When numbers are very large or very small, writing them out in full becomes cumbersome and error-prone (one slip in counting the zeros is enough). It is then convenient to use scientific notation: every number is written in the form

a10nwith1a<10,a\cdot 10^n \qquad \text{with}\quad 1 \leq a < 10,

where aa is the mantissa (a number with a single digit before the decimal point) and nn is an integer, positive for large numbers and negative for small ones. A few examples from the scales of nature:

  • Electron mass: 9,11031  kg9{,}1\cdot 10^{-31}\;\text{kg}
  • Atomic nucleus radius: 1015  m\sim 10^{-15}\;\text{m}
  • Earth’s radius: 6,4106  m6{,}4\cdot 10^6\;\text{m}
  • Earth-Sun distance: 1,51011  m1{,}5\cdot 10^{11}\;\text{m}
  • Sun’s mass: 21030  kg2\cdot 10^{30}\;\text{kg}

The order of magnitude of a number is the nearest power of 10. It is a quick way of saying “how large” a quantity is, ignoring the details. For instance, the Earth’s radius is of order 107  m10^7\;\text{m}: more precisely it equals 6,4106  m6{,}4\cdot 10^6\;\text{m}, but since 6,4>103,26{,}4 > \sqrt{10} \approx 3{,}2 the mantissa “rounds” upward, and the nearest power of 10 is 10710^7 rather than 10610^6. The criterion, in general, is exactly this: the mantissa is compared with 103,2\sqrt{10}\approx 3{,}2 to decide which power to round towards.

Sensitivity to orders of magnitude

In physics it is essential to develop an “intuition” for orders of magnitude. If a calculation gives the mass of the Moon as 5  kg5\;\text{kg}, it is immediately clear there is an error, without even redoing the sums: the result should be of order 1022  kg10^{22}\;\text{kg}. Comparing the order of magnitude of a result with what is expected is the first, fastest check of any calculation.

Collegamenti

Argomenti: Grandezze fisiche e misura Concetti: Notazione scientifica e ordini di grandezza Competenze: Stime di Fermi

Esercizi collegati: Problema — Volume di un parallelepipedo · Problema — Capelli in testa · Problema — Mar Adriatico