Because the objects in the solar system have their own orbits, they are not visible at different times of the year in the same way that deep-sky objects are. However, this page still provides background information on the common solar system targets you might view through the telescope.
Object | Type | Discovered | Brightness | Apparent Size | Size (Rel to Earth) | Suggested Telescope | Observing Notes | Notes | Links for More Information |
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Moon | moon | Antiquity | -12.6 - -2.5 | 30' | 0.27 Earth | any | Best observed near first/third quarter, since side illumination shows crater/highlands; use filter to limit light | Consists of dark "seas" (maria) and bright "highlands" (terrae); albedo is ~10% -- similar to coal | Space.com![]() ![]() ![]() ![]() |
Mercury | planet | Antiquity | -2.6 - 5.7 | 5-13'' | 0.38 Earth | >= 8" | Only visible during dawn/dusk due to interior orbit; shows phases | No atmosphere; ice thought to exist in permanently shrouded craters at poles; anomolies in orbit confirmed general relativity; | Space.com![]() ![]() ![]() ![]() |
Venus | planet | Antiquity | -5 - -3.8 | 10-63'' | 0.95 Earth | >= 6" | Brightest planet in the sky; only visible near sunset/sunrise due to interior orbit; shows phases | Hottest planet in solar system 870F; greenhouse runaway atmosphere | Space.com![]() ![]() ![]() ![]() |
Mars | planet | Antiquity | -2.9 - 1.8 | 3-25'' | 0.53 Earth | >= 8" | Distinctive red color and relative brightness make it easy to find | Home to tallest mountain in solar system, Olympus Mons; | Space.com![]() ![]() ![]() ![]() |
Jupiter | planet | Antiquity | -2.9 - -1.6 | 30-50'' | 11.2 Earth | >= 8" | Can see Galilean Moons and red spot with telescope, use Jupiter Tracker![]() |
Most massive planet; has 63 moons and tenuous rings; | Space.com![]() ![]() ![]() ![]() |
Saturn | planet | Antiquity | -0.5 - 1.5 | 14-21'' | 9.4 Earth | >= 8" | Can see rings easily in telescope | rings made of billions of particles of ice and rock, ranging in size from a grain of sugar to the size of a house | Space.com![]() ![]() ![]() ![]() |
Uranus | planet | William Herschel 1781 | 5.3 - 6.0 | 3-4'' | 4.0 Earth | >= 10" | Beautiful aqua color; hard to find unless using tracking/finding with 10" | pronounced "YOOR-a-nus", not "your anus"; rotation axis is perpendicular to its orbital axis; first planet discovered in modern times | Space.com![]() ![]() ![]() ![]() |
Neptune | planet | Urbain Le Verrier 1846 | 7.8 - 8.0 | 2-2.5'' | 3.9 Earth | >= 10" | Dark blue/purple; hard to find unless using tracking/finding with 10" | Using Newtonian Gravitation to understand anomolies in Uranus' orbit, Neptune was found where predicted to be | Space.com![]() ![]() ![]() ![]() |
Pluto | dwarf planet | Clyde Tombaugh 1930 | 13.6 - | 0.06-0.1'' | 0.18 Earth | Good luck! | Extremely faint, probably need >16" telescope with good tracking | Highly elliptical orbit and out of the plane of the solar system; originally classified as a planet, reclassified as a dwarf planet in 2006 due to similarity with many many other kuiper belt objects | Space.com![]() ![]() ![]() ![]() |
Ceres | dwarf planet | Guiseppi Piazzi 1801 | 6.6 - | 0.3-0.8'' | 0.08 Earth | >= 10" | Probably need >10" telescope with good tracking | Largest of the asteroid belt objects; classified as a planet in 1801 but reclassified as an asteroid in the 1850s due to discovery of several other asteroids | Space.com![]() ![]() ![]() ![]() |