A Little Planet

Mercury - March 5, 2012
Mercury - March 5, 2012

It was a next day with the clear sky above us. It was also a good time to look at Mercury. It is able to observe only if the seeing is excellent and the planet is at a suitable distance from Sun, so I was quite happy when I had seen its phase.

Object Name: Mercury
Object Type: planet
Location: PÅ‚aza, Poland
Date: 05.03.2012
Media: graphite pencil, white paper, inverted in Photoshop CS2

Mercury in the Evening, Near Eastern Elongation

I was able to observe Mercury on March 19, 2011 (00:00 U.T.) over the western horizon (~23.5*) using my friend’s excellent Meade 8-inch (20-cm) F/10 ACF SCT at 120x. I was impressed with the fact that albedo features were visible over the planet while using an aperture down to 4 inches (10 cm) at a friend’s observatory. The seeing over the western horizon at sunset (twilight) was very erratic but while airing for moments of steady seeing I was rewarded by the features noted below.

Date (U.T.): March 19, 2011
Time (U.T.): 00:00
CM 77.8*W, Ls 128.5*, De -5.3*, Ds 0.1*
-0.7m, p 60%, 6.7″
Instrument: Meade 8-inch (20-cm) F/10 ACF SCT
Magnification: 120x
Filters: None (IL)
Seeing (1-10): 4-6, Antoniadi (I-V): III-IV

A digital image produced in Photoshop CS5.

Carlos E. Hernandez

Mercury in Broad Daylight

Mercury in Broad Daylight

Daytime observation of Mercury
Sketch and Details by Carlos E. Hernandez

Daytime Observation of Mercury

I was able to make a daytime observation of Mercury on August 22, 2009 (20:00 U.T.) using an 8-inch (20-cm) F/15 Maksutov-Cassegrain (286x). I was with a friend and suggested that we try hunting Mercury down in the daytime sky. There was a thin haze in the daytime sky so we thought that we may not be able to see it. We first centered his instrument (fitted with a solar filter) on the Sun then offset it by approximately two hours in right ascension (RA) and Mercury was in the field. Mercury was visible at a quarter phase (55%) and albedo features were noted over the illuminated disk.

My observation reminded me of the historic observations made by Antoniadi and Schiaparelli over the end of the nineteenth century and early twentieth century. These classic astronomers made their observations of Mercury in the daytime as observing this planet is difficult in a darkened sky as it is never more than 28 degrees from the Sun. Schiaparelli and Antoniadi erroneously believed that the rotation period of Mercury was 88 days (instead of 58.6 days) and therefore locked in with it’s revolution period. It was not until 1965 when the radio telescope discovered the true rotation period.

A digital image produced in Photoshop CS3.

BE CAREFUL TO NEVER OBSERVE MERCURY IN THE DAYTIME UNLESS YOUR INSTRUMENT HAS A SOLAR FILTER PLACED UPON IT UNTIL THE PLANET IS IN THE FIELD OF VIEW!

Carlos E. Hernandez

Crescent Moon and Planet Gathering

Conjunction

Crescent Moon and Planet Gathering
Sketch and Details by Carlos E. Hernandez

I was fortunate to have witnessed the grouping of the Moon, Mercury, and Jupiter again on December 29, 2008 (23:15 U.T.) with the addition of Venus. The Waxing Crescent Moon was now above the pair of Mercury and Jupiter. Mercury (-0.75m) was approximately 7.5 degrees above the western horizon, Jupiter (-1.51m) ~10 degrees, the Moon ~15 degrees, and Venus (-4.25m) ~33 degrees. Earthshine was easily visible over the unilluminated portion of the Moon. This grouping was very striking against a pastel blue sky with lavender clouds below over the western horizon.

A digital image produced using Gimp.

