Comet 53P/Van Biesbroeck July 9, 2016 with plotted syndynes
Comet 53P/Van Biesbroeck about 70 days past perihelion
Time Stamp: 2016 07 09, 9:25:59 UT
Motion: 0.22"/min in PA 229.0°
Stack of 4 x 600 seconds
Coma 81" x 50" extended PA 255 degrees
Tail 0.1 arc minutes PA 260 degrees
Charles Bell H47 Vicksburg
0.3-m Schmidt-Cassegrain + CCD + R band filter
Magnitude 15.3 R with 9.35 arc sec aperture radius
I am seeing a concentration of large particles like a spline that line up near a zero velocity syndyne with beta of 0.0010 with about 1 mm diameter.
Assuming dust density = 1000 kg/m^3, dust particle radius = 5.67E-4meters or about 567 microns
According to the width of the tail, there appears to be a range of smaller dust particles.
Plotted syndynes: beta: 0.0010, 0.0100, 0.1000, 0.2000
Ephemeris data:
t - T = +70.45192 days
delta = 1.564 AU
r = 2.494 AU
Elongation = 149.6 degrees
Phase = 11.9 degrees
PsAng = 245.4 degrees
PsAMV = 260.1 degrees
PlAng = -2.8 degrees, earth below comet orbit plane
Comet 53P/Van Biesbroeck July 9, 2016 with plotted syndynes
Comet 53P/Van Biesbroeck about 70 days past perihelion
Time Stamp: 2016 07 09, 9:25:59 UT
Motion: 0.22"/min in PA 229.0°
Stack of 4 x 600 seconds
Coma 81" x 50" extended PA 255 degrees
Tail 0.1 arc minutes PA 260 degrees
Charles Bell H47 Vicksburg
0.3-m Schmidt-Cassegrain + CCD + R band filter
Magnitude 15.3 R with 9.35 arc sec aperture radius
I am seeing a concentration of large particles like a spline that line up near a zero velocity syndyne with beta of 0.0010 with about 1 mm diameter.
Assuming dust density = 1000 kg/m^3, dust particle radius = 5.67E-4meters or about 567 microns
According to the width of the tail, there appears to be a range of smaller dust particles.
Plotted syndynes: beta: 0.0010, 0.0100, 0.1000, 0.2000
Ephemeris data:
t - T = +70.45192 days
delta = 1.564 AU
r = 2.494 AU
Elongation = 149.6 degrees
Phase = 11.9 degrees
PsAng = 245.4 degrees
PsAMV = 260.1 degrees
PlAng = -2.8 degrees, earth below comet orbit plane