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Sir Christopher Wren 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 | 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 Astronomy Quotes The Planet Venus Back in 1686, a French scholar by the name of Bernard de Fontenelle, wrote, "I can tell from here...what the inhabitants of Venus are like; they resemble the Moors of Granada; a small black people, burned by the sun, full of wit and fire, always in love, writing verse, fond of music, arranging festivals, dances, and tournaments every day." Nice try, Bernard, but you had it all wrong. Back in those days, it was generally accepted that Venus was much like Earth. Venus is about the size of Earth, but that's pretty much where all resemblance ends. Almost all of the planets in our solar system travel around the sun in a counterclockwise direction…all of them except Venus and Uranus, that is. Venus (as well as Uranus) travels clockwise. All of the planets except Venus and Uranus rotate on their axis in a counterclockwise direction. Venus and Uranus rotate clockwise. Venus also rotates really slowly, too. A "day" on Venus would equal about 243 Earth days. Venus is covered by a thick layer of clouds that make studying the surface very difficult. In the last 30 years, however, astronomers have learned how to "see" through the thick cloud cover. In 1962, Mariner 2 was the first spacecraft to go by Venus. Since then, there have been 20 more missions. The first hard landing on Venus was done by Venera 4 in 1967. The first soft landing was done by Venera 7 in 1970. In 1989, the Magellan spacecraft probe was launched. Magellan rotated around Venus from 1990 to 1995. It then burned up in the atmosphere of Venus. Magellan bounced radar signals off the surface of Venus and transmitted the data back to Earth. |
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Famous Astronomy Quotes 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.
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