What are Messier Objects Tiffany Alago March 1

What are Messier Objects? Tiffany Alago March 1, 2009 Prof. Layden ASTR 309

Introduction Throughout the night as the earth rotates our sky changes, and so does the sky where we stand. The information that continues is the results of a Messier marathon. How many Messier objects can you see in one night? The answer is you never know for sure. If you ask yourself that question everyday, you would most likely get a different answer each day.

Purpose The purpose of this project is to give a brief description of Messier objects: What are they? What are some different types? To show what do some look like. What’s important or interesting about them?

Goals Part of the work of this project was to take the best quality pictures possible. In order to achieve this goal one had to put in practice and improve the skills learned in class, which includes: Planning your night – what are you observing and when are you going to observe it? Checking and predicting the weather. Proper use of the CCD camera. Proper use of the 0. 5 m telescope.

Messier Objects Charles Messier is the first astronomer to come up with a systematic catalogue of deep sky objects. In the Messier catalog there are currently 110 deep sky objects. Some of the types of deep sky objects include: Galaxies – spiral, irregular, elliptical Nebulae – planetary, diffuse Globular clusters Open clusters

Messier Marathon

M 35 Open cluster Right Ascension: 06 h 08. 9 m Declination: +24° 20 m Visual Brightness: 5. 3 mag Apparent Dimension: 28. 0 arc min Exposure time of image: 12 s

M 35 This open cluster is located in Gemini. Discovered by Philippe Loys de Cheseaux. Was catagolized in 1745 or 1746. At a distance of 2, 800 light years Includes several hundreds of stars. Last count was of 513 stars Of intermediate age. Includes some post-main sequence stars: with some red and orange giants of spectral type G to K

M 42 Star forming Nebulae Right Ascension: 05 h 35. 4 m Declination: -05° 27 m Visual Brightness: 4. 0 mag Apparent Dimension: 85 x 60 arc min Exposure time of image: 12 s

M 42 Is an emission and reflection nebula, with an open cluster in Orion. Also known as the Orion Nebula. Is one of the brightest starforming nebulae and one of the brightest diffusion nebulae in the sky It is a big object, considered to cover four times the area of the full moon. Located 1, 600 light years away. Is a very turbulent cloud of gas and dust, hence it’s gaseous nature.

M 42 This nebula is said to be located in the sword of Orion. Under good night sky conditions it can be clearly visible to the naked eye. Is considered one of the brightest of all deep sky objects and is one of the most studied.

M 44 Open Cluster Right Ascension: 08 h 40. 1 m Declination: +19° 59 m Visual Brightness: 3. 7 mag Apparent Dimension: 95. 0 arc min Exposure time of image: 4 s

M 44 Also known as Praesepe or the Beehive cluster. Includes about 200 stars. Is about 577 light years away. Has an estimated age of about 730 million years old. Contains some red giants, white dwarfs and one blue star.

M 44 Mythology behind M 44 is that “Greeks and Romans saw this "nebula" as the manger (Greek: Phatne) associated with two asses who eat from it; Asellus Borealis, the Northern Ass and Asellus Australis, the Southern Ass. Erathosthenes reported that these were the asses on which the gods Dionysos and Silenus rode into the battle against the Titans.

M 44 The titans were frightened by the animals' braying so that the gods won. As a reward, the asses were put in sky together with Phatne. ” (Frommert and Krongberg)

M 53 Globular Cluster Right Ascension: 13 h 12. 9 m Declination: +18° 10 m Visual Brightness: 7. 3 mag Apparent Dimension: 13. 0 arc min Exposure time of image: 20 s

M 53 Discovered by John Elert Bode in 1775. Is 60, 000 light years away from the galactic center. Is a globular cluster (NGC 5024) in Coma Berenice. Is below average of “metallicity” compared to other globular clusters. Has stars within the horizontal branch and some red giants. Contains 47 known RR Lyrae variable stars!!!

