Introduction
WR 25, also known as HD 93162, 2MASS J10441038-5943111, Hen 3-478, SAO 238408, XMMU J104410.3-594311, CD-59°3282,PPM 339385, PPM 339385, Trumpler 16 177, GSC 08626-01989 and UBV 9882, is a binary star system located in the Carina constellation. WR 25 has a mass of 98 Solar Masses, a radius of 20.24 Solar Radius, a luminosity of 2,400,000 Solar Luminosity, an orbital period of 207.85 Earth Days and a temperature of 50,100 Kelvin or 49827 degrees Celsius or 89720 degrees Fahrenheit. WR 25 is located 6425.281 Light Years from Earth inside The Carina Nebula. 
Information about WR 25
The Main Star of WR 25 is 2.4 Million Fold the brightest of The Sun. WR 25 contains a Wolf-Rayet Stars, giving it the name WR 25. 

Introduction
Sneden's Star, also known as BPS CS 22892-0052 or HE 2214-1654, is an Old Population II Star located inside the Aquarius Constellation. Sneden's star has mass of 1.13 Solar Masses, a radius of 13.8 Solar Radius and a surface gravity of 1.15 Centimetre-gram-second system of units. Sneden's Star is 13 Billion Years Old and has temperature of 4690 Kelvin or 4417 degrees Celsius or 7982 degrees Fahrenheit. Sneden's Star is around 17,000 Light Years from Earth. 
Information about Sneden's Star
Sneden's Star was discovered in 1995 by American Astrophysicist Timothy C. Beers using the Curtis Schmidt Telescope in Chile. Over the years of it's knowing-of, Sneden's Star has been observed to contain 53 Elements inside of it, which is only beaten by The Sun as far as observed chemical elements goes.

Introduction
Are you stuck in the past with your old and rusty Supernova 1000? Do you want to upgrade to a more futuristic, hip and cool Supernova? Well boy, do I have the deal for you! Introducing, Supernova 2000!
Supernova 2000
Supernova 2000, also known as Supernova 2000a and SN 2000A, is a Type 1A Supernova located inside NGC 7674. That's all folks!

Introduction
Supernova 2010, also known as Supernova 2010it and SN 2010it, is a Type 1A Supernova located inside NGC 1417. 

Introduction
Are you tired of your old, outdated and lame Supernova? Is your old Supernova acting up? Is your old Supernova an eye sore? Well no worries my friend. For The Supernova 1000 is here! 
​Supernova 1000
Supernova 1000, also known as Supernova 1000+0216 and SN 1000+0216 is a Super Extreme Remote Superluminous Supernova was exploded in June of 2006 and November of 2006. It was so big that it was still detectable in November of 2008. 

Introduction
A Supernova is big, but is it the largest nova? Not at all, for there is an even more extreme supernova. This astronomical event is known as a Hypernova.
​

Introduction
Supernova 185, also known as SN 185, SNR G315.0-02.3, SNR G315.4-02.3, 1ES 1436-62.4, 1RXS J144254.3-622815, 3FHL J1443.0-6227e, AJG 27, 3A 1438-626, GPS 1438-624, MSH 14-6-03 and 2FHL J1443.2-6221e is a Type 1A Supernova located inside The Centaurus Constellation and The Circinus Constellation. Supernova 185 is located inside The Milky Way Galaxy 9100 Light Years from Earth. The Supernova 185 explosion event occurred on December 7th 185 AD and was seen by Ancient Chinese Astronomers and Emperor Lo Yang. 

Introduction
Champagne Supernova, also known as W49B, SNR G043.3-00.2, 1ES 1908+09.0, 3C 398, 3C 398.0, 4C 09.63, 3FHL J1911.0+0905, 3CR 398, AJG 95, 2FGL J1911.0+0905, 3FGL J1910.9+0906 and 2FHL J1911.0+0905, is a Nebula that is a Supernova Remnant from likely a Type 1B Supernova or Type 1C Supernova located inside The Aquila Constellation. Champagne Supernova is located 33,000 Light Years from Earth. The Supernova is believed to have occurred 1,000 Years Ago and is also believed to have left a Black Hole Remnant. 

