koronisfamily.com
Identify observable asteroids from list of targets of interest
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Observer circumstances
Observer location:
Boambee
Carbuncle Hill Observatory
Cerro Tololo Observatory
Cornell Hartung-Boothroyd Obs.
Foggy Bottom Observatory
Lowell Obs. Anderson Mesa
Mauna Kea
Oakley Observatory
Palmer Divide Observatory
Santana Observatory
Vassar College Observatory
Wallace Observatory
Whitin Observatory
Latitude
, East longitude
Local date at start of night (yyyy mm dd):
Time zone for output:
(UT-12 hr)
(UT-11 hr)
(UT-10 hr)
(UT-9 hr)
PST (UT-8 hr)
PDT (UT-7 hr)
MST (UT-7 hr)
MDT (UT-6 hr)
CST (UT-6 hr)
CDT (UT-5 hr)
EST (UT-5 hr)
EDT (UT-4 hr)
(UT-3 hr)
(UT-2 hr)
(UT-1 hr)
UT
(UT+1 hr)
(UT+2 hr)
(UT+3 hr)
(UT+4 hr)
(UT+5 hr)
(UT+6 hr)
(UT+7 hr)
(UT+8 hr)
(UT+9 hr)
(UT+10 hr)
(UT+11 hr)
(UT+12 hr)
Size for
DSS finder charts
(arcminutes):
Width
, Height
Target list
:
Highest-priority objects
A. Koronis family spin vectors
B. Koronis family phase curves
C. Koronis family spin periods
D. Koronis family shapes
E. Koronis family 5 to 10 km
F. Control Group III
G. Karin cluster
H. Koronis family(Mothe-Diniz)
Misc. non-Koronis objects
Possible class projects
Criteria for "observable objects"
Predicted mean
V
magnitude
brighter than
and also
fainter than
Object altitude
above
degrees
Sun altitude
below
degrees
Moon
must be either
at least
degrees away from object,
or
at least
degrees from the object
and also
less than
% lit
Additional object selection criteria
Minimum time span observable
if not specified in targets file: observable at least
hours
(Select
for specified span length to override targets file values in all cases)
Observable starting
no later than
minutes after start of night
Observable until
at least
minutes before end of night
H
magnitude brighter than
and also
fainter than
H
magnitude for selection and for predicted
V
magnitudes:
use Koronis program
H
and
G
if available
use IAU
H
and
G
in all cases
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$Revision: 2.16 $
Credits
Copyright (c) 2009 Stephen M. Slivan. All rights reserved.