Observing the planets of our solar system with a telescope is an enjoyable part of amateur astronomy. And unlike other forms of observing, such as deep-sky, it can be done from the center of a city as well as out in the country. No travel required. If it is clear (a rarity here in the Pacific Northwest) I can quickly set up one of my telescopes on the balcony and start observing. So here are a few tips on viewing our neighbors in the Solar System.
Any decent quality telescope over 60 millimeters (about 2.5 inches) will show some detail on Jupiter, the phases of Venus and Mercury and the rings of Saturn. If I just want a quick look I will go with my 90mm APO refractor. But better viewing can be had with 150mm (6 inch) and larger instruments. This is because the planets are small and to tweak out fine detail we will need to use high powers. And since at best you can use 50X per inch of aperture, you can see the need for size.
The actual telescope type is of lesser importance, but I personally like to use either reflectors or apochromatic (color free) refractors. Some excellent choices for a planetary scope are:
– a Maksutov Cassegrain of 150mm or greater
– a Newtonian Reflector of 150mm or greater
– a Schmidt-Cassegrain of 200mm or greater (this is what I use at the moment)
– a Apochromatic Refractor of 130mm or greater (expensive though)
But don’t despair if your scope isn’t listed here. Remember the best telescope is the one you use, so please use what you have. There are ways to squeeze more performance out of any optics.
One word is all that is really needed here, STEADY. As long as it is stable, and you don’t mind pushing it along, a Dobsonian mount, or a non-motorized alt-az with no slow motion controls will work fine. Of course it is irritating to wait for the image to stabilize again after you nudge the scope along. That is why a well built, steady, motorized mount is much nicer since the planet will remain in your field of view for as long as you want to view it. But again using what you have is more important.
Since the planets are small, a lot of magnification is required to observe fine detail. But you can’t go overboard either. On the best nights, with the steadiest skies, the maximum usable magnification you can use is 50X per inch of aperture (8 inch scope, 400X).
But those nights are far and few between. More often than not you will find your maximum magnification will be about 25X per inch. On my 8 inch I my most used eyepiece for planetary work is a 9mm Orthoscopic, which offers about 222X on that scope. This combination has afforded me outstanding views of
Jupiter, Saturn and Mars.
Keep in mind that eyepieces are expensive. You can but some good all-round eyepieces and a quality Barlow and those can offer you years of viewing pleasure. But if high contrast, high detailed views are what you want I suggest a few Orthoscopic eyepieces. They can be had for around $100 each. Highly recommended.
A quick word on magnification. To figure out the magnification a given eyepiece will provide on a given telescope use the following formula.
Magnification = focal length of telescope divided by the focal length of the eyepiece. So my 8 inch Schmidt Cassegrain has a focal length of 2000mm. If I use my 9mm Ortho we find, 2000/9 = 222.22X.
If I use the same eyepiece with my 91mm refractor what do we get? It has an f ratio of f6.6. So 6.6 x 91mm = 600 so a focal length of 600. Then 600mm divided by 9mm = 66.66X.
Although optional, a set of color filters can really help pull out different details on the planets. Here are some filters I can suggest with their Wratten numbers.
– #12 Yellow – Deepens blues and brings out reds and yellows on Jupiter and Saturn, also improves surface detail on Mars. Best on 150mm or greater scopes.
– #80A Blue – This filter can really pull the detail out on Jupiter’s cloud belt and Great Red Spot. Also useful on Saturn, enhancing contrast.
– #58 Green – Adds contrast and detail to the belt structure on Jupiter and Saturn. Also useful on the Martian polar caps. Best on 200mm or greater scopes.
– #25A Red – Fantastic filter for increased contrast on Jupiter. Really makes the belts “pop out”. Also very nice on Mars. Only recommended for scopes greater than 200mm. OR
– #21 Orange – Does somewhat the same as the #25 Red, just not as well, but can be used with smaller scopes.
