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An Overview of New Worlds, New Horizons in Astronomy and Astrophysics About the National Academies
2020 VISION An Overview of New Worlds, New Horizons in Astronomy and Astrophysics About the National Academies The National Academies—comprising the National Academy of Sciences, the National Academy of Engineering, the Institute of Medicine, and the National Research Council—work together to enlist the nation’s top scientists, engineers, health professionals, and other experts to study specific issues in science, technology, and medicine that underlie many questions of national importance. The results of their deliberations have inspired some of the nation’s most significant and lasting efforts to improve the health, education, and welfare of the United States and have provided independent advice on issues that affect people’s lives worldwide. To learn more about the Academies’ activities, check the website at www.nationalacademies.org. Copyright 2011 by the National Academy of Sciences. All rights reserved. Printed in the United States of America This study was supported by Contract NNX08AN97G between the National Academy of Sciences and the National Aeronautics and Space Administration, Contract AST-0743899 between the National Academy of Sciences and the National Science Foundation, and Contract DE-FG02-08ER41542 between the National Academy of Sciences and the U.S. Department of Energy. Support for this study was also provided by the Vesto Slipher Fund. Any opinions, findings, conclusions, or recommendations expressed in this publication are those of the authors and do not necessarily reflect the views of the agencies that provided support for the project. 2020 VISION An Overview of New Worlds, New Horizons in Astronomy and Astrophysics Committee for a Decadal Survey of Astronomy and Astrophysics ROGER D. -
Experiencing Hubble
PRESCOTT ASTRONOMY CLUB PRESENTS EXPERIENCING HUBBLE John Carter August 7, 2019 GET OUT LOOK UP • When Galaxies Collide https://www.youtube.com/watch?v=HP3x7TgvgR8 • How Hubble Images Get Color https://www.youtube.com/watch? time_continue=3&v=WSG0MnmUsEY Experiencing Hubble Sagittarius Star Cloud 1. 12,000 stars 2. ½ percent of full Moon area. 3. Not one star in the image can be seen by the naked eye. 4. Color of star reflects its surface temperature. Eagle Nebula. M 16 1. Messier 16 is a conspicuous region of active star formation, appearing in the constellation Serpens Cauda. This giant cloud of interstellar gas and dust is commonly known as the Eagle Nebula, and has already created a cluster of young stars. The nebula is also referred to the Star Queen Nebula and as IC 4703; the cluster is NGC 6611. With an overall visual magnitude of 6.4, and an apparent diameter of 7', the Eagle Nebula's star cluster is best seen with low power telescopes. The brightest star in the cluster has an apparent magnitude of +8.24, easily visible with good binoculars. A 4" scope reveals about 20 stars in an uneven background of fainter stars and nebulosity; three nebulous concentrations can be glimpsed under good conditions. Under very good conditions, suggestions of dark obscuring matter can be seen to the north of the cluster. In an 8" telescope at low power, M 16 is an impressive object. The nebula extends much farther out, to a diameter of over 30'. It is filled with dark regions and globules, including a peculiar dark column and a luminous rim around the cluster. -
The Flint River Observer a Frac Special Edition The
1 How it happened is an intriguing tale. Many astronomers considered the change to be a long- THE overdue step in advancing astronomy as a science -- and as many others regarded it as a deception perpetrated by the International Astronomical FLINT RIVER Union (IAU). Curiously, both sides were right. I’ve written about it before, but this Special OBSERVER Edition of the Observer is broader in scope. Written 22 yrs. after the event, it tells both sides of NEWSLETTER OF THE FLINT the story in far greater depth than previously. RIVER ASTRONOMY CLUB (Incidentally, this project began as a brief “This ‘n That” newsletter item about an article that An Affiliate of the appeared in Astronomy Magazine but quickly grew Astronomical League into something much larger. You’ll see what I was writing about on p. 6.) Special Edition October, 2018 -Bill __________________________________________ * * * A FRAC SPECIAL EDITION THE PLUTO QUESTION: What is a Planet? Beginnings. The discovery of Neptune by William Lassell in 1846 brought the solar system’s planet total to eight. However, wobbles in the by Bill Warren orbital paths of Uranus and Neptune led the American astronomer, founder and director of __________________ Lowell Observatory, Percival Lowell, to conclude that a ninth planet -- he called it Planet X – lay Introduction. If you were born before 1990, you somewhere beyond Neptune and was tugging probably remember how upset people were when gravitationally on that planet and Uranus. Lowell Pluto was removed from the solar system’s family died in 1916, but in 1929 Vesto Slipher, his of planets in 1996. -
115 Abell Galaxy Cluster # 373
