Absolute distance measurements can be performed with an interferometric method that uses only a single tunable laser. This method has one major drawback, because a small target movement of the order of one wavelength during a measurement will be interpreted as a movement of one synthetic wavelength. This effect is usually mitigated by adding a second (nonscanning) laser. We show that absolute distance measurements can be performed with only one laser if the movements encountered are smooth, on the time scale of one measurement. In this case the movement errors can be compensated with a simple algorithm that combines several subsequent measurements. Several different techniques can be used to measure absolute distances, among which are time-of-flight measurements, high-frequency modulation schemes, and interferometric methods. Of these, only the last two have the potential to achieve resolutions below a millimeter over several hundred meters. Most of these methods are not truly absolute distance measurements, but systems that are sensitive to changes on the scale of a certain synthetic wavelength. The total distance can be calculated only with a priori (low-resolution) knowledge of the distance or by cascading a number of systems with decreasing synthetic wavelengths. 1,2 Truly absolute, single-stage distance measurements can be made by sweeping a laser over a known wavelength range and measuring the phase difference interferometrically during the sweep, usually called frequency-sweeping interferometry. 3,4 This method suffers from a basic drawback that has large consequences if the target moves during a measurement. A movement of the target over one optical wavelength is interpreted as the movement over one synthetic wavelength. This problem is usually solved by adding a second laser, which reduces the sensitivity to movements of the order of the synthetic wavelength itself. 5,6 We explore a solution without a second laser, by measuring in the presence of movements and correcting for the movement errors in the data analysis. Our intended application is absolute distance metrology between satellites. The Darwin Space Interferometer, for example, would require knowledge of the absolute distance between two satellites with an accuracy of better than 100 m over a distance of 250 m. Consider an optical interferometer with a fixed optical path length difference L that is equipped to measure phase as a function of time. For fixed or slowly changing optical frequency , the phase is proportional to both the length and the frequency. Because the phase is usually measured modulo 2, the absolute phase is unknown. By unwrapping the phase over time it is, however, possible to measure phase differences. If the light source is a tunable laser that is swept from optical frequency 1 to 2 , the total phase difference will bewith c the speed of light, ⌬ the frequency difference of the sweep, and ⌳ the so-called synthetic wavelength defined byReversing Eq. (1), the length L should be calculated asThe length is thus directly proporti...