Just imagining I was captain of this ship...
Friday, April 27, 2012
Thursday, April 5, 2012
Mars Drawing
Today was a strange day at work...too many people not getting along with each other; a colleague who had a death in the family; and our department saddened by the suicide of a student. It was one of those days where I felt that "I'd like to buy the world a coke"...Maybe I am showing my age with that little jingle, but certainly everyone needs to take a deep breath and look up at the night sky we are so fortunate to have here in Arizona.
Mars is currently 12.11 arcseconds in diameter and still shining at magnitude -0.6. Mars is .773 astronomical units from Earth, or 6 minutes 25.6 seconds in light time. My sketch was completed this evening at 8:44 PM MST (0344 UT, April 6th). At the top is the North Polar Cap, and there was quite a bit of haze in the southern polar region.
And, while I never thought I would say something like this, a big shout out to the Governor of AZ for vetoing the electronic billboard legislation! Our legislature quickly passed this asinine bill at the urging of Clear Channel Communications, and fortunately the Governor had a rare moment of clarity and realized that not only was the multi-million dollar astronomy related industry threatened, but these electronic billboards are safety hazards as well. But I digress...back to the night skies...
While it is nearly full moon, I opened up my observatory and spent a little time observing Mars again this evening. Using my 12" LX200 SCT I was treated to a night of exceptionally good seeing. Using an 8mm eyepiece I was observing Mars at a magnification of 380X without any image breakdown. I did try a 5mm eyepiece (608X), however, there was nothing visible at that power that I could not see much sharper at 380X. Below left is my sketch, and at right a simulated view courtesy of CalSky.
Sunday, March 18, 2012
Night and Day
The wonderful thing about having a small home based observatory is that there is virtually no set-up or preparation involved in observing. Simply head outside, roll off the roof and wake the telescope mount from hibernation. After a long day of work it is simply a 30 foot walk out the backdoor and I am relaxing under the night sky.
Earlier this week I was at a meeting with University of Arizona Astronomer Carl Hergenrother, who maintains an excellent blog called The Transient Sky which deals with comets, asteroids and meteors. I highly recommend a visit to his site. Carl reminded me that Comet C/2009 P1 Garradd was still fairly bright in the evening sky in the northeast. I have been following this comet since late August 2011, when I first sketched it at magnitude 8.2 and have since made about a half-dozen sketches of it. I remarked to Carl that I was amazed at how long this comet had remained fairly bright. He indicated that the sustained brightness is a result of a rather large comet that did not approach the Sun very closely. He remarked that had it come closer, it may have become a "Great Comet."
I last visited this comet in early February (see this post) and decided to have another look. The comet is currently heading for a rendezvous with the Big Dipper asterism in Ursa Major and is well placed for observation much of the night. Below is a diagram of the comets orbit (courtesy JPL).
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Below is my sketch of Comet C/2009 P1 Garradd completed at 0420 UT on 3/15/2012 (9:20 PM MST 3/14/12). At the time of my sketch, the comet was 1.301 AU from Earth and 1.91 AU from the Sun.
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As you can see, I was not disappointed in the mighty comet. It is moving along at a stately pace of approximately 3.27 arcseconds per min and is currently sporting two diffuse tails. The tail to the east appears much broader and more diffuse than the tail to the west. I made this observation using my recently acquired TEC 8 inch f/20 Maksutov, with a 35mm Panoptic eyepiece yielding a magnification of 116x. Current estimates place the comet at approximately magnitude 7.4. I will be in Portal, AZ this coming weekend under magnitude 7+ skies and am very excited to have a look at Comet Garradd under truly dark skies. Look for a follow up sketch next week.
Of course, the Lost Pleiad Observatory is a round the clock operation and until I invent a way to see the deep sky in the daytime (in visible light), I still observe our nearest star, the Sun every chance I get. Below is a sketch I made of the Sun using my dedicated Hydrogen Alpha telescope on March 17th. Happy St. Patrick's Day!
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Sunday, March 4, 2012
Mars - Still Curious
While NASA may be struggling to budget for future Mars exploration, as Astronomer-in-Chief of the Lost Pleiad Observatory, I remain curious. In 154 days, on August 6th 2012, the Mars Science Laboratory, nicknamed Curiosity, will touch down on the red planet and if all goes well begin to enthrall us with information and data. While we wait for this exciting event, I continue to do what I can to keep an eye on Mars.

Last night I made my first decent sketch of Mars with my TEC 8 inch f/20 Maksutov Cassegrain. I plan to write a review of this scope one day, but it is really a very specialized instrument that delivers excellent contrast, a large image scale, and sharp views. It is well regarded as a high end planetary instrument. The telescope is about 16 years old, and I believe that it is slightly out of collimation. I do mean slightly, and I will likely wait until this summer when I am in Colorado to personally deliver the scope to TEC for a tune-up. You can see from these pictures that despite its age, it is in good used shape.
Even with a waxing gibbous moon, last nights seeing conditions were slightly above average, with reasonably stable skies allowing me to use a magnification of 253x. My sketch was completed at 0447 UT on March 4th (9:47 PM MST, March 3rd), with Mars central meridian at 315.8 degrees. Currently at Magnitude -1.2, Mars is .6739 AU from earth, or 5 minutes and 36 seconds in light time. It subtends an angle of only 13.89 arcseconds, which is not very large when it comes to discerning dusky low contrast surface features.
