The Position of Saturn in the Night Sky

Moon near Saturn Dates, October 2007 to December 2008

The orbit of Saturn shown at two/three year intervals between the years 1993 and 2020 AD. The orbit of the Earth is seen close to the centre, marked at various dates by a blue-green globe (the orbits are not shown to scale). The dates in blue are the dates of Saturn's opposition to the Sun, i.e. when the planet is closest to the Earth and appears at its brightest for the year. The images in the grey circles show how the planet appears from the Earth (orientated with Celestial North at the top). The points of Saturn's perihelion (i.e. its closest point to the Sun) and aphelion (its most distant point from the Sun) are also marked. The constellation in which Saturn appears, as seen from the Earth, is shown in green. The First Point of Aries is the 'zero point' from which the longitudes of the planets are measured (diagram based on a graphic by space artist David A Hardy).

 

Animation showing the varying aspect of Saturn's rings at various opposition dates from 1993 to 2020, with additional orbital and observational details. The image is shown with Celestial North up (note that astronomical telescopes will normally show images inverted).

Saturn images adapted from NASA JPL's Solar System Simulator ('SPACE')

Saturn's rings contribute a great deal to its brightness, and in fact, from the vantage point of the Earth, they are not always fully on view. About every 13 to 16 years, the rings are edgewise-on to the Earth's line-of-sight, when they are only seen as a thin line in telescopes - or sometimes not at all - and the planet appears much dimmer in the sky. Saturn takes a little less than 29.5 years to orbit the Sun, and during this time we see the rings from different angles.

The rings were wide open in 2002-3 and Saturn's Southern hemisphere is currently tipped in our direction. The rings have been closing up in recent years, showing a narrower and narrower aspect, with Saturn becoming rather dimmer at each successive opposition, and the rings will appear edge-on to the Earth in September 2009 (although the planet will appear very close to the Sun at this particular time). They will then slowly open up again and be fully on view some eight years later (October 2017), when Saturn's Northern hemisphere will be tipped our way.

Note that when the rings are wide open (i.e. when Saturn is brightest) the planet is seen in the constellations of Taurus or Gemini (when its Southern hemisphere is facing Earth) or in Scorpius, Ophiuchus or Sagittarius (when its Northern hemisphere faces Earth). Edge-on ring aspects occur when the planet is on the Aquarius/Pisces border (when oppositions take place around September) or in Leo (oppositions taking place around March).

Where is Saturn now?

 

Having spent the period from July 2005 to August 2006 in the constellation of Cancer, Saturn crossed the boundary into Leo on 30 August 2006. This diagram shows the apparent path of the planet through to late 2009. Periods of non-visibility (i.e. when the planet/constellation passes behind the Sun as seen from the Earth) are shown as a dashed line. Note that by the time Saturn reaches the tail-end of the Lion (i.e. South of the star Denebola) the rings will be seen edgewise-on to our line of sight (this diagram applies to the Northern hemisphere; for the Southern hemisphere view, click here).

Printer-friendly versions of this chart are available for Northern and Southern hemisphere views.

Like the other solar system planets, Saturn's orbit is somewhat elliptical, which means that its apparent size at opposition varies slightly throughout its 29.5 year orbit. When it is closest to the Sun (at perihelion), it lies some 9.03 Astronomical Units (AU) from the Sun; when furthest away (aphelion) it is 10.06 AU from the Sun (where 1 AU = 149,597,870 km or 92,955,807 statute miles). At perihelic oppositions, Saturn is some 743 million miles (1,197 million kms) from the Earth, whilst at aphelic oppositions it lies some 1027 million miles (1,654 million kms) from the Earth.

Saturn reaches opposition every 378 days, i.e. about 13 days later in each successive year.