WINTER Medium-scope challenges 271 # # 115 Abell Galaxy Cluster # 373 Target Type RA Dec. Constellation Magnitude Size Chart AGCS 373 Galaxy cluster 03 38.5 –35 27.0 Fornax – 180 ′ 5.22 Chart 5.22 Abell Galaxy Cluster (South) 373 272 Cosmic Challenge WINTER Nestled in the southeast corner of the dim early winter western suburbs. Deep photographs reveal that NGC constellation Fornax, adjacent to the distinctive triangle 1316 contains many dust clouds and is surrounded by a formed by 6th-magnitude Chi-1 ( 1), Chi-2 ( 2), and complex envelope of faint material, several loops of Chi-3 ( 3) Fornacis, is an attractive cluster of galaxies which appear to engulf a smaller galaxy, NGC 1317, 6 ′ known as Abell Galaxy Cluster – Southern Supplement to the north. Astronomers consider this to be a case of (AGCS) 373. In addition to his research that led to the galactic cannibalism, with the larger NGC 1316 discovery of more than 80 new planetary nebulae in the devouring its smaller companion. The merger is further 1950s, George Abell also examined the overall structure signaled by strong radio emissions being telegraphed of the universe. He did so by studying and cataloging from the scene. 2,712 galaxy clusters that had been captured on the In my 8-inch reflector, NGC 1316 appears as a then-new National Geographic Society–Palomar bright, slightly oval disk with a distinctly brighter Observatory Sky Survey taken with the 48-inch Samuel nucleus. NGC 1317, about 12th magnitude and 2 ′ Oschin Schmidt camera at Palomar Observatory. In across, is visible in a 6-inch scope, although averted 1958, he published the results of his study as a paper vision may be needed to pick it out. -
Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed Individual Bright Stars in Andromeda
The Resolution: Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed individual bright stars in Andromeda • Calculated the distance using the Period-Luminosity Relation for Cepheid Variable Stars The Resolution: Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed individual bright stars in Andromeda • Calculated the distance using the Period-Luminosity Relation for Cepheid Variable Stars 1. MEASURED magnitude & Period The Resolution: Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed individual bright stars in Andromeda • Calculated the distance using the Period-Luminosity Relation for Cepheid Variable Stars 1. MEASURED magnitude & Period 2. CALCULATED Luminosity The Resolution: Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed individual bright stars in Andromeda • Calculated the distance using the Period-Luminosity Relation for Cepheid Variable Stars 1. MEASURED magnitude & Period 2. CALCULATED Luminosity 3. CALCULATED Distance The Resolution: Edwin Hubble (1889-1953) Measured Distance to Andromeda Galaxy (M31) • Noticed individual bright stars in Andromeda • Calculated the distance using the Period-Luminosity Relation for Cepheid Variable Stars 1. MEASURED magnitude & Period 2. CALCULATED Luminosity 3. CALCULATED Distance • Result was MUCH farther than expected... • (2.3 Million Ly - well beyond Milky Way) Henrietta Leavitt & Period-Luminosity Relation Cepheid Variables: Bright stars whose Luminosity (energy output) varies every -
What If the Mars Rover Does Find Lostgenius Whomerits Aplaceon Thepodium
Thursday, August 30, 2012 THE IRISH TIMES 11 ScienceScience EditorTodayDick Ahlstrom e-mail [email protected] CORMAC Ó What if the Mars Rover does find RAIFEARTAIGH Lost genius Proof of who merits a place on the podium Who knows about Vesto Slipher, life? the astronomer who inspired the work of Edwin Hubble? NE OF the great surprises of 20th century science was the discovery that Oour universe is expanding. The finding caused a paradigm shift in cosmology and eventually led to today’s “Big Bang” model of the origin of the universe. It is therefore quite puzzling that a scientist who played a key role in the discovery remains virtually unknown to scientists and the general public alike. Step forward Vesto Slipher, the American astronomer who first established that the most distant objects in the sky are moving away from one another at high speed. Vesto Melvin Slipher was born in the US state of Indiana in 1875. He was educated at Indiana University and took up a position at the Lowell Observatory in Arizona after receiving his degree in 1901. There, he showed himself to be an astronomer of exceptional talent. In particular, he pioneered a method of measuring the motion of stars with the use of a spectrograph, an instrument that analyses the spectrum of light emitted by a body. Slipher used his new technique to study the attempting to answer questions “A laser on Curiosity’s mast cre- many details about the analysis of Is there anything out there? An Kevin Nolan, lecturer in physics at most enigmatic astronomical objects of the BECCA WILSON about Martian life. -
Victoria Centre
ROYAL ASTRONOMICAL SOCIETY OF CANADA: VICTORIA CENTRE New Moon through the Trees, by Diane Bell The Littlest AGM After changing our society’s year end to December 31st, to be more in sync with RASC National and the rest of Western Civilization, the next step was having an annual general meeting, to fulfill our obligations to the BC Society’s Act. The February 13th meeting was chosen to do double duty as our monthly meeting and what President Reg Dunkley promised as a 5 minute AGM, to vote on the financials I prepared as the outgoing treasurer. SKYNEWS March 2019 ISSUE #406 Page 1 ROYAL ASTRONOMICAL SOCIETY OF CANADA: VICTORIA CENTRE The dining wasn’t what we’ve come to expect for our annual general meetings. In fact there was no food to be had at all, other than the usual snacks served in the astronomy teacher’s lounge for our after meeting social. Having just had our banquet in November, it was considered a bit gauche to have another one so soon, let alone the organizing required to make it happen on short notice. The weather was also unkind, as the meeting was scheduled at the end of a week of snow for the BC South Coast, something local denizens are generally less than prepared for. 19 RASC Victoria members were present and another 16 provided proxy votes so we could achieve quorum (there are currently 285 RASC Victoria Centre members). One of the proxy votes was made from as far away as Tasmania! The SkyNews Editor provided his proxy vote and watched the meeting via UTube, from his home, on the snowy plateau of North Saanich, where his summer tire equipped car remained parked for the week. -
Extra! Extra! Read All About the Universe!
