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What's Happening at Insight Observatory...

Saturday, November 16, 2013

Comets ISON and Lovejoy Now Visible to Naked Eye

According to reports from Space.com and Sky and Telescope magazine, the much-anticipated Comet ISON is now visible to the naked eye according to reports from many observers. Comet ISON - the potential "comet of the century" - has suddenly brightened in an outburst of activity with just two weeks to go before it literally grazes the surface of the sun.  In recent months, Comet ISON has repeatedly befuddled forecasters trying to anticipate just how bright it will ultimately become. 

Comet ISON imaged by Julian Durnwalder on 11-10-2013 using itelescope.net's T21 in Mayhill, New Mexico
Comet ISON imaged by Julian Durnwalder on 11-10-2013
using itelescope.net's T21 in Mayhill, New Mexico

But earlier this week, the comet's brightening trend again seemed to sputter and stall, but more recent observations suggest a sudden and radical upsurge in brightness. Comet ISON has brightened suddenly in the last few days to 5th magnitude as of November 15th - a popsicle-shaped comet with a round, sharp-edged, bright green head and a long, thin, dim tail. It's speeding sunward near the bright star Spica in Virgo and Mercury low in the east just before dawn. The comet passes less than 2° from Spica on the mornings of November 17th and 18th for the Americas, accelerating every day toward its November 28th perihelion and trial by fire.

According to veteran comet observer, John Bortle, Comet ISON was shining only at magnitude +8.5 on Monday (Nov. 11) morning - more than six times too dim to be visible to the unaided eye. But by Wednesday morning, the comet’s brightness had increased three-fold brightening to +7.3.

In just 72 hours, Comet ISON increased nearly 16 times in brightness. Carl Hergenrother, acting co-coordinator of the comet section of the Association of Lunar and Planetary Observers, has confirmed Bortle's observations. "ISON has dramatically brightened over the past few days," Hergenrother told SPACE.com via email. "The latest observations put the comet around magnitude 5.7 to 6.1 which is a 2+ magnitude increase from this weekend. My own observations from this morning in 10x50 and 30x125 binoculars show a nice 'lollipop' comet with a very condensed blue-green head and a long narrow tail. The tail was over 1 degree in length even in the 10x50s. The comet may continue to brighten as the outburst is still in its early stages."

Meanwhile, Comet Lovejoy glows only a little less bright much higher before dawn. Both comets are visible in binoculars despite moonlight returning to the morning sky. They're being detected naked-eye by skilled observers under good conditions.

As of Nov. 6, based on a consensus of worldwide observers, Comet Lovejoy had reached magnitude 6.5, which is considered to be the threshold of naked-eye visibility in a dark sky, far from any bright lights.

The new comet is getting progressively brighter with each passing day. This is because while en route to its Dec. 22 rendezvous with the sun, Lovejoy will make its close approach with Earth on Tuesday, when it will pass within 36.9 million miles (59.4 million km) of the planet.

At its best around that time, Comet Lovejoy "might" become as bright as magnitude 4.5, still a moderately faint object, yet bright enough to be glimpsed with the naked eye and certainly a fine object for binoculars and small telescopes. Unfortunately, the moon will be two days past full that morning and well up in the west, lighting up the sky, probably preventing any naked-eye viewing opportunity.
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Saturday, July 13, 2013

Blake Planetarium Receives Grant from itelescope.net

With a generous research grant awarded from iTelescope.net, a research project utilizing remote robotic telescopes for astronomy education called "Discovering our Milky Way Galaxy" will be a collaboration between the W. Russell Blake Planetarium, Insight Observatory, iTelescope.net and a group of students in grades 6-8. The planetarium will place a large printout of the Milky Way Galaxy, the way we see it from Earth, on the outside wall of the planetarium. The printout of the Milky Way will cover the view from both hemispheres. The students will be paired in groups of two and each group will be assigned a deep-sky object in or near the visible arm of the visible Milky Way. 

Northern Arm of Milky Way Galaxy imaged from iTelescope.net's New Mexico Skies location
Northern Arm of Milky Way Galaxy imaged from iTelescope.net's New Mexico Skies location

They will be in charge of imaging this object and writing a paragraph about it. When the images are returned, Michael Petrasko and Muir Evenden, Co-Project Directors from Insight Observatory will assist them with processing the images. The final pictures of the students' deep-sky objects will be placed along with the image of the Milky Way on the outside of the planetarium for all of the school and visitors to see and learn from.

