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Night Photography December 2011
Night Photography December 2011 Max Lyons http://www.tawbaware.com Agenda ● Photography at different times of night ● Moon ● Stars ● Software and technology ● Tips, Tricks and Equipment Blue Hour ● Blue Hour: “The period of twilight each morning and evening where there is neither full daylight nor complete darkness. The time is considered special because of the quality of the light at this time of day." 35 minutes after sunset, sun about 7 degrees below horizon Twilight ● Twilight: “the period between sunset and sunrise during which there is natural light provided by the upper atmosphere, which receives direct sunlight and scatters part of it towards the earth's surface" Credit: Why Not a Duck / Wikimedia Commons Light After The Sun Sets ● Civil Twilight: Sun is 0 to 6 degrees below horizon ● Nautical Twilight: Sun is 6 to 12 degrees below horizon ● Astronomical Twilight: Sun is 12-18 degrees below horizon ● Night: Sun is more than 18 degrees below horizon Blue Hour ● Some of the best “sunset” shots happen after most of the photographers have packed up their gear and gone home! Top: 1 minute before sunset, sun on horizon Bottom: 30 minutes after sunset, sun about 6 degrees below horizon Blue Hour ● If conditions are right, clouds “light up” just after sunset 10 minutes after sunset, sun about 2 degrees below horizon Blue Hour ● Clouds take on pink glow just after sunset 10 minutes after sunset, sun about 2 degrees below horizon Blue Hour ● Twilight provides even, soft illumination...and the opportunity for longer exposures 15 minutes after sunset, sun about 3.5 degrees below horizon ISO 100, F11, 2 seconds Blue Hour ● Great time to shoot objects illuminated by artificial light: buildings, statues, monuments, etc. -
Sky at Night 55 Moore Marathon - Observing Guide
The Sky at Night 55 Moore Marathon - Observing Guide... Thanks for taking part in the Sky at Night’s Moore Marathon - our 55th anniversary challenge. This guide has been designed to help you fi nd the 55 selected objects in the marathon. We would like you to tell us which of our 55 selected objects you’ve managed to fi nd. If you’ve managed to grab any images of them, then you can share them via our Flickr group at... www.fl ickr.com/groups/bbcskyatnight Remember too that you can keep up with the programme itself at... www.bbc.co.uk/skyatnight The guide has been written for the month of April, when British Summer Time is in force. When we talk about time in the marathon, we mean British Summer Time (BST) - that’s the same time as shown on your clock or watch. BST comes into force during 2012 on March 25th. On this day the clocks go forward by one hour. Please remember that for programme inclusion, we need your completed QUICK or DETAILED forms back by April 24th. Object No. Guide Page Object No. Guide Page Object No. Guide Page 1 2 21 4 41 4 2 2 22 11 42 4 3 2 23 15 43 2 4 2 24 15 44 8 5 4 25 4 45 9 6 4 26 11 46 9 7 8 27 14 47 9 8 8 28 14 48 9 9 8 29 14 49 4 10 4 30 9 50 2 11 4 31 15 51 4 12 9 32 11 52 15 13 10 33 4 53 15 14 10 34 13 54 13 15 10 35 2 55 11 16 10 36 4 17 13 37 2 18 11 38 4 19 14 39 4 20 13 40 11 Page 1 1 The Moon Rating - Easy Best seen with - Naked Eye Visibility - 1-9 April before midnight, 10-17 early hours, 22-30 early evening (programme deadline 24th April) The fi rst object is our very own Moon. -
Explorethe Impact That Killed the Dinosaursp. 26