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Moon near Saturn Dates, October 2007 to December 2008

On one or two days in each month, the Moon can be used as our celestial guide to help in locating Saturn in the sky. Use the following table to determine on which dates to see the Moon in the vicinity of the planet:

Date Range

(World)

Conjunction (Geocentric)

Moon Phase

Date & Time

Separation

2007

Oct 7/8

Oct 7, 16:00 UT

1°.3

Waning Crescent

Nov 3/4

Nov 4, 03:05 UT

1°.8

Waning Crescent

Dec 1

Dec 1, 13:09 UT

.4

Last Quarter

Dec 28/29

Dec 28, 22:24 UT

.8

Waning Gibbous

2008

Jan 24/25

Jan 25, 06:14 UT

.9

Waning Gibbous

Feb 21

Feb 21, 11:49 UT

.8

Full

Mar 19/20

Mar 19, 15:19 UT

.6

Waxing Gibbous

Apr 15/16

Apr 15, 18:29 UT

.6

Waxing Gibbous

May 12/13

May 12, 23:55 UT

.8

Waxing Gibbous

Jun 9

Jun 9, 09:14 UT

.1

Waxing Crescent

Jul 6/7

Jul 6, 22:15 UT

.5

Waxing Crescent

Aug 3/4

Aug 3, 13:30 UT

.8

Waxing Crescent

Sep 27/28

Sep 27, 19:41 UT

4°.5

Waning Crescent

Oct 24/25

Oct 25, 08:05 UT

.0

Waning Crescent

Nov 21/22

Nov 21, 18:21 UT

.6

Waning Crescent

Dec 18/19

Dec 19, 03:21 UT

.0

Last Quarter

 

The Moon made several close approaches to Saturn during 2007, such as on this occasion, photographed by the author on March 2nd, when the Moon came to within 1° of the planet (geocentric measurement). The photo was obtained by pointing a tripod-mounted digital SLR camera through the eyepiece of an 8-inch reflecting telescope set at 81x magnification. Since the Moon is many times brighter than Saturn, two separate photos were required in order to capture the Moon and Saturn at their correct exposures. From the author's location in the South-western United Kingdom, the Moon was seen to pass just to the North of the planet (note that the image is inverted, since it was taken through an astronomical telescope).

During 2007, the Moon also passed in front of Saturn - in an event called a lunar occultation - on several occasions when seen from various parts of the world. Saturn is not involved in any occultations during 2008.

Moon near Saturn dates for the period from October 2007 to December 2008. The Date Range shows the range of dates worldwide (allowing for Time Zone differences across East and West hemispheres). Note that the Date, Time and Separation of conjunction (i.e. when the two bodies are at the same celestial longitude) are measured from the Earth's centre (geocentric) and not from the Earth's surface (times are given in Universal Time [UT], equivalent to GMT). The Moon Phase shows whether the Moon is waxing (between New Moon and Full Moon), waning (between Full Moon and New Moon), at crescent phase (less than half of the lunar disk illuminated) or gibbous phase (more than half but less than fully illuminated).

The Moon moves relatively quickly against the background stars (in an Eastward direction, at about its own angular width [0º.5] each hour, or about 12º.2 per day) and because it is relatively close to the Earth, an effect called parallax causes it to appear in a slightly different position (against the background stars) when seen from any two locations on the globe at any given instant; the further apart the locations, the greater the Moon's apparent displacement against the background stars. Therefore, for any given date and time listed in the table, the Moon will appear closer to Saturn when seen from some locations than from others. For this reason, the dates shown in the table should be used only for general guidance.

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The Naked-eye appearance of Saturn

Naked Eye Planet Index

Planetary Movements through the Zodiac

Positions of the Superior Planets:

Mars, 2007-2008

Jupiter, 2006-2008

Uranus, 2006-2018

Neptune, 2006-2023

Pluto, 2006-2022

Current Position of the Sun and the Brighter Naked-Eye Planets (Star Map)


 

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Copyright © Martin J. Powell, Nov 2005 with amendments Sep 2007; minor update Jan 2008


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