Welcome to SkyEye, your guide to this month's celestial events.
Date | 45° N | 30° S | Event | |
---|---|---|---|---|
1 | Wed | Mercury at greatest elongation east | ||
2 | Thu | |||
3 | Fri | |||
4 | Sat | |||
5 | Sun | New Moon | ||
6 | Mon | Moonless skies favour this year's return of the Phoenicids (theoretical peak activity: from 15:30 UT). | ||
Moon occults Mars: visible from about 22:30 UT in Cuba, Manitoba, and central and southeastern United States. | ||||
7 | Tue | Similarly, observers of the poorly-studied Puppid-Velids enjoy dark skies. | ||
8 | Wed | |||
9 | Thu | |||
10 | Fri | |||
11 | Sat | |||
12 | Sun | |||
13 | Mon | First Quarter Moon at apogee | ||
14 | Tue | The waxing gibbous Moon leaves the second half of the night dark for observing the ever-reliable Geminids (theoretical peak activity: from 11:00 UT). | ||
15 | Wed | |||
16 | Thu | Jupiter at east quadrature | ||
17 | Fri | |||
18 | Sat | Uranus at east quadrature | ||
19 | Sun | |||
20 | Mon | Mercury at inferior conjunction | ||
21 | Tue | Full Moon | ||
A total lunar eclipse is visible from the Americas, most of the Pacific Ocean, most of Australasia and Asia, most of Europe, western Africa and much of the Atlantic Ocean. | ||||
Solstice | ||||
22 | Wed | Impossibly light skies obliterate the Ursids this year. | ||
23 | Thu | |||
24 | Fri | |||
25 | Sat | Perigee | ||
26 | Sun | |||
27 | Mon | |||
28 | Tue | Last Quarter Moon | ||
29 | Wed | |||
30 | Thu | |||
31 | Fri |
The word planet is derived from the Greek word for "wanderer." Unlike the background stars, planets seem to move around the sky, keeping mostly to a narrow track called the ecliptic, the path of the Sun across the stars. Dwarf planets and small solar-system bodies including comets, are not so constrained, often moving far above or below the ecliptic.
Constellations are patterns of stars in the sky. The International Astronomical Union (IAU) recognises 88 different constellations. The brightest stars as seen from the Earth are easy to spot but do you know their proper names? With a set of binoculars you can look for fainter objects such as nebulae and galaxies or some of the closest stars to the Sun.
Descriptions of the sky for observers in both the northern and southern hemispheres are available for the following times this month. Subtract one hour from your local time if summer (daylight savings) time is in effect.
Local Time | Northern Hemisphere | Southern Hemisphere |
---|---|---|
1730 hours (1830 hours summer time) | 45° N | 30° S |
1930 hours (2030 hours summer time) | 45° N | 30° S |
2130 hours (2230 hours summer time) | 45° N | 30° S |
2330 hours (0030 hours summer time) | 45° N | 30° S |
0130 hours (0230 hours summer time) | 45° N | 30° S |
0330 hours (0430 hours summer time) | 45° N | 30° S |
0530 hours (0630 hours summer time) | 45° N | 30° S |
Much of this information can be found in this month's issue of your favourite amateur astronomy magazine available in your local bookshop. Another excellent source is the current edition of the Astronomical Calendar by Guy Ottewell and published by the Universal Workshop at Furman University.
The SkyEye banner features a collision of galaxy clusters and is courtesy of NASA, ESA, CXC, M. Bradac (University of California, Santa Barbara) and S. Allen (Stanford University). When MACS J0025.4-1222 was formed, gravity caused the ordinary matter in the colliding galaxy clusters to slow down whereas the dark matter, which at best interacts only weakly with itself, continued on its original course. Thus, this object provides both confirmation of the existence of dark matter and a further understanding of its properties. This image is a composite of Hubble Space Telescope and Chandra X-ray Observatory data where dark matter is coloured blue (mapped by Hubble using gravitational lensing techniques) and ordinary matter is coloured pink (mapped by Chandra detecting X-rays from gas heated by the collision).