[net.astro] StarDate: January 26 Hubble's Variable Nebula

dipper@utastro.UUCP (Debbie Byrd) (01/26/85)

This is the anniversary of the first picture taken with the Palomar
200-inch telescope.  More on what it photographed -- after this.

January 26  Hubble's Variable Nebula

On this date in the year 1949, the Palomar 200-inch telescope took its
first picture -- of a strange object called Hubble's Variable Nebula.

This object is a cloud in space -- discovered in the year 1783 by Sir
William Herschel.  It now bears Edwin Hubble's name -- not Herschel's
-- because Hubble found out in 1916 that the cloud changes from month
to month.  The changes aren't just in size and brightness -- they're
also in the actual appearance of the nebula itself.  It's thought that
changing light conditions and moving shadows cast on the cloud are due
to some dark masses drifting in the space nearby.

There's also a variable "star" associated with this cloud in space --
which still is being intensely studied by astronomers today.  The
object R -- that's the letter R in the constellation Monoceros -- was
discussed at a conference held in Tucson about a year ago -- a
conference on protostars and protoplanets -- or stars and planets in
the process of being born.  R Mon, like some other stars now known,
appears to have solid material near it -- maybe a disk, although that's
not yet known.  At any rate, although this material doesn't extend as
great a distance as some other similar disks found in the past year or
so, there's enough mass near R Mon to equal about the combined masses
of the giant planets in our solar system -- Jupiter, Saturn, Uranus and
Neptune.  We don't know yet -- but this material may someday become
planets for the faraway star, R Mon.


Script by Deborah Byrd.

(c) Copyright 1984, 1985 McDonald Observatory, University of Texas at Austin