Kolloqium: Gegenseitige Jupitermondereignisse - Beobachtungen 2014/15 : PHEMU at Jupiter-V (Amalthea)
Eine Herausforderung ist die Auflösung der Mondscheibchen. Bei Ganymed ist das gut möglich
was possible to observe eclipses and occultation between the jovian
Nice observations were possible like here an eclipse of Ganymede by Io
Eine zweite Herausforderung definiert der IMCCE selbst. ...Verfinsterungen jenseits der 4 großen Galileischen Monde.
Many amateurs take the ephemeris from the side of the IMCCE. The IMCCE published informations about the 4 bright Galileian Moons and also about the weak moons inside the Io-orbit.
The biggest one of this small moons is Jupiter-V Amalthea. But:
-Amalthea has only 14mag, that´s 2 million times weaker than Jupiter
-max. distance from the planet is only one Jupiter-diameter
-The moon is exremly fast. He surrounds the planet in only 11 houes abnd 57 minutes
Needed for a success:
-a eclipse near the maximum elongation to freeze the moon-position for longer exposures
-a eclipse with no other Galileian-Moons in the field of view
-a eclipse with a high Jupiter near the meridian to reduce seeing-effects-a eclipse some month before and after the opposition to get distance from the eclipsing moon
5 possible eclipses where found. 3 in March, 2 in April and 1 in May.
The common solution is to mask the planet.
But its also possible to rise the contrast with a filter.
-The moon is bright in IR by red sulfur from Io
-in Methan band the Jupiter has a weak reflektion
Common CCD have 10% sensitivity at 890nm
Whats needed fo success:
-big telescope. Available is a 80cm Telescope at Bavarian Public Observatory Munich.
-a special filter for the Methan-band at 890nm
-sensitive CCD in IR
weather was only good on 2 days in
April. For the observation the pictures
were made with 30s each.
The eclipse was predicted with 2,7min so 5 pictures without Amalthea are expected.
The observation was 30min or 120 pictures. First all pictures were added to get the right position of Amalthea:
3 pictures of 30 seconds were combined to get one frame for this animation.
The measured value for the eclipse is 20:17:01 UT - 20:19:03 UT.
This fits good to the predicted times 20:16:33 - 20:19:14 UT.
It´s the first eclipse of Amalthea seen by an Amateur, I presume. And the first without masking the planet.
A second observation was possible at the 7. April
animation 4 pictures each 20s were
But between 19:51:45 and 19:53:59 UT no eclipse was visible.
Also at minutes before and after no eclipse was registrated.