CCD Imaging
Below are the details and photos of crescents captured by a CCD camera with filters using special telescope, and then the observer made some image processing to enhance the results. All these pictures were taken during broad daylight!
Ramadan 1427 AH:-
- Observer Name: Joachim Schulte in den Baumen
- Month Name: Ramadan 1427 AH.
- Equipment: CCD and 5" Professional Lunar Crescent Observation Telescope.
- Location: Sonneberg, Germany.
- Longitude: 11.2 E
- Latitude: 50.4 N
- Elevation: 640 m
- Topocentric Conjunction: 22 September 2006 CE, at 11:09 UT.
- Geocentric Conjunction: 22 September 2006 CE, at 11:45 UT.
- Photo Time: 23 September 2006 CE, at 13:00 UT (15:00 LT).
- Topocentric Age (At Photo Time): 25 hours and 51 minutes.
- Geocentric Age (At Photo Time): 25 hours and 15 minutes.
- Lag time: 08 minutes.
- Elongation (At Photo Time): 11.7 degrees.
- Relative Azimuth (at Photo Time): 13.3 degree.
- Relative Altitude (at Photo Time): 3.5 degrees.
- Moon Altitude (at Photo Time): 30.7 degrees.
- Sun Altitude (at Photo Time): 34.1 degrees.
- Note: The observer was not able to see the crescent even through the telescope! It was only captured by the CCD after image processing.
- Source of Observation: ICOP.
Ramadan 1428 AH:-
- Observer Name: Peter Aniol
- Month Name: Ramadan 1428 AH.
- Equipment: CCD and 4" Astelco Lunar Crescent Telescope.
- Location: Alpes-De-Haute Provence, France.
- Longitude: 05.85 E
- Latitude: 44.0 N
- Elevation: 568 m
- Topocentric Conjunction: 11 September 2007 CE, at 12:36 UT.
- Geocentric Conjunction: 11 September 2007 CE, at 12:44 UT.
- Photo Time: 12 September 2007 CE, at 09:32 UT (11:32 LT).
- Topocentric Age (At Photo Time): 20 hours and 56 minutes.
- Geocentric Age (At Photo Time): 20 hours and 48 minutes.
- Lag time: 12 minutes.
- Elongation (At Photo Time): 10.7 degrees.
- Relative Azimuth (at Photo Time): 5.2 degree.
- Relative Altitude (at Photo Time): 9.8 degrees.
- Moon Altitude (at Photo Time): 32.3 degrees.
- Sun Altitude (at Photo Time): 42.1 degrees.
- Note: The observer was not able to see the crescent even through the telescope! It was only captured by the CCD after image processing.
- Source of Observation: ICOP.
Thul Keadah 1428 AH:-
- Observer Name: Peter Aniol
- Month Name: Thul Keadah 1428 AH.
- Equipment: CCD and 4" Astelco Lunar Crescent Telescope.
- Location: Alpes-De-Haute Provence, France.
- Longitude: 05.85 E
- Latitude: 44.0 N
- Elevation: 568 m
- Topocentric Conjunction: 09 November 2007 CE, at 22:56 UT.
- Geocentric Conjunction: 09 November 2007 CE, at 23:03 UT.
- Photo Time: 10 November 2007 CE, at 10:52 UT (11:52 LT).
- Topocentric Age (At Photo Time): 11 hours and 56 minutes.
- Geocentric Age (At Photo Time): 11 hours and 49 minutes.
- Lag time: MINUS 11 minutes.
- Elongation (At Photo Time): 8.0 degrees.
- Relative Azimuth (at Photo Time): 3.3 degree.
- Relative Altitude (at Photo Time): 7.4 degrees.
- Moon Altitude (at Photo Time): 21.1 degrees.
- Sun Altitude (at Photo Time): 28.5 degrees.
- Note: The observer was not able to see the crescent even through the telescope! It was only captured by the CCD after image processing.
- Source of Observation: ICOP.
Definitions
Topocentric Age: Time elapsed from the topocentric conjunction up to the time of interest.
Geocentric Age: Time elapsed from the geocentric conjunction up to the time of interest.
Lag time: Time difference between sunset and moonset, or from moonrise and sunrise for waning crescent
Elongation: Topocentric angular separation between the centers of Sun and Moon. It is called Arc of Light as well (ARCL).
Relative Azimuth: Topocentric azimuth difference between Sun and Moon. It is called Delta Azimuth as well (DAZ).
Relative Altitude:Topocentric altitude difference between Sun and Moon. It is called Arc of Vision as well (ARCV).
Moon Altitude: Topocentric Moon airless altitude not corrected for refraction.
Sun Altitude: Topocentric Sun airless altitude not corrected for refraction.
Note from ICOP Memeber Mr. Qamar Uddin: "Please could you also make a special mention of the fact that those "World
Records Crescent Observations" are carried out by astronomy experts, who have a
lot of experience of knowing when and where to look (possibly with optical aids
to find the moon)! So, that ordinary Muslims may not "blame" themselves for not
seeing the crescent at the same time/location."
By Mohammad Odeh. Copyright © 1998-2007 Islamic Crescents' Observation Project (ICOP), All Rights Reserved. This material may not be reproduced in any form without permission. For more information Kindly send E-mail