Transit of VenusNo one alive today has seen this sight, and it happens only twice this century. For the first time since 1882, Venus will glide across (transit) the face of the Sun on June 8th, taking 6 hours 12 minutes to complete its journey. The entire transit is visible from Europe, Africa (except the far west), the Middle East, and Asia (except the far east). For observers in eastern and central North America, the Sun rises with the transit in progress. The article "The Transit of Venus:
Where to See It" will help you determine whether or not you'll be able to see this event from your area.
A magnified view of the Sun (which requires a proper solar filter) will reveal the black dot of Venus slowly moving across the Sun’s face from celestial east to west. Perhaps the most interesting aspect of the transit is watching Venus enter and exit the solar disk — a process that takes about 20 minutes.
Eye safety is a prime consideration when you’re viewing the solar surface (with or without Venus in transit). Always use a safe solar filer or an indirect projection technique, even when the Sun is low on the horizon. Visit "The Sun" section of Sky & Telescope's Web site to learn how to safely view our star.
By the way, the second and final Venus transit of the 21st century occurs in 2012; the next pair of transits doesn't take place until 2117 and 2125.
Solar and Lunar Eclipses
Two weeks later, on the night of May 4–5, a total lunar eclipse is visible from Europe, Asia, Africa, and Australia. Totality lasts for 76 minutes, with mideclipse occurring at 20:30 Universal Time (10:30 p.m. in Cape Town, South Africa). At least some part of Earth's dark shadow (the umbra) touches the Moon for 3 hours 24 minutes. Western Europe, western Africa, and eastern South America will see the Moon rise already eclipsed, while in eastern Asia and Australia the Moon sets as the eclipse ends.
A partial solar eclipse occurs in western Alaska at sunset on October 13th and across Japan, the northeastern tip of China, and eastern Russia on the 14th. Greatest eclipse occurs in Alaska, west of Anchorage, where more than 90 percent of the solar diameter is obscured as the Sun sets.
The second total lunar eclipse of 2004 is visible from the Americas, Europe, most of Africa, and western Asia on the night of October 27–28. Canada and the continental US will see all of totality (weather permitting), but Hawaii will experience only a partial eclipse, as the Moon rises after totality has ended. At 9:14 p.m. Eastern Daylight Time on the 27th (subtract 3 hours for Pacific Time, add 4 hours for Greenwich or Universal time) the Earth’s umbra touches the left side of the Moon. The dark notch grows until it covers the entire lunar surface at 10:23 p.m. Since the envelope of air surrounding our planet bends some of the Sun’s light into the Earth’s shadow, the Moon will probably remain visible during totality. If our atmosphere is relatively clear, the Moon will be bathed in the reddish glow from sunrises and sunsets around the world. But if the air is thick with clouds, the Moon may look dull gray and dim. Totality ends at 11:45 p.m., and the Moon departs the Earth’s umbra at 12:54 a.m.
Additional details about these and other upcoming eclipses, as well as information about how to observe and photograph these breathtaking celestial spectacles, are available in the "Eclipses" section of this Web site.
Comets in 2004
Comet C/2002 T7 (LINEAR), discovered in October 2002, remains faint until after perihelion (its closest approach to the Sun) in late April 2004. By mid-May, Comet LINEAR may become at least as bright as 4th or 3rd magnitude, and Southern Hemisphere observers will be able to see it in the southwest shortly after sunset. At this time it’ll join another comet — Comet C/2001 Q4 (NEAT) — that southern skywatchers will have been observing for some time.
Comet NEAT was discovered in August 2001, but it’s visible mainly from south of the equator until late April 2004. Then the comet begins a rapid rise through the winter sky, moving past the bright stars Sirius and Procyon in early May and M44 (the Beehive Cluster in Cancer) at midmonth before entering the constellation Ursa Major in late May. During this time, C/2001/Q4 may become at least a 3rd-magnitude object, making it easy to spot after twilight in the west.
More information about both comets is available in the online article "Two Comets in 2004."
Occultations of Jupiter and VenusAs the Moon glides eastward through the sky, it occasionally occults (passes in front of) a star or planet, snuffing out its light. The star or planet reappears on the Moon’s opposite side up to an hour later.
Beginning about 3:45 a.m. Eastern Standard Time on the morning of December 7th, the Moon occults Jupiter for observers from the Rocky Mountains eastward in North America. This will be a spectacular event, easily visible in binoculars and small telescopes. The giant planet and several of its four bright satellites will disappear behind the bright lunar limb of the waning crescent Moon, reappearing from behind the dark limb up to an hour later.
Three other planetary occultations in 2004 deserve mention, though all are daytime events. On May 21st, Europeans see the Moon hide Venus beginning around 11:00 Universal Time. For skywatchers in northeastern US and eastern Canada, the Moon covers Jupiter beginning about 12:00 p.m. EST on November 9th. Finally, on November 10th, observers in Australia and New Zealand see an occultation of Venus starting at approximately 1:00 UT (noon in Sydney, Australia).
The Moon also hides bright stars on a regular basis. The best of these occultations for the coming year are described in the article "Lunar Occultation Highlights for 2004."
Detailed descriptions of upcoming celestial events appear monthly in Sky & Telescope magazine. A summary of these events, plus any late-breaking observing stories, can be found in the Observing section of this Web site.