While at
Sproul Observatory, he made
astrometric measurements of
Barnard's Star and in the 1960s reported a periodic "wobble" in its motion, apparently due to
planetary companions. It was not until several decades had passed that a consensus had formed that this had been a spurious detection. In 1973 astronomers
George Gatewood of the
Allegheny Observatory and
Heinrich Eichhorn of the
University of Florida, using data obtained with improved equipment on the 30-inch Thaw Refractor telescope, did not detect any planets but instead detected a change in the color-dependent image scale of the images obtained from the 24-inch refractor telescope at the
Sproul Observatory used by Van de Kamp in his study. Astronomer
John L. Hershey found that this anomaly apparently occurred after each time the
objective lens was removed, cleaned, and replaced. Hundreds more stars showed "wobbles" like
Barnard's Star's when photographs before and after cleaning were compared – a virtual impossibility. while modern radial velocity curves place a limit on the planets much smaller than claimed by Van de Kamp. A study in 2018 suggested that there was a planet orbiting Barnard's Star (
Barnard's Star b), albeit of much lower mass than Van de Kamp could have detected; Additionally, three other candidate low-mass planets were proposed in this study. All of these planets orbit closer to the star than the
habitable zone. However, the indicated masses of the planets are again far below those capable of detection by Van de Kamp. ==Other work==