Water (H2O)

As an extremely stable compound of two abundant elements, water (often as water ice or water vapor) is almost ubiquitous in the Solar System. It is essential for life support and agriculture. It is valuable as a solvent or feedstock for chemical processes and also a convenient source of H2 and O2 by electrolysis. Forms a eutectic with ammonia that is believed to be responsible for much cryovolcanism.

Melting Point (at 101 kPa): 273 K
Vapor pressure of Solid at Melting Point: 611 Pa
Triple Point: 273.16 K at 612 Pa
Critical Temperature: 647.1 K
Critical Pressure: 22.06 MPa
Liquid Density at Boiling Point: 999.84 kg/m3

Reactivity Table. Only reactions exoergic at normal temperatures (<300 K) considered.

Rxn with:

H2O

O2

CH4

NH3

H2S

HF

HCl

H2

N2

Possible:

N/A

N

N

some (rev)

some dissoc

some dissoc

full dissoc

N

N

Rxn with:

C

CO2

Fe

FeS

MgSiO3

SiO2

NaCl

CaSO4

Al2O3

Possible:

N

rev

Y

N

N

N

dissoc

dissoc

N

Notes: N = no; Y = yes; dissoc = dissociation; rev = reversible.

Abundance in the Solar System:

Body:

The Moon

Mars

Venus

Asteroids

Jup/Saturn

Presence:

Rare

Common

Common

Common

Common

Body:

Ganymede

Europa

Titan

Ur/Neptune

Triton

Presence:

Common

Common

Common

Common

Common

Uses:
Life support- essential
Agriculture-essential
Source of H2 & O2 by electrolysis
Feedstock for manufacture of many other hydrogen compounds (CH4 and other organics, NH3, HCl, HF, H2SO4)
Useful polar solvent

Likely Sources:
Occurs naturally in most environments

Likely Methods of Preparation:
[Reduction of metal oxides with hydrogen]

Last updated 9th April 2003.

Go to the products page
Go to the processes page
Go to the Exochemistry Site main page