Being comfortable makes any type of observing far better. I have 2 different chairs that I use for observing. Also be sure to dress right. Remember you will be standing still so you will need warmer clothes than you think.
I hope you enjoy your travels through our solar system with your telescope. As your experience grows you may be interested in learning to sketch what you see or even get into planetary imaging. The sky truly is the limit.
Visually, Venus has been known for thousands of years, appearing as one of the brightest objects in the night sky. Images from Earthbound telescopes show its various phases, which were first noted by Galileo and were one of the key arguments for a heliocentric solar system.
The surface of Venus is unseen from Earth due to extensive cloud cover; the atmosphere of Venus being discovered in the eighteenth century and subsequently found to consist mainly of carbon dioxide. The clouds were also determined by spectroscopy (measuring the spectrum of the light from the planet) to contain sulphuric acid droplets, hence being very corrosive.
In 1924, bolometry (measurement of infrared radiation) indicated that the cloud tops had a temperature of about -43 degrees Celsius. Also wind speeds measured by cloud motions were recorded at 220 miles per hour. In 1956, radio astronomy enabled measurement of the temperature of the surface of Venus, which was found to be 327 degrees Celsius, but as far as Earth based observations went at this time, this was about all we could learn about the planet.
Then in the early 1960’s, the radio telescope at Goldstone in California revealed that Venus had a 243 day retrograde rotation; in other words it orbits counter-clockwise around the Sun, but rotates itself in a clockwise direction. It is the only terrestrial planet to exhibit such behaviour.
The retrograde Venusian day is so long that it is actually longer than its year (224.7 days) and may be a significant factor in Venus having practically no magnetic field. Despite this, Venus does have an ionosphere close to its surface, but whereas the ionosphere of the Earth is due to its intrinsic magnetic field, the ionosphere on Venus is due to interactions of the solar wind.
In the early 1970s, the Goldstone telescope also made radio images of the surface of Venus and various features were identified. Although the radar images had poor resolution, they did reveal light areas of rough terrain and darker regions of smooth plains.
Thanks to the use of large radio telescopes and optical telescopes watching the ‘twinkle’ of stars, we have indeed confirmed a number of planets outside of our own solar system. However, we have never actually seen most of these planets, and can only gauge their existence and possible composition based upon the nature of light given off from their host stars.
This twinkle that I speak of is actually the bending of a star’s light as a planet passes in front of it. Given that twinkle, and how it refracts light, we can even hazard a fairly accurate guess as to the composition of the crossing body. This allows us, in truth, to explore our reality from the Safety of Earth.
However, this is only the first step. Just because we know a planet is at a certain star, doesn’t mean we, as Humans, should abandon our race to the stars. We must confirm these guesses, and take closer looks. We will be bound to simple guesses and many questions, if we choose to remain here on Earth.
Only by sharing our encounters, and thoughts on this subject, will we ever make progress. Indeed, the same rule applies for science fiction. We need these things, not just for the sake of entertainment, but for pure introspection. As we are exposed to more ideas, more often, we will be open to the possibilities and more supportive (as a people) of space exploration and travel.
As we close our minds, and becoming incredibly skeptical, we stop technological progress, and we eventual spur on to some period of stagnation. Space Travel has brought us numerous devices and raw knowledge that have spurred our civilization onwards.
From the Space Program, we’ve gained everything from Cordless Power Tools, to Smoke Detectors, to Landsat Satellites leased for agricultural work, to numerous other improvements, the returns are there. And these first early steps will lead to the greatest return of all, discovery of a new habitable planet and freedom from our solar system!
Thus, we need to support the Space Program. To do this, we need to, firstly, make sure our representation knows how we feel. We can also support this by seeing more science fiction films, visiting museums, and keeping open minds.
This might not seem to be of any connection, but if these sources of entertainment and knowledge (or potential knowledge) do well, far more people can see them. Thus, people may become exposed to concepts they were not even aware of. As a result, they may become vivid supporters of the Space Program, just like you!