How to make the most of your observations of the worlds of the Solar System.

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Published: Monday, 15 July 2024 at 08:49 AM


Observing the planets in the night sky is a wonderful aspect of astronomy, and in this guide we’ll reveal our top tips for making the most out of the worlds of our Solar System

Today, the sensitivity and size of imaging equipment has improved immeasurably.

Yet even in the 21st Century, there are still areas of amateur astronomy where visual observers can make valuable contributions.

Find out which planets are visible in the night sky tonight

Observing the planets is one of the joys of astronomy. Credit: ARUIZHU/istock/getty images

If you are observing the planets, there are many specialist techniques that will enable you to obtain reliable results.

In this guide we’ll show you how to observe the most rewarding planets for study: Venus, Mars, Jupiter and Saturn.

Throughout the guide, we’ll mention which telescope filters you may wish to use to improve your observations. You can find out more about this in our guide to telescope filters for observing the planets.

Venus

Venus Dmitry Ardashev, Zaprudnya, Russia, 29 April 2023 Equipment: QHY 187M mono CMOS camera, TS-Optics UNC 10-inch f/5 Newtonian, Sky-Watcher EQ6-R mount
Venus, photographed by Dmitry Ardashev, Zaprudnya, Russia, 29 April 2023

Venus can be a challenging object for visual observers, yet in the 1960s it was such astronomers who helped to establish that the planet’s clouds have a three-day rotation period.

When observing the planets, you’ll find that each Solar System world has its own characteristics and specific attributes to enjoy.

With Venus, a visual observer can obtain disc drawings that correctly show the phase and to record elusive cloud markings. 

A cursory telescopic view of Venus will reveal a bright white disc with a phase.

The bright cusp caps covering the poles may be glimpsed, but that will probably be the only detail.

Don’t be put off, though: with time and patience subtle cloud markings come into view.

Venus’s fast-moving cloud formations, recorded through Schuler and Baader ultraviolet filters in 2018. Credit: Sebastian Voltmer / CCDGuide.com
Venus’s fast-moving cloud formations, recorded through Schuler and Baader ultraviolet filters in 2018. Credit: Sebastian Voltmer / CCDGuide.com

The first thing to do is to find the correct magnification: one that gives a reasonable disc size and is suitable for the seeing conditions.

I find 130-160x to be about right. Venus is also best observed in bright skies, as this reduces the glare from the disc. 

As with all planets, don’t expect to see all the fine details at once – you will need to engage with your visual system (one of the most remarkable adaptive optics kits on Earth).

Venus can be seen with the naked eye, appearing like a bright star in the morning or evening sky. Here it sits below a crescent Moon. Credit: Pete Lawrence
Venus can be seen with the naked eye, appearing like a bright star in the morning or evening sky. Here it sits below a crescent Moon. Credit: Pete Lawrence

Ask yourself what you can see on the disc and slowly your eyes will respond.

Spend about 15 minutes looking at the planet’s disc before you start drawing.

To sketch Venus you’ll need a circle 50mm in diameter. Draw in the phase and then, with a 2B pencil, gently shade in the subtle cloud markings.

Eyepiece filters are a great help as they allow you to see into different depths of the atmosphere.

Red and blue filters help to enhance cloud markings, while a yellow filter will bring out the polar collars.

Find out more in our guide to the different ways to observe Venus.

To observe the Schröter effect, be prepared to catch Venus half-lit – it will be earlier than expected. Credit: Konstantin von Poschinger / CCDGuide.com
To observe the Schröter effect, be prepared to catch Venus half-lit – it will be earlier than expected. Credit: Konstantin von Poschinger / CCDGuide.com

The Schröter effect

Look at Venus when it’s predicted to be at half phase and you’ll notice that the phase is actually slightly less than half.

This is the Schröter effect, where the planet’s observed phase is always less than the theoretical one, and it is particularly prominent in a blue filter. 

The phenomenon was first recorded by Johann Schröter in the 1790s and is due to light being scattered in the thick atmosphere.

You can record it for yourself: on your drawing, simply measure the distance (in mm) with a ruler from the limb to the terminator and divide this distance by 50 to get the observed phase of Venus.

