Saturn Opposition 2003

 
 


Saturn is one of the splendors of the night sky. Few people forget their first glimpse through a telescope at the planet and its expansive rings hovering against the velvet background of space.

While the best views of Saturn will be during the cold winter months, few will disagree that it is worth the trouble to venture out into the frosty air to experience Saturn Shadingthe beauty of this, the most recognizable celestial object. 

Saturn begins to rise high in the evening sky in late October and reaches opposition (where the Sun and Saturn appear in opposite directions from Earth's perspective) on December 31st . 

Text Box:  Saturn with its rings will be 1.8 times larger than Mars was at its recent opposition. Mars was 25 arc seconds in diameter (angular size) during the opposition in 2003. Saturn with its rings will be about 46 arc seconds in angular size. Even though Saturn is much further away than Mars, Saturn is much larger. Mars was about 35 million miles away at opposition where as Saturn will be about 800 million miles away.

 Viewing specifics for opposition 2003 are as follows:

Opposition Specifics:
Date:
December 31, 2003
Magnitude: -0.3
Diameter: 20.7"
Declination: +23 degrees

Saturn's next opposition will not be until  January 13, 2005.

During the 2003 opposition the orientation of the rings will be particularly good. This year’s opposition  will reveal an optimal view with little or no shadowing on the planet and nearly optimal brightness.

Any telescope with at least a 30x magnification will reveal the rings. But the views become truly exquisite with a 100-200 mm (approximately 4-8 inch) aperture instrument.

Text Box:  You will be able to easily see a gap in the rings known as Cassini's Division. There is another division near the outer edge which can be seen in the larger telescopes. That feature is called the Encke's Division. You will also be able to see belts on the planet itself.  For approximately one to four months either side of opposition, Saturn's shadow across its rings is very apparent.

Saturn's rings are the planet's most endearing telescopic feature. Throughout the 2003-2004 viewing cycle, the rings display themselves to Earth through an average tilt of -25 degrees. Due to the ring tilt, we see the rings and moons of Saturn from south of the ring plane.  Saturn’s rings are incredibly thin for their size. The ring thickness is about 3,280 feet or nearly 2/3 of a mile.

At last count, Saturn had 31 moons. The largest, Titan is easily visible in any telescope. At west and east maximum elongation the moon appears as an 8th magnitude object orbiting approximately 5 ring diameters from the planet. Saturn's other visible moons are Enceladus, Tethys, Dione, and Rhea.

Saturn is the second largest planet in our solar system with a  diameter of 74,900 miles which is 9.5 times larger than Earth’s diameter.  To put it into perspective, Saturn and its rings would just fit in the distance between Earth and the Moon.  It is the sixth planet in the solar system at distance of  840 million miles from the Sun.  The rotational period for Saturn is 10 hours, 39 minutes, meaning one there are a little over 10 hours in each Saturnian day. 

Its atmosphere is primarily composed of hydrogen, with small amounts of helium and methane. It can be said that it is some what cold and windy on Saturn, with  velocities reaching 1,100 miles an hour at the equator and average  atmospheric temperatures of about -220 degrees Fahrenheit.  Keeping that in mind is sure to make you feel warmer as you view Saturn in the cold winter months.   

It was Galileo in the early 1600’s who was the first to observe Saturn's rings with his 20-power telescope. Interestingly, he was quite confused by the ring apparition through his poor quality optics. Originally he speculated that the rings were "handles" or large moons on either side of the planet. In 1655, Dutch astronomer, Christiaan Huygens was the first to correctly discern the nature of the rings of Saturn. It was not until 1675 that Italian Astronomer Giovanni Domenico Cassini was able to resolve the main division in the ring structure, thus bearing his name.

On July 1, 2004, the Cassini/Huygens spacecraft will arrive at Saturn and begin a detailed study of the planet and its largest moon Titan, stay tuned…