How Far Away Is That?
How Far Can Your Telescope See ?
How Big Is It Compared To Earth?
How Many Moons Does It Have?
by: Larry McNish
Page last updated April 26, 2023
(Page originally created Apr 14, 2004)
I often get asked these questions when showing family, friends and the general public
celestial targets in my telescope.
Keep these tables handy and you'll never struggle for an answer again!
1. How Far Away Is That?
The following table lists many Solar System objects by distance:
For the solar system objects the distance given is an approximation based on
the differences of the semi-major axes of their orbits. For the inner planets
this is too "near" given that they are in inferior conjunction when this
happens - you may wish to use a different number - somewhere between inferior
conjunction and perhaps greatest elongation. (See the diagram in Section 8 below.) For the outer planets, this is
also too "near" given that this only happens at opposition. Pluto's distance is
also adjusted considering it's current position at nearly the distance of Neptune.
However, the people asking the question are not usually seeking an explanation
of solar system geometry, but a simple "guesstimate".
| Object |
A.U. |
Miles |
Say. . . |
Kilometers |
Say. . . |
Light Time |
| Sun | 1 | 92,955,807.27054 | 93 Million mi |
149,597,870.696 | 150 Million km | 8.31 min |
| Moon | 0.00257 | 238,917 | 240 Thousand mi | 384,500 | 400 Thousand km | 1.282 sec |
| Mercury | 1-0.39 = | 56,730,000 | 57 Million mi | 91,500,000 | 92 Million km | 5.08 min |
| Venus | 1-0.72 = | 26,040,000 | 26 Million mi | 42,000,000 | 42 Million km | 2.33 min |
| Mars | 1.5-1 = | 46,500,000 | 47 Million mi | 75,000,000 | 75 Million km | 4.17 min |
| The average asteroid | (Ceres) 2.767-1 = | 164,331,000 | 160 Million mi | 265,050,000 | 265 Million km | 14.73 min |
| Jupiter | 5.2-1 = | 390,600,000 | 390 Million mi | 630,000,000 | 630 Million km | 35.00 min |
| Saturn | 9.6-1 = | 799,800,000 | 800 Million mi | 1,290,000,000 | 1 Billion km | 71.67 min |
| Uranus | 19.1-1 = | 1,683,300,000 | 2 Billion mi | 2,715,000,000 | 3 Billion km | 2.51 hr. |
| Neptune | 30.0-1 = | 2,697,000,000 | 3 Billion mi | 4,350,000,000 | 4 Billion km | 4.03 hr. |
| Pluto | 39.5-1 = | 3,580,000,000 | 4 Billion mi | 5,760,000,000 | 6 Billion km | 5.33 hr. |
| Orcus (2004 DW) | 39.4-1 = | 3,570,000,000 | 4 Billion mi | 5,745,000,000 | 6 Billion km | 5.32 hr. |
| Varuna (2000 WR106) | 43.1-1 = | 3,913,000,000 | 4 Billion mi | 6,298,000,000 | 6 Billion km | 5.83 hr. |
| Haumea (2003 EL61) | 43.3-1 = | 3,930,000,000 | 4 Billion mi | 6,328,000,000 | 6 Billion km | 5.86 hr. |
| Quaoar (2002 LM60) | 43.5-1 = | 3,950,000,000 | 4 Billion mi | 6,358,000,000 | 6 Billion km | 5.89 hr. |
| 15760 (1992 QB1) | 43.7-1 = | 3,970,000,000 | 4 Billion mi | 6,388,000,000 | 6 Billion km | 5.91 hr. |
| Makemake (2005 FY9) | 45.7-1 = | 4,160,000,000 | 4 Billion mi | 6,687,000,000 | 7 Billion km | 6.19 hr. |
| Eris (2003 UB313) | 67.7-1 = | 6,200,000,000 | 6 Billion mi | 9,978,000,000 | 10 Billion km | 9.24 hr. |
| Sedna (2003 VB12) | 494.5-1 = | 45,900,000,000 | 46 Billion mi | 73,830,000,000 | 74 Billion km | 68.36 hr. |
| The average meteor | 50-100 Km (in the Earth's atmosphere) |
| The Shuttle | 350 Km |
| The International Space Station | 380 Km |
| Geostationary satellites | 35,790 Km (about 100 times further than the ISS but only 1/10 the way to the Moon) |
| The average comet | 100,000,000 miles (~1 A.U.) |
Also see: The Solar System for comparisons of Solar System bodies
Also see: The Kuiper Belt home page
Also see: Trans-Neptunian Objects at Wikipedia.