EXPLORE the impact that killed the dinosaurs p. 26 DECEMBER 2016 The world’s best-selling astronomy magazine Understanding cannibal star systems p. 20 How moon dust will put a ring around Mars p. 46 Discover colorful star clusters p. 32 www.Astronomy.com AND MORE BONUS Vol. 44 Astronomy on Tap becomes a hit p. 58 ONLINE • CONTENT Issue 12 Meet the master of stellar vistas p. 52 CODE p. 3 iOptron’s new mount tested p. 62 ÛiÃÌÊÊÞÕÀÊiÞḭ°° ...and share the dividends for a lifetime. Tele Vue APO refractors earn a high yield of happy owners. 35 years of hand-building scopes with care and dedication is why we see comments like: “Thanks to all at Tele Vue for such wonderful products.” The care that goes into building every Tele Vue telescope is evident from the first time you focus an image. What goes unseen are the hours of work that led to that moment. Hand-fitted rack & pinion focusers must withstand 10lb. deflection testing along their travel, yet operate buttery-smooth, without gear lash or image TV-60 shift. Optics are fitted, spaced, and aligned using proprietary techniques to form breathtaking low-power views, spectacular high-power planetary performance, or stunning wide-field images. When you purchase a TV-76 Tele Vue telescope you’re not so much buying a telescope as acquiring a lifetime observing companion. Comments from recent warranty cards UÊ/6Èä®ÊºÊV>ÌÊÌ >ÊÞÕÊiÕ} ÊvÀÊ«ÀÛ`}ÊiÊÜÌ ÊÃÕV ʵÕ>ÌÞtÊ/ ÃÊÃV«iÊÜÊ}ÛiÊiÊ>Êlifetime TV-85 of observing happiness.” —M.E.,Canada U/6ÇȮʺ½ÛiÊÜ>Ìi`Ê>Ê/6ÊÃV«iÊvÀÊ{äÊÞi>ÀðÊ>ÞtÊ`]ʽÊÛiÀÜ ii`tÊLove, Love, Love Ìtt»p °°]" U/6nx®ÊºPerfect form, perfect function, perfectÊÌiiÃV«i]Ê>`ÊÊ``½ÌÊ >ÛiÊÌÊÜ>ÌÊxÊÞi>ÀÃÊÌÊ}iÌÊÌt»p,° °]/8 U/6nx®Êº/ >ÊÞÕÊvÀÊ>}ÊÃÕV Êbeautiful equipment available. -
Sample Chapter
REVIEW COPY NOT FOR PUBLIC USE First light on Morro Rock from Montaña de Oro Chapter 12 central coast 212 Photographing California VOL. 2 – SOUTH central coast 213 Morro Rock & Morro Strand State Beach Morro Bay State Park The volcanic plug, Morro Rock, towers 581 feet above the adjacent ocean and Although Morro Rock itself is techni- beach. There are over two miles of sandy beach north of Morro Rock. The beach cally within Morro Bay State Park, another close to the rock offers a very gradual slope towards the water. From the southern section of the same park next to Morro end of the beach, low tide can provide you with wet sand to capture Morro Rock Bay, south of town, provides better views and its reflection. A minus low tide is even better. of the rock. There are no trails on Morro Photo advice: The Bay itself provides a Rock and climbing is prohib- better mirror surface before afternoon ited, as it is a sacred site to local winds come up and in winter months with Salinan and Chumash tribes. less fog. The mud flats south of the town You can drive up to its base, of Morro Bay provide excellent habitat for though, and park at Coleman birds such as egrets and herons. Park. In the spring, you may find sea otters with pups here in Getting there: From downtown Morro the relatively calm waters of the Bay, take Main Street south to the vicin- entrance to the Bay. ity of the Morro Bay Golf Course and the Morro Bay State Park campground. -
Photo by David Townsend
Partners in Palo Duro Canyon Foundation On the Edge! Photo by David Townsend 1 Hi Ho! New Golf Carts for Park Hosts Photo by Eddie Tubbs Partners recently purchased for Palo Duro Canyon State Park three new golf carts to be used exclusively by Park hosts. “Exclusively” means that the carts will not be used for trail maintenance, trail rescues (emergencies being the exception), or other tasks required by the Park. Wouldn’t you like to drive one? To qualify as a Park host or other volunteer position contact Jeff Davis or Lindsay Pannell at (488) 2727, ext. 2007. E-mail: [email protected]. or [email protected]. Photos by Eddie Tubbs 2 The invention and implementation of the railroad provided a unique opportunity. Cattle bosses realized they could sell each head of cattle for ten times the amount in distant cities like Chicago. Ranches like Goodnight’s JA Ranch right here in Palo Duro Canyon took advantage of the opportunity. Thus the age of cattle drives and the iconic era of the cowboy was truly born. Most Texas ranchers began with longhorns Joseph Allen because of their plentiful numbers and ability Park Superintendent to survive hard trail drives. Today, we have four members of the Longhorns and Longjohns official longhorn herd of Texas. The old- timers, T-Bone and Brisket, are joined by two The year 1886 ushered in the “Great Die- new yearlings, Chicken and Waffles. Not a Up,” a bitterly cold blizzard that swept week passed after the babies journeyed from through the Great Plains, killing 90% of the South Texas to the Panhandle that we were northern herds. -
