Quote:
Originally Posted by mswhin63
I am no expert but was looking at the proportion of the comet compared to the larger one below looks the same or very close (ball x tail) as the tails only appear when it gets closer to the sun I assume the comet would be about the same.
Hey I might be totally out of league though. I am still learning.
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One thing i have learnt is that its like looking at asterisms, some things that are brighter seem closer but not necessarily so.....
Comet sizes can come down to a number of factors, size of the nucleus, gas/dust production, distance, intrinsic brightnesses......until an orbit is determined then anything about the comet can only be speculative.
Gotta start somewhere!
So if you went to the CBAT pages, find Comets, then dig up the orbital ephemerides you can compare their DELTA which is Earth-Comet distance.
http://www.cfa.harvard.edu/iau/Ephem...ts/2009U6.html
http://www.cfa.harvard.edu/iau/Ephem...ets/0081P.html
C/2009 U6
Date TT R. A. (2000) Decl. Delta r Elong Phs m1
2009 10 26 09 41.54 +13 09.2
1.788 1.711 69.3 32.9 16.6
2009 10 31 09 52.04 +12 54.9
1.767 1.736 71.8 32.9 16.6
2009 11 05 10 02.04 +12 42.6
1.745 1.761 74.4 32.9 16.7
81P/ Wild
2009 10 26 09 42.01 +12 39.3
2.092 1.969 69.0 28.1 13.0
2009 10 31 09 52.98 +11 47.6
2.020 1.943 71.2 28.9 12.9
2009 11 05 10 03.98 +10 54.0
1.949 1.917 73.4 29.7 12.7
Notice the difference in Delta (highlighted in red) in AU , so 81P is further away at the moment, but is much more active, so it's brightness will be higher. Elongation is the Comets angle from the Sun as seen from Earth.
r = Perihelion distance (closest approach to the sun) in A.U.
m1 is the predicted visual magnitude.
Don't worry too much about phase angle, thats better explained looking at an orbital simulation.
Hope this helps!