Do this for all of your drawings and you can plot the decreasing phase against time on a graph and show how the effect changes over the course of an elongation.

Mars

Mars photographed by Martin Lewis
Credit: Martin Lewis

The ochre disc of Mars is full of subtle, slowly changing features.

Mars is a world of vast volcanoes, continent-sized canyons and majestic deserts.

It’s not uncommon for fogs to collect in the basins such as Hellas and Argyre, and the volcanoes attract brilliant clouds at their summits.

Martian meteorology changes over the course of a few hours, and it can all be recorded and studied visually.

The well-defined Martian seasons produce different phenomena.

During the apparition in 2013-14, it was springtime in the northern hemisphere, and the brilliant north polar cap shrank dramatically as it sublimated away.

Mars at Opposition, 2016 John Chumack, Dayton, Ohio, USA. Equipment: C8, Qhy5IIL CCD, 2x barlow.
Mars at Opposition, 2016 John Chumack, Dayton, Ohio, USA. Equipment: C8, Qhy5IIL CCD, 2x barlow.

Recording the retreat and advance of the polar caps is important as it reveals information about the Martian climate. 

The dust-storm season occurs during spring and summer in the southern hemisphere.

Telescopically, these storms resemble small orange clouds, and they can engulf the entire planet.

It may take many months for the dust to clear and afterwards there may be changes to the dark albedo features.

You can track the progress of large dust storms, recording their size and changes to local surroundings. A green filter helps enhance them.

Mars tolerates high magnification well because red light is less affected by Earth’s turbulent atmosphere.

At powers of 300x, dark albedo features like the Syrtis Major will show a multitude of subtle structure.

The triangular Syrtis Major can be seen in centre of this image of Mars. Note: south is up in the image. Credit: Pete Lawrence
The triangular Syrtis Major can be seen in centre of this image of Mars. Note: south is up in the image. Credit: Pete Lawrence

Drawing Mars requires some patience.

You can’t spend any longer than 15 minutes doing so as Mars’s rotation will have moved the features away from where you’ve placed them in the drawing.

Sketch the phase first if it is present, then the polar caps. Spend seven minutes putting down the obvious features and use the remaining time to put in any bright clouds you can see.

A blue Wratten No 80A filter helps to enhance white clouds. Aim to make two to three drawings over a night to show how the clouds change.

For more info, read our guide on how to observe Mars.

Jupiter

Jupiter imaged in August 2022, showing its famous Great Red Spot. Credit: Pete Lawrence
Jupiter imaged in August 2022, showing its famous Great Red Spot. Credit: Pete Lawrence

The restless clouds of Jupiter have generated plenty of work for visual observers for hundreds of years.

Through a telescope, this gas giant is differentiated into darker belts and brighter zones.

Powerful jet streams carry large storms along, presenting us with an ever-changing cloudscape.

Jupiter has a large disc and magnifications of 160x or more are sufficient to reveal a lot of fine detail.

A red filter helps to enhance bluer features like festoons along the equator.

Conversely a blue filter helps to enhance redder objects like the belts and the Great Red Spot.

A yellow filter gives good all-round contrast.

It takes practice to record Jupiter correctly, but doing so will really hone your observational skills.

Jupiter, Josh French, Grampound Road, Cornwall, 8 November 2022 Equipment: ZWO ASI 462MC camera, Orion Skyquest XX12g GoTo Truss Tube Dobsonian and mount
Jupiter, Josh French, Grampound Road, Cornwall, 8 November 2022

A Jupiter drawing requires the correct blank: this planet is appreciably flattened due to its rapid rotation, so the standard blank is 64mm wide but only 60mm high. 

Like Mars, Jupiter rotates quickly; in this case you have 10 minutes to make your sketch.

First draw the main belts and large storms, recording the ones near the preceding edge first as these
will vanish soonest.

Spend the remaining time adding in the finer details.

Belts and zones in Jupiter’s atmosphere. Start by locating the main features, then use these to navigate to more ambiguous regions. Credit: BBC Sky at Night Magazine

Great Red Spot

Jupiter’s most famous and persistent storm is the Great Red Spot, a vast hurricane situated in Jupiter’s South Tropical Zone.

