Tag Archives: Newtonian

IOTA Announcement – Occultation By Neptune’s Moon Triton – 5 October 2017

Greetings, fellow astrophiles!

The following recently came across the ASRAS email list from ASRAS and IOTA member Brad Timerson. If you’ve the gear for it, this is an excellent chance to contribute to some far-out science.

There will be an occultation of a 12.5-mag. star by Neptune’s large satellite Triton the early evening of October 5th (just before 8pm EDT) that will be visible from east of the Appalachian Mountains. It’s the brightest star to be occulted by Triton since the Voyager flyby showed that the satellite has a substantial atmosphere with interesting dark plumes. The occultation will allow us to learn more about the atmosphere, and its variation with altitude and latitude. Sofia plans to fly over the Atlantic, to try to catch the central flash, where Triton’s whole atmosphere will focus/amplify the star’s light, probing deeper parts of the atmosphere. This might also be observed from Florida, but observations anywhere from the East Coast area are sought, to sample a wide range of latitudes of Triton’s atmosphere. Details of the occultation are available at MIT’s Web site for the event at hubble.mit.edu/prediction.html.

The central time for the Rochester area is within several seconds of 7:55:40 pm EDT on October 5th. For an observer near the center of the path, the event could last as long as 3 minutes. Because the Rochester area is north of that path, any occultation or atmospheric dimming would likely last some fraction of that time. You should plan to record the event for about 10 minutes before and after the time shown here.

A main challenge of the event will be to record Triton and the target star with a good signal, preferably with clear separation between 8th-mag. Neptune less than a quarter arc minute away. You will need good scale to separate the objects well enough. More observing tips are given on the MIT web site. The target star is about a magnitude brighter than Triton.

Telescopes as small as 8″ Newtonians will show the target star. (see included image from a European observer) For occultation work, we don’t need to “see” the occulting body (Triton in this case), just the object being occulted. Low light and/or integrating video cameras are best for this observation. However, standard astronomical cameras operated in a mode so as to produce images as quickly as possible will also work. Testing ahead of time to determine the correct exposure to just barely detect Triton should be done. This is to insure that the light from nearby Neptune doesn’t overwhelm that of the nearby moon and star at the time of the event.

Target star, Neptune, and Triton.

I plan on using my 10″ Meade LX200GPS at either f/6.3 (focal reducer) or at the normal f/10 prime focus. I will be using a Watec 120N+ low light video camera and integrating for 64 or 128 frames (2 seconds and 4 seconds). I’m still experimenting and might even need longer integration times.

Triton occults 4UC 410-143659, 5 October 2017 – visible regions from Earth.

Everyone with suitable equipment is encouraged to try this event. And I would appreciate it if this message is forwarded to any nearby universities that might have the ability to observe this event. If individual images are taken (instead of video) the exact time for each exposure is required (don’t depend on the computer’s internal clock. Use a GPS-based time). For analysis, it may be possible to measure the light level on individual images or the images can be combined into a video and measuring software used on the video.

Please contact me (EMAIL) for additional information or to submit observations.

CNYO Observing Log: TACNY Jr. Cafe And Solar Session @ The MOST, 17 May 2014

The May 17th TACNY Jr. Cafe Scientifique featured New Moon Telescope’s and CNYO’s own Ryan Goodson. His lecture, “Monster Telescopes And How They Are Built,” took attending students and adults on a 70-minute tour of the history of large-aperture telescopes. The lecture focused specifically on the Dobsonian philosophy that Ryan and NMT have developed upon to produce a novel design in scope assembly that many in the amateur astronomy community have taken notice of (when not commenting on the quality of the woodwork!).

The history and recent developments of the kind of telescope made famous by Isaac Newton – the Newtonian Reflector. We will begin the discussion from the perspective of the great Newton in the 1600s with his humble 1 1/2″ reflector, then journey through time to the present day, when amateur astronomers can often be seen in fields with telescopes large enough to rival or often surpass the size and quality of many professional observatories. We will focus on how the telescope is built, from the choice of wood to the installation of advanced electronics, finishing the discussion with what they are ultimately able to show us.

From Newton’s own telescope (perhaps he called it a “Me”ian scope), to the use of the PLOP program for optimizing mirror cells, to the new trend of GOTO-ing Dobsonian designs for tracking and imaging applications, Ryan gave the audience a broad sampling of topics important to scoped builders and users, all in a manner that didn’t bury non-scope owners in the jargon of the field.

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Ryan loading the rocker box of a 16″ Dob.

As is always the case at Jr. Cafe lectures, the kids were full of interest and great questions (as I’ve said before, nothing makes me feel more hopeful about the future of U.S. science than having a student ask a question I have to think hard about before answering).

But Wait! There’s More!

To take full advantage of the number of attendees and attending scopes, CNYO also hosted a solar session at the very beginning of the Creekwalk (next to the MOST) immediately after Ryan’s lecture. Over a two-hour period, approximately 45 lecture attendees and passers-by stopped to take in the sights of out nearest star. On a day that featured a few thick pockets of high-altitude clouds and otherwise perfect blue skies, the Coronado PST in attendance allowed us to follow a few significant prominences that changed shape considerably over the course of only 15 minutes (which was made more impressive to some of the new observers when we mentioned that these prominences were more easily measured in Earth diameters than in miles or kilometers).

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The Sun on May 17th, 2014. From NASA/SOHO

CNYO would like to specifically thank the NASA Night Sky Network for providing a (timely) Solar Kit that has already seen quite a bit of use these past few months at the capable hands of Larry Slosberg. I also want to thank Stephen Ramsden of the Charlie Bates Solar Astronomy Project for handing me several pairs of solar shades (at NEAF 2014) that also saw considerable use to those not lined up behind the scopes.

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