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OUR OBSERVATIONS
Our group was able to conduct several observations of the star during its eclipses and to visually approximate its magnitude. To do this, we chose several non-variable stars, whose magnitudes we knew, and compared them with the magnitude of Algol. Our observations are recorded in Table 1.
| Date (JD UT) | Comparison Stars | Estimated Magnitude | Remarks | |||
| Name | m | Name | m | |||
| 2452509.560 | Alpha Per | 1.80 | Beta Ari | 2.64 | 2.20 | Before eclipse |
| 2452511.468 | Beta And | 2.06 | Eps Cas | 3.38 | 3.00 | Beginning of eclipse |
| 2452511.468 | Gamma And | 2.18 | Alpha Tri | 3.41 | 3.41 | Eclipsed |
| | |
| The Constelation of Perseus. Algol is the bright star in the middle. | Algol and the region around it. | Algol |
We were also able to take a picture of Algol using a CCD camera and a Schmidt telescope at the National Astronomical Observatory in Rozhen, Bulgaria. Unfortunately, due to poor weather conditions, we were unable to picture a minimum. We also took photographic pictures of the Perseus constellation and the near regions at the National Astronomical Observatory and Planetarium of Gabrovo.