Also see: New Horizons - NASA's Pluto-Kuiper Belt Mission
Also see: Discovery of Eris (formerly nicknamed Xena)
Also see: Discovery of Dysnomia (formerly nicknamed Gabrielle - Eris' moon)
2. How Far Can Your Telescope See ?
The following table lists some deep sky objects by distance:
| Object |
Distance |
| The Pleiades M45 | 380 LY (Light Years) |
| The Dumbbell nebula M27 | 1,250 LY |
| The Orion Nebula M42, M43 | 1,600 LY |
| The Ring Nebula M57 | 2,300 LY |
| The Lagoon nebula M8 | 5,200 LY |
| The Crab nebula M1 | 6,300 LY |
| Globular Cluster M13 | 25,000 LY |
| The Andromeda Galaxy M31,M32,M110 | 2.9 Million LY |
| Galaxies M81, M82 | 12 Million LY |
| The Whirlpool Galaxy M51 | 37 Million LY |
| The Sombrero Galaxy M104 | 50 Million LY |
| Stars within the galaxy | Thousands of Light Years |
| Messier objects | Closest M45=380 LY, The most distant Messier objects=60 Million LY |
| The Finest 110 NGC objects | Closest NGCxxx =? the most distant (NGCxxx) =? |
| Other Galaxies | Hundreds of Millions of Light Years |
| Quasars | Billions of Light Years |
3. How Big Is It Compared To Earth?
The following table shows Solar System objects (o) relative to Earth (e)
by Diameter and Volume:
| Object |
Diam (km) |
Do/De |
Diameter Comment |
Vo/Ve |
Volume Comment |
| Earth | 12756 | 1 | | 1 | |
| Moon | 3475 | 0.272421 | 1/4 of Earth | 0.0203 | 50 times smaller |
| Sun | 1392530 | 109.1667 | 110 times | 1,300,979 | a million times larger |
| Mercury | 4879 | 0.382487 | 1/3 | 0.0562 | 18 times smaller |
| Venus | 12104 | 0.948887 | a tiny bit smaller | 0.857 | a little smaller |
| Mars | 6792 | 0.532455 | 1/2 | 0.151 | about 7 times smaller |
| Jupiter | 142980 | 11.20884 | 11 times | 1,321.33 | 1300 times larger |
| Saturn | 120540 | 9.449671 | 9 times | 763.59 | 800 times larger |
| Uranus | 51120 | 4.007526 | 4 times like Neptune | 63.08 | 60 times larger like Neptune |
| Neptune | 49530 | 3.882879 | 4 times like Uranus | 57.74 | 60 times larger like Uranus |
| Pluto | 2370 | 0.1858 | 1/5 | 0.0059 | a "speck" about 1% of Earth |
| Orcus (2004 DW) | ~1500 | 0.1176 | 1/9 | 0.0016 | a "speck" less than 1% of Earth |
| Varuna (2000 WR106) | ~800 | 0.0627 | 1/16 | 0.0002 | a "tiny speck" much less than 1% of Earth |
| Haumea (2003 EL61) | ~1500 | 0.1176 | 1/9 | 0.0016 | a "speck" less than 1% of Earth |
| Quaoar (2002 LM60) | ~1260 | 0.09878 | 1/10 | 0.0010 | a "speck" less than 1/10% of Earth |
| 15760 (1992 QB1) | ~? | | | | a "speck" less than 1% of Earth |
| Makemake (2005 FY9) | ~1900 | 0.1489 | 1/7 | 0.0033 | a "speck" less than 1% of Earth |
| Eris (2003 UB313) | 2330 | 0.1827 | 1/5 | 0.0035 | a "speck" about 1% of Earth |
| Sedna (2003 VB12) | ~1600 | 0.1254 | 1/8 | 0.0020 | a "speck" less than 1% of Earth |
| The average asteroid | | | tiny | | same |
| The average meteor | | | like a grain of sand | | same |
| The average comet | | | tiny nucleus, huge coma | | same |
And a special note - all the planets could fit between the Earth and the Moon.

Yes, it's true. See: http://www.universetoday.com/115672/you-could-fit-all-the-planets-between-the-earth-and-the-moon/
Also see: The Solar System for comparisons of Solar System bodies
Also see: http://www.rense.com/general72/size.htm for a comparison between the Earth and other planets and the Sun and other stars.
4. How Many Moons Does It Have?
| Object |
# of Moons |
Names (arranged closest to furthest) |
| Mercury | 0 | |
| Venus | 0 | |
| Earth | 1 | Luna, the Moon |
| Mars | 2 | Phobos and Deimos (both very small and hard to observe even with the largest telescopes) |
| Jupiter | 80 | Possibly 95 moons. 4 big ones - Io, Europa, Ganymede, Callisto (can be seen in binoculars) |
| Saturn | 83 | 6 big ones - Enceladus, Tethys, Dione, Rhea, Titan, and Iapetus |
| Uranus | 27 | 5 big ones - Miranda, Ariel, Umbriel, Titania, and Oberon |
| Neptune | 14 | 3 big ones - Proteus, Triton, and Nereid (The 14th moon S/2004 N1 was discovererd July 1, 2013 by Mark Showalter of the SETI Institute in Mountain View, Calif. using the Hubble space telescope. |
| sub-total | 207 | |
| Pluto | 5 | 1 big one - Charon, and 4 small ones - Nix, Hydra, "S/2011 (134340) 1" or "P4" now named Kerberos, discovered
July 20, 2011, and "S/2012 (134340) 1" or "P5" now named Styx, discovered on images taken by Hubble's Wide Field Camera 3 on June 26, 27, 29, and July 7 and 9, 2012.
