Quick Find Conversion Table

1 - 33
petawatts to picowatts
1= 1.0E+27
2= 2.0E+27
3= 3.0E+27
4= 4.0E+27
5= 5.0E+27
6= 6.0E+27
7= 7.0E+27
8= 8.0E+27
9= 9.0E+27
10= 1.0E+28
11= 1.1E+28
12= 1.2E+28
13= 1.3E+28
14= 1.4E+28
15= 1.5E+28
16= 1.6E+28
17= 1.7E+28
18= 1.8E+28
19= 1.9E+28
20= 2.0E+28
21= 2.1E+28
22= 2.2E+28
23= 2.3E+28
24= 2.4E+28
25= 2.5E+28
26= 2.6E+28
27= 2.7E+28
28= 2.8E+28
29= 2.9E+28
30= 3.0E+28
31= 3.1E+28
32= 3.2E+28
33= 3.3E+28
34 - 66
petawatts to picowatts
34= 3.4E+28
35= 3.5E+28
36= 3.6E+28
37= 3.7E+28
38= 3.8E+28
39= 3.9E+28
40= 4.0E+28
41= 4.1E+28
42= 4.2E+28
43= 4.3E+28
44= 4.4E+28
45= 4.5E+28
46= 4.6E+28
47= 4.7E+28
48= 4.8E+28
49= 4.9E+28
50= 5.0E+28
51= 5.1E+28
52= 5.2E+28
53= 5.3E+28
54= 5.4E+28
55= 5.5E+28
56= 5.6E+28
57= 5.7E+28
58= 5.8E+28
59= 5.9E+28
60= 6.0E+28
61= 6.1E+28
62= 6.2E+28
63= 6.3E+28
64= 6.4E+28
65= 6.5E+28
66= 6.6E+28
67 - 99
petawatts to picowatts
67= 6.7E+28
68= 6.8E+28
69= 6.9E+28
70= 7.0E+28
71= 7.1E+28
72= 7.2E+28
73= 7.3E+28
74= 7.4E+28
75= 7.5E+28
76= 7.6E+28
77= 7.7E+28
78= 7.8E+28
79= 7.9E+28
80= 8.0E+28
81= 8.1E+28
82= 8.2E+28
83= 8.3E+28
84= 8.4E+28
85= 8.5E+28
86= 8.6E+28
87= 8.7E+28
88= 8.8E+28
89= 8.9E+28
90= 9.0E+28
91= 9.1E+28
92= 9.2E+28
93= 9.3E+28
94= 9.4E+28
95= 9.5E+28
96= 9.6E+28
97= 9.7E+28
98= 9.8E+28
99= 9.9E+28

Popular conversions

Popular units

petawatts

The petawatt (PW) is equal to one quadrillion (1015) watts and can be produced by the current generation of lasers for time-scales on the order of picoseconds (10−12 s). One such laser is the Lawrence Livermore's Nova laser, which achieved a power output of 1.25 PW (1.25×1015 W) by a process called chirped pulse amplification. The duration of the pulse was roughly 0.5 ps (5×10−13 s), giving a total energy of 600 J.

picowatts

The picowatt (pW), not to be confused with the much larger petawatt (PW), is equal to one trillionth (10−12) of a watt. Technologically important powers that are measured in picowatts are typically used in reference to radio and radar receivers, acoustics and in the science of radio astronomy.