| Pressure of Air at 25 degree Torr | Molecular Density molec/cm3 | Molecular Incident Rate molec/cm2-sec | Mean Free Path cm | Time to Form a Monolayer second (8x1014molec/cm2) |
| 760 | 2.46x1019 | 2.88x1023 | 6.7x10-6 | 2.9x10-9 |
| 1 | 3.25x1016 | 3.78x1020 | 5.1x10-3 | 2.2x10-6 |
| 10-3 | 3.25x1013 | 3.78x1017 | 5.1 | 2.2x10-3 |
| 10-6 | 3.25x1010 | 3.78x1014 | 5.1x103 | 2.2 |
| 10-9 | 3.25x107 | 3.78x1011 | 5.1x106 | 2.2x103 |
| 10-12 | 3.25x104 | 3.78x108 | 5.1x109 | 2.2x106 |
| 10-15 | 3.25x10 | 3.78x105 | 5.1x1012 | 2.2x109 |
| Degree of Vacuum | Pressure Range (Pa) : 1 Pa = 7.5x10-3 Torr |
| Low Vacuum (LV) | 3.3x103 < P < 105 |
| Medium Vacuum | 10-1 < P < 3.3x103 |
| High Vacuum (HV) | 10-4 < P < 10-1 |
| Very High Vacuum | 10-7 < P < 10-4 |
| Ultrahigh Vacuum (UHV) | 10-10 < P < 10-7 |
| Extremely High Vacuum (XHV) | P < 10-10 |
2. Natural Vacuum: No natural high vacuum is known on earth. Some of these applications are very vital. Human beings are pumping to about 740 Torr during respiration, and may achieve pressures as low as 300 Torr by suction. The octopus is able to achieve pressures of about 100 Torr. In space the pressure decreases with the altitude from the pressure of 760 Torr at sea level. Up to 100 km altitude (troposphere and stratosphere) the pressure decreases quite regularly by a factor of 10 per 15 km altitude, which results in a pressure of 10-3 Torr at about 90 km altitude. The ionosphere (100-400 km) contains a large number of ionized atoms, and its pressure decreases only by a factor of 10 every 100-200 km. This decrease results in a pressure of about 10-10 Torr at an altitude of 1,000 km. About 400 km ultrahigh vacuum conditions exist. At 10,000 km a pressure of about 10-13 Torr exists. The pressure measured on space crafts are determined by the spacecraft velocity and gas particle concentration.
