Light Pollution in the Pfalz an International Problem!

Size: px
Start display at page:

Download "Light Pollution in the Pfalz an International Problem!"

Transcription

1 Light Pollution in the Pfalz an International Problem! The Nature Park Pfälzer Wald and the French/German UNESCO biosphere reserve Pfälzer Wald /Vosges du Nord are a relatively dark region in the Southwest of Germany, though densely populated and therefore bright areas are close by. A group of 6 students (Stefan Altschuck, Fabian Friedelt, Alexander Gust, Katja Hoffmeister, Nico Lörsch and Marcel Schäfer) of landscape planning at the Technical University Kaiserslautern (Prof. Dr. K. Tobias) studied during the summer semester 2015 possible dark places in the UNESCO biosphere reserve and took there measurements of the sky brightness. Together with more students an excursion into the Pfälzer Wald was planned in the night July 16/17.

2 Meeting and departure in Kaiserslautern Burgruine Lindelbrunn First station was the castle Lindelbrunn (alt. 438 m) near Vorderweidenthal. Twilight was not yet ended, but the light domes were clearly visible.

3 Allsky picture taken at Burgruine Lindelbrunn, exp. time 30s, 1:2.8, 800 ISO This allsky picture has been transformed to horizontal coordinates with the interpretation of the light domes given under the picture. And a comparison with VIIRS data from December 2014.

4 Very prominent in the South is the light dome of Strasbourg ( inh.) at a distance of about 65 km. The more reddened color indicates a farther away light dome. The light domes of Karlsruhe and the Rhein-Neckar-Region (Ludwigshafen, Mannheim and Heidelberg) with much more inhabitants and nearer (see list) are less prominent, indicating that Strasbourg is much brighter illuminated.

5 Distance Inhabitants Frankfurt/Mainz km 1,5 Mio. Ludwigshafen/Mannheim/Heidelberg 56 km 1,2 Mio. Karlsruhe 40 km Strasbourg 65 km Pirmasens 22 km Ramstein 40 km Kaiserslautern 35 km Fisheye pictures taken towards the South and towards the North The horizon towards the North is still bright due to the twilight. But a bright light source of whiter color is visible at the horizon. Later during the night the sky was covered but from a viewpoint about 13 km further to the North (Luitpoldsturm, alt. 607 m) the bright light source could be separated in individual beams. Light source in the North (Ramstein) from Burgruine Lindelbrunn and Luitpoldturm Luitpoldturm/Hermersbergerhof The night before (July 15/16) the sky was clear near the P south of Hermersbergerhof but due to the limited horizon view, light domes are less conspicuous. However the domes of Strasbourg in the South, of the Rhein-Neckar area in the East and Ramstein in the North can be recognized.

6 Allsky picture taken at the parking south of Hermersbergerhof (m= 21.2 mag/arcsec²) Generally the region of the Pfälzerwald in the foreground appears dark, while the background sky is illuminated. Many of the villages have changed the lighting to full cut-off 4000 K LED lighting. The brightness levels are however very different!

7 LED street lighting in Bundenthal (left) is about 3-4 times brighter than in Vorderweidenthal

8 The bright light in the North is the lighting of Ramstein Airbase which is also the brightest point on the DMSP and VIIRS pictures. It is due to indirect lighting from flood lighting towards a reflector with the light beam larger than the reflector. This is an unnecessary waste of energy and could be easily avoided, by applying one of these simple measures: Switch-off of the outer flood lamps Shielding the outer lamps that the light is only directed towards the reflector Decreasing the distance between luminaires and the reflector that less or no light will pass by the reflector Increasing the area of the reflector Is the illumination of the church in Fischbach, the biosphere house and the house of sustainable development at Johanniskreuz during all the night sustainable? Nike-Stellung/Braunsberg The potential observing platform Nike-Stellung is mainly dominated by the lights from Pirmasens. A. Hänel, 7/2015

Sustainable outdoor lighting for reducing energy and light waste

Sustainable outdoor lighting for reducing energy and light waste Sustainable outdoor lighting for reducing energy and light waste IEECB16, Frankfurt 16-18 March 2016 Andreas Hänel, Planetarium, Museum am Schölerberg, Osnabrück, Germany Lambros Doulos, National Technical

