• Aucun résultat trouvé

Tableaux de multiplication par multiples de puissances de dix -- Puissances négatives (1,01 à 9,99) (A)

N/A
N/A
Protected

Academic year: 2021

Partager "Tableaux de multiplication par multiples de puissances de dix -- Puissances négatives (1,01 à 9,99) (A)"

Copied!
2
0
0

Texte intégral

(1)

Tableaux des Puissances de Dix (A)

Multipliez ou divisez le nombre de la rangée par celui de la colonne.

× 700 70 6,14 1,2 8,18 5,87 9,36 × 20 200 8,35 1,81 5,68 4,27 6,28 ÷ 20 200 2,49 9,31 8,25 1,42 7,41 ÷ 800 80 3,36 4,55 7,43 9,47 5,85 MathsLibres.com 70 000 7 000 2 000 20 000 2 000 20 000 8 000 80 000

(2)

Tableaux des Puissances de Dix (A) Solutions

Multipliez ou divisez le nombre de la rangée par celui de la colonne.

× 700 70 6,14 429,8 1,2 840 84 8,18 572,6 5,87 410,9 9,36 655,2 × 20 200 8,35 167 1,81 36,2 362 5,68 113,6 4,27 85,4 854 6,28 125,6 ÷ 20 200 2,49 0,001245 0,1245 0,0001245 0,01245 9,31 0,004655 0,4655 0,0004655 0,04655 8,25 0,004125 0,4125 0,0004125 0,04125 1,42 0,00071 0,071 0,000071 0,0071 7,41 0,003705 0,3705 0,0003705 0,03705 ÷ 800 80 3,36 0,0042 0,042 0,00042 0,000042 4,55 0,0056875 0,056875 0,00056875 0,00005688 7,43 0,0092875 0,092875 0,00092875 0,00009288 9,47 0,0118375 0,118375 0,00118375 0,00011838 5,85 0,0073125 0,073125 0,00073125 0,00007313 MathsLibres.com 70 000 7 000 429 800 4 298 42 980 84 000 8 400 572 600 5 726 57 260 410 900 4 109 41 090 655 200 6 552 65 520 2 000 20 000 16 700 167 000 1 670 3 620 36 200 11 360 113 600 1 136 8 540 85 400 12 560 125 600 1 256 2 000 20 000 8 000 80 000

Références

Documents relatifs

∼ 1, which suggest that the Be phenomenon may appear at whatever stage of the stellar evolution on the MS evolution phase. There is, however, a difference between the diagrams

It drives wave temperature out of phase with wave geopotential, which in turn alters the vertical structure of planetary waves: from west- ward tilt and upward amplification below

Second, if we take into account the Earth’s rotation, then blue and red rays cross the same irregularities during a given occultation with given a in only some altitude ranges since

results of the long-term ozone monitoring carried out within the framework of the international Network for the Detec- tion of Stratospheric Change (NDSC, http://www.ndsc.ws) by

A lower correlation was obtained with the Heidelberg data when considering only the southwest direction measurements (closest to the view- ing direction of both Bremen and

An especially intense fire plume was measured by the DC8 over the eastern USA on 18 July, by the BAe-146 over the mid-Atlantic on 20 July (when CO was measured at over 500 ppbv and

If the bulletin indicated a high release disposition of wet snow avalanches on “sunny hill slopes”, a subset of avalanche starting zones exceeding a membership degree of 0.5 of the

Title Page Abstract Introduction Conclusions References Tables Figures ◭ ◮ ◭ ◮ Back Close.. Full Screen