Photochemistry

Photochemistry is when molecules are hit by high energy light (usually Ultraviolet light) which breaks molecular bonds, and creates molecular fragments. These are usually highly reactive, and combine with other molecules. Mars' atmosphere is so thin, that some of these unstable fragments can last minutes or hours. Further, long lived, stable species are created (such as CO or O₂) which last for a long time in the Martian atmosphere.

There are three major gases in the Martian atmosphere Carbon dioxide (CO₂), Nitrogen (N₂), and Water (H₂O). The major photochemistry in the Martian atmosphere are based on these.

There are two areas where this occurs: the lower atmosphere (from UV light), and the edge of space (which has UV light, and also particles of the solar wind). These are both discussed below.

Our current models of the Martian atmosphere overestimate the amount of CO, and underestimate the amount of O₃ by significant amounts. This is an area of active research.

Lower Atmosphere

Nitrogen Photo-Dissociation

Nitrogen has a powerful bond, which makes it difficult for UV light to break it apart. Thus, species from the breakup of N₂ in the Martian atmosphere are quite rare, and play only a minor part in these exotic chemistries.

The major reaction is: N₂ + hv --> N + N(²D). (With wavelengths from 80 to 100 nm.)

• The '²D' means that the nitrogen's 'D' orbital is highly excited.
• The 'hv' represents high energy light.
• The 'h' is the Plank constant.
• The 'V' is the wavelength of the light.

N(²D) + CO₂ --> NO + CO

N + O --> NO + hv.

These cause further reactions:

N + NO --> N₂ + O

N + H₂O --> NO + OH

NO + H₂O --> NO₂ + OH

Note that NO₂ weakly dissolves in water, forming nitrous acid, and will be permanently lost to the atmosphere if it is absorbed in the soil.

The presence of these nitrogen species act as a catalyst, helping to react CO and O₂ to form CO₂ and atomic Oxygen.

Nitric acid (HNO₂) and peroxynitric acid (HO₂NO₂) are also formed but tend to break up quickly.

Carbon Dioxide Photo-Disassociation

Carbon dioxide plays a large part of these exotic chemistries, due to it pre-eminent proportion of the Martian atmosphere.

CO₂ + hV --> CO + O(¹D) (Where the D orbital is highly excited.)

OH + O --> O2 + H

If the hydrogen atom reaches the edge of space it is easily lost.

CO + OH --> CO₂ + H

If the atomic hydrogen manages to find an O₂, molecule, it may react thus:

H + O₂ = HO₂.

HO₂ is called hydroperoxyl, hydrogen superoxide, peroxyl radical, hydrogen dioxide, or dioxidanyl. It quickly reacts with any Ozone it encounters.

HO₂ + O₃ --> HO + O₂ + O₂

It may also encounter atomic oxygen:

HO₂ + O --> OH + O₂

Finally, if Carbon monoxide encounters atomic oxygen:

CO + O --> CO₂. (This can also be synthesized via series of other reactions.)

Water Photo-Disassociation

The most interesting series of reactions flows from the break up of water in the Martian atmosphere.

H₂O + hV --> OH + H. (The wavelength of the light must be under 200 nm.)

This atomic hydrogen is highly reactive. Water is confined to the lower atmosphere, so this hydrogen has plenty of time to react.

H₂O + O(¹D) --> OH + OH

These reactions also occur:

HO₂ + O --> OH + O₂

CO + OH --> CO₂ + H

The atomic hydrogen and OH (hydroxide) is created in significant quantities, and are used in many of the reactions described above. However, since the water on Mars is confined to the lower atmosphere, these chemical species are common in the LOWER atmosphere. (Altho, they may be moved higher by winds.)

Sulphur & Chlorine Chemistries

On Earth, sulphur dioxide (SO₂) is the most common gas produced by volcanoes. Searching for this gas would be a strong indication of active vulcanism on Mars. However, despite careful searching, no sulphur compounds have been found in the Martian air.

If sulphur dioxide does appear, it undergoes the following:

SO₂ + hV --> SO + O SO + hV --> S + O

These rapidly react: S + O₂ --> SO + O SO + O₂ --> SO₂ + O SO + OH --> SO2 + H SO + H₂O --> OH

These reactions keep SO₂ in equilibrium, with SO₂ being the dominate sulphur species up to ~45 km. Above this, SO becomes the dominate species.

The major sink for sulphur is:

SO₂ + OH --> HSO₃ (Using some other particle as a catalyst.) HSO₃ + O2 --> SO₃ + HO₂ SO₃ + H₂O + H₂O --> H₂SO₄ + H₂O

Sulphuric acid (H₂SO₄) can either condense at the surface, or be dissolved in water and enter the water table, being lost to the atmosphere. It has been estimated that the half life of sulphur compounds in the Martian atmosphere is ~2 years. This suggests that Martian vulcanism must be ~1,500 times less on Mars than on Earth.

Chlorine is likewise released by volcanoes, but perchlorates from the surface dust may also be a source in the Martian air. Chlorine is removed from the air by this reaction:

Cl + HO₂ --> HCl + O₂

Hydrochloric acid (HCl) will react with water or the surface and soon be removed. There are indications of tiny amounts of HCl in the Martian air, but it is a negligible player in the photo-chemistries described above.

The Methane Controversy

Methane (CH₄) may have been detected on Mars. (Most detections are at the error limits of the instruments finding it.) If it does exist, it will be broken up by reacting with OH or O(¹D). Its expected lifetime in the atmosphere is ~300 years, so any methane formed will have plenty of time to be well mixed in the Martian atmosphere. This makes the methane spikes found by Curiosity hard to explain, unless they took place very near the lander.