What is it?
An Imposter, is one who poses as someone or something that they are not. Perhaps like a mocking bird who mimics the voice of another bird in order to draw in prey for the hunt. This can happen in space as well; more specifically with supernovae. This fake is known as a supernova imposter. Supernova imposters are interstellar explosions that at first are thought and seen to be supernovae, alas this explosion is not the result of the death of the host star. Therefore instead of being classified as supernova, which would require a stars death, this explosion is called a Supernova Imposter. They are also known as Type V Supernovae, Extra-Powerful Novae, Eta Carinae analogs and giant eruptions of luminous blue variables or LBV. Some discovered Supernova Imposters are The Great Eruption of Eta Carinae, SN 1954J, SN 2008S and NGC 6946. 

​PS: This Supernova is Sus

Introduction
The King Supernova, also known as King Supernova, SN 1993J, AAVSO 0947+69, ICRF J095524.7+690113, INTREF 395 and PBC J0955.1+6904, is a Type II Supernova inside The Ursa Major Constellation. The King Supernova is located inside The M81 Galaxy. The King Supernova is the second-brightest Supernova ever discovered in the twentieth century. The King Supernova was discovered on March 28th, 1993 by Astronomer F. Garcia.  The King Supernova came from a K-Type Supergiant Star that had a Super Totally Awesome Explosion, resulting in The Creation of The King Supernova!

Introduction
Tycho's Supernova, also known as SN 1572, HR 92, SN 1572A, SNR G120.1+01.4, SNR G120.2+01.4, 1ES 0022+63.8, 1RXS J002509.2+640946, B Cas, BD+63 39a, 8C 0022+638, 4C 63.01, 3C 10, 3C 10.0, 2C 34, RRF 1174, 1XRS 00224+638, 2U 0022+63, 3A 0022+638, 3CR 10, 3U 0022+63, 4U 0022+63, AJG 112, ASB 1, BG 0022+63, CTB 4, KR 101, VRO 63.00.01, [DGW65] 3, PBC J0024.9+6407, F3R 3628, WB 0022+6351, CGPSE 107 and GB6 B0022+6352, is a Type 1A Supernova located inside The Cassiopeia Constellation. Tycho's Supernova is inside The Milky Way Galaxy. Tycho's Supernova is from 8000 to 9800 Light Years from Earth. Tycho's Supernova appeared in November 1572, The same year England and France sign an anti-Spanish Military Convenant. 

List of All 110 Messier Objects
1. Crab Nebula(M1)
2. NGC 7089 (M2)
3. NGC 5272 (M3)
4. NGC 6121 (M4)
5. NGC 5904 (M5)
6. Butterfly Cluster (M6)
7. Ptolemy Cluster (M7)
8. Lagoon Nebula (M8)
9. NGC 6333(M9)
10. NGC 6254 (M10)
11. Wild Duck Cluster (M11)
12. NGC 6218 (M12)
13. Great Globular Cluster in Hercules (M13)
14. NGC 6402 (M14)
15. NGC 7078 (M15)
16. Eagle Nebula (M16)
17. Omega, Swan, Horseshoe or Lobster Nebula (M17)
18. NGC 6613 (M18)
19. NGC 6273 (M19)
20. Trifid Nebula (M20)
21. NGC 6531 (M21)
22. Sagittarius Cluster (M22)
23. NGC 6494 (M23)
24. Sagittarius Star Cloud (M24)
25. IC 4725 (M25)
26. NGC 6694 (M26)
27. Dumbbell Nebula (M27)
28. NGC 6626 (M28)
29. Cooling Tower (M29)
30. NGC 7099 (M30)
31. Andromeda Galaxy (M31)
32. NGC 221 (M32)
33. Triangulum Galaxy (M33)
34. NGC 1039 (M34)
35. NGC 2168 (M35)
36. NGC 1960 (M36)
37. NGC 2099 (M37)
38. NGC 1912 (M38)
39. NGC 7092 (M39)
40. Winnecke 4 (M40)
41. NGC 2287 (M41)
42. Orion Nebula (M42)
43. De Mairan's Nebula (M43)
44. Beehive Cluster (M44)
45.Pleiades (M45)
46. NGC 2437 (M46)
47. NGC 2422 (M47)
48. NGC 2548 (M48)
49. NGC 4472 (M49)
50. NGC 2323 (M50)
51. Whirlpool Galaxy (M51)
52. NGC 7654 (M52)
53. NGC 5024 (M53)
54. NGC 6715 (M54)
55. NGC 6809 (M55)
56. NGC 6779 (M56)
57. Ring Nebula (M57)
58. NGC 4579 (M58)
59. NGC 4621 (M59)
60. NGC 4649 (M60)
​61. NGC 4303 (M61)
62. NGC 6266 (M62)
63. Sunflower Galaxy (M63)
64. Black Eye Galaxy (M64)
65. Leo Triplet NGC 3623 (M65)
66. Leo Triplet NGC 3627 (M66)
67. NGC 2682 (M67)
68. NGC 4590 (M68)
69. NGC 6637 (M69)
70. NGC 6681 (M70)
71. NGC 6838 (M71)
72. NGC 6981 (M72)
73. NGC 6994 (M73)
74. Phantom Galaxy (M74)
75. NGC 6864 (M75)
76. Little Dumbbell Nebula (M76)
77. Cetus A (M77)
78. NGC 2068 (M78)
79. NGC 1904 (M79)
80. NGC 6093 (M80)
81. Bode's Galaxy (M81)
82. Cigar Galaxy (M82)
83. Southern Pinwheel Galaxy (M83)
84. NGC 4374 (M84)
85. NGC 4382 (M85)
86. NGC 4406 (M86)
87. Virgo A (M87)
88. NGC 4501 (M88)
89. NGC 4552 (M89)
90. NGC 4569 (M90)
91. NGC 4548 (M91)
92. NGC 6341 (M92)
93. NGC 2447 (M93)
94. Croc's Eye or Cat's Eye (M94)
95. NGC 3351 (M95)
96. NGC 3368 (M96)
97. Owl Nebula (M97)
98. NGC 4192 (M98)
99. NGC 4254 (M99)
100. NGC 4321 (M100)
101. Pinwheel Galaxy (M101)
102. Spindle Galaxy (M102)
103. NGC 581 (M103)
104. Sombrero Galaxy (M104)
105. NGC 3379 (M105)
106. NGC 4258 (M106)
107. NGC 6171 (M107)
108. NGC 3556 (M108)
109. NGC 3992 (M109)
​110. NGC 205 (M110)

