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![]() Right: The crescent Moon, Venus, and Jupiter all appeared together in the early morning hours of April 23rd, 1998. A similar show -- minus Jupiter -- will take place on May 17th through 19th, 1999. This image appears courtesy of S. Barnes, Sky Optics, copyright 1998 all rights reserved.
![]() On Monday the 17th, about an hour after sunset, the delicate crescent Moon will lie just 13 degrees directly beneath Venus. The next night, Tuesday the 18th, will be even better when the Moon and Venus will be almost side by side, separated by a scant 7.6 degrees. Die-hard Star Wars fans camping out for tickets on the eve of the premier shouldn't miss this spectacle. Finally, on May 19th, the crescent Moon will climb higher in the sky, appearing approximately 20 degrees above the brilliant planet.
Next week's close encounter in the evening sky should be an enjoyable sight. But there's more: Cradled in the arms of the slim crescent Moon will appear the ghostly outline of the full Moon, a dim glow that astronomers call "Earthshine." Like all the planets we see in the night sky, the Moon does not shine by its own light. It reflects sunlight. The side of the Moon facing the sun shines brightly, and the side facing away is nearly dark. The only significant illumination on the "dark side of the Moon" (no relation to the Dark Side of the Force) is due to Earthshine -- sunlight that bounces off the Earth and falls on the lunar surface. A slender crescent Moon with Earthshine is widely regarded as one of the most delicate and beautiful sights in the night sky. It will be difficult to see from urban areas, but should be easy to view from dark sky locations. ![]() Most moviegoers won't have a telescope with them as they slowly approach the ticket counter, but for those who do, a look at Venus through a modest-sized instrument will be a rewarding sight. Because Venus is closer to the sun than Earth, it appears from our vantage point to have phases like the Moon. As viewed through a telescope on May 19th Venus will look like a tiny quarter Moon approximately 19 arcseconds across. Sixty percent of the visible disk will be illuminated. If you do look at Venus through a telescope don't expect to see any surface features. The planet is completely veiled by clouds. In fact, that's why Venus is so bright. Its dense cloud layer reflects most of the sunlight shining down on the planet. Venus is about the same size as Earth and not much closer to the sun than our own planet. For this reason it was once thought that the two planets were similar, and that advanced life might even be found on Venus. Today we know that this is not the case. ![]() The pressure of Venus's atmosphere at the surface is 90 atmospheres, about the same as the pressure at a depth of 1 km in Earth's oceans. The air is consists mainly of carbon dioxide and there are several layers of clouds many kilometers thick composed of sulfuric acid. This dense atmosphere produces a runaway greenhouse effect that raises the surface temperature to over 850 o F -- hot enough to melt lead. This makes Venus's surface hotter than Mercury's, despite being nearly twice as far from the Sun. For more information about Venus and the Moon, visit The Nine Planets by Bill Arnett and SEDS. |
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Venus: Just Passing By -- Astronomy Picture of the Day, May 1, 1998 A rare double-conjunction eclipse -- Astronomy Picture of the Day, Apr. 28, 1998 A Venus Landing -- Astronomy Picture of the Day, Jan. 24, 1999 Venus's Once Molten Surface -- Astronomy Picture of the Day, Jan. 10, 1999 Why is Venus so bright? -- from EarthSky.com NASA's Magellan Mission to Venus -- from JPL The Nine Planets: the Moon -- from SEDS The Nine Planets: Venus -- from SEDS The Solar System Photo Gallery -- from the National Space Science Data Center |
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