The research project is slated to take place in October 2013. Planetarium Instructor, Monica Ares, will have the students come to the planetarium for an overview of the project and to look at the Milky Way on the dome. They will pair up and use iPads to fill out a form through Insight Observatory's website with their image request, exposure time, and telescope location. The form will also require a paragraph about the object. The students will return a week later to process their images in the computer lab. The photos will then be printed and overlaid on the image of the Milky Way along the outside of the planetarium.

The goal of the project is for students and teachers to understand not only what lies beyond our own night sky but also how we use the clues of distant objects to help us understand our own galaxy. Since we cannot take a picture of our entire Milky Way galaxy, we can study the images we capture of distant galaxies, both edge-on, and front-facing to better understand the part of the Milky Way that we can see in our sky. We can also study nebulae both within our galaxy and those that we see in distant galaxies to help us understand the life cycle of our stars and our ever-changing universe. We hope to create a permanent display of both the Galaxy Project and the Milky Way Project using digital posters on the outside of the planetarium.
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Saturday, May 18, 2013

The Galaxy Project - What Lies Beyond Our Stars

Ms. Campbell's 6th-grade class at Plymouth Community Intermediate School in Plymouth, Massachusetts, was part of an exciting collaboration with the W. Russell Blake Planetarium and the Insight Observatory to image objects beyond the visible stars in our night sky. The students were given access to high-powered remote robotic telescopes for astronomy education located in New Mexico and Spain, facilitated by Insight Observatory. Each group was asked to image an item in deep space found near the patch of sky containing the constellations of Ursa Major, Leo, Coma Berenices, Canes Venatici, and Virgo.

Display of Galaxies Imaged by PCIS Students
Display of Galaxies Imaged by PCIS Students

The images that the students took of galaxies, a globular cluster, and a planetary nebula are breathtaking!  A large printout of the night sky, along with the students' images, is on display near the entrance of the planetarium. This hands-on experience not only taught the students a great deal about remote imaging with a telescope, but it also enabled them to grasp the profoundness of the images they captured.

Special thanks to Monica Ares, Planetarium Program Instructor, Michael Petrasko, Insight Observatory Project Developer, and Kellianne Campbell, 6th Grade Teacher at PCIS. Together, they designed this amazing opportunity for our students that they hope will grow in the years to come. Below are a few of the images the students acquired by using a 17" telescope remotely in Mayhill, New Mexico, with all image exposure times at 5 minutes. You can view all of the images the students acquired on the Insight Observatory's Image Gallery page.

M51 - Image by Mark R. & Peter H.
M51 - Image by Mark R. & Peter H.

The Whirlpool Galaxy (also known as NGC 5194) is an interacting grand-design spiral galaxy in the constellation Canes Venatici. Recently, it is estimated to be 15 and 35 million light-years from our own Milky Way Galaxy. The galaxy and its companion (NGC 5195) are easily observed by amateur astronomers, and the two galaxies may even be seen with binoculars under dark skies and good seeing conditions. The Whirlpool Galaxy is also a popular target for professional astronomers, who study it to further understand galaxy structure (particularly structure associated with the spiral arms) and galaxy interactions.  

M97 - Image by Bianca T. & Cassidy B.
M97 - Image by Bianca T. & Cassidy B.

The Owl Nebula (also known as Messier 97, NGC 3587) is a planetary nebula in the constellation Ursa Major. It was discovered by Pierre Méchain in 1781. M97 is regarded as one of the more complex of the planetaries. The 16th magnitude central star has about 0.7 solar mass, and the nebula itself has about 0.15 solar mass. The nebula formed roughly 6,000 years ago. The nebula gets its name from the appearance of owl-like "eyes" when viewed through a large 200mm telescope under dark sky conditions with the aid of a so-called "nebula filter." The eyes are also (albeit not so easily) visible in photographs of the nebula.

NGC 4565 - Image by Olivia F. & Nachelle S.
NGC 4565 - Image by Olivia F. & Nachelle S.

NGC 4565 (also known as the Needle Galaxy or Caldwell 38) is an edge-on spiral galaxy about 30 to 50 million light-years away in the constellation Coma Berenices. The 10th magnitude galaxy sits perpendicular to our own Milky Way galaxy and is almost directly above the North Galactic Pole (in the same way Polaris is located above the North Pole). It is known as the Needle Galaxy for its narrow profile. First spotted in 1785 by Sir William Herschel (1738–1822), this is one of the most famous examples of an edge-on spiral galaxy. "Visible through a small telescope, some sky enthusiasts consider NGC 4565 to be a prominent celestial masterpiece Messier missed."
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