Calhoun Stargaze - October, 2019
Calhoun Stargaze - October, 2019 After experiencing almost two full weeks of clear October weather, with the New Moon period at month end approaching, the weather pattern went back to being unpredictable. The forecast for the weekend of the Calhoun StarGaze wasn’t very promising. But those who could make it down south early to Calhoun on Tuesday and Wednesday nights were lucky. Unfortunately, I had to work Thursday morning,,,,, Thursday 10/24/2019: Having packed up the camper and astronomy gear the night before, I left Pittsburgh around noon and after a couple of stops to gas-up the SUV, and pickup lunch, I arrived at the park right at 4pm. On the drive down, along I79 in the mountains, the fall tree colors were spectacular. There were 8 of us on the ridge, Ed K from the Kiski Astronomers, Frank W from Pgh, Nate from Tenn, John D of the Calhoun Stargaze committee, and Chuck from OH, and a couple of other campers that I didn’t have time to meet. Also, Warren and Stephanie had their RV down in the campground. Ed saved me my usual spot and introduced everyone there to the 'Pittsburgh Chair' concept. LOL! According to those who were there earlier in the week, both Tuesday and Wednesday nights were excellent! Chuck, John, and Ed told me that Wednesday night was chilly, no dew, but everything was covered by frost at dawn. Shortly after I arrived at Calhoun, Park Board members Donnie and Roger, along with additional help started work on installing new electrical conduit along the ridgeline and placed a new wooden power post (with 8 new duplex 110v outlets) toward the center section of the ridge. -
Joe Orman's Naked-Eye
Joe Orman’s Naked‐Eye 100 Title Description All‐Night Sky Stay up all night and watch the sky change as the earth turns. This faint patch of light is the farthest thing visible to the naked eye, over Andromeda Galaxy 2 million light‐years away! This red giant star in Scorpius is sometimes close to Mars, and they look Antares, The Rival Of Mars the same‐ bright and pink. Crepuscular rays converging on the antisolar point; often very faint and Anticrepuscular Rays diffuse. Follow the curve of the Big Dipper's handle to a bright star‐ Arcturus in Arc To Arcturus Bootes. ISS, HST etc. look like stars moving steadily across the sky. Check Artificial Satellites heavens‐above.com for visibility. Usually too faint to see, but on April13, 2029, asteroid 2004MN will Asteroids make a close naked‐eye pass. Bright glow around the sun or moon, colorless and only a few degrees Aureole across. Northern Lights. From the southern U.S., can occasionally be seen as a Aurora Borealis reddish glow in the northern sky. Sunlight peeking between the mountains of the moon during a total Bailey's Beads solar eclipse. A band of pink above the horizon; look opposite the sun just before Belt Of Venus sunrise or just after sunset Betelgeuse The Hunter's left shoulder is a red giant star, bright and pink to the eye. The body and tail of Ursa Major, the Big Bear. Close to Polaris in the Big Dipper northern sky. The star where the dipper's handle bends, Mizar, has a fainter Big Dipper Double‐Star companion Alcor‐ a good test of vision. -
“Running Man” Nebula
