Home Page Updated on December 16, 2020
MisV0858
|
R.A. | 17h57m57s.52 | |
Decl. | -28o25'18".5 | (2000.0) |
Mag. | 12.7-16.0Rc | |
Type | M | |
Period | 220 | |
Epoch | 2450681 |
Digitized Sky Survey GIF image (15 x 15 arcmin)
It was discovered by Seiichi Yoshida on images taken by Ken-ichi Kadota, Ageo City, Saitama, Japan.
MisV0857 is 36 arcsec from MisV0858.
Stefan Huemmerich and Klaus Bernhard revealed that it is a Mira type variable with a period of 220 days, brightness range of 12.7-16.0 mag(Rc), using the MACHO project data.
14.2 +--------------------------------------------------------+ | * | | | | * | | * | | | | | | | | | | | | | | | | | | v v | | | | | | | | | | | | | | | | v | 15.6 +--------------------------------------------------------+ 2451261 2451615 1999 Mar. 23 2000 Mar. 11
Date | Mag | Filter | Observer |
---|---|---|---|
1999 Apr. 8.75742 | [15.0 | C | Ken-ichi Kadota |
1999 Apr. 8.75797 | [15.0 | C | Ken-ichi Kadota |
1999 Apr. 30.74247 | [15.0 | C | Ken-ichi Kadota |
1999 Sept. 23.43274 | [15.5 | C | Ken-ichi Kadota |
1999 Sept. 23.43324 | [15.5 | C | Ken-ichi Kadota |
2000 Feb. 24.83672 | 14.4 | C | Ken-ichi Kadota |
2000 Feb. 24.83728 | 14.3 | C | Ken-ichi Kadota |
2000 Feb. 24.83799 | 14.4 | C | Ken-ichi Kadota |
2000 Feb. 24.83854 | 14.5 | C | Ken-ichi Kadota |