COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 2988 Konkoly Observatory Budapest 20 February 1987 HU ISSN 0374 - 0676 UBV OBSERVATION OF NOVA ANDROMEDAE 1986 M. Suzuki (Ena City, Gifu, Japan) discovered a nova of m = 8.0 at alpha = 23h09.5m, delta = +47d10' (equinox 1950.0) on Dec. 5.44 (UT), 1986. After the maximum light, we observed the nova in UBV colours with the 40-cm reflector of the Science Museum of Kawasaki on Dec. 11 (UT), 7 And was used as the comparison star. The obtained differential magnitudes in the sense of Nova - 7 And are given in Table I, which are also plotted in Figure l. Table I UBV Photoelectric Observations of Nova Andromedae 1986 1986 Dec. 11(UT) G. M. T Hel. JD DU mag DB mag DV mag 2446775 8 45.6 0.8650 2.1827 2.8020 2.9739 9 15.7 0.8859 2.1805 2.7903 2.9653 10 5.5 0.9205 2.1893 2.7813 2.9520 10 25.2 0.9342 2.1749 2.7837 2.9582 10 42.3 0.9461 2.1825 2.7831 2.9612 11 6.5 0.9629 2.1818 2.7861 2.9757 11 25.6 0.9761 2.1995 2.7686 2.9728 11 48.3 0.9919 2.1752 2.7484 2.9546 12 16.5 1.0115 2.1437 2.7272 2.9307 12 40.0 1.0278 2.1349 2.6687 2.8860 12 57.7 1.0401 2.1484 2.6703 2.8925 Our observation indicates the existence of some increasing light. It is also found that the B-V colour is becoming redder with time while the U-B bluer. [FIGURE 1] Figure 1. Light and colour variations of Nova Andromeda 1986 on Dec. 11. We would like to express our hearty thanks to Prof. M. Kitamura of Tokyo Astronomical Observatory for his encouragement. SHIGERU OHMORI and TOSHIYA KAGA JAPOA (Japan Amateur Photoelectric Observers Association) c/o Geology Division Education Centre of Kanagawa Prefecture, Fujisawa City, Fujisawa 4210, Kanagawa, 251 Japan.