NGC 1975 the “Running Man” nebula Robbin Jones took this image of the “The Running Man” nebula in Orion Oct 17 with his MallinCam DS10cTEC color CMOS camera on a Celestron 8" SCT XLT scope. Image was made using an Orion Skyglow imaging filter with 30 15 second exposures live stacked at 3 different histogram white points of 255, 200 and 150. Most of us are familiar with M 42 the great Orion Nebula but we often overlook other nearby treasures. NGC 1975 sets just above the famous nebula. Its composed of a cloud of interstellar dust superimposed on a background area of reflection nebulae. It is part of a larger region composed of NGC 1973, 1975 and 1977 lying about 1,500 light years away in Orion. See more at https://apod.nasa.gov/apod/ap141219.html Contents: 1 The Running Man Nebular by Robbin Jones 2 Upcoming Events 3 Zoom Meeting Tues Dec 8th - Dr. Emily Levesque “The Last Star Gazers” Links to previous Zoom meetings - 2021 Astronomical League calendars 4 President’s Message – by Tamara Green Board meeting report - Texas Star Party May 2-9 5-6 The Grand Conjunction of Jupiter and Saturn and how it affected the history of astronomy 7-9 Throwing Shade – by Brad Young - observing Earth’s shadow 10 New Ancient Egyptian Constellations discovered – Ron Coates Make a Rainbow Sundial by John Land 11 Star & Constellation Word Search by John Blaesi 12 Treasurer’s Report – John Newton 13 Club Contacts and Ideas Wanted for Club Zoom meetings Astronomy Club Events Check our website www.AstroTulsa.com events section for updates Members ONLY Events continue with Social Distancing Guidelines in Effect We are limiting our Observatory nights to our MEMBERS ONLY. -
Watch for Earth's Shadow and the Belt of Venus in Both the Evening
Watch for Earth’s shadow and the Belt of Venus In both the evening and morning sky, try watching for Earth’s shadow, a blue-grey darkness in the direction opposite the Sun, darker than the twilight sky. Like all worlds orbiting a Sun, Earth casts a shadow. Earth's shadow extends about 1.4 million km into space. You might not realize it, but, from Earth's surface, you can see the shadow. In fact, it's easy to see, and you've probably already seen it, many times, as day changes to night. That's because night itself is a shadow. When night falls, you're standing within the shadow of Earth. The best time to watch for Earth's shadow is when it's creeping up on your part of Earth … The pink band above the shadow – in the east after Image taken at the Woomera missile range in Australia sunset, or west before dawn – is called the Belt of Venus. The Moon phase shifts throughout the month, and sometimes you won’t find the Moon in the night sky. Earth’s shadow, on the other hand, is more reliable. It can be seen any clear evening, ascending in the eastern sky at the same rate that the Sun sets below the western horizon. The shadow of the Earth is big. You might have to turn your head to see the whole thing. And the shadow is curved, just as the shadow of any round object is curved. Earth’s shadow extends hundreds of thousands of miles into space, so far that it can touch the Moon. -
Night Photography in the Great Outdoors
Collier’s Guide to Night Photography in the Great Outdoors Text and Photography by Grant Collier Collier Publishing Arvada, CO CP Acknowledgements About the Author I learned most of the information in this book by experimenting with different equipment, camera settings, and shooting techniques over 12 years. However, I wanted to ensure that this book was as thorough as possible, so I scoured the web for any other tips and pointers that might be useful. I would like to thank the following photographers for the advice they have provided to ensure that capturing a good shot in the dark is more than just a shot in the dark! David Kingham, Tony Kuyper, Floris Van Breugel, Mike Berenson, Nat Coalson, Steven Christenson, Ian Norman, Allister Benn, Royce Bair, John Mumaw, Mikko Lagerstedt, Jeffrey Sullivan, Brad Goldpaint, Thomas O’Brien, Phil Hart, Tony Prower, Marc Adamus, René Pirolt, Todd Salat, and Jason Hatfield. ©2015 Grant Collier All photos ©2015 Grant Collier Design by Grant Collier ISBN # 978-1-935694-17-5 Published by Collier Publishing LLC http://www.collierpublishing.com This book may not be reproduced in full or in part by any means (with the exception of short quotes for purpose of review) without permission of the publisher. Cover Photo: The aurora borealis lights up the night sky over Wiseman, Alaska. Title Page: A waterfall flows beneath Kirkjufell mountain in Iceland, as the northern lights dance in the sky. Author Page: Grant stands in the opening of Wilson Arch near Moab, Utah on an autumn night. Back Cover: The Milky Way provides a dramatic backdrop to a ruin in Canyonlands National Park. -