M 64 Spiral Galaxy Right Ascension: 12 h 56. 7 m Declination: +21° 41 m Visual Brightness: 8. 5 mag Apparent Dimension: 9. 3 x 54 arc min Exposure time of image: 45 s

M 64 Also known as the Blackeye galaxy or the Sleeping Beauty Galaxy. Was discovered by Eward Pigott in 1779. A characteristic feature of this galaxy is the dark dust pattern that surrounds it. The distance of has not been very well determined. Includes cepheid variable stars!!!

M 65 Spiral Galaxy Right Ascension: 11 h 18. 9 m Declination: +13° 05 m Visual Brightness: 9. 3 mag Apparent Dimension: 8 x 1. 5 arc min Exposure time of image: 30 s

M 65 Discovered in 1980 by Charles Messier. Has a luminous disk populated by old stars. Also is NCG 3623 within Leo. Located 35 million light years away. Forms part of the Leo Triplett (M 66 and NGC 3628).

M 66 Spiral Galaxy Right Ascension: 11 h 20. 2 m Declination: +12° 59 m Visual Brightness: 8. 9 mag Apparent Dimension: 8 x 2. 5 arc min Exposure time of image: 20 s

M 66 Discovered by Charles Messier in 1780. Is NGC 3627 in Leo and also forms part of the Leo Triplett. It’s spiral arms are deformed as result of encounters with other members of the Leo Triplett. Is 35 million light years away.

M 67 Open Cluster Right Ascension: 08 h 50. 4 m Declination: +11° 49 m Visual Brightness: 6. 1 mag Apparent Dimension: 30 arc min Exposure time of image: 20 s

M 67 Discovered by Johann Gottfried Koehler approximately in 1779. The oldest of Messier’s open clusters. Close to 3. 2 billion years old. Is NGC 2682 within Cancer. Expected death… in another 5 billion years!! Has a red giant branch and a main sequence that end in hot blue. Has counted till now 500 stars, 200 of them being white dwarfs! Is the perfect object to observe when studying sun-like type stars.

M 81 Spiral Galaxy Right Ascension: 09 h 55. 6 m Declination: +69° 04 m Visual Brightness: 6. 9 mag Apparent Dimension: 21 x 10 arc min Exposure time of image: 65 s

M 81 Also known as the Bode’s Galaxy. NGC 3031 in Ursa Major. Discovered by Johann Elert Bode in 1774. Has a distance of 11 million light years away. On March 28, 1993 a type II supernova occurred in M 81, which was discovered by the Spanish amateur astronomer Francisco Garcia Diaz!!! Has a population of 210(+/- 30) globular clusters!! Is the cause for M 82 initial deformation from an encounter millions of years ago.

M 82 Irregular Galaxy Right Ascension: 09 h 55. 8 m Declination: +69° 41 m Visual Brightness: 8. 4 mag Apparent Dimension: 9 x 4 arc min Exposure time of image: 18 s

M 82 As M 81, it was also Only 12 million light years discovered by Johann Elert away. Bode in 1774. Has one true and one false NGC 3034 in Ursa Major. supernova reported: Famous for it’s heavy False: (1986 D) - a starforming activity. slightly variable 2 micrometer source had Prototype member of the fooled the discoverers. class of Star Bursting True: (2004 am) – Galaxies!!! discovered at the Lick Observatory.

M 94 Spiral Galaxy Right Ascension: 12 h 50. 9 m Declination: +41° 07 m Visual Brightness: 8. 2 mag Apparent Dimension: 7 x 3 arc min Exposure time of image: 40 s

M 94 NGC 4736 in Canes Venatici. Discovered by Pierre Méchain in 1781. Has an extremely bright inner region surrounded by a ring of active starforming regions. The distance has yet to be fully determined. Relatively young/adult cluster. One of the relatively rare galaxies in which two “waves" of stellar formation can be observed.

M 95 Spiral Galaxy Right Ascension: 10 h 44. 0 m Declination: +11° 42 m Visual Brightness: 9. 7 mag Apparent Dimension: 4. 4 x 3. 3 arc min Exposure time of image: 60 s

M 95 Discovered by Pierre Méchain in 1781. Is 41 million light years away. Is NGC 3351 within Leo. Has cepheid variables!!! Is a barred spiral galaxy. Was one of the galaxies in the key project of the Hubble Space Telescope for One of the faintest the determination of the Messier objects. Hubble constant.