This by the way, is the allure of observing Mars. It is the only planet in our solar system where we can directly observe the surface. Venus, Jupiter, Saturn, Uranus, Neptune...these planets only show us their cloud tops. It is fun while sitting and observing Mars through a telescope to think back to the times when Astronomers such as Percival Lowell were making detailed visual observations of Mars and speculating on canals, water and plant life. Without the benefit of missions to Mars to see the Martian environment up-close we would still be wondering. Who knows what secrets Mars has yet to share with us? I, for one, remain curious.

Last night I made my first decent sketch of Mars with my TEC 8 inch f/20 Maksutov Cassegrain. I plan to write a review of this scope one day, but it is really a very specialized instrument that delivers excellent contrast, a large image scale, and sharp views. It is well regarded as a high end planetary instrument. The telescope is about 16 years old, and I believe that it is slightly out of collimation. I do mean slightly, and I will likely wait until this summer when I am in Colorado to personally deliver the scope to TEC for a tune-up. You can see from these pictures that despite its age, it is in good used shape.![]() |
| Click to enlarge |
This by the way, is the allure of observing Mars. It is the only planet in our solar system where we can directly observe the surface. Venus, Jupiter, Saturn, Uranus, Neptune...these planets only show us their cloud tops. It is fun while sitting and observing Mars through a telescope to think back to the times when Astronomers such as Percival Lowell were making detailed visual observations of Mars and speculating on canals, water and plant life. Without the benefit of missions to Mars to see the Martian environment up-close we would still be wondering. Who knows what secrets Mars has yet to share with us? I, for one, remain curious.
Thursday, March 1, 2012
Optimus Prime on space exploration
There is nothing to be said about this video...turn on your volume, watch it full screen and of course...
Autobots! Transform...and Roll Out!
Autobots! Transform...and Roll Out!
Saturday, February 18, 2012
Back to the drawing board
My life has been super busy- In addition to a new job, I have a new telescope(yipee) and next week is my sons Bar Mitzvah for which he has been studying for a year...but that is fodder for another post or three when I get the chance. This morning we have the clearest skies we have had in about a week and I decided that before I did any of the 100 things I need to get done today that I was going to make a sketch of the Sun. I love solar observing and sketching what I see and somehow we are mid-way through February and I had only managed three solar sketches this year! Finally, I present number four!
My sketch was completed at 1640 UT (9:40 MST) under clear skies, with average transparency. There does seem to be a bit of humidity in the air as evidenced by the whitish color of our sky (typically our skies are a picturesque blue), as well as the water dripping off of the roof. Regardless, the skies were still better than average and I was able to see much more detail that I could reasonably sketch. Believe it or not, the infrequency of my sketching has also left me a bit out of practice...so this took a bit longer than usual and I am not quite as thrilled with the detail on paper. The Sun was at an altitude of approximately 29 degrees, and an azimuth of approximately 129 degrees.
There are not many active regions on the face with AR 11420 quite near the meridian and containing a dark spot. Just above this AR 11419 contains two smaller spots and is somewhat brighter. To the east of these regions is a bright plage region that may be developing as evidenced by a strong dark filament within. 11418 near the SW limb is unremarkable. Perhaps the most interesting feature of the day is the beautiful "filaprom" on the SE limb. I do not know if this is the technical name, but this feature was very much 3D in my telescope as the filament and prominence were very clearly connected.
Below is a comparison image from the Big Bear Solar Observatory from 1659 UT, about 20 minutes following my sketch. Big Bear maintains a very nice webpage of recent images.
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There are not many active regions on the face with AR 11420 quite near the meridian and containing a dark spot. Just above this AR 11419 contains two smaller spots and is somewhat brighter. To the east of these regions is a bright plage region that may be developing as evidenced by a strong dark filament within. 11418 near the SW limb is unremarkable. Perhaps the most interesting feature of the day is the beautiful "filaprom" on the SE limb. I do not know if this is the technical name, but this feature was very much 3D in my telescope as the filament and prominence were very clearly connected.
Below is a comparison image from the Big Bear Solar Observatory from 1659 UT, about 20 minutes following my sketch. Big Bear maintains a very nice webpage of recent images.
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| Click to enlarge |
Saturday, February 11, 2012
SDO does it again
No time for a lengthy post, but I had to share this video released from the Solar Dynamics Observatory. Incidentally, today marks the second anniversary of the SDO launch....Just think, it is only over the past year and a half that humans have been able to observe the dynamic behavior of our star in high definition!
According to SDO: "As if it could not make up its mind . . . darker, cooler plasma slid and shifted back and forth above the Sun's surface seen here for 30 hours (Feb. 7-8, 2012) in extreme ultraviolet light. An active region rotating into view provides a bright backdrop to the gyrating streams of plasma. The particles are being pulled this way and that by competing magnetic forces. They are tracking along strands of magnetic field lines. This kind of detailed solar observation with high-resolution frames and a four-minute cadence was not possible until SDO, which launched two years ago on Feb. 11, 2010."
According to SDO: "As if it could not make up its mind . . . darker, cooler plasma slid and shifted back and forth above the Sun's surface seen here for 30 hours (Feb. 7-8, 2012) in extreme ultraviolet light. An active region rotating into view provides a bright backdrop to the gyrating streams of plasma. The particles are being pulled this way and that by competing magnetic forces. They are tracking along strands of magnetic field lines. This kind of detailed solar observation with high-resolution frames and a four-minute cadence was not possible until SDO, which launched two years ago on Feb. 11, 2010."
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