,034th 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: 0.971-1.054 Solar Masses (1,017-1,104 Jupiter Masses; 323,305-350,941 Earth Masses; 1,931-2,096 Septillion Tonnes)
* Radius: 487-551 Solar Radius (678,237,108-767,368,884 km in Diameter; 2.26687-2.56477 AU; 237,169-303,601 Solar Areas or 115,501,303-167,284,151 Solar Volumes)
* Luminosity: 9,163-14,711 Solar Luminosities
* Temperature: 2,559-2,708 Kelvin (2,286-2,435 °C; 4,147-4,415 °F)
* Spectral Type: C8,9-C9,10 or M9III-M10III
* Right Ascension: 18h 28m 00.6184s
* Declination: -16° 45' 32.817"
* Apparent Magnitude (V): +11.5
* Variable Star Type: Mira Variable Star
* Evolutionary Stage: Asymptotic Giant Branch

### Other Designations

V4020 Sagittarii, AK Sagittarii, HD 170034, IRAS 18251-1647, IRC -20484, 2MASS J18280062-1645328
UDF 2457

UDF 2457, Also Named **Preg Sector B4-53**, is an Red Dwarf Stars in The Constellation Fornax, The Star is Located at 61,227 Light Years Away From Earth

## Information

* Mass: 0.626 Solar Masses
* Radius: 0.567 Solar Radius
* Luminosity: 7.18% Solar Luminosities
* Temperature: 3,962 Kelvin (3,689 °C; 6,672 °F)
* Age: 1.8 Billion Years
* Spectral Type: M0V
* Metallicity [Fe/H]: +0.21 dex
* Right Ascension: 03h 32m 38.788s
* Declination: -27° 48' 10.03"
* Apparent Magnitude (V): +25.023
* Estimated Value: 6,726 CR
* Total Population: 1,153
V781 Cassiopeiae

Object type: Yellow supergiant star
Number of stars: 1
Total mass: 18-24 Solar Masses (18,855-25,140 Jupiter Masses; 5,993,298-7,991,064 Earth Masses; 35,792-47,723 Septillion Tonnes)
Distance from the sun: ~14,400 ly

V781 Cassiopeiae, Also Named **HD 12399**, **BD +63° 277** or **IRAS 02000+6359**, is a Yellow Supergiant Stars in The Constellation Cassiopeia, The Star is Located at Around 14,400 Light Years Away From Earth

The name HD 12399 derives directly from the fact that the star is the 12,399th 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 9635 derives directly from the fact that the star is the 9,635th stars in the Hipparcos catalogue, and The name SAO 12102 derives directly from the fact that the star is the 12,102nd stars in the Smithsonian Astrophysical Star catalogue

## Information

* Mass: 18-24 Solar Masses (18,855-25,140 Jupiter Masses; 5,993,298-7,991,064 Earth Masses; 35,792-47,723 Septillion Tonnes)
* Radius: 311-358 Solar Radius (433,124,724-498,580,872 km in Diameter; 1.44763-1.6664 AU; 96,721-128,164 Solar Areas or 30,080,231-45,882,712 Solar Volumes)
* Luminosity: 68,357-102,173 Solar Luminosities
* Temperature: 5,292-5,454 Kelvin (5,019-5,181 °C; 9,066-9,358 °F)
* Spectral Type: G6Ia-G8Ia
* Right Ascension: 02h 03m 49.1245s
* Declination: +64° 14' 14.953"
* Apparent Magnitude (V): +7.49

### Other Designations

V781 Cassiopeiae, HD 12399, HIP 9635, SAO 12102, BD +63° 277, IRAS 02000+6359, TYC 4041-724-1, 2MASS J02034911+6414146
V1890 Cygni

V1890 Cygni is a Red Supergiant Stars in The Constellation Cygnus, The Star is Located at 21,081 Light Years Away From Earth

## Information

* Mass: 20.64-23.19 Solar Masses (21,620-24,292 Jupiter Masses; 6,872,315-7,721,366 Earth Masses; 41,042-46,113 Septillion Tonnes)
* Radius: 843-951 Solar Radius (1,174,032,612-1,324,442,484 km in Diameter; 3.92396-4.42668 AU; 710,649-904,401 Solar Areas or 599,077,107-860,085,351 Solar Volumes)
* Luminosity: 105,400-148,000 Solar Luminosities
* Temperature: 3,582-3,671 Kelvin (3,309-3,398 °C; 5,988-6,148 °F)
* Spectral Type: M3Iab-M4Iab
* Right Ascension: 20h 57m 46.8512s
* Declination: +35° 58' 02.845"
* Apparent Magnitude (V): +11.9968
* Variable Star Type: Semi-Regular Variable Star
Ten Most Terrible Disasters