Extra! Extra! Read All About the Universe! Barb Mattson (USRA/GSFC) JHU Space Grant July 8, 2013 1 Nature of Supernovae You will receive the Cosmic Times posters at the end of this workshop Gallery Walk Take a tour of the Cosmic Times posters Gallery Walk ' • ' Start at one Cosmic Times poster station Ø Cosmic Times poster Ø 3 versions of the newsletter: early edition (7-8 grade), home edition (9-10 grade), late edition (11-12 grade, same readings as on posters) • ' At each poster, use the chart paper to record the answers to the following two questions, as they relate to that issue of Cosmic Times Ø What big questions are facing scientists? Ø What answers have scientists just found? • ' You will have 4 minutes at the first poster, and 2 minutes at each subsequent poster • ' Return to first poster and prepare a 1-minute summary of all the responses (write it down!) The year is 1919… ' • What’s going on? • What’s going on in science? • What is your view of the Universe? ª Infinite ª Unchanging/static ª Ageless ' 5 1919 – Einstein’s Gravity • ' What is Gravity? • ' Gravity is curved space- time. Ø Gravity bends light. Ø Amount of deflection ' differs from Newton’s prediction. ' ➜ 1919 Solar Eclipse verified Einstein’s prediction. 1919 – Einstein’s Gravity • What is Gravity? • Gravity is curved space- time. Ø Gravity bends light. Ø Amount of deflection differs from Newton’s prediction. ➜ 1919 Solar Eclipse verified Einstein’s prediction. Fundamental science concepts: motions of the Earth, Moon & Sun, solar eclipse, gravity, curved space-time 1929 - Expanding Universe ' • Vesto Slipher showed the “nebulae” were red- shifted. -
Hubbles Spies the Beautiful Galaxy IC 335 24 December 2014
Hubbles spies the beautiful galaxy IC 335 24 December 2014 very low. Hence, the population of stars in S0 galaxies consists mainly of aging stars, very similar to the star population in elliptical galaxies. As S0 galaxies have only ill-defined spiral arms they are easily mistaken for elliptical galaxies if they are seen inclined face-on or edge-on as IC 335 here. And indeed, despite the morphological differences between S0 and elliptical class galaxies, they share some common characteristics, like typical sizes and spectral features. Both classes are also deemed "early-type" galaxies, because they are evolving passively. However, while elliptical galaxies may be passively evolving when we observe them, they have usually had violent interactions with other galaxies in their past. In contrast, S0 galaxies are either aging and Credit: ESA/Hubble and NASA fading spiral galaxies, which never had any interactions with other galaxies, or they are the aging result of a single merger between two spiral galaxies in the past. The exact nature of these This new NASA/ESA Hubble Space Telescope galaxies is still a matter of debate. image shows the galaxy IC 335 in front of a backdrop of distant galaxies. IC 335 is part of a galaxy group containing three other galaxies, and Provided by NASA located in the Fornax Galaxy Cluster 60 million light-years away. As seen in this image, the disk of IC 335 appears edge-on from the vantage point of Earth. This makes it harder for astronomers to classify it, as most of the characteristics of a galaxy's morphology—the arms of a spiral or the bar across the center—are only visible on its face. -
Mar / Apr 2017 1
Let’s see, does HGO’s roof roll off to the left or the right? If I didn’t know it would be difficult to tell! Even Stuart conceded the snow was too deep for observatory 2 Event Calendar—Main Events access. 3 SVAS Guest Speaker Schedule 4 Getting Acquainted with the SVAS Candidates 8 Seven Earth-Size Planets Around single Star! NASA I really enjoy beautiful winter scenes, and with HGO 10 Hubble Sees the Beautiful Galaxy IC335 and RJMO as the center piece, it couldn’t get any better! 11 SVAS ATM Connection 13 Solar Eclipse Provides Coronal Glimpse, Space Place 15 SVAS Main Events Looking forward to some great spring observing, 16 Classifieds 17 SVAS Officers, Board, Members , Application Observer Editor Mar / Apr 2017 1 March 17, Fri, SVAS Annual Election Meeting, 8:00pm. Sacramento City College, Mohr Hall Room 3, 3835 Freeport Boulevard, Sacramento, CA. There will be no speaker this month. March 25, Sat Blue Canyon, weather permitting. March 27, Monday New Moon. April 21 , Fri, SVAS General Meeting, 8:00pm. Sacramento City College, Mohr Hall Room 3, 3835 Freeport Boulevard, Sacramento, CA. April 22 & 29, Sat , Blue Canyon, weather permitting. Yes two dates this month! Let’s hope the snow clears. April 25, Tuesday New Moon. Mar 25 Apr 22 & 29 May 27 Jun 24 July 21-23 Star B Q Aug 19 Sept 16 & 23 Oct 21 Nov 18 Dec 16 Contact Wayne Lord Mar / Apr 2017 2 April 21, 2017, Bill Goff will discuss some of the types of variables, why amateur observations are important, opportu- nities for pro/am collaboration and some exciting recent develop- ments. -
