[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-chat 9] Mira Comparison stars
- Date: Wed, 29 Jan 1997 09:33:40 -0500 (EST)
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: hz642@cleveland.Freenet.Edu (Robert J. Modic)
- Subject: [vsnet-chat 9] Mira Comparison stars
- Reply-To: hz642@cleveland.Freenet.Edu (Robert J. Modic)
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
I'd like to clarify the remarks I made yesterday about Alpha
Cet and other comparison stars for Mira. First, I assumed that
most observers are making estimates of Mira naked eye now that it
is mag ~2.6. Secondly, I assumed that these estimates where made
with the stars in focus. In this case, the Purkinje effect will
cause Alpha Cet to appear ~0.2 mag or more brighter than its V mag.
Defocusing the stars and using averted vision will cause the opposite
to occur, as Brian Skiff mentioned. I observed Mira, Alpha Cet, and
Beta Ari last night using these two methods. With direct vision and
in focus, Alpha Cet was ~ 0.3 mag brighter than Beta Ari. Using
a little averted vision, Alpha was 0.1 to 0.2 mag brighter. Viewed
out of focus (I wear glasses) and with plenty of a.v., Alpha was
~0.15 mag fainter than Beta Ari.
Finally, my suggestion of Beta Cet as a good comparison star
for Mira was based on its V mag and color. Obviously, when Mira
is in the SW from mid-northern latitudes, Beta Cet is too low to be
a useful comp star. But when Mira is in the SE or when viewed from the
southern hemisphere, Beta Cet is a good choice. Alpha Ari is a good
alternative for us northerners.
Regards,
Robert J. Modic
AAVSO
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp