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CCD Images - Session 28 (2002-10-02)

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Bullet NGC 7317-7320 Galaxy Cluster (Stephan's Quintet)
Bullet M32 Galaxy
Bullet M110 Galaxy
Bullet M31 Spiral Galaxy - Nucleus 
Bullet NGC 206 Emission Knot in M31
Bullet HD209458 (star to extra-solar planet system)
Bullet Variable Stars 
 
 
> Notes from CCD Session 28

NGC 7317-7320 Galaxy Cluster (Stephan's Quintet)

Stephan's Quintet (Pegasus)
NGC 7317 (Mag +14.8), NGC 7318A (Mag +14.6), NGC 7318B (Mag +14.0), 
NGC 7319 (Mag +14.6), NGC 7320 (Mag +13.6), NGC 7320C (Mag +16.6) 
Image
2002-10-02  21:44 to 21:51h UT
CCD Image, 2 x 2 min exposure (2x2 binning)
11.4 x 7.6 arc min  (#28003 & 28005)
 

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M32 Galaxy

M32 Galaxy (Andromeda)
Image
2002-10-03  00:44 to 00:54h UT
CCD Image, 2 x 5 min exposure (2x2 binning)
11.4 x 7.6 arc min  (#28240-41)

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M110 Galaxy

M110 Galaxy (Andromeda)
Image
2002-10-03  01:03 to 01:14h UT
CCD Image, 2 x 5 min exposure (2x2 binning)
11.4 x 7.6 arc min  (#28243-44)

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M31 Spiral Galaxy - Nucleus

Nucleus of M31 Galaxy ( Andromeda)
Image
2002-10-03  00:44 to 00:54h UT
CCD Image, 2 x 5 min exposure (2x2 binning), 
11.4 x 7.6 arc min  (#28240-41)
  
Nucleus of M31 Galaxy (Andromeda) - Enhanced
Image
2002-10-03  00:44 to 00:54h UT
CCD Image, 2 x 5 min exposure (2x2 binning), 
Mid-range brighten & Unsharp Masked
11.4 x 7.6 arc min  (#28240-41)

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NGC 206 Emission Knot/Cluster in M31

NGC 206 Emission Knot in M31 arms (Andromeda)
Image
2002-10-03  01:16 to 01:27h UT
CCD Image Mosaic, 5 min exposure (2x2 binning), 2x1 mosaic
Processing : Smoothed, Linear Stretch 
10.5 x 13.2 arc min  (#28245-46)

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HD209458 (star to extra-solar planet system)

HD 209458 has a transiting Jupiter mass short period extrasolar planet.(HD 209458-b). Every 3.5 days, the planet produces a dimming of the star of 1.7 % that lasts for about 3 hours. The dimming has been detected by Castellano and Laughlin using almost identical equipment to me (ie 8" telescope and ST-7E CCD camera), which presents me the opportunity to me to also have a go at trying to detect a extrasolar planet lying at a distance of  1.45 x 1015 km (47.08 parsecs, 153.5 light years) from Earth..

As a prelude to a future attempt to detect the planet an initial image of HD 209458 was taken :

HD209458 (Pegasus)
Image
2002-10-02  22:04h UT
CCD Image, 7 x 5 sec exposure (2x2 binning)
11.4 x 7.6 arc min  (#28010-16)

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Variable Stars 

 

R And, Mira-type variable (Andromeda)
baseline magnitude estimate
Image
2002-10-02  23:34h UT
CCD Image, 3 x 5 sec exposure (2x2 binning)
11.4 x 7.6 arc min  (#28160-62)
  
R And, Mira-type variable (Andromeda)
baseline reference image 30 sec exposure
Image 
2002-10-02  23:36h UT
CCD Image, 3 x 30 sec exposure (2x2 binning)
11.4 x 7.6 arc min  (#28166-68)

More Variable Stars baseline images were taken (And, Lac, Peg). Click on link to see them.

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This Web Page: CCD Images - Session 28 (2002-10-02 to 2002-10-03)
Last Updated : 2015-05-16
Site Owner : David Richards
Home Page : David's Astronomy Web Site