Related Experiment Video
Updated: Aug 8, 2026

Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2018 JULY-SEPTEMBER
1Center for Solar System Studies-Palmer Divide Station, 446 Sycamore Ave., Eaton, CO 80615 USA.
None:
Lightcurves for 12 main-belt asteroids were obtained at the Center for Solar System Studies-Palmer Divide Station (CS3-PDS) from 2018 July-September. Analysis of a larger amplitude lightcurve in 2018 for 5175 Ables lead to new analysis and results for earlier apparitions. The Hungaria asteroid (37378) 2001 VU76 is possibly a super-fast rotator with a period and size that put it just above the so-called "spin barrier."
Related Concept Videos
Attenuated Total Reflectance (ATR) Infrared Spectroscopy: Overview
The ATR process begins by directing a beam...
Atomic Emission Spectroscopy: Interference
Atomic Emission Spectroscopy: Lab
Flame Photometry: Overview
Flame Photometry: Lab
Relative Motion Analysis using Rotating Axes
However, to express the relative position of point B relative to point A, an additional frame of reference, denoted as x'y', is necessary. This additional frame not only translates but also rotates relative to the fixed frame, making it instrumental in...