Introduction
Ogma, also known as HD 149026, Ogma, BD+38°2787, GSC 03063-01587, HIP 80838 and SAO 65349, is a Yellow Subgiant star located inside The Hercules Constellation. Ogma has a planet orbiting it called b Smetrios. Ogma has a mass of 1.345 Solar Masses, a radius of 1.541 Solar Radiuses and a luminosity of 3.03 Solar Luminosities. Ogma has a surface gravity of 4.189 centimeter-gram-second system of units and a temperature of 6147 Kelvin. Ogma is 2.6 Billion Years Old. Ogma is 250 Light Years from The Sun. 

Introduction
Peacock Star, also known as Peacock, α-Pav, HR 7790, HD 193924, NSV 13060,  HIP 100751, CD-57° 9674, FK5 764, SAO 246574 and TYC 8785-1898-1, is a Binary Star located inside The Pavo Constellation. Peacock has a mass of 5.91 Solar Masses, a radius of 4.83 Solar Radiuses and a luminosity of 2200 Solar Luminosities. Peacock has a surface gravity of 3.94 centimeter-gram-second system of units and a temperature of 17,711 Kelvin. Peacock Star is 48 Million Years Old. Peacock is 179 Light Years from The Sun.  

Introduction
Navi, also known as Gamma Cassiopeiae, Tsih, γ Cas, 27 Cassiopeiae, ADS 782, BD+59°144, FK5 32, HD 5394, HIP 4427, HR 264, SAO 11482, WDS 00567+6043 and AAVSO 0050+60, is a subgiant star located inside Cassiopeia Constellation. Navi has a mass of 17 Solar Masses, a radius of 10 Solar Radiuses and a luminosity of 34,000 Solar Luminosities. Navi has a surface gravity of 3.5 centimeter-gram-second system of units and a temperature of 25,000 Kelvin. Navi is 8 Million Years Old. Navi is 550 Light Years from The Sun. 

Introduction
Meissa, also known as, λ Orionis, 39 Orionis, 101 G. Orionis, BD+09°879, HIP 26207 and SAO 112921, is a Multiple Star located inside The Orion Constellation. Meissa is 1,100 Light Years away from Earth. The two main stars are Meissa A, an O8 Giant Star and Meissa A, a B-Class Main Sequence Star. Very Cool!
Meissa A
Meissa A, also known as HD 36861 and HR 1879 is a O8 Giant Star. Meissa A has a mass of 279 Solar Masses, a solar radius of 4.2 Solar Radiuses and a luminosity of 165,000 Solar Luminosities. Meissa A has a surface gravity of 3.9 centimeter-gram-second system of units and a temperature of 37,689 Kelvin. 
Meissa B
Meissa B, also known as HD 36862 and HR 1880, is a B-Class Main Sequence Star. Meissa B has a mass of 10.3 Solar Masses, a radius of 4.2 Solar Radiuses and a luminosity of 6300 Solar Luminosities.  Meissa has a surface gravity of 4.21 centimeter-gram-second system of units and a temperature of 25,400 Kelvin. Meissa B is 1.8 Million Years Old. 

