IYA2009 - 2009 IS THE INTERNATIONAL YEAR OF ASTRONOMY
Commemorating glorious events particularly the 400th anniversary of Galileo’s invention of the telescope
Slogan - The Universe, Yours to Discover
|Events during April
· Lyrids meteor shower 19th to 25th April with a maximum on the 22nd. Conditions for viewing are favourable this year.
· The Moon: Full - 9th, New - 25th
· The constellation of Leo is dominant in the April night sky and this year is graced by the presence of Saturn.
If in doubt about where to find Leo, find the pointers of The Plough and look in the opposite direction from Polaris.
(Also see Constellation Map 1).
· If you are lucky enough to be near the equator on an April evening, you will be able to see the best known northern constellation,
Ursa Major, and the best known southern constellation, the Southern Cross, above
the horizon at the same time.
|For observors in tropical and northern latitudes, Mercury becomes visible low in the western evening sky after the
first ten days of April. For northern observors this is the most favourable evening apparition of 2009. The planet is at greatest eastern elongation on
26th April. Mercury will fade in brightness from -1.2 magnitude on 11th April to +1.0 magnitude by the end of the month.
The best times to observe Mercury in the northen hemisphere are when it is an evening star in the spring and a morning star in the autumn. In midsummer
the lighter skies make visibility difficult near the horizon.
The best times to observe Mercury are when it is an evening star in the spring and a morning star in the autumn. In midsummer
the lighter skies make visibility difficult near the horizon.
|Venus passed through inferior conjunction on the 27th March. It
is now visible in the eastern morning sky before sunrise with a magnitude brightening throughout April from -4.1 to -4.5. During the latter half of April, Venus and
Mars are just a few degrees apart (4 to 5š on the 21st-22nd).
On the 8th June 2004, Venus was at inferior conjunction
and transited the sun. Transits of Venus are rare, taking place at greater
than 100 year intervals and usually in pairs. The last two transits of Venus were in 1874 and 1882. June's transit
began at 7.20h and lasted 6 hours until 13.20h, the total event visible from Europe as a small black disc crossing
the lower part of the Sun from left to right. The next transit will be in late June 2012. After that, transits of Venus
won't occur again until 2117 and 2125.
Before and after inferior conjuction, when Venus is
the closest it comes to the Earth, are the times at which the planet is most brilliant and can be seen setting or rising
4 hours after or before the Sun. The dates of the next two inferior conjunctions are October 28th 2010 and October 26th 2018.
|To observors in the tropics and southern latitudes, at magnitude +1.2 and moving eastwards in Capricorn then Pisces,
Mars is visible as a morning object low above the eastern horizon prior to the brightening twilight inhibiting observation.
Mars passes just 0.43š south of Uranus on 15th April but is not visible in northern latitudes until later in the year.
At opposition on the 28th August 2003, Mars was only 56 million kilometres from the Earth. It showed a
disc of 25.1 seconds of arc across which is almost as large as it can ever appear. Mars started 2003 at 310 million kilometres from
the earth at 4.5 seconds of arc and 1.6 magnitude. By opposition it brightened 50 times to reach -2.9 magnitude but faded to 0
magnitude by December. Even to the naked eye Mars was a striking object in the summer and autumn sky, easily identifiable by its
reddish hue in an area of sky poor in bright stars. Mars will not be as close again until 2018.
These favourable oppositions occur every 15 or 17 years but other oppositions occur at average intervals of 2 years 2 months during
which time the planet makes a complete circle of the Earth. In general Mars is observable every other year, being too close to the sun for favourable conditions
during other times. Brightness at opposition varies from -1.0 to -2.9 magnitude, and when furthest from the earth it fades to 1.7 magnitude. The planet can be
identified by its orange-red colour.
As in 2003, Mars comes nearest to the Earth at oppositions at the end of August. At these times it can be brighter than Jupiter,
although low in the sky in Aquarius for northern observors. In the northern hemisphere, the planet may be better seen at oppostions during autumn and winter months
when it is higher in the sky.
|At magnitude -2.1, Jupiter continues to be visible in the eastern morning sky.
Being 770 million kilometres from the sun, the difference in brightness between opposition and conjunction varies less than with Mars, from
about -2.8 to -1.8 magnitude. Always a bright planet, Jupiter comes to opposition a month later each year, moving approximately from one zodiacal constellation to the next.
The 4 largest moons of Jupiter are easily visible through a small telescope, ranging from 4.6 to 5.6 in magnitude. The innermost, Io, takes 1.8 days
to orbit the planet making its motion easily detectable within a few minutes.
|At opposition on the 8th March, Saturn is still visible throughout the night
from the fall of darkness until early morning. At magnitude +0.5 the planet remains in Leo.
Saturnīs rings continue to close with the south pole presented towards Earth and the far side of the rings no longer appearing clear of the planetīs body. This year the
Earth will pass through the ring plane making the rings invisible for a short while. This will be the first time since 1997 that the planetīs magnitude has faded to
Saturn moves more slowly than Jupiter and can remain in the same constellation for several years. The brightness of the planet depends on the
aspect of its rings, as well as its distance from Earth and the Sun.
The planet crossed the equator into the northern hemisphere in 1996 where it will remain until 2010 with the southern side of the ring system
facing the earth. Because of its distance, its brightness varies little between opposition and conjunction but is affected by the huge ring system. Seen edge on the
rings contribute little or no light.
Every 15 years the plane of Saturn's rings passes through the sun, illuminating first the north and then the south side. For a few days the
rings are edge on to the sun. About the same time the Earth passes through the ring plane and, depending on the Earth's position, this may happen just once or 3 times.
During 1995/96 there was a triple crossing and the next will be 2038/39. The next single crossings will be in 2009 and 2025.
Saturn's largest moon, Titan, is visible in small telescopes orbiting outside of the ring system.
|Brightness varies slightly reaching 5.6 magnitude at opposition. This is bright enough to see with the naked eye but identifying it against the stars is difficult.
|Neptune has an average magnitude of 7.9 which varies little with changing distance.
|No longer an offical planet and never brighter than +13 magnitude, Pluto is only visible through powerful
First quarter: 2nd
Full moon: 9th
Last quarter: 17th
New moon: 25th