More information

The Effect of a Small Nearby Village (Großmugl) on Night Sky Brightness

The Effect of a Small Nearby Village (Großmugl) on Night Sky Brightness Sky Brightness Measurements with a Digital Camera: The Effect of a Small Nearby Village (Großmugl) on Night Sky Brightness Georg Zotti Wiener Arbeitsgemeinschaft für Astronomie & Österreichischer Astronomischer

More information

Stars and Galaxies Phys1403 Lab - Constellations

Stars and Galaxies Phys1403 Lab - Constellations Stars and Galaxies Phys1403 Lab - Constellations Instructions: You can work in a group of 2 or 3 students. Part 1: Using the Charts in the Planetarium Table 1 has a list of constellations showing its stick

More information

Planetarium Based Laboratory Activity Constellations

Planetarium Based Laboratory Activity Constellations Planetarium Based Laboratory Activity Constellations Instructions: You can work in a group of 2 or 3 students. Part 1: Using the Charts in the Planetarium Table 1 has a list of constellations showing its

More information

News from Germany: LED street lighting comparison SQM and SQM-L

News from Germany: LED street lighting comparison SQM and SQM-L News from Germany: LED street lighting comparison SQM and SQM-L Wien, 23rd August 2008 Fachgruppe DARK SKY der Vereinigung der Sternfreunde Andreas Hänel Planetarium, Museum am Schölerberg, Osnabrück LED

More information

UNIVERSITY OF HONG KONG

UNIVERSITY OF HONG KONG LIGHT POLLUTION UNIVERSITY OF HONG KONG The function of all outdoor lighting is to enhance the visibility or the aesthetics in the night-time environment. The light should go to where it is needed. If

More information

Identification and verification of Dark Sky Parks in Germany

Identification and verification of Dark Sky Parks in Germany Identification and verification of Dark Sky Parks in Germany Dark-Sky Parks Symposium Montsec June 2011 Working Group DARK SKY der Vereinigung der Sternfreunde Andreas Hänel Planetarium, Museum am Schölerberg,

More information

Dark Sky Parks in Germany

Dark Sky Parks in Germany Dark Sky Parks in Germany 11th European Symposium for the Protection of the Night Sky Working Group DARK SKY der Vereinigung der Sternfreunde Andreas Hänel Planetarium, Museum am Schölerberg, Osnabrück

More information

Night Skies and Photic Environment Resource Summary Bandelier National Monument

Night Skies and Photic Environment Resource Summary Bandelier National Monument Night Skies and Photic Environment Resource Summary Bandelier National Monument National Park Service U.S. Department of the Interior Natural Resource Stewardship and Science Natural Sounds & Night Skies

More information

Demonstrating Light Pollution and Shielding

Demonstrating Light Pollution and Shielding Demonstrating Light Pollution and Shielding This demonstration will illustrate the effects of lighting on our view of the night sky and how shielding can reduce light pollution while at the same time making

More information

2.2 The Reason for Seasons

2.2 The Reason for Seasons 2.2 The Reason for Seasons Our goals for learning: What causes the seasons? How does the orientation of Earth's axis change with time? Thought Question TRUE OR FALSE? Earth is closer to the Sun in summer

More information

11th European Symposium for the Protection of the Night Sky. Kolláth Zoltán

11th European Symposium for the Protection of the Night Sky. Kolláth Zoltán 11th European Symposium for the Protection of the Night Sky Kolláth Zoltán Update Hungarian parks Dark Sky Parks in Hungary IDSPs recognized by IDA: 2009: (Nominated in Armagh, 2009) Zselic Starry sky

More information

Transcontinental Australia Dark Sky Quality Survey

Transcontinental Australia Dark Sky Quality Survey Transcontinental Australia Dark Sky Quality Survey ALAN 2016 4 TH INTERNATIONAL CONFERENCE ON ARTIFICIAL LIGHT AT NIGHT SEPTEMBER 26-28, 2016 CLUJ-NAPOCA, ROMANIA Kellie Pendoley PhD Ellen Boylen Robert

More information

Dark Skies Outreach to Sub-Saharan Africa Program

Dark Skies Outreach to Sub-Saharan Africa Program (This lesson was adapted from an activity by the International Dark-Sky Association: www.darksky.org.) Grades: 5 th 12 th grade Overview: Students each build a Magnitude Reader. They use the reader to

More information

The Sun s center is much hotter than the surface. The Sun looks large and bright in the sky. Other stars look much smaller.