The Atlas Star
The Atlas Star, also known as Atlas, 27 Tau, BD+23° 557, FK5 142, HD 23850, HIP 17847, HR 1178 and SAO 76228 is a Triple Star system located inside The Taurus Constellation. The Atlas star is a part of The Pleiades Star Cluster or M45. The Atlas Star can be split precisely to Atlas A and Atlas B, Atlas C is not precise enough for specific measurements.
Atlas A
Atlas A has a mass of 4.74 Solar Masses and a radius of 2 Solar Radiuses. Atlas A has a surface gravity of 3.483 centimeter-gram-second system of units and temperature of 13,446 Kelvin. 
Atlas B
Atlas B has a mass of 3.42 Solar Masses. 

Introduction
Maia, also known as 20 Tauri, HR 1149, BD+23°516, HD 23408, HIP 17573, SAO 76155, GC 4500, NSV 01279 and WDS J03458+2422, is a Blue Giant Star located inside The Taurus Galaxy. Maia fourth brightest star inside M45 or The Pleiades Star Cluster. Maia has a mass of 5 Solar Masses, a radius of 6.04 Solar Radiuses and a luminosity of 850 Solar Luminosities. Maia has a temperature of 12,600 Kelvin.
Maia in The Classical World
In The Traditional Classical World Religion, Maia was the oldest of the seven sister known as The Pleiades. The Pleiades were the daughters of Atlas, The Titan who was punished by Zeus to hold the weight of The Universe on his back. Maia, in fact, was impregnated by The King of The gods, Zeus, and begot The Messenger god, Hermes. 

Introduction
La Superba, also known as The Superb, Y Canum Venaticorum, HR 4846, HD 110914, BD+46°1817, FK5 1327, HIP 62223, SAO 44317, GC 17342 and 152 Schjellerup, is a Red Giant Star located inside The Canes Venatici Constellation. La Superba is a carbon star giving it a Super Red Color. La Superba might hath a mass of 3 Solar Masses, a radius of 307 Solar Radiuses and a luminosity of 4853 Solar Radiuses. La Superba has a temperature of 2750 Kelvin. La Superba is 760 Light Years from The Sun.

Introduction
Hamal, also known as Hemal, Ras Hammel, El Nath, Arietis, α Ari, Alpha Arietis, Alpha Ari, 13 Arietis, 13 Ari, BD+22 306, FK5 74, GC 2538, GJ 84.3, GJ 9072, HD 12929, HIP 9884, HR 617, LTT 10711, NLTT 7032, PPM 91373 and SAO 75151, is a Red Giant Star located inside The Aries Constellation. Hamal is the brightest star inside The Aries Constellation and 50th Brightest Star in the night sky. Hamal has a mass of 1.5 Solar Masses, a radius of 14.9 Solar Radiuses and a luminosity of 91 Solar Luminosities. Hamal has a surface gravity of 2.57 centimeter-gram-second system of units and a temperature of 4480 Kelvin. Hamal is 3.4 Billion Years Old. Hamal is 65.8 Light Years from The Sun. 

Introduction
Pollux, also known as β Geminorum, 78 Geminorum, BD+28°1463, GCTP 1826.00, Gliese 286, HD 62509, HIP 37826, HR 2990, LFT 548, LHS 1945, LTT 12065 and SAO 79666, is an Orange-Hued Giant Star located inside The Gemini Constellation. Pollux is the brightest star in Gemini and the closest giant to The Sun. Pollux has a mass of 1.91 Solar Masses, a radius of 9.06 Solar Radiuses and a luminosity of 32.7 Solar Luminosities. Pollux has a surface gravity of 2.685 Centimetre-Gram-Second System of Units and a temperature of 4586 Kelvin. Pollux is 724 Million Years Old. Pollux is 33.78 Light Years from The Sun. 
Profile of Pollux
Pollux is twofold or double the mass of The Sun and ninefold the radius of The Sun. Pollux has evolved from its initial A-Type Main Sequence Star phase due to it using up its hydrogen core. Pollux is believed to possess a Planetary System effectively making it part of a Solar System like ours. The Planet known as Pollux B was found orbiting Pollux on June 16th, 2006. Pollux was observed being 2.3 fold the mass of Jupiter and having a revolution around Pollux of 590 Earth Days. 