M 98 Spiral Galaxy Right Ascension: 12 h 13. 8 m Declination: +14° 54 m Visual Brightness: 10. 1 mag Apparent Dimension: 9. 5 x 3. 2 arc min Exposure time of image: 25 s Look close, zoom in… it’s there

M 98 Is NGC 4192 in Coma Berenices. Discovered by Pierre Méchain in 1781. It has been argued to be a Virgo Cluster member. “Shows a chaotic, diffuse disk, containing some blue regions of newly formed stars, and a huge quantity of occulting dust. ” (Frommert and Kronberg) Also one of the faintest Messier objects.

M 105 Elliptical Galaxy Right Ascension: 10 h 47. 8 m Declination: +12° 35 m Visual Brightness: 9. 3 mag Apparent Dimension: 2. 0 arc min Exposure time of image: 75 s

M 105 Discovered by Pierre Méchain in 1781. Is NGC 3379 in Leo. Only 38 million light years away. Contains a massive central object of about 50 million solar masses.

M 106 Spiral Galaxy Right Ascension: 12 h 19. 0 m Declination: +47° 18 m Visual Brightness: 8. 4 mag Apparent Dimension: 19 x 8 arc min Exposure time of image: 25 s

M 106 NGC 4258 in Canes Venatici. Discovered by Pierre Méchain in 1781. Has a distance of 21 to 25 million light years. It resembles somewhat the Andromeda galaxy M 31. The arms have bright blue star clusters that must have been recently formed. The active center also emits jets!!! A supernova, 1981 K, occurred in M 106 in August 1981.

M 108 Spiral Galaxy Right Ascension: 11 h 11. 5 m Declination: +55° 40 m Visual Brightness: 10. 0 mag Apparent Dimension: 8 x 1 arc min Exposure time of image: 90 s

M 108 NGC 3556 within Ursa Major. Discovered by Pierre Méchain in 1781. Appears to have no bulge and no pronounced core at all. Approximately 45 million light years away. Has a a detail-rich mottled disk with heavy obscuration along the major axis. A type II supernova 1969 B occurred in M 108 on Jan 23, 1969.

Sky conditions the night of the Messier Marathon. At 11 pm sky was clear. Not very dark, some light pollution. The moon was in a smaller phase (meaning not full and not too bright). Around 3 am we started getting some patches of clouds. At 4: 10 pm the sky was fully clouded and seemed less darker.

Conclusion All of these images where taken at the Bowling Green State University Observatory with the 0. 5 meter telescope. To get a quality image while taking pictures with a CCD camera a lot of things need to be considered: Visual magnitude of object Lof the object in the sky Exposure time Highest count possible with CCD camera Filters being used. The goal is to take the best picture possible when using the CCD camera and the factors mentioned before affect the focus and saturation of the image. It take practice, comfort and patience to achieve this goal.

Works Cited Frommert, Hartmut, and Christine Kronberg. “The Messier Catalog. ” The Munich Astro Archive. 30 Aug. 2007. SEDS. 28 Feb. 2009 < http: //www. maa. clell. de> However I used a more specific link created from this website. One for each Messier object, which are the following: http: //www. maa. clell. de/Messier/E/m 035. html http: //www. maa. clell. de/Messier/E/m 042. html http: //www. maa. clell. de/Messier/E/m 044. html http: //www. maa. clell. de/Messier/E/m 053. html http: //www. maa. clell. de/Messier/E/m 064. html http: //www. maa. clell. de/Messier/E/m 065. html

Works Cited http: //www. maa. clell. de/Messier/E/m 066. html http: //www. maa. clell. de/Messier/E/m 067. html http: //www. maa. clell. de/Messier/E/m 081. html http: //www. maa. clell. de/Messier/E/m 082. html http: //www. maa. clell. de/Messier/E/m 094. html http: //www. maa. clell. de/Messier/E/m 095. html http: //www. maa. clell. de/Messier/E/m 098. html http: //www. maa. clell. de/Messier/E/m 105. html http: //www. maa. clell. de/Messier/E/m 106. html http: //www. maa. clell. de/Messier/E/m 108. html