Asteroid (99) Dike Occultation Dec. 1 am, Delmarva to Mongolia

Hundreds of telescopes are in this path, also over Washington, Pittsburgh, Cleveland, and Detroit

Accuweather indicates conditions may be good in the Maryland - n. VA - DC region, but poor towards the northwest

The 8.9-mag. star is in a rich Milky Way field in Auriga

New: 2005 Nov. 28

Accuweather forecasts about 40% cirrus in the Washington, DC region, 
so chances look good for being able to see this relatively bright 
star over 40 deg. above the northwestern horizon in our area.  
Chances are poorer for areas northwest of our region.

If you have a 2-inch or larger telescope, we need your help to 
observe the occultation of 8.9-mag. SAO 58354 = HIP 26902 by 
the 69-km asteroid (99) Dike, visible Thursday morning Dec. 1st in a 
path passing over the southern Delmarva Peninsula, southern and 
western Maryland, northern Virginia, and Washington, DC at 10:15 UT 
= 5:15 am EST Nov. 11; at 10:16 UT over n.e. West Virginia, south-
central & western Penn. (Pittsburgh at s. limit, Erie and Harrisburg 
north of the northern limit but within the 1-sigma uncertainty zone 
where an occultation is possible); n.e. Ohio, s.w. Ontario, and 
eastern and northern Michigan (Detroit just s. of the s. limit); at 
10:17 UT (4:17 am CST), over western Upper Michigan, extreme n.e. 
Minnesota, western Ontario, and eastern Manitoba n.e. of Winnipeg; 
then the path extends across n.w. Canada, northern Alaska, eastern 
Siberia, n.e. China, and s.e. Mongolia (10:26 UT), rather forbidding 
lands with no known occultation observers.
For more information about this event, see Steve Preston's Web site. 
It has detailed finder charts of different scales to easily locate 
the star.  Guy Nason has prepared some quite detailed maps of the 
path from eastern Manitoba to the Atlantic:

Maryland, e. & n. Virginia, n.e. W.Va.
Pennsylvania & n.e. Ohio
Michigan & n.e. Minn.
w. Ontario & e. Manitoba
Power Point file with all four maps.

If you can help us observe this occultation, either from your home 
or observatory, or as a mobile observer, please inform me and Derek 
Breit (e-mail breit_ideas@hotmail.com ).  For coordinating coverage 
of this occultation, a list of stations sorted by distance in km 
from the predicted central line, are on Derek Breit's Web site.
You can search for your, or your town's or observatory's, name to 
see just when the occultation is predicted for your area (that time 
should be accurate to within 15 seconds or so), the probability for 
having an occultation there, and the predicted Sun and star 
altitudes at the time.  If your station is not in the list, send me 
and/or Derek Breit your coordinates, or your street address, and we 
can add it. Derek will update his Web site with information 
indicating which distances from the central line (or "chords") will 
have observers trying to time the occultation.  For information 
about timing occultations, click here 
with some more good information by Guy Nason here.

Let me know your plans, whether you plan to observe from a fixed 
site or are mobile, needing a line to aim for.  During the next 
nights, I'll distribute an edited down list of stations from Derek 
Breit's more extensive list including only those who have said that 
they will try to observe this good event.  I hope to try to observe 
the occultation from multiple sites across the path, probably mostly 
near US 301 from s. of Bowie to the Nice Bridge, but may select a 
different area, depending on the weather.  If any others in Maryland 
or DC-region want to help me with this, let me know. 

Guy Nason also is organizing observers in southwestern Ontario; for 
details, including a more detailed map of that area, click here. 

You can see the path superimposed on very detailed 
maps and satellite imagery on Charlie Ridgway's Web site.  
For general information about his site, click here, 
while for the map specifically for the Dike occultation,
click here.  
On this site, you can enter a distance from the central line in km 
in a special "offset" box (just write over the default value of 1000 
given there) and it will plot gray lines at that distance north and 
south of the central line. 

Type your distance number (in km) in the box just to the left of the
"Plot Offsets" box at the bottom of the map.  You need to type a
number with no sign, then two gray lines are plotted; zoom in on the
gray line northeast of the yellow central line if your distance is +
and on the gray line southwest of the central line if your distance
is -.  You can move the map by grabbing it (left-clicking and
holding down) and you can zoom in or out by left-clicking on the
scale in the upper left part of the map (+ on that scale means "zoom
in" for more detail over a smaller area).  You can toggle between
"map" (showing town and road names), "satellite" for satellite 
imagery, and "hybrid" for both together.  

The target star is 3.4 deg. west-southwest of 3rd-mag. theta Aurigae 
at J2000 RA 5h 42m 41.5s, Dec +36 deg. 08' 59"; the target star is 
two deg. southwest of 5th-mag. upsilon Aurigae and only 5' southeast 
of an 8th-mag. star, and 30' north and a little east of a 7th-mag. 
star; there's a distinctive pattern of other 9th-mag. stars near the 
target star in this rich winter Milky Way field that will help 
locate the target.  The spectral class of the target star is B5.  
If an occultation occurrs, it would last up to 5 seconds with a 5-
magnitude drop. 

There are other occultations soon in the Mid-Atlantic region,
but this is the best asteroidal occultation passing over the 
Washington, DC area this year, so it deserves a special effort.  If 
the weather forecast remains good enough, plan to go to bed a little 
earlier than usual Wed. night so you can get up a little earlier to 
try this good event.  

David Dunham
e-mail home dunham@starpower.net; office david.dunham@jhuapl.edu