The Sun s center is much hotter than the surface. The Sun looks large and bright in the sky. Other stars look much smaller. The Sun A star is a huge ball of hot, glowing gases. The Sun is a star. The width of the Sun is equal to the width of 100 Earths placed side by side. The Sun is extremely hot. The surface of the Sun has

More information

The Moon Project: Moon Rise and Set

The Moon Project: Moon Rise and Set The Project: Rise and Set The Project: Rise and Set The by Mary Barrett The is really just one size The light grows larger every day It always stays the same, Exactly as it ought'er, But here on Earth

More information

Teacher Activity Packet: Observation Guide

Teacher Activity Packet: Observation Guide Teacher Activity Packet: Observation Guide Encourage your students to participate in a world-wide citizen science campaign to observe and record the magnitude of visible stars as a means of measuring light

More information

Constellations In ancient times, constellations only referred to the brightest stars that appeared to form groups, representing mythological figures.

Constellations In ancient times, constellations only referred to the brightest stars that appeared to form groups, representing mythological figures. Chapter 2: The Sky Constellations In ancient times, constellations only referred to the brightest stars that appeared to form groups, representing mythological figures. Constellations Today, constellations

More information

Using a Quantitative Measure to Achieve a Qualitative Lighting Design Effect! Introduction What is Luminance?

Using a Quantitative Measure to Achieve a Qualitative Lighting Design Effect! Introduction What is Luminance? Using a Quantitative Measure to Achieve a Qualitative Lighting Design Effect! Introduction What is Luminance? Luminance in a simple language is the measurement unit of brightness. In realty brightness

More information

Exploring The Planets: Jupiter

Exploring The Planets: Jupiter Exploring The Planets: Jupiter By Encyclopaedia Britannica, adapted by Newsela staff on 08.28.17 Word Count 691 Level 800L New Horizons spacecraft took this collection of images of Jupiter and Io in 2007.

More information

Performance and Results from the Globe at Night Sky Brightness Monitoring Network

Performance and Results from the Globe at Night Sky Brightness Monitoring Network Performance and Results from the Globe at Night Sky Brightness Monitoring Network Dr Chu-wing SO, The University of Hong Kong Dr Chun Shing Jason PUN, The University of Hong Kong Sze-leung CHEUNG, IAU

More information

Name: Earth and Space Assessment Study Guide. Assessment Date : Term Rotation Revolution

Name: Earth and Space Assessment Study Guide. Assessment Date : Term Rotation Revolution Name: Earth and Space Assessment Study Guide Assessment Date : Earth s Rotation and Revolution Term Rotation Revolution Brief Definition Earth s Time to Complete One complete spin on an axis 24 hours (or

More information

UNIVERSITY OF HAWAI I SYSTEM TESTIMONY

UNIVERSITY OF HAWAI I SYSTEM TESTIMONY UNIVERSITY OF HAWAI I SYSTEM TESTIMONY HB 1835: RELATING TO THE DEPARTMENT OF TRANSPORTATION Testimony Presented Before the House Committee on Transportation February 15, 2006 by Richard J. Wainscoat,

More information

Which graph best shows the relationship between intensity of insolation and position on the Earth's surface? A) B) C) D)

Which graph best shows the relationship between intensity of insolation and position on the Earth's surface? A) B) C) D) 1. The hottest climates on Earth are located near the Equator because this region A) is usually closest to the Sun B) reflects the greatest amount of insolation C) receives the most hours of daylight D)

More information

Ricardo Moreno, Rosa M Ros,

Ricardo Moreno, Rosa M Ros, Preparation of one astronomical observation Ricardo Moreno, Rosa M Ros, Beatriz García, Francis Berthomieu International Astronomical Union Colegio Retamar de Madrid, España Universidad Politécnica de

More information

Efficiency Works. February 6, Night Sky Initiative

Efficiency Works. February 6, Night Sky Initiative Efficiency Works February 6, 2018 Night Sky Initiative 1 Purpose Nature in the City Objective CP2: Work cross-departmentally and with external partners toward a darker night sky. Night Sky Initiative Goals:

More information

5. A particular star has an angle of parallax of 0.2 arcsecond. What is the distance to this star? A) 50 pc B) 2 pc C) 5 pc D) 0.