Messenger’s Focus

Mercury

Mercury
Sketch and Details by Carl Roussell

Name: Mercury
Type: Planet
Location: Hamilton, Ontario, Canada
Date: Sep 18,2008
Medie: graphite pencils om plain paper
Telescope15cm f/8 refractor, 300x,
Filters: W21 and W23A

Note: Trying to find and name features on Mercury is challenging and will let you feel like to astronomers of the past. The light patch on the is in the right place to Apollonia, and the two dark patches Solotudo Argiphontae (north) and Tricerna (south)

A Freckle on the Sun

Mercury-Solar Transit

Mercury-Solar Transit
Sketch and Commentary by Jeremy Perez
Move cursor over sketch to see labels.

On Wednesday, November 8th, 2006, Mercury was due for a solar transit. Now, in my neck of the woods, that just happens to be a work day. So I planned to set up the scope during lunch in the parking lot, or outside the lunchroom. The only thing I needed was a solar filter. A couple years ago, a very kind and generous amateur astronomer from Phoenix, Scott Kroeppler, sent me a couple small Baader solar film samples. Other than some casual, unmagnified looks at the sun, I hadn’t put them to good use. Until now. I stayed up the night before, rigging these two 1-inch square pieces of solar film and a sewing hoop to an 8 inch square piece of foam core. I wasn’t sure if it would work, but the next morning, I pulled into the parking lot at work, put my mangy, home-made solar cap on the front, and got a handheld look at the sun for the first time through my own scope. Not only did it work great, but I was pleasantly surprised to see a huge sun spot easing over the solar limb.

So I got to work, and then about 15 minutes before the beginning of the transit, I put it all together on the patio outside the lunch room where I had the best opening between all the trees. I didn’t start quite early enough, because by the time I got everything set up and the solar cap taped on securely, Mercury was already well inside the solar disc. It looked just like a printed period against blue-white filtered circle of the sun. It had entered just south of the massive sunspot I noticed earlier. A couple fainter sunspots rested on the opposite side. At that point, I made my first solar sketch, and noted how easy it would be to really exaggerate distances and proportions across the sun’s face. I was excited to see that light, textured, filamentary features were visible around the sunspots. As I studied these features, I noticed that it didn’t take long for Mercury’s motion to become apparent.

Over the next 45 minutes, I invited passing coworkers to have a look. They all seemed happy to get a look at the transit, particularly after reading about it in the newspaper the day before. As folks walked up to the eyepiece, I tried to coach them a bit with the sketch to be sure they didn’t confuse the sunspot for Mercury. Quite a few commented on how very tiny the little planet appeared. Several of them were even able to make out the two relatively faint sunspots over on the western limb as well. After a little more than an hour, I moved the scope to an out-of-the-way spot, and went back to work.

At about 20 minutes before the end of the transit, I raced outside to find that the sun was completely hidden behind trees where I had the scope set up. With a bit of scouting, I moved the whole thing into the parking lot about a hundred yards to the north where I had a clear vantage. And here I got to watch that perfect little dot edge closer to the western edge of the sun. At about four Mercury diameters from the edge, the whole shebang began to sink behind a tree-lined ridge a mile to the west. So I missed seeing Mercury merge with and disappear into the darkness on the other side of the sun. It was still a fascinating event to witness, and since Mercury won’t do this again until 2016, I’m glad I was able to fit it in.

The sketch at the top of this post was overlayed onto a digitally generated disc with limb darkening that estimates what I saw through the eyepiece. The next time I sketch the sun this way, I’m sure I’ll want to include the lighter features, which will mean generating that limb darkening manually and erasing through it.

Subject Mercury – Solar Transit
Classification Planetary/Solar
Date/Time November 8, 2006, 12:33 – 04:54 PM MST (November 8, 2006, 07:33 – 11:54 UT)
Observing Loc. Flagstaff, AZ
Instrument Orion SVP 6LT Reflector (150 mm dia./1200 mm F/L)
Eyepieces/Mag. 25 mm (48X)
Conditions Clear, breezy
Seeing Ant. IV