Solar
& Planetary LtE Now in May 2024
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¤••••• Subject
: Mars:
Received:
Hi,
Here are my first images of Mars
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240531/FMl31May24.png
Thanks,
Frank
J MELILLO (
¤••••• Subject
: Mars 31 May 0447UT IR
Received:
Hi all,
Seeing
was poor this morning, possibly a result of strong Jetstream overhead.
Aurorae
Sinus is just below centre, with Solis Lacus still visible at upper right.
Mare
Erythraeum is to the upper left of centre.
I have
been watching the light area below the pole, initially thinking it might be the
artefact that is sometimes seen, but the asymmetric appearance in this image
may possibly indicate some dust near the south pole.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240531/CFs31May24.png
Best regards,
¤••••• Subject
: Mars 30 May 0515UT IR RGB
Received:
Hi all,
A later start this morning, with the view almost the same
longitude as yesterday.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240530/CFs30May24.png
Best regards,
¤••••• Subject
: Mars 29 May 0442UT IR RGB
Received:
Hi all,
I had below average seeing this morning. I wasn’t overly happy
with the final RGB, but during processing,
I did
seem to notice a suspicious yellowish tinge to the upper left near the
terminator. But certainly not definite, and hope to get a better look at that
region tomorrow.
The
image is centred on Valles Marineris/Ophir with
Solis Lacus upper right of centre and Aurorae Sinus just left of centre.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240529/CFs29May24.png
Best regards,
¤••••• Subject
: Saturn 20240528_IR
Received:
Saturn IR image on
Best
regards,
Tomio AKUTSU (
¤••••• Subject
: Mars 20240528_R
Received:
Mars R image on
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240528/Ak28May24.png
Best
regards,
Tomio AKUTSU (
¤••••• Subject
: Mars 27 May 0457UT IR RGB
Received:
Hi all,
Some periods of very good seeing this morning.
Similar
view to the last few days, with Solis Lacus upper left of centre and Valles
Marineris extending in from centre left.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240527/CFs27May24.png
Best regards,
¤••••• Subject
: RE: Mars 26 May 0511UT IR RGB
Received:
Hi all,
If you
can kindly replace the image set from yesterday with this updated version.
The time
at upper left was incorrect.All other info remains the same.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240526/CFs26May24p.png
Thanks
and best regards,
¤••••• Subject
: Mars 20240526
Received:
Mars image on
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240526/Ak26May24.png
Best
regards,
Tomio AKUTSU (
¤••••• Subject
: Re: Mars 26 May 0511UT IR RGB
Received:
Thanks,
I'm not
sure of which features I'm seeing, but I think it's
Aquilae Fretum that's unusually prominent just north of the eastern end of Mare
Sirenum. Also, a westward extension of Phoenicis Lacus that has been present
for the last few apparitions is still seen, and Phasis (just west of Solis
Lacus) is dark.
Roger
Roger VENABLE (
¤••••• Subject
: Mars 26 May 0511UT IR RGB
Received:
Hi all,
Another very pleasant morning in the observatory, with good
seeing despite a moderate Jetstream.
View is
similar to the last few days with Solis Lacus upper left of centre and Valles
Marineris centre left.
I
forgot to mention yesterday that Mars has attained 5 arc-seconds.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240526/CFs26May24.png
Best
regards,
¤••••• Subject
: Saturn 20240525
Received:
Saturn images on
Best
regards,
Tomio AKUTSU (
¤••••• Subject
: Mars 20240525
Received:
Mars images on
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240525/Ak25May24.png
Best
regards,
Tomio AKUTSU (
¤••••• Subject
: Mars 25 May 0414UT IR
Received:
Hi all,
With
strong Jetstream this morning, the unexpectedly good conditions I had for
Saturn did not persist, and I just ran a series of IR’s on Mars.
Solis
Lacus is upper left of centre with Valles Marineris extending in from the
centre left.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240525/CFs25May24.png
Best
regards,
¤••••• Subject
: Saturn 20240523
Received:
Saturn image on
Best
regards,
Tomio AKUTSU (
¤••••• Subject
: Mars 20240523
Received:
Mars image on
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240523/Ak23May24.png
Best
regards,
Tomio AKUTSU (
¤••••• Subject
: Mars 22 May 0451UT IR RGB
Received:
Hi all,
Image
set from this morning with M Sirenum still prominent above centre.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240522/CFs22May24.png
Best
regards,
¤••••• Subject
: The colors of Saturn in 2023-22 (III) Indices and more
UV data
Received:
Hi all, here are more UV data and some indices, where
dividing one band with another brings interesting stuff.
1) Since last
year I'm using a shorter UV-pass filter than the Chroma Bessel U, the Asahi
340. Used with the T620 AstroQueyras without barlow at
an altitude of 3000 meters, the filter succesfully detected the increase of
albedo of the planet before 350 nm. Actually on that band, the southern
hemisphere around 40°S is brighter than the rings !
My photometry of that filter failed (the only one) so I have
evaluated the expected value by looking at the Saturn spectrum inside the
passband of the filter. While in the U band the albedo is around 20%, through
the UV340 it raises to 0,22.
The Chroma U used at the AstroQueyras Observatory looks to
produce more contrast between the EZ and the rest of the globe, maybe because
at that good site, shorter wavelengths are caught, despite the filter and the
camera being exactly the same.