5. A particular star has an angle of parallax of 0.2 arcsecond. What is the distance to this star? A) 50 pc B) 2 pc C) 5 pc D) 0. Name: Date: 1. How far away is the nearest star beyond the Sun, in parsecs? A) between 1 and 2 pc B) about 12 pc C) about 4 pc D) between 1/2 and 1 pc 2. Parallax of a nearby star is used to estimate its

More information

8.9 Observing Celestial Objects from Earth

8.9 Observing Celestial Objects from Earth 8.9 Observing Celestial Objects from Earth Celestial objects are visible from Earth both by day and by night. In the daytime you can see the Sun and, sometimes, the Moon. Looking up at the night sky on

More information

[04] Seasons, Phases, and Eclipses (9/7/17)

[04] Seasons, Phases, and Eclipses (9/7/17) 1 [04] Seasons, Phases, and Eclipses (9/7/17) Upcoming Items Homework #2 due next lecture. Read Ch. 3.3 and do the self-study quizzes for next lecture, and skim 2.4, 3.1, 3.2, & 3.4. https://pbs.twimg.com/media/dh69il_u0aenivq.jpg:large

More information

Teacher Activity Packet: Observation Guide Campaign Dates that use Leo: March and April 11 20

Teacher Activity Packet: Observation Guide Campaign Dates that use Leo: March and April 11 20 Teacher Activity Packet: Observation Guide Encourage your students to participate in a worldwide citizen science campaign to observe and record the magnitude of visible stars as a means of measuring light

More information

ì<(sk$m)=cdfdhh< +^-Ä-U-Ä-U

ì<(sk$m)=cdfdhh< +^-Ä-U-Ä-U Standards Preview Earth Sciences Standard Set 4. Earth Sciences 4. Objects in the sky move in regular and predictable patterns. As a basis for understanding this concept: 4.a. Students know the patterns

More information

Stars and Planets GPS S4E1 A-D: Students will compare and contrast the physical attributes of stars, star patterns, and planets. Ms.

Stars and Planets GPS S4E1 A-D: Students will compare and contrast the physical attributes of stars, star patterns, and planets. Ms. Stars and Planets GPS S4E1 A-D: Students will compare and contrast the physical attributes of stars, star patterns, and planets. Ms. D AngeloD Physical Attributes of Stars Number Size Color Pattern A star

More information

About Light Pollution

About Light Pollution About Light Pollution Rappahannock Astronomy Club Presented by Scott Busby Member, Rappahannock Astronomy Club Presentation Agenda Introduction to Light Pollution How many Stars Can You See? Our Atmosphere

More information

Environmental Teaching Methods Natural Resources 310

Environmental Teaching Methods Natural Resources 310 Page 1 Student I.D. #11201571 Environmental Teaching Methods Natural Resources 310 Assignment 2 Writing an Environmental Education Unit Plan August 7, 2002 Page 2 NRES 310 Assignment 2: Writing an Environmental

More information

Tourism and Dark-Sky Places in Europe

Tourism and Dark-Sky Places in Europe Tourism and Dark-Sky Places in Europe Dark-Sky Parks Symposium Lastovo September 2010 Working Group DARK SKY der Vereinigung der Sternfreunde Andreas Hänel Planetarium, Museum am Schölerberg, Osnabrück

More information

The Hertzsprung-Russell Diagram and Stellar Evolution

The Hertzsprung-Russell Diagram and Stellar Evolution The Hertzsprung-Russell Diagram and Stellar Evolution Names: The H-R Diagram and Stellar Properties Activity 1. In which corner of the diagram (upper right, upper left, lower right, or lower left) would

More information

Star Gazing. Part 1. Name: What do you know about stars? Is the Sun a star? Why do we only see some stars at night?

