Fremont Peak 1/6/03
by David Kingsley
I was one of the half dozen or so observers who went down to the Peak
last night (Monday 1/6/02). I had a great time from sundown to
about 2:30 in the morning under the best observing conditions I have
seen in several months: clear skies, good transparency, temperatures
in the 50s throughout the night, zero problem with dew (humiditygot
down to 28% during the night). I was concerned about wind levels at
the Peak after Jeff's report from Saturday night/Sunday morning, and
Peter's report that wind was howling everywhere in the park except
Coulter on Sunday night. In contrast, when I arrived between 4 and
5 pm on Monday, it was almost dead calm everywhere in the park,
including the SW lot, Coulter row, and over by the observatory. It
stayed surprisingly calm all night, with mild breezes at the couple
of mile an hour most of the time until I left around 3 am.
Highlights for me during eight solid hours or so of observing:
- Some wonderful detail on the moon as we were waiting for it to get
dark. Taruntius showed great relief on the edge of Mare
Fecunditatis. The entire central 2/3 or so of the crater floor has
been raised up higher than the rest of the floor near the crater rim,
like a giant piston pushing up inside an oversized cylinder. A
central peak sits atop the center of the piston, giving lots of
different heights, shadows, and highlights in a very 3 dimensional
view.
Further from the terminator, the eastern edge of the beautiful
crater Langrenus showed an interesting feature I had never seen
before. Although most of the crater was fully illuminated, there was
an obvious inky black spot on the inner side of the eastern wall
that looked just like a black cave entrance. I had recently read
about a similar cave illusion that shows up in Copernicus when the
sun hits the terraced walls just right (O'Meara article in Jan or
Feb Sky and Tel). It was very interesting to see a similar
apparent cave opening show up in a completely different crater.
- Despite a bit of moon in the west, I spent a lot of time hunting
down new extragalactic globulars in M31. I think transparency last
night was better than it had been on several other nights of the
project, but the seeing was somewhat softer. I ended up working at a
magnification of about 400x (barlowed 9 mm Nagler with 14.5 inch
Starmaster scope), which gave good views even though I would often
have to wait a few seconds for the image to stabilize. Under these
conditions, my limiting magnitude turned out to be very similar to
what it had been at LSA in October and Fremont Peak on Thanksgiving
day (faintest extragalactic glob about visual magnitude 16.1). With
last nights new glob catches, and some others from various observing
sessions in December, I finally crossed the half century mark on
the extragalactic globular project. I have now logged 52 total
globular clusters found around M31 (not counting three or four other
candidates that I had previously logged, but which are now thought
not to be globs based on additional studies since the Hodge atlas was
prepared). I have a handful of M31 candidates left, and a smaller
list of possible targets in other galaxies. And as spring and summer
comes, I am looking forward to logging some remaining globs from our
own Galaxy too.
- There was a lot of beautiful action on Jupiter last night!
Every 6 years, the orbital plane of Jupiter is lined up with Earths
in such a way that Jupiter's moons show mutual eclipses and
occultations,. Bob Cz. alerted me to a mutual shadow eclipse that was
supposed to take place about 1:15 am. I checked the usual chart of
mutual events in the recent Sky and Telescope article and saw that
there was also going to be an occultation of Io by Europa starting
about 10:30 pm. We swung the scopes over periodically during the
night, and had some great views when the seeing would momentarily
stabilize. Io and Europa hung together off the following edge of
Jupiter around 10:15 pm, first looking like a tight double star, than
coming into elongated apparent contact. The superimposed moons
obviously could not be visually split during during the occultation,
but their different colors were apparent at high power in the
superimposed image. (Io slightly yellow-reddish, and Europa
whitish, the two colors reflecting their different cell surfaces of
sulfur volcanoes on Io and cracked ice on Europa). The contrasting
colors made a joined object that was yellow/red at one end and white
at the other. Shortly after the moons had moved together, Europa's
shadow showed up on Jupiter, a beautiful black dot almost perfectly
centered between the two main belts of Jupiter. Io's shadow then
joined the scene, initially trailing Europa's shadow but gradually
overtaking it during the transit because of the faster orbital time
of Io. It was very interesting to see the difference in the shadows
marching down the central lane of Jupiter at high magnification.
Io is both larger and closer to Jupiter than Europa, and its shadow
was obviously larger, blacker and sharper looking than Europas during
the double shadow transit. I checked the scene again around
1:15 and 1:30 am, the time during which the shadow of Europa was
supposed to eclipse Io against the face of Jupiter (second "mutual
event" of the night). Unfortunately, the seeing had softened during
the night, and this second mutual event took place when the moons
themselves were transiting the face of Jupiter. Although the moons
were visible when transiting at the edge of Jupiter, I could not seem
them well enough on the face of Jupiter to view the eclipse of Io's
disc by Europa's shadow. The shadows themselves were still very
obvious however, and the bigger blacker dot of Io's shadow had
obviously outraced the smaller shadow of Europa, now leading instead
of trailing because of the faster orbital time of Io. What a great
combination of events, and a beautiful demonstration of surfaces,
sizes, and orbits around the King of Planets.
- I chased down three separate comets during the night using
finder charts taken from the Skyhound observing site (see
http://www.skyhound.com/sh/comets.html). C/2002 V1 (NEAT) in Pisces
was the brightest and biggest, currently estimated at mag 7.3.
C2001 HT50 (LINEAR-NEAT) in Hydra and C/2001 RX14 (LINEAR) were much
dimmer and smaller (around mag 10 or 11). HT50 was an asymmetric,
chevron-shaped nebulosity, and obviously changed position during
the time between an initial sketch and when I checked back about an
hour later. Getting to C/2001 RX14 (LINEAR ) turned out to be much
more interesting than the comet itself. The starting point for my
star hop was the M106 galaxy in Ursa Major, a beautiful sight that
I had never seen before with 14.5 inches of aperture. In traveling
from M106 to the comet, I chanced on at least 3 or 4 other pretty
NGC galaxies hiding here and there among the star fields. When the
eyepiece is full of UMa galaxies, you know spring can't be too far
away.
I enjoyed lots of other objects during the night, including some nice
views at various galaxies Jamie Dillon was tracking down. Thanks to
everyone for the shared views, Jamie for the calendar, and Bob Cz.
for inviting me to come over and observe near the observatory instead
of at Coulter. After lots of rainy weather, and then recently
being blown out of Coe on New Year's day, and fogged out of Dino
Point on Sunday, it was wonderful to be under clear skies again with
the 14.5 inch scope.
Definitely my best night since LSA, and a very satisfying mix of
both shallow and deep sky objects.
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