Kuiper Belt Object Sizes and Distances from Occultation Observations
- 23 April 2003
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 589 (2), L97-L100
- https://doi.org/10.1086/375852
Abstract
There are several observational campaigns under way to detect kilometer size foreground Kuiper Belt Objects (KBOs) through their occultation of background stars. The interpretation of an occultation light curve, unfortunately, is affected by a geometric degeneracy such that one is unable to determine the KBO size independent of its distance. This degeneracy can be broken through a precise measurement of the relative velocity obtained from simultaneous observations of individual events. While an array of telescopes spread over an area of few square kilometers can be employed, it is unlikely that the relative velocity can be measured to the required accuracy to help break this geometric degeneracy. The presence of diffraction fringes in KBO occultation light curves, when projected sizes of occulted stars are smaller than the Fresnel scale, improves determination of size and distance significantly. In this regard, we discuss the potential role of a dedicated satellite mission for KBO occultation observations. If dwarf stars at the V-band magnitudes of 14th and fainter can be monitored at time intervals of 0.1 seconds with normalized flux errors at the level of 1%, the occultation observations will allow individual KBO sizes and distances to be determined at the level of a few percent or better.Comment: 4 pages, 2 figures, To appear in ApJ LetterKeywords
This publication has 12 references indexed in Scilit:
- Occultation Searches for Kuiper Belt ObjectsThe Astrophysical Journal, 2003
- Kuiper Belt Objects: Relics from the Accretion Disk of the SunAnnual Review of Astronomy and Astrophysics, 2002
- Planet Formation in the Outer Solar SystemPublications of the Astronomical Society of the Pacific, 2002
- A Detection Method for Small Kuiper Belt Objects: The Search for Stellar OccultationsIcarus, 2000
- Occultations by Kuiper belt objectsMonthly Notices of the Royal Astronomical Society, 1997
- PROBING PLANETARY ATMOSPHERES WITH STELLAR OCCULTATIONSAnnual Review of Earth and Planetary Sciences, 1996
- MACHO velocities from satellite-based parallaxesThe Astrophysical Journal, 1994
- Stellar occultations by small bodies - Diffraction effectsThe Astronomical Journal, 1987
- Can ‘invisible’ bodies be observed in the Solar System?Nature, 1976
- The Advanced Theory of Statistics. Vol. 3.Published by JSTOR ,1969