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 |
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 NinePlanets Wikipedia Solarviews |
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 NinePlanets Wikipedia Solarviews |
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 NinePlanets Wikipedia Solarviews |
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 NinePlanets Wikipedia Solarviews |
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 NinePlanets Wikipedia Solarviews |
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 NinePlanets Wikipedia Solarviews |
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 NinePlanets Wikipedia Solarviews |
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 NinePlanets Wikipedia Solarviews |
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 NinePlanets Wikipedia Solarviews |
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 NinePlanets Wikipedia Solarviews |