Binocular Challenges
This page intentionally left blank Cosmic Challenge Listing more than 500 sky targets, both near and far, in 187 challenges, this observing guide will test novice astronomers and advanced veterans alike. Its unique mix of Solar System and deep-sky targets will have observers hunting for the Apollo lunar landing sites, searching for satellites orbiting the outermost planets, and exploring hundreds of star clusters, nebulae, distant galaxies, and quasars. Each target object is accompanied by a rating indicating how difficult the object is to find, an in-depth visual description, an illustration showing how the object realistically looks, and a detailed finder chart to help you find each challenge quickly and effectively. The guide introduces objects often overlooked in other observing guides and features targets visible in a variety of conditions, from the inner city to the dark countryside. Challenges are provided for viewing by the naked eye, through binoculars, to the largest backyard telescopes. Philip S. Harrington is the author of eight previous books for the amateur astronomer, including Touring the Universe through Binoculars, Star Ware, and Star Watch. He is also a contributing editor for Astronomy magazine, where he has authored the magazine’s monthly “Binocular Universe” column and “Phil Harrington’s Challenge Objects,” a quarterly online column on Astronomy.com. He is an Adjunct Professor at Dowling College and Suffolk County Community College, New York, where he teaches courses in stellar and planetary astronomy. Cosmic Challenge The Ultimate Observing List for Amateurs PHILIP S. HARRINGTON CAMBRIDGE UNIVERSITY PRESS Cambridge, New York, Melbourne, Madrid, Cape Town, Singapore, Sao˜ Paulo, Delhi, Dubai, Tokyo, Mexico City Cambridge University Press The Edinburgh Building, Cambridge CB2 8RU, UK Published in the United States of America by Cambridge University Press, New York www.cambridge.org Information on this title: www.cambridge.org/9780521899369 C P. -
A Galaxy Classification Grid That Better Recognises Early-Type Galaxy
MNRAS 000,1– ?? (2019) Preprint 24 July 2019 Compiled using MNRAS LATEX style file v3.0 A galaxy classification grid that better recognises early-type galaxy morphology Alister W. Graham? Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122, Australia. Accepted 2019 June 7. Received 2019 June 7; in original form 2019 April 26 ABSTRACT A modified galaxy classification scheme for local galaxies is presented. It builds upon the Aitken-Jeans nebula sequence, by expanding the Jeans-Hubble tuning fork diagram, which it- self contained key ingredients from Curtis and Reynolds. The two-dimensional grid of galaxy morphological types presented here, with elements from de Vaucouleurs’ three-dimensional classification volume, has an increased emphasis on the often overlooked bars and continua of disc sizes in early-type galaxies — features not fully captured by past tuning forks, tridents, or combs. The grid encompasses nuclear discs in elliptical (E) galaxies, intermediate-scale discs in ellicular (ES) galaxies, and large-scale discs in lenticular (S0) galaxies, while the E4-E7 class is made redundant given that these galaxies are lenticular galaxies. Today, these struc- tures continue to be neglected, or surprise researchers, perhaps partly due to our indoctrination to galaxy morphology through the tuning fork diagram. To better understand the current and proposed classification schemes — whose origins reside in solar/planetary formation models — a holistic overview is given. This provides due credit to some of the lesser known pioneers, presents some rationale for the grid, and reveals the incremental nature of, and some of the lesser known connections in, the field of galaxy morphology.