Then,
in the scientific litterature (Karkoschka, Sanchez-Lavega...) we find 2
indices:
2) Dividing blue by red produces a color
index, where we measure how red or how blue are the Saturn latitudes. The index
correctly shows that the southern winter hemisphere was noticeably bluer over
the past years, and it also correctly shows that it has reddened in 2023 in
comparison with 2022 (from blue to green).
Let's see how it turns in 2024, the winter hemisphere looks
bluer to me than last year so far...
3) Dividing CH4 by UV. This should be done
with a UVB filter (in the litterature we find data from the F275M HST filter),
but of course it is impossible from the ground.
To the contrary of Jupiter however, the aspect of Saturn in
UVA is much closer to that of UVB, so I tried it anyways. This index measures
how high/opaque are the clouds, and without any surprise the Equatorial Zone is
occupied by noticeably higher and thicker clouds than elsewhere. Ricardo again,
I don't know if it is acceptable on Saturn to measure this index through UVA ?
On the
next time I will send my data about the rings
Best
wishes
Christophe
Christophe PELLIER (
Planetary
astronomy and imaging
¤••••• Subject
: Mars 21 May 0429UT IR
Received:
Hi all,
Due to
time limitations today I limited the session to IR captures.
Seeing had
also deteriorated from the earlier Saturn session, possibly due to a pre-dawn breeze that had developed.
M
Sirenum is the most prominent feature above centre.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240521/CFs21May24.png
Best
regards,
¤••••• Subject
: Mars 20240520
Received:
Mars image on
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240520/Ak20May24.png
Best
regards,
Tomio AKUTSU (
¤••••• Subject
: Saturn 20240520
Received:
Saturn image on
Best
regards,
Tomio AKUTSU (
¤••••• Subject
: Mars 20 May 0447UT IR RGB
Received:
Hi all,
Image set
from this morning. M Sirenum above centre.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240520/CFs20May24.png
Best
regards,
¤••••• Subject
: Mars 2024/05/17-Kumamori
Received:
Mars IR image on
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240517/Km17May24.png
Best
regards,
Teruaki KUMAMORI (Osaka, JAPAN)
¤••••• Subject
: Mars 19 May 0418UT IR
Received:
Hi all,
Conditions
were poor this morning and I was only able to use a limited number of IR
captures.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240519/CFs19May24.png
Best
regards,
¤••••• Subject
: Mars 15 May 0520UT IR RGB
Received:
Hi all,
I have
been clouded out the last few mornings, and although clear this morning, seeing
was below average.
I did
not feel that the RGB data was good enough and stuck with the best IR captures
of the morning.
M Cimmerium
is the most prominent feature.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240515/CFs15May24.png
Best
regards,
¤••••• Subject
: Mars 11 May 0533UT IR RGB
Received:
Hi all,
Having
had to abort an earlier session due to cloud build up,
I
realised it was clearing and went back out to the observatory.
The sky
was already brightening, and I struggled with the B captures.
The
image is centred on Mare Tyrrenhum and Syrtis Minor, with Hesperia quite
obvious.
Syrtis
Major to the right. Some regions of
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240511/CFs11May24.png
Best
regards,
¤••••• Subject
: Mars 6 May 0456UT IR RGB
Received:
Hi all,
Image
set from yesterday morning under fairly decent conditions.
Looking down on
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240506/CFs06May24.png
Best
regards,
¤••••• Subject
: Saturn 20240506
Received:
Saturn image on
Best
regards,
Tomio AKUTSU (
¤••••• Subject
: Mars
20240506
Received:
Mars IR image on
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240506/Ak06May24.png
Best
regards,
Tomio AKUTSU (
¤••••• Subject
: Mars
5 May 0452UT IR RGB
Received:
Hi all,
I was a
bit sidetracked this morning with chasing Eta Aquariids but did manage this
image set towards sunrise. Conditions were not bad until the end of the G run
and then went badly downhill for the B’s, so the B is very poor.
Tried to put the RGB together as best I could.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240505/CFs05May24.png
Best
regards,
¤••••• Subject
: Mars
4 May 0501UT IR
Received:
Hi all,
Another
session where I had to stay with IR, as clouds were
moving in.
A pity
as I had some very nice conditions for Saturn a bit earlier.
Syrtis
Major coming into view at lower left and
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240504/CFs04May24.png
Best
regards,
¤••••• Subject
: Mars
3 May 0503UT IR
Received:
Hi all,
As with
Saturn, I had generally poor conditions this morning, with some improvement
right at the end of the session. Due to the conditions I only captured IR data.
As with
yesterday, some light areas are seen in
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240503/CFs03May24.png
Best
regards,
¤••••• Subject
: Mars
2 May 0440UT RGB IR
Received:
Hi all,
With
conditions being noticeably poorer this morning, I just ran a series of IR
captures.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240502/CFs02May24.png
Best
regards,
¤••••• Subject
: Mars
1 May 0512UT RGB IR
Received:
Hi all,
Being a bit later, very similar to yesterday.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240501/CFs01May24.png
Best
regards,
¤••••• Subject
: Mars
30 April 0452UT RGB IR
Received:
Hi all,
I had
limited time this morning, and just ran a series of IR captures.
Conditions
were again fairly decent.
https://www.kwasan.kyoto-u.ac.jp/~cmo/cmons/2024/240430/CFs30Apr24.png
Best
regards,