Star Gazing. Part 1. Name: What do you know about stars? Is the Sun a star? Why do we only see some stars at night? Star Gazing Name: Part 1 What do you know about stars? Is the Sun a star? Why do we only see some stars at night? Castor Betelgeuse Rigel Pollux Procyon Sirius The picture above shows the stars as seen

More information

LIGHT POLLUTION MEASUREMENT: A PROJECT WORK FOR SECONDARY SCHOOL STUDENTS

LIGHT POLLUTION MEASUREMENT: A PROJECT WORK FOR SECONDARY SCHOOL STUDENTS Light pollution measurement: a project work for secondary school students LIGHT POLLUTION MEASUREMENT: A PROJECT WORK FOR SECONDARY SCHOOL STUDENTS I. Döményné Ságodi 1, A. Dömény 2 1 Garay János Grammar

More information

German data sets for comparing ambulance location models

German data sets for comparing ambulance location models German data sets for comparing ambulance location models Melanie Reuter-Oppermann a, Christiane Bernath a a Karlsruhe Service Research Institute (KSRI), Karlsruhe Institute of Technology, Germany Abstract

More information

Constellations and Asterisms

Constellations and Asterisms Constellations and Asterisms Constellations When ancient people looked at the sky they saw patterns and gave names to apparent groups of stars. Constellation patterns have been found on tablets over 4000

More information

Blackbody Radiation OBJECTIVES

Blackbody Radiation OBJECTIVES Name Class Date Skills Practice Lab Blackbody Radiation A perfect absorber of radiation also happens to be a perfect radiator of that radiation as well. Such objects are called blackbodies, because darker

More information

STAR PROPERTIES. How Many Stars in Leo? How Many Stars in Orion? How Many Stars in Ursa Major? How Many Stars in Gemini? 4/30/15.

STAR PROPERTIES. How Many Stars in Leo? How Many Stars in Orion? How Many Stars in Ursa Major? How Many Stars in Gemini? 4/30/15. 4/30/15 Contela7ons STAR PROPERTIES How Many Stars in Orion? 25 8 100 >1,000,000 50 21 100 >1,000,000 Scorpius Canis Minor Canis Major Leo How Many Stars in Leo? 25 16 100 >1,000,000 How Many Stars in

More information

Effective August 2007 All indicators in Standard / 14

Effective August 2007 All indicators in Standard / 14 8-4.1 Summarize the characteristics and movements of objects in the solar system (including planets, moons, asteroids, comets, and meteors). Taxonomy level: 2.4-B Understand Conceptual Knowledge Previous/Future

More information

CHAPTER 2 Strand 1: Structure and Motion within the Solar System

CHAPTER 2 Strand 1: Structure and Motion within the Solar System CHAPTER 2 Strand 1: Structure and Motion within the Solar System Chapter Outline 2.1 EARTH, MOON, AND SUN SYSTEM (6.1.1) 2.2 GRAVITY AND INERTIA (6.1.2) 2.3 SCALE OF SOLAR SYSTEM (6.1.3) 2.4 REFERENCES

More information

Community Survey. 1 of What type of street lighting do you prefer? Response Percent. Response Count

Community Survey. 1 of What type of street lighting do you prefer? Response Percent. Response Count Community Survey 1. What type of street lighting do you prefer? Percent LED (between Rowland Boulevard and Adele Drive) 60.0% 54 Induction (between Arthur Drive and Yukon Way) 45.6% 41 answered question

More information

Key Concepts Solar System, Movements, Shadows Recall that Earth is one of many planets in the solar system that orbit the Sun.

Key Concepts Solar System, Movements, Shadows Recall that Earth is one of many planets in the solar system that orbit the Sun. Key Concepts Solar System, Movements, Shadows 4-3.1 Recall that Earth is one of many planets in the solar system that orbit the Sun. It is essential for students to know that Earth is a planet that orbits

More information

Exercise 1: Earth s Moon

Exercise 1: Earth s Moon PHYS1014 Physical Science Summer 2013 Professor Kenny L. Tapp Exercise 1: Earth s Moon Complete and submit this packet, securely stapled, at the beginning of Exam 1. PART I --- Online Video Lecture from

More information

MiSP Astronomy Seasons Worksheet #1 L1

MiSP Astronomy Seasons Worksheet #1 L1 MiSP Astronomy Seasons Worksheet #1 L1 Name Date CHANGING HOURS OF DAYLIGHT ON LONG ISLAND Introduction You sometimes hear people say, Days are longer in the summer and shorter in the winter. That is a

More information

MiSP Astronomy - Seasons Worksheet #1 L2

MiSP Astronomy - Seasons Worksheet #1 L2 MiSP Astronomy - Seasons Worksheet #1 L2 Name Date Changing Hours of Daylight on Long Island (L 1, 2, 3) Introduction You sometimes hear people say, Days are longer in the summer and shorter in the winter.

