Dust storms¶
Energy and power · level 6, lesson 6 of 6
A question to start¶
In June 2018, a dust storm spread across the whole of Mars. Opportunity, on solar power for 14 years, went silent and never spoke again. How dark does a dust storm make the sky?
The idea¶
Scientists measure how dusty the sky is by its optical depth, \(\tau\) (tau). Sunlight coming straight through the air is cut down by a factor
for the Sun overhead. Each 1 of optical depth cuts the direct beam to \(e^{-1} = 37\%\).
| Sky | \(\tau\), about | Direct sunlight getting through |
|---|---|---|
| Clear Mars sky | 0.3 to 0.5 | 61 to 74% |
| A dusty day | 1 | 37% |
| A big regional storm | 3 | 5% |
| The 2018 storm over Opportunity | about 11 | 0.002% |
Not all the light is lost: dust also scatters light sideways, and some of that reaches the ground as dim, diffuse daylight. Even so, in the thickest part of the 2018 storm, only a tiny share of the usual sunlight reached Opportunity's panels. It could not charge its batteries, and its heaters could not keep it warm.
Planet-wide storms like 2018's come every few Mars years, usually in the dusty season (southern spring and summer), and can last for months. A city on solar power alone would need to store enough energy, or keep a second source, to get through one.
Worked examples¶
1. A dusty day. At \(\tau = 1\), with 586 W/m² above the air and the Sun overhead, the direct beam is \(586 \times 0.37 = 216\) W/m².
2. A regional storm. At \(\tau = 3\): \(586 \times e^{-3} = 586 \times 0.050 = 29\) W/m² direct.
3. The 2018 storm. \(e^{-10.8} = 2\times10^{-5}\). Of 586 W/m², about 0.01 W/m² came straight through. Diffuse light added more, but still only a few percent of a clear day.
Try it¶
- What does optical depth measure?
- Find the share of direct sunlight getting through at \(\tau = 2\).
- A panel gives 1,000 Wh a sol in a clear sky at \(\tau = 0.5\). Roughly what might it give at \(\tau = 2.5\), counting only the direct beam?
- Why could a nuclear power unit keep a city going through a storm?
Answers
- How much the dust in the sky blocks the direct sunlight.
- \(e^{-2} = 0.135\), about 14%.
- \(1000 \times e^{-2.5}/e^{-0.5} = 1000 \times e^{-2} = 135\) Wh (in reality diffuse light adds some).
- It does not need sunlight: its heat comes from atomic nuclei.
Common mistake¶
"Twice the dust, half the light." Optical depth works by multiplying: doubling \(\tau\) from 2 to 4 cuts the direct light from 14% to 2%, not from 14% to 7%.
Where it leads¶
- Back: Dust on the panels · Next level: Storing energy
- Level 6 page · Energy and power topic page
- Getting through a storm: Through a dust storm. How dust storms grow: Air and fluids. The figures: NASA's Opportunity mission page and Opportunity's last images, used to measure the tau of 10.8.