Among his contributions were attempts to determine
longitude. Determining longitude at sea was one of the major scientific problems of the seventeenth century, and Van Langren devoted much of his work to finding a practical solution. As early as 1621 he proposed that longitude could be calculated by observing the
Moon, particularly by tracking how the illumination of lunar mountains and craters changed during the lunar cycle. of statistical data, showing the wide range of estimates of the distance in longitude between
Toledo and
Rome.|left To show the magnitude of the problem, he created the first (known)
graph of statistical data, showing the wide range of estimates of the distance in longitude between
Toledo and
Rome. He believed he could improve the accuracy of longitude determination, particularly at sea, by observing peaks and craters of the
Moon as they appear and disappear, not only during eclipses of the Moon but also in the course of the entire lunation. His proposed method required accurate observations and detailed mapping of the lunar surface, which led him to undertake systematic studies of the Moon. He named crater
Langrenus on the
Moon after himself, and the name has been preserved to this day. ==External links==