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Galileo Galilei
The Constellations
There were originally 48 ancient constellations. The naming of the constellations began in the Middle East many centuries ago, but all societies named constellations, and the origins are mostly shrouded in time.
The ancient Greeks added stories and verses, and the ancient Romans gave the constellations Latin names. The ancient constellations are made up of only the brightest stars in the sky. Astronomers later broke the constellation Argo into three parts, so there are now 50 ancient constellations.
It was during the early part of the twentieth century, and astronomers of the International Astronomical Union (IAU) adopted another 38 modern constellations. (This is the same group who recently decided that Pluto is not a planet.)
The members of the IAU drew rectangular borders around all of the 88 constellations. There are informal constellations, or "asterisms" -- like Ursa Major holding the "Big Dipper" -- that young people who are interested in astronomy first learn to identify.
The names of the 88 constellations:
1. Andromeda
2. Antlia
3. Apus
4. Aquarius
5. Aquila
6. Ara
7. Aries
8. Auriga
9. Boötes
10. Caelum
11. Camelopardalis
12. Cancer
13. Canes Venatici
14. Canis Major
15. Canis Minor
16. Capricornus
17. Carina
18. Cassiopeia
19. Centaurus
20. Cepheus
21. Cetus
22. Chamaeleon
23. Circinus
24. Columba
25. Coma Berenices
26. Corona Austrina
27. Corona Borealis
| 28. Corvus
29. Crater
30. Crux
31. Cygnus
32. Delphinus
33. Dorado
34. Draco
35. Equuleus
36. Eridanus
37. Fornax
38. Gemini
39. Grus
40. Hercules
41. Horologium
42. Hydra
43. Hydrus
44. Indus
45. Lacerta
46. Leo
47. Leo Minor
48. Lepus
49. Libra
50. Lupus
51. Lynx
52. Lyra
53. Mensa
54. Microscopium
| 55. Monoceros
56. Musca
57. Norma
58. Octans
59. Ophiuchus
60. Orion
61. Pavo
62. Pegasus
63. Perseus
64. Phoenix
65. Pictor
66. Pisces
67. Piscis Austrinus
68. Puppis
69. Pyxis
70. Reticulum
71. Sagitta
72. Sagittarius
73. Scorpius
74. Sculptor
75. Scutum
76. Serpens
77. Sextans
78. Taurus
79. Telescopium
80. Triangulum
81. Triangulum Australe
82. Tucana
83. Ursa Major
84. Ursa Minor
85. Vela
86. Virgo
87. Volans
88. Vulpecula
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A few of the constellations do actually resemble what they are supposed to represent, but most of them don't. The purpose of the names for constellations is not usually to name them for what they portray, but rather to honor or represent.
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Famous Meteorites
The Planet Saturn
The planet Saturn resembles the planet Jupiter in many ways. Saturn is also a planet that has very little if any solid matter. It is believed that there is a hard rocky core, but that belief is unproven (albeit very probable) theory. Saturn, like Jupiter, is made up of gases and liquids. There is an internal heat source. We know this because Saturn radiates more energy than it receives.
Saturn rotates fast. It makes one complete revolution once every 10 or 11 hours. Saturn rotates around the sun once every 29.5 years. Because it rotates so fast, Saturn is flattened at the poles, making it an almost oblate planet.
The space probes, Pioneer 11, Mariner 11 and 12, and Voyager I and II, provide the best and most accurate information to astronomers about the planet Saturn, even though the Hubble space telescope takes very good images of Saturn. The space probes get "up close and personal," so to speak, and have provided information about Saturn that nothing else could have provided.
Wind velocity on Saturn is extreme. Wind speeds of more than 1,118 mph have been recorded. Unlike the winds on Jupiter, however, wind speeds on Saturn do not seem to be closely related to the positions of the belts and bands.
The rings around Saturn are one of the most interesting features. Really high-resolution pictures taken on the Voyager missions tell us that the rings are actually made up of hundreds of thousands of very small rings. The evidence suggests that the rings are composed of particles that are mostly ice crystals. A lot has been learned about the rings of Saturn over the last 20 or so years, but there is so much about them that is still a mystery. |
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More articles:
The Planet Venus
Astrophotography by Jerry Lodriguss
Carl Sagan - Wikipedia, the free encyclopedia
Glow-in-the-dark constellations
Venus - Wikipedia, the free encyclopedia
Space Travel
Our Sun
There is nothing remarkable about our sun in the scheme of things. It is very similar to millions of other stars (and our sun is a star) in the universe. You might even call our sun an "average" star.
The energy source for our sun is nuclear fusion. If the total energy output of the sun for just one second could be captured, it would provide the United States with enough energy at the current level of usage for nine million years.
There is a hard core at the center of the sun. The core is so dense and the sun is so large that energy released in the center of the sun takes 50 million years to reach the surface. That means that if the sun suddenly stopped producing any energy at all at the core today, it would be another 50 million years before we noticed it here on earth.
Our sun has been producing radiant and thermal energy for the last four or five billion years. There is enough hydrogen for it to continue producing energy for at least another hundred billion years. In about 10-20 billion years, the sun will begin to expand. It will engulf the closest planets (including Earth), and then it will be a giant red star. In another few billion years after that, our sun will become what is known as a dwarf star.
Most people think of the sun as this large (huge), constant featureless fireball in the sky. The large part is right, but the constant (or steady) and the featureless parts are all wrong. Sunspots are a feature of the sun that was first noted by Theophrastus about 325 BC. A moderate-size sunspot is about the size of Earth. Sunspots come and go over a period of days or weeks.
Related Topics: The Planet Uranus,
The Demotion of Pluto, The Planet Mars
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