When a minor planet (asteroid, planetoid) passes in
front of a star, the star will be occulted for a short while, typically
for a few seconds. Exact measurements from various places make it possible
to determine the asteroid's size and shape. Such occultations can often
be observed with small instruments, e.g. binoculars. The predicted times frequently
differ from the real ones. The event can sometimes come
unexpectedly, making it difficult to obtain the correct time.
This applet, written and provided by Klaus Nagel, simulates an occultation. It shows a view of the night
sky through a telescope. One of the stars will be occulted, within a two minute time
period, for a few seconds. Place the mouse pointer anywhere within the simulated field of view and
click the mouse when you notice the occultation, and then again
when you notice the star reappear. The real occultation times, your
measurements, and the deviations will be displayed three seconds later. This gives an idea of your
Personal Equation (PE) and its variance. This can then be applied to refine a real
occultation timing, and therefore obtain a more accurate result.
The star to be occulted is located near the centre. It will be marked
red for three seconds when you push the button Display.
The other button will Start
a new trial.
If you require specific occultation data for your locality, or details of occultations
involving fainter stars, please get in touch with the Director of the
Occultation Section giving your geographical location. Graphical representations of
each occultation will be available at the Occultation Sections web-site before
the event is due to take place. Please visit the UK's definitive site for
lunar and asteroidal occultations: www.asterocc.org.uk