Lesson
The theory — Scale of the Universe Explorer
An order of magnitude is one factor of ten. Write a length as 10a metres and its size collapses into a single number, a — and equal steps across the ruler above are equal multiplications, not equal distances.
What each symbol means
a- the exponent in
10am — the only number you need to place something on this ruler. A bacterium is10−6m, so its a is −6; Everest is104m, so its a is 4. N:M- a ratio, written so the larger object comes first and the smaller is scaled to 1. Bacterium to virus is
101 : 1— the bacterium is ten times the length. decade- one factor of ten, and the unit the ratio table counts in. The gap between two objects is
a − bdecades, so a difference of 3 decades means a thousandfold, not threefold.
Where the formula comes from
- To compare two sizes you divide them:
10ametres by10bmetres. - Dividing powers of the same base subtracts the exponents, so
10a / 10b = 10a−b. The division itself never has to be carried out — and that is the whole reason a logarithmic ruler is usable at these extremes. - The ratio is therefore
10a−b : 1, anda − bis the number of decades between the two. That subtraction is what the table above prints: the Sun's radius against Everest is8.847 − 4.000 = 4.847 decades.
How to read what you see
Drag to pan, and scroll or pinch to zoom; the ruler is marked in powers of ten, so one step is one factor of ten wherever you are on it. The table lists pairs of objects three ways at once — the two names, the ratio as N:M, and the exponent subtraction that produced it. Reading a row backwards is often the more surprising direction: a bacterium against an atom is 104 : 1, so an atom is ten thousand times shorter than a single cell of the simplest life there is.
- Assumes
- One representative length per object, which is a genuine simplification rather than a rounding: bacteria span more than a decade among themselves, and “human cell” covers both a red blood cell and a neuron a metre long. The ruler also measures length only. Mass, age and energy each span their own, quite different, number of decades.
- Breaks when
- Two objects inside the same decade land almost on top of each other, so this is the wrong instrument for comparing things of similar size — it is built for exactly the comparisons a linear ruler cannot show. And the smallest label is not a size at all: the Planck length is not the width of any object, it is the scale at which our current description of space stops giving reliable answers.
Problem solved in full
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The ratio of the Sun's and Moon's mean distances by subtracting exponents 6 steps
The Moon's mean distance is 3.844×10⁸ m and the Sun's is 1.4960×10¹¹ m. Get the ratio by subtracting exponents instead of dividing — then use it to predict how many times larger the Sun is than the Moon, and work out why the prediction misses.
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Two measured means, one per orbit. Neither number comes off the ruler above; the ruler was built from them.
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Divide these as written and you are pushing twelve digits around. Put each distance on the exponent instead — a number written as 10x keeps all of its size in x. Those two values, rounded to three decimals, are exactly the positions the ruler holds for the Moon's and the Sun's distance.
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Powers of ten divide by subtracting. Click the Earth-Sun distance and Earth-Moon distance labels on the ruler — this tool has no preset buttons, the labels themselves are the control. The Exponent math column then prints this subtraction, and the N:M column the ratio it stands for.
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An exponent is not yet a ratio. Split it — the whole part 2 counts the decades, the leftover 0.590 supplies the leading digits, because 100.590 = 3.890. Dividing the two original distances the long way gives 389.18, and agreeing to three figures is the receipt that the trip through logarithms lost nothing.
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Now spend the ratio on something it was not asked for. From here the Sun and Moon look almost the same size, and a disc's angular size is roughly its diameter over its distance — so if the two discs matched exactly, the radius ratio would be forced to equal the distance ratio. Measured radii disagree: 400.43 against the 389.18 the distances demand, larger by 2.9%.
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The 2.9% is not an arithmetic slip. It is the two discs failing to match, and the fix is to stop assuming they do: put the radii and distances into the angle itself. The Moon is the smaller disc on average, which is not the way the coincidence is usually told.
Answer
2.590 decades — a distance ratio of 3.89×10² : 1. The radius ratio is 400.43, larger by 2.9%, so on average the Moon is the smaller disc. That average is not what decides an eclipse. The Moon's distance swings between 363,300 km and 405,500 km, so its disc swings from 32.88′ down to 29.46′, while the Sun's moves only between 32.52′ and 31.45′. The two ranges overlap. Near perigee the Moon's disc is the larger one and covers the Sun completely — a total eclipse; near apogee it is too small and leaves a ring of Sun around it — an annular eclipse. The 2.590 decades is what makes the two discs agree to within 3% at all; the wobble around it decides which eclipse you get, and the ruler above computes none of that.
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Learning path
Orders of magnitude
References (2)
- The Planck length, as measured — 1.616 255 × 10⁻³⁵ m, which the page rounds to 10⁻³⁵ m: NIST/CODATA, “Planck length”, Fundamental Physical Constants.
- The scale of the observable universe comes from the cosmological parameters here: Planck Collaboration, “Planck 2018 results. VI. Cosmological parameters.” Astronomy & Astrophysics 641, A6, 2020.