November2016 .Pdf
WESTCHESTER AMATEUR ASTRONOMERS November 2016 Celebrating Halloween In This Issue . Courtesy of Scott Nammacher is this ghostly image of IC63 in pg. 2 Events for November Cassiopeia. IC63 is an emission/reflection nebula associated with nd pg. 3 Almanac the 2 magnitude star Gamma Cassiopeia. The nebula lies at a pg. 4 In Memoriam: Mario Palmieri distance of about 600 light years. pg. 5 WAA Goes to Astronomy Camp Scott took this image with his 12.5" Planewave scope and a SBIG pg. 12 Is Proxima Centauri's 'Earth-like' 10XME camera—160 min (10 minute subs) in each of Ha and Planet Actually like Earth at All? OIII. He used MaximDL for capture and stacking and Photoshop pg. 13 The Belt of Venus to combine and finish. Scott did a 4-color version using Ha and pg. 14 Active Regions 2599 and 2598 OIII, but elected to convert the finished work to B&W for effect. SERVING THE ASTRONOMY COMMUNITY SINCE 1986 1 WESTCHESTER AMATEUR ASTRONOMERS November 2016 Events for November Emmanouil Makrakis - Scarsdale Claudia & Kevin Parrington Family - Harrison WAA November Lecture Elaine Miller - Pound Ridge “Astrophotography Image Processing Hans Minnich - Bronx with PixInsight.” Bob Kelly - Ardsley Friday November 4th, 7:30pm Kevin Mathisson - Millwood Leinhard Lecture Hall, Pace University, Pleasantville, NY Astrophotographer and WAA-member, Olivier Pra- che, will briefly introduce the image processing soft- ware, PixInsight, and its purpose. He will go through a digital color image development process using Pix- Insight to highlight how the tools function and how to use them. Olivier has been watching the sky since the mid- 1970’s and started imaging around 2003. -
Tropospheric Haze and Colors of the Clear Twilight Sky
Research Article Vol. 56, No. 19 / July 1 2017 / Applied Optics G179 Tropospheric haze and colors of the clear twilight sky RAYMOND L. LEE,JR.* AND DUNCAN C. MOLLNER Mathematics and Science Division, United States Naval Academy, Annapolis, Maryland 21402, USA *Corresponding author: [email protected] Received 31 January 2017; revised 21 March 2017; accepted 23 March 2017; posted 24 March 2017 (Doc. ID 285879); published 12 June 2017 At the earth’s surface, clear-sky colors during civil twilights depend on the combined spectral effects of molecular scattering, extinction by tropospheric aerosols, and absorption by ozone. Molecular scattering alone cannot pro- duce the most vivid twilight colors near the solar horizon, for which aerosol scattering and absorption are also required. However, less well known are haze aerosols’ effects on twilight sky colors at larger scattering angles, including near the antisolar horizon. To analyze this range of colors, we compare 3D Monte Carlo simulations of skylight spectra with hyperspectral measurements of clear twilight skies over a wide range of aerosol optical depths. Our combined measurements and simulations indicate that (a) the purest antisolar twilight colors would occur in a purely molecular, multiple-scattering atmosphere, whereas (b) the most vivid solar-sky colors require at least some turbidity. Taken together, these results suggest that multiple scattering plays an important role in determining the redness of the antitwilight arch. © 2017 Optical Society of America OCIS codes: (010.1290) Atmospheric optics; (010.1310) Atmospheric scattering; (010.1690) Color; (010.3920) Meteorology; (330.1730) Colorimetry. https://doi.org/10.1364/AO.56.00G179 τ 1.