Visible to a 5-inch scope, the Great Red Spot drifts in longitude at varying speeds; this drift rate can be measured. 

When the storm is visible, watch as it moves towards the central meridian.

When you think its centre is on the meridian, record the time.

Use freeware software WinJUPOS to convert the time into longitude and repeat this whenever you observe the Great Red Spot.

You can plot the resulting longitudes against time and look at how quickly the spot is moving in Jupiter’s atmosphere.

Find out more in our guide on how to observe Jupiter.

Saturn

Saturn at opposition Padraig Connor, Belfast, Northern Ireland, 18th July 2022 Equipment: ZWO ASI224MC planetary camera, SkyWatcher 200P, Dobsonian mount
Saturn at oppositionPadraig Connor, Belfast, Northern Ireland, 18th July 2022Equipment: ZWO ASI224MC planetary camera, SkyWatcher 200P, Dobsonian mount

It is often said that majestic Saturn is a ‘quieter’ Jupiter. The belts and zones of Saturn’s atmosphere are less well defined, but the storms that this planet can produce are even more ferocious. 

Watching and charting storm activity is one of the main tasks for visual observers of Saturn.

Storms are seasonal, occurring every 30 years, and usually take the form of a large white oval on Saturn’s equator.

Recently Saturn has produced storms in living memory: quite unexpectedly in late 2010 a large storm erupted in the planet’s northern hemisphere, lasting into 2011.

This powerful storm churned up the North Tropical Zone, reminding us of the need for a constant vigil if we’re to catch the next outbreak.

Saturn Robbie Smith, Stevenage, Hertfordshire, 15 August 2023 Equipment: ZWO ASI178MC colour CMOS camera, Celestron C9.25 XLT Schmidt-Cassegrain, Sky-Watcher EQ6-R Pro mount
Saturn by Robbie Smith, Stevenage, Hertfordshire, 15 August 2023

To really view Saturn, you’ll need to use a power of 160x times or more; 250x is a good all-round magnification.

Drawing Saturn requires five accurately placed ellipses – so don’t try to do it free-hand, use a carefully produced blank. 

Saturn is also a quick spinner, so spend about eight minutes drawing in the main features on the disc and the rings, and use the final four minutes to finish the fine details such as the fainter belts and shadows.

Filters work well for Saturn: yellow enhances the contrast between belts and zones, while light blue helps to emphasise redder features.

Also watch out for a bi-coloured aspect of Saturn’s rings: occasionally Saturn’s outermost ring, the A-Ring, appears brighter in a blue filter than in a red one.

Although rare, this phenomenon has been reported by visual observers and is worth keeping an eye out for.

Find out more in our guide on how to observe Saturn.

A range of eyepieces will serve you well for observing the planets
A range of eyepieces will serve you well for observing the planets

Best astronomy accessories for observing the planets

Eyepieces

A selection of medium- and high-power eyepieces, giving a range of magnifications to suit your seeing conditions. A useful range is 160-190x for low power, 200-250x for medium power and 300x-plus for high power.

Find out more in our guide on how to build an eyepiece collection.

Filters 

These help to enhance different features on planetary discs. Red, blue and yellow filters are invaluable.

Pencils 

Some planetary features are more subtle than others, so you’ll need range of pencils from HB to 6B, to capture as many as possible.

Red Light

White light destroys night vision, so always use a red light to draw.

WINJUPOS

This essential free software (www.jupos.org/gh/download.htm) displays the features present on Jupiter or Saturn’s disc at any date and time, and gives you the planetary longitudes for both gas giants so you can record the location of details.

It is especially helpful as these planets have three systems of longitude due to their different bands of rotation.

When observing the planets, a log book will help you keep track of what you see.
When observing the planets, a log book will help you keep track of what you see.

Keeping a log book

Keeping a log book is an essential skill for any visual observer.

It will keep your observations in a logical structure and you’ll be able to look back and see how your drawing skills have developed.

Your log book should be a sturdy bound notebook, and every observation should include the following information: 

Find out more in our guide on keeping an astronomical log book.

Keep us up to date with your adventures observing the planets by emailing contactus@skyatnightmagazine.com