List of Solar System extremes

This article describes extreme locations of the Solar System. Entries listed in bold are Solar System-wide extremes.

By feature

Record Data Feature Ref.
Largest canyon 4000 km long, 200 km wide Valles Marineris, Mars
Tallest mountain 21.9–26 km (13.6–16.2 mi)

25 km (16 mi)

Olympus Mons, Mars

Unnamed mountain, Máni

Tallest volcano 25 km (15.5 mi) Olympus Mons, Mars
Tallest cliff 20 km (12.4 mi) Verona Rupes, Miranda, Uranus
Largest impact crater 2,700 km (1,700 mi) North Polar Basin, Mars

By class

Type Average density Average temperature Average surface gravity
Lowest Highest Lowest Highest Lowest Highest
Star 1.4 g/cm3

Sun

5778 K

Sun

274 m/s2

Sun

Major planet 0.7 g/cm3Saturn 5.51 g/cm3
Earth

73 K

Neptune

733 K

Venus

3.70 m/s2
Mercury

23.1 m/s2
Jupiter

Dwarf planet 1.4 ±0.2 g/cm3 Orcus 2.52 ±0.05 g/cm3 Eris 30 K

Makemake

167 K

Ceres

≈0.2 m/s2 Orcus 0.8 m/s2Eris
Major moon of major or dwarf planet 0.98 g/cm3
Tethys
3.53 g/cm3
Io
38 K
Triton
250 K
Moon
0.064 m/s2Mimas 1.796 m/s2Io
Type Escape velocity Mass Volume
(radius)
Lowest Highest Lowest Highest Lowest Highest
Star 617.7 km/s
Sun

332,830 MEarth
Sun

695,000 km
Sun

Major planet 4.3 km/s
Mercury
59.5 km/s
Jupiter
0.055 MEarth
Mercury
318 MEarth
Jupiter
2500 km
Mercury
69911 km
Jupiter
Dwarf planet ≈0.43 km/s
Orcus
1.3 km/s
Eris
0.0000916 MEarth
Orcus
0.0028 MEarth
Eris
487.3 km
Ceres
1187 km
Pluto
Major moon of major or dwarf planet 0.16 km/s
Mimas
2.74 km/s
Ganymede
0.000006 MEarth
Mimas
0.0250 MEarth
Ganymede
198 km
Mimas
2634 km
Ganymede
Extreme characteristic Major planet Dwarf planet Major moon
(of a major or dwarf planet)
Densest atmosphere Venus
Pluto Titan

By object

Astronomical body Elevation
(height above/below datum)
Elevation
(height above/below base)
Surface temperature
Highest Lowest Highest Lowest Highest Lowest
Sun N/A 5,000,000 K
In a solar flare

1240 K
In a sunspot

Mercury 3 kilometres (1.9 mi)
Caloris Montes, northwest Caloris Basin rim mountains

723 K
Dayside of Mercury

89 K
Permanently shaded polar craters

Venus 11 kilometres (6.8 mi)
Maxwell Montes, Ishtar Terra

3 kilometres (1.9 mi)
Diana Chasma, Aphrodite Terra

755 K
lowlands of Venus

644 K
Maxwell Montes, Ishtar Terra

Earth 8,848 metres (29,029 ft)
Mount Everest, Nepal - Tibet, China

10,971 metres (35,994 ft)
Challenger Deep, Mariana Trench, Pacific Ocean

10,200 metres (33,500 ft)
Mauna Kea, Hawaii, United States of America

7 kilometres (4.3 mi)
Mariana Trench, Pacific Ocean

330 K
Furnace Creek Ranch,
Death Valley, United States
(more info)
184 K
Vostok Station, Antarctica
(more info)
Mars 27 kilometres (17 mi)
Olympus Mons, Tharsis
6 kilometres (3.7 mi)
Hellas Planitia

24 kilometres (15 mi)
Olympus Mons, Tharsis
9 kilometres (5.6 mi)
Melas Chasma, Valles Marineris

293 K
Martian equator in midsummer day

120 K
Martian poles in the depths of winter night

Jupiter N/A 152 K

110 K

Saturn N/A 143 K

82 K

Uranus N/A 68 K

59 K

Neptune N/A 53 K
50 K
Moon 10,786 metres (35,387 ft)
5.4125°, 201.3665°
9.06 kilometres (5.63 mi)
Antoniadi Crater (-172.58°E, 70.38°S)
400 K
midday on the equator
26 K
Permanently shadowed southwestern edge of the northern polar zone Hermite Crater in winter solstice
Io 17.3 kilometres (10.7 mi)
Boosaule Montes
Europa 2 kilometres (1.2 mi)
conical mountain (34.5N, 169.5W)
132 K
Subsolar temperature
Ganymede 156 K
Subsolar temperature
80 K
Nighttime temperature
Callisto 168 K
Subsolar temperature
80 K
Predawn nighttime temperature
Titan 2 km (1.2 mi)
Mithrim Montes, Xanadu
Mimas
Enceladus 110 K
Tiger Stripes
Tethys
Dione
Rhea
Iapetus 20 kilometres (12 mi)Voyager Mountains, equatorial ridge and bulge

Ariel
Umbriel
Titania
Oberon
Miranda 20 kilometers (12 mi)

Verona Rupes

Triton
Nereid
Proteus
Charon
Ceres 4.5 kilometres (2.8 mi)
Ahuna Mons

235 K

Pluto 3.4 km (2.1 mi)
Norgay Montes, Tombaugh Regio
45 K

35 K

Eris 41 K

30 K

Makemake
Haumea
The bodies included in this table are: (1) planemos; (2) major planets, dwarf planets, or moons of major or dwarf planets, or stars; (3) hydrostatically round so as to be able to provide a geodetic datum line.

By distance

See also

See also

  • Extremes on Earth

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