Asteroid Ceres approaches Earth
February is a special occasion for the solar system's biggest asteroid. Not only is 1 Ceres making its closest approach to Earth since 1857, but it also will not get this close again for at least another millennium.
The long-term gravitational tugs of the planets conspire to modify Ceres' orbit just enough for this month's record-breaking event. Still, the difference between the asteroid's appearance now and at other favorable oppositions isn't huge. In 9 years, Ceres will be only 1.2 percent farther away.
You can follow Ceres through binoculars from your backyard. It sails through northern Leo during February, in a region without a lot of bright stars. Simply use the finder chart to pick out the pattern of nearby stars, then look for the interloper.
You may think this close approach will give you a chance to see Ceres without optical aid. You'd be right -- although not by much. At opposition, Ceres glows at magnitude 6.9 in a sparse starfield. Sharp-eyed observers under the darkest skies have seen objects this faint before. However, you'll have a better chance just 3 years from now. Ceres will then brighten to magnitude 6.7 thanks to the "opposition effect." The Sun-Earth-asteroid angle then will be closer to a straight line than during this month's slightly crooked arrangement. The better alignment in 2012 will increase Ceres' brightness more than the greater distance will decrease it.
On Friday Jan 30, 09 we are presented with a nice opportunity to catch Venus in broad day light.
On this day the Moon and Venus would be rising almost together. At about 10:00 a.m. if the sky is clear it should not be difficult to see the brightening lunar crescent well above the eastern horizon. Venus would be about two and quarter degrees south of the Moon. If one uses a small pair of binoculars one should be able to see these in the same field of view.
The best opportunity, however, comes when they will be crossing the meridian, an imaginary arc that passes through the north pole, the point right overhead and then the south pole. Close to the time is crosses the meridian (called transit time) time face due south and look strait up and then bend your neck down slightly southwards. You should be able to spot the Moon and then continue further down a bit and you can spot Venus.
Venus Rise, Transit and set times (in IST) for some cities in India are
rise transit set
Chennai 9h 01m 15h 12m 21h 26m
Bangalore 9h 25m 15h 27m 21h 28m
Jaipur 9h 32m 15h 34m 21h 36m
Kolkata 8h 42m 14h 44m 20h 46m
Mumbai 9h 44m 15h 46m 21h 47m
New Delhi 9h 26m 15h 28m 21h 30m
Pune 9h 39m 15h 41m 21h 43m
If you missed the event, never mind. Wait till it gets dark. It would be a magnificent view of the Moon and Venus next to each other above the western horizon.
Annular Solar Eclipse of January 26
The first solar eclipse of 2009 occurs at the Moon's ascending node in western Capricornus. An annular eclipse will be visible from a wide track that traverses the Indian Ocean and western Indonesia. A partial eclipse will be seen within the much larger path of the Moon's penumbral shadow, which includes the southern third of Africa, Madagascar, Australia except Tasmania, southeast India, Southeast Asia and Indonesia. (Figure 1).
The annular path begins in the South Atlantic at 06:06 UT when the Moon's antumbral shadow meets Earth and forms a 363 kilometre wide corridor. Traveling eastward, the shadow quickly sweeps south of the African continent, missing it by approximately 900 kilometres. Slowly curving to the northeast the path crosses the southern Indian Ocean. Greatest eclipse[1] takes place at 07:58:39 UT when the eclipse magnitude[2] will reach 0.9282. At this instant, the annular duration is 7 minutes 54 seconds, the path width is 280 kilometres and the Sun is 73° above the flat horizon formed by the open ocean. The central track continues northeast where it finally encounters land in the form of the Cocos Islands and onward to southern Sumatra and western Java (Figure 2). At 09:40 UT, the central line duration is 6 minutes 18 seconds and the Sun's altitude at 25°. In its final minutes, the antumbral shadow cuts across central Borneo and clips the northwestern edge of Celebes before ending just short of Mindanao, Philippines at 09:52 UT. During a 3 hour 46 minute trajectory across our planet, the Moon's antumbra travels approximately 14,500 kilometres and covers 0.9% of Earth's surface area. Path coordinates and central line circumstances are presented in Table 1.
Partial phases of the eclipse are visible primarily from southern Africa, Australia, Southeast Asia and Indonesia. Local circumstances for a number of cities are listed in Table 2. All times are given in Universal Time. The Sun's altitude and azimuth, the eclipse magnitude and obscuration[3] are all given at the instant of maximum eclipse.
This is the 50th eclipse of Saros 131. The family began with an unusually long series of 22 partial eclipses starting on 1125 Aug 01. The first central eclipse was total in the Northern Hemisphere on 1522 Mar 27. It was followed by 5 more total eclipses before the series produce 5 hybrid eclipses from 1630 to 1702. The first annular eclipse of Saros 131 occurred on 1720 Aug 04. The series will produce 29 more annular eclipses the last of which is 2243 Jun 18. Saros 131 terminates on 2369 Sep 02 after a string of 7 partial eclipses. Complete details for 70 eclipses in the series may be found at:
Launch Conference of the International Year of Astronomy
UNESCO, Paris, France, January 15-16 2009
2009 has been declared International Year of Astronomy by the General Assembly of the UN (United Nations Organization).
The Opening ceremony of the International Year of Astronomy will take place in Paris, January 15-16, 2009, under the aegis of the UN, the UNESCO (United Nations Educational, Scientific and Cultural Organisation), the IAU (International Astronomical Union). It is also supported by a number of sponsors including French and international organizations and institutions .
About 600 participants are expected, among them eminent scientists (including Nobel Prize winners), and also about 200 young students from over 100 countries, participating to the International Year IYA2009. Attendance is on invitation only.
Comets for both morning and evening
January lets us do an end run around the Moon's bright glare. When it washes out the sky near one interplanetary fuzzball, a second one comes into view on the sky's other side. Newcomer C/2007 N3 (Lulin) glides in the Moon-free morning skies during January's first 2 weeks, then the returning Comet 85P/Boethin becomes a prime evening target after midmonth.
Lulin tips the scales of Libra, between ruddy Antares and blue-white Spica. Glowing at 8th magnitude, this primordial snowball hails from the distant Oort Cloud. The comet makes its closest approach to the Sun January 10, but it will continue to brighten as it approaches Earth. It's destined never to return to the inner solar system. You'll need an 8-inch telescope to spy this comet from the suburbs, but a 4-inch will reveal it under a dark sky