In a February 2013 on-line poll to vote for names for the last two moons, "Vulcan" and "Cerberus" (or "Kerberos") (for P4 and P5) won the competition.
The July 2, 2013 IAU official announcement of the names for P4 and P5 is here. |
| Ceres | 0 | |
| Eris (2003 UB313) | 1 | Dysnomia discovered on September 10, 2005 |
| Haumea (2003 EL61) | 2 | Hi'iaka discovered on January 26, 2005, and Namaka discovered on June 30, 2005 |
| Makemake (2005 FY9) | 0 | |
| sub-total | 8 | |
| Orcus (2004 DW) | 1 | Vanth discovered on November 13, 2005 (announced on February 22, 2007) |
| Quaoar (2002 LM60) | 1 | Weywot discovered on February 14, 2006 (announced on February 22, 2007) |
| sub-total | 2 | |
| Total | 217 | (and counting. . .) |
From: http://skyandtelescope.com/observing/objects/planets/article_827_1.asp (as of January 2006).
Two new moons for Pluto? See: ASTRONOMICAL HIGHLIGHTS for November 2005
and Astronomy Picture of the Day for 2005 November 3
Two new moons for Uranus ("Cupid" and "Mab") December 22, 2005 see: http://hubblesite.org/newscenter/newsdesk/archive/releases/2005/33/
and http://www.astronomy.com/asy/default.aspx?c=a&id=3821
Note that these two "new moons", "Mab" and "Cupid" are just "new" names for two discovered in 2003 -
S/2003 U1 and S/2003 U2 - so the total is still 27 for Uranus.
Saturn - 47, 49, 50 or ?? - see the article: http://saturn.jpl.nasa.gov/multimedia/images/image-details.cfm?imageID=1700
Most Recent: http://www.skyandtelescope.com/observing/objects/planets/A_Guide_to_Planetary_Satellites.html July 2013

from: http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=2823
Also see: The Solar System for comparisons of Solar System bodies
Other KBOs with Moons:
At least 12 KBOs have companions, and more are being discovered all the time. They are often called "binary KBOs" because the two objects have similar size, so it's not clear which is the "KBO" and which is the "moon!"
"Santa" has a moon nicknamed "Rudolph".
There are also more than 100 asteroids with moons and some "double asteroids"
see http://www.johnstonsarchive.net/astro/asteroidmoons.html
Some Asteroids with Moons:
| Asteroid |
# of Moons |
Name(s) |
| 243 Ida | 1 | Dactyl (discovered February 1994) |
| 762 Pulcova | 1 | |
| 90 Antiope | | actually a double asteroid! |
| 87 Sylvia | 2 | Romulus and Remus |
| 2001 SN263 / 153591 | 2 | S/2008 (153591) 1 and S/2008 (153591) 2 |
| 216 Kleopatra | 3 | |
| 45 Eugenia | 3 | Petit-Prince and another designated S/2004 (45) (3rd discovered in 2007) |
| 87 Sylvia | 3 | (2001) |
| 93 Minerva | 3 | (2009) |
| 3749 Balam | 3 | (2008) |
5. The Brightest Asteroids
The ones brighter than about magnitude +9 can be seen with binoculars under good conditions.
The dimmer ones (higher magnitudes) will require a telescope.
| # | Name | Magnitude |
| 4 | Vesta | 7.6 |
| 1 | Ceres | 8.7 |
| 2 | Pallas | 9.1 |
| 20 | Massalia | 10.1 |
| 11 | Parthenope | 10.1 |
| 3 | Juno | 10.3 |
| 344 | Desiderata | 10.3 |
| 51 | Nemausa | 10.3 |
| 44 | Nysa | 10.5 |
| 88 | Thisbe | 10.5 |
| 5 | Astraea | 10.5 |
| 17 | Thetis | 10.6 |
| 89 | Julia | 10.7 |
| 7 | Iris | 10.7 |
| 8 | Flora | 10.7 |
| 19 | Fortuna | 10.8 |
| 15 | Eunomia | 10.9 |
| 16 | Psyche | 10.9 |
| 387 | Aquitania | 10.9 |
| 324 | Bamberga | 11.0 |
6. Saturn's biggest moons

7. Jupiter's biggest moons

8. Solar System Geometry
 |
| IC | - Inferior Conjunction |
| GEW | - Greatest Elongation West |
| SC | - Superior Conjunction |
| GEE | - Greatest Elongation East |
| O | - Opposition |
| WQ | - Western Quadrature |
| C | - Conjunction |
| EQ | - Eastern Quadrature |
|
Note that the distance between Earth and any other planet varies greatly.
For Mercury and Venus it ranges from IC to SC (on the other side of the Sun).
For Mars, Jupiter, Saturn, Uranus, Neptune and the Plutoids it ranges from O to C.
9. Retrograde Motion Examples:
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