The Hubble Space Telescope and the Messier objects
The famous Hubble Space Telescope is certainly one of the most innovative
tools of the astronomers in the 1990s decade; the present author is just
now going to predict (and is convinced it deserves) that it might win the
title "Photographer of the Decade" for the 1990, as Voyager 2 was
nominated for the 1980. Its most spectacular results, together with an
open and intelligent public relations policy of the Space Telescope
Science Institute, has provided astronomers with a great flood of data
and high-quality images, and an outstanding popularity, especially as all
the materials get public domain two years after they were obtained.
The Hubble results have revolutionized the state of knowledge in virtually
any branch of astronomy -- not that every good result comes from the HST,
but as these data are available publicly, they are used if ever possible;
from planets, comets, and asteroids to stars, clusters, nebulae, and
galaxies, every sort of objects in the sky were investigated, often
obtaining most revolutionary results.
Among the most outstanding achievements are observations of objects from
Messier's catalog, as those are outstanding representatives of all types
of Deep-Sky objects. Because not every author has made his results
available to the public domain, we cannot present a comprehensive review
here at the moment. But we have tried to link into our catalog some of
the most interesting achievements.
There's but one fact on the Hubble Telescope's optics which must be kept
in mind: The Hubble telescope has a very long focal length of 190 feet (58 m),
and thus a one degree field measures one full meter in the space telescope's
focal plane, and one arc minute about 1.7 cm. As its detectors are very much
smaller, their fields of view are actually small, so that only photos of small
portions of extended objects like most of Messier's catalog can be obtained.
Moreover, the Hubble Space Telescope is not only an astronomical instrument
(though the telescope makes up its biggest part) but also a sophisticated
spacecraft. As a spacecraft, it has proven to be very reliable, and was
so well operated that the technological operations did virtually never concern
the scientific program (at least up to November 1999 when it shut down itself
because the fourth of 6 gyroscopes failed - only to be recovered in the
third servicing mission, STS-103, in December 1999).
The Hubble Space Telescope (HST) was originally projected under the name
"Large Space Telescope" (LST) and then simply "Space Telescope" (ST), and
developed since the 1970s.
Indeed, Hubble is one of the more important in a considerably long list of
orbiting telescopes,
or astronomy satellites. It is the second of four in a NASA series of large
orbiting observatories, observing in the visible light, together with
the Compton Gamma Ray Telescope (CGRO) observing in Gamma-ray light,
the Chandra X-ray Observatory (CXO), and
the Spitzer Space Telescope (SST) observing in
Infrared.
Here's a list of links to the Hubble observations of Messier objects we
could collect with our pages:
M1:
Jeff Hester and
Paul Scowen of the
Arizona State University, Tempe, Arizona, have obtained
gorgeous images of the Crab Nebula
with the Hubble Space Telescope. These images have been reproduced
previously in Sky and Telescope of January 1995, and have provided
some new and significant insight into the internal processes of this
supernova remnant. Some views of fine detail
have been extracted, which are e.g. suitable for computer screen background.
On May 30, 1996, new studies of the same
authors have provided some new insight into the dynamics and changes of the
Crab nebula and its pulsar.
Studies of June 2000 of 1995 images reveal details
of the Heart of the Crab Nebula.
Multispectral image from October 2006, created
from optical Hubble, X-ray Chandra, and infrared Spitzer exposures.
M33: Discovery of the hot young giant stars
which excite the huge
emission nebula NGC 595 in M33 to shine.
The giant diffuse nebula NGC 604 in M33
has been photographed with the HST, resolving about 200 hot young massive
stars.
M84:
A massive central object in M84 was
detected in the heart of this Virgo Cluster lenticular when in early 1997
the newly installed Space Telescope Imaging Spectrograph (STIS) was used
to investigate this galaxy.
M96:
Nial R. Tanvir used the HST to detect and investigate Cepheid variables
in this galaxy. HST image of M96
M100:
This grand-design spiral was among the first objects
photographed after the HST refurbishment
by the crew of the Shutle mission STS-61 in December 1993.
Moreover, this galaxy is the home of the first
Cepheid variables discovered
in the Virgo cluster of galaxies, giving a distance
of 50-60 million light years, and a Hubble constant of 80+/-17.
However, with the refinement of the distance scale by ESA's astrometric
Hipparcos satellite, this value must be refined by about 10 percent, and
current estimates for H0 are closer to 67+/-7.
We know of more good Hubble results concerning Messier objects.
They are listed below, and we would like to get images and more
information for inclusion here:
M101: The distance of M101 has been
determined as 24 million light years (27 if corrected for Hipparcos data),
again with Cepheids (again, within the
H0 Key Project).
A HST image of M101 was in a semi-recent issue of Astronomy magazine.
Also, there were older images which are not yet on SEDS, e.g. in the slide
sets of the Astronomical Society of the Pacific, including more
photos of M42, M77, M87, and others which still await being included here.
Some Hubble images of non-Messier objects have also found their way into our
service: