Nature October 7th 1875
In No.5 of “Publicazioni del Reale Osservatorio di Brera in
Milano”, Herr Tempel has laid down the stars from the Pleiades, from the
Durchmusterung , and traced the outline of the nebula near Merope as it
appeared to him with a magnifying power of twenty four on a telescope of four
inches aperture. The outline is shown to be elliptical, one extremity of the
longer axis, the northern one, at Merope, and the inclination of this axis to
the circle of declination about 18 degrees, so that as referred to Merope, the
angle of position of the longer axis is 198 degrees.
M Wolf, of the Observatory of Paris, observing with the
telescope of 0.31m aperture in March
1874, perceived two nuclei, one almost concentric with Merope, the other and
brighter of the two at a distance of about seven seconds, on the same parallel,
following. From the month of November
1874 to the end of February 1875 the nebula could not be seen notwithstanding
the very favourable atmospheric conditions, and at the same time M Stephan was
unable to detect it with the telescope of 0.80m. M Wolf concludes that the
nebula is certainly variable and that its period is pretty short.
Herr Tempel remarks that generally the nebula has been much
more readily seen with small telescopes than with large ones, and doubt has
been expressed as to any real variability of light; yet it is not easy to
understand, except upon this supposition, why the nebula should be visible at
certain times in a particular telescope and invisible at others, the
circumstances of the sky appearing to be about the same in all cases.