Introduction
Denebola, also known as Deneb Aleet, β Leonis, 94 Leo, BD+15°2383, FK5 444, GCTP 2738.00, GJ 448, HD 102647, HIP 57632, HR 4534, LHS 2462, LTT 13249 and SAO 99809, is an A-Type Main Sequence Star located in The Leo Constellation (Lion Constellation). Denebola has a mass of 1.78 Solar Masses, a radius of 1.728 Solar Radiuses and a luminosity of 15 Solar Luminosities. Denebola has a surface gravity of 4.0 Centimetre-Gram-Second System of Units and a temperature of 8500 Kelvin. Denebola is is about 100 Million Years Old to 380 Million Years Old. Denebola is 36 Light Years from The Sun.
Profile of Denebola
Denebola is almost to two fold the mass of The Sun and 15 fold the luminosity of The Sun. Denebola is the second-brightest star in The Leo Constellation. The Traditional Name in Arabic, Denebola, is a condensed name of the full name Deneb Alased, which translated means The Tail of The Lion. Which is cool because Denebola is in The Lion Constellation, Leo Constellation. In Traditional Astrology, Denebola is believed to have inflicted misfortune and dishonor to man. In Ancient China, Chinese Astronomers said that Denebola, known to them as Wǔdìzuò-yī or 五帝座, was the First Star of The Five Star collective known as Seat of The Five Emperors. 

Introduction
Alcor, also known as g Ursae Majoris, 80 Ursae Majoris, BD+55 1603, CCDM J13240+5456D, GC 18155, HD 116842, HIP 65477, HR 5062, PPM 34021, SAO 28751 and WDS J13239+5456C, is a binary star system that is fainter companion of the quadruple star system Mizar that is located inside The Ursa Major Constellation. Alcor is 81.7 Light Years from The Sun. Alcor is split inside two camps, Alcor A and Alcor B. Alcor A
Alcor A has a mass of 1.84 Solar Masses, a radius of 1.846 Solar Radiuses and a luminosity of 14.03 Solar Luminosities. Alcor A has a surface gravity of 4.25 Centimetre-Gram-Second System of Units and a temperature of 8221 Kelvin. 
Alcor B
Alcor B has a mass of 0.25 Solar Masses and is 0.5 Billion Years Old. Alcor B is a Main Sequence Red Dwarf. 
Profile of Alcor
Alcor A and Alcor B are 1.2 Light Years apart from each other.  

Introduction
Gacrux, also known as Gacrux, CD−56 4504, γ Crucis, Gl 470, HD 108903, HIP 61084, HR 4763, LTT 4752 andSAO 240019, is a Red Giant Star located inside The Crux Constellation. Gacrux is the 26th brightest star in the night sky. Gacrux has a mass of 1.5 Solar Masses, a radius of 84 Solar Radiuses and a luminosity of 820 Solar Luminosities. Gacrux has temperature of 3626 Kelvin. Gacrux is 88.6 Light Years from The Sun making it the closest Giant Star to The Sun.
Profile of Gacrux
Gacrux is in its post Main Sequence Star phase and is projected to become a white dwarf at some point in the future just like The Sun. Gacrux is 84 fold the radius of The Sun. Gacrux was known in The Classical World, The Roman World and in Classical China. Gacrux is featured in the flags of some of The Nations of The World. These nations include Brazil, Australia, New Zealand and Papua New Guinea. 

Introduction
Alpha Pegasi, also known as Markab, Marchab, 54 Pegasi, HR 8781, BD +14°4926, HD 218045, SAO 108378, FK5 871 and HIP 113963, is an A-type subgiant star located in The Pegasus Constellation. Alpha Pegasi is the third-brightest star within the Pegasus Constellation. Alpha Pegasi has a mass of 3 Solar Masses, a radius of 4.72 Solar Radiuses and a luminosity of 160 Solar Luminosities. Alpha Pegasi has a surface gravity of 3.51 Centimetre-Gram-Second System of Units and a temperature of 9765 Kelvin. Alpha Pegasi is 133 Light Years from The Sun. 
Profile of Alpha Pegasi
Alpha Pegasi has used up its hydrogen core and is beginning it's post main sequence part of its life. This has given it a radius five fold that of The Sun. Alpha Pegasi's Traditional name, Markab is Arabic for the The Saddle of the horse.