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 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.
  
- M4: 
  White dwarfs (September 1995);
  Old planet discovered near white dwarf and
  pulsar (July 2003)
  
- M8:
  Hubble Views the Hourglass Nebula in M8
  (January 1997)
- M14:
  Search for Nova of 1938 (October 1990)
- M15:
  Dense Core of the globular cluster,
  similar to active galactic nuclei (November 1995);
  M15 and its Planetary Nebula Pease 1
  (August 2000)
  
- M16: Gas Pillars and Evaporating 
  Gaseous Globules in the Eagle Nebula
  (November 1995);
  screen sized crops
  
- M17: Star formation in the central part of the 
  Omega Nebula M17 (April 2002);
  Turbulent Gas in M17 (April 2003)
- M20: Observation of 
  Star birth in the Trifid Nebula (1999)
  
- M22: HST 
  finds hints for planet-sized objects in M22.
- M27:
  A close-up of M27 obtained in November 2002 (2003).
  
- M31: Discovery of the Andromeda Galaxy's
  double nucleus (1993).
  Investigation of M31's brightest 
  globular cluster, G1 (1996).
  
- M32:
  The Nucleus of M32 (1992).
  Discovery of blue giant stars near the nucleus 
  of M32 (1999).
- 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.
- M42: 
  early pre-repair photos (1993),
  Proplyd discovery photos (June 1994),
  Mosaic and closeups (November 1995),
  Trapezium cluster and Proplyds (January 1997),
  OMC 1 molecular cloud (NIC, May 1997),
  Trapezium in IR (August 2000),
  Proplyds under hot radiation (April 2001)
  
  
- M45:
  Barnard's Merope Nebula, IC 349,
  Distance to M45 star (June 2004)
- M51:
  Hubble photos of M51, especially of its core 
  ("X" or "y" structure in the core of M51) have been taken before and after its 
  repair in December 1993 by the crew of the Space Shuttle mission STS-61. 
  The HST also recorded 
  Supernova 1994I in M51.
  In 2001, new images of inner spiral arms
  of M51 revealed unprecedented detail of spiral arms and dust clouds.
  
- M57:
  HST image of M57;
  Oct 98 HST image.
- M60:
  HST image of M60's center
- M64: 
  IR image of M64 central region taken by
  Nicmos-3 (PR 99-10 from March 18, 1999);
  Optical image of M64's central region, 
  WFPC-2 (PR 2004-04 from February 5, 2004)
- M77: 
  Early HST photos of M77's core (Oct 1990).
  The active nucleus of this 
  Seyfert II galaxy was revealed by the HST early after its refurbishment
  in December 1993.
  
- M80:
  Gorgeous image of M80 from the Hubble 
  Heritage Project, showing various types of stars including Blue Stragglers.
  July 1999.
- M81:
  Cepheid variables in M81 (June 1993).
- M82:
  M82 image by Hubble, September 1997
  (processed by Mischa Schirmer), and press release.
  
- M83:
  M83 images by HST WFPC2.
- 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.
- M87:
  The "Smoking Gun" (June 1994),
  M87's active nucleus, surrounded by an accretion disk.
  In addition, R. Mark Elowitz 
  has provided a well-processed HST image of 
  M87's jet.
  M87's jet by HST and NRAO (Oct 1999)
  New view of M87's nucleus and jet (Aug 2000).
  Finally, we have an older (pre-repair) 
  image of M87 and its jet.
  
- M91:
  M91 spiral arms, with an asteroid captured
  and discovered on flyby.
- 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.
  
- M101:
  
- M102/NGC 5866:
   Hubble Sees Galaxy on Edge
- M104:
  Hubble Mosaic of the Majestic Sombrero Galaxy.
- M105:
  Central Massive Dark Object (Jan 1997)
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:
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:
Links to materials of, from, and about the Hubble Space Telescope:
Hartmut Frommert 
Christine Kronberg
[contact]
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Last Modification: February 6, 2007