This is Top 10 Natural Disasters is Depending Severity from Disasters

# Content

## Number Ten: April 2015 Nepal earthquake

The April 2015 Nepal earthquake is a Richter Magnitude 8.1 earthquakes struck Kathmandu, Nepal on April 25, 2015, The earthquake is triggered landslides and avalanches, caused devastating damages

### Information

* Earthquake magnitude: 8.1
* Total damages: $8.8 Billion dollars
* Casualties: 8,964 deaths and 21,952 injuries
Timeline of a 71 Jupiter Masses Brown Dwarfs

This is Timeline of a 71 Jupiter Masses Brown Dwarfs, The Brown Dwarf Have 2 Planets

## Information

* Mass: 71 Jupiter Masses
* Radius: 1.64 Jupiter Radius
* Initial Temperature: 2,150 °C (2,423 Kelvin)
* Initial Spectral Type: M9.5V

## Planet Information

* Planet A: 1.09 Earth Radius, 1.37 Earth Masses, 0.079 AU, Terrestrial Planet
* Planet B: 0.76 Jupiter Radius, 1.07 Jupiter Masses, 0.187 AU, Gas Giant
Westerlund 1-26

Object type: Red hypergiant star
Number of stars: 1
Total mass: 30-40 Solar Masses (31,425-41,900 Jupiter Masses; 9,988,830-13,318,440 Earth Masses; 59,654-79,539 Septillion Tonnes)
Distance from the sun: ~14,200 ly

Westerlund 1-26 is a Red Hypergiant Stars in The Super Star Cluster Westerlund 1, The Star is Located at Around 14,200 Light Years Away From Earth

If Westerlund 1-26 was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, Mars, Ceres, and even Jupiter

## Information

* Mass: 30-40 Solar Masses (31,425-41,900 Jupiter Masses; 9,988,830-13,318,440 Earth Masses; 59,654-79,539 Septillion Tonnes)
* Radius: 1,518-1,842 Solar Radius (2,114,094,312-2,565,323,928 km in Diameter; 7.06592-8.57407 AU; 2,304,324-3,392,964 Solar Areas or 3,497,963,832-6,249,839,688 Solar Volumes)
* Luminosity: 272,567-480,594 Solar Luminosities
* Temperature: 3,385-3,541 Kelvin (3,112-3,268 °C; 5,633-5,914 °F)
* Spectral Type: M4Ia0-M5Ia0
* Right Ascension: 16h 47m 05.4077s
* Declination: -45° 50' 36.617"
* Apparent Magnitude (B): +22.1
* Apparent Magnitude (V): +16.79
* Apparent Magnitude (R): +12.63
* Apparent Magnitude (G): +11.31
* Apparent Magnitude (I): +9.19
* Apparent Magnitude (J): +4.309
* Apparent Magnitude (H): +1.351
* Variable Star Type: Semi-Regular Variable Star
V354 Cephei

Object type: Red supergiant star
Number of stars: 1
Total mass: 30-40 Solar Masses (31,425-41,900 Jupiter Masses; 9,988,830-13,318,440 Earth Masses; 59,654-79,539 Septillion Tonnes)
Distance from the sun: ~16,000 ly

V354 Cephei, Also Named **IRAS 22317+5838**, is a Red Supergiant Stars in The Constellation Cepheus, The Star is Located at Around 16,000 Light Years Away From Earth

If V354 Cephei was placed into center of the solar system, that It's will engulf Mercury, Venus, Earth, Mars, Ceres, and even Jupiter

## Information

* Mass: 30-40 Solar Masses (31,425-41,900 Jupiter Masses; 9,988,830-13,318,440 Earth Masses; 59,654-79,539 Septillion Tonnes)
* Radius: 1,447-1,608 Solar Radius (2,015,213,748-2,239,435,872 km in Diameter; 6.73544-7.48485 AU; 2,093,809-2,585,664 Solar Areas or 3,029,741,623-4,157,747,712 Solar Volumes)
* Luminosity: 309,167-447,082 Solar Luminosities
* Temperature: 3,578-3,722 Kelvin (3,305-3,449 °C; 5,981-6,240 °F)
* Spectral Type: M2Ia-M3Ia
* Right Ascension: 22h 33m 34.6356s
* Declination: +58° 53' 47.124"
* Apparent Magnitude (V): +10.9
* Apparent Magnitude (G): +8.201
* Apparent Magnitude (J): +3.915
* Apparent Magnitude (H): +2.565
* Apparent Magnitude (K): +1.869
* Variable Star Type: Semi-Regular Variable Star or Slow Irregular Variable Star

### Other Designations

V354 Cephei, IRAS 22317+5838, IRC +60361, RAFGL 2922, TYC 3995-449-1, 2MASS J22333464+5853470