More information

Earth, Sun, and Stars

Earth, Sun, and Stars Earth, Sun, and Stars Daily Patterns Earth Spins Earth is always moving, even though you don t feel it. One way Earth moves is by spinning around an imaginary line. One end of the line would come out of

More information

Influence of moon light on tip-tilt sensing accuracy using STRAP

Influence of moon light on tip-tilt sensing accuracy using STRAP Keck Adaptive Optics Note 425 Influence of moon light on tip-tilt sensing accuracy using STRAP Stephan Kellner, David Le Mignant and Marcos van Dam Version 1.0: 2 October 2006 Abstract AO observations

More information

The full, blue supermoon is coming to the night sky near you

The full, blue supermoon is coming to the night sky near you The full, blue supermoon is coming to the night sky near you By Shannon Schmoll, The Conversation, adapted by Newsela staff on 01.30.18 Word Count 872 Level 980L Image 1. A picture of the moon. It shows

More information

Page Eclipses INTERACTIVE. Lunar phases

Page Eclipses INTERACTIVE. Lunar phases Page 30 1.4 Eclipses INTERACTIVE Lunar phases An eclipse occurs when the Moon happens to lie exactly between the Earth and the Sun, or when the Earth lies exactly between the Sun and the Moon, so that

More information

Patterns on Earth 4.8C

Patterns on Earth 4.8C Have you ever made shadow puppets? If you put your hand between a flashlight and a wall, you will make a shadow. You might have made a rabbit shape or some other animal shape with your hands. Your hand

More information

Lecture 8. October 25, 2017 Lab 5

Lecture 8. October 25, 2017 Lab 5 Lecture 8 October 25, 2017 Lab 5 News Lab 2 & 3 Handed back next week (I hope). Lab 4 Due today Lab 5 (Transiting Exoplanets) Handed out and observing will start Friday. Due November 8 (or later) Stellar

More information

INSPIRATION FROM NATURE

INSPIRATION FROM NATURE INSPIRATION FROM NATURE STORK LITTLE BROTHER Dimmension drawings 137 650 280 2 Main technical data Voltage, V Frequency, Hz Nominal current, ma Power, W Total luminous Flux, Lm Efficiency, Lm/W Power factor,

More information

The control of light pollution in Italy

The control of light pollution in Italy The control of light pollution in Italy Fabio Falchi CieloBuio - Coordinamento per la protezione del cielo notturno www.cielobuio.org ISTIL Istituto di Scienza e Tecnologia dell Inquinamento Luminoso www.istil.eu

More information

Objectives. Duration: one week

Objectives. Duration: one week Objectives At the conclusion of the lesson, students will be able to: 1. Analyze data to describe the motion of the sun including equinox and solstice paths in the sky for an Ancient Culture 2. Use alt-azimuth

More information

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Pearson Education, Inc.

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Pearson Education, Inc. Chapter 2 Lecture The Cosmic Perspective Seventh Edition Discovering the Universe for Yourself Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the

More information

Introduction to Astronomy Laboratory Exercise #1. Intro to the Sky

Introduction to Astronomy Laboratory Exercise #1. Intro to the Sky Introduction to Astronomy Laboratory Exercise #1 Partners Intro to the Sky Date Section Purpose: To develop familiarity with the daytime and nighttime sky through the use of Stellarium. Equipment: Computer

More information

PHYS 160 Astronomy Test #1 Fall 2017 Version B

PHYS 160 Astronomy Test #1 Fall 2017 Version B PHYS 160 Astronomy Test #1 Fall 2017 Version B 1 I. True/False (1 point each) Circle the T if the statement is true, or F if the statement is false on your answer sheet. 1. An object has the same weight,

More information

Agenda. LAB (Inst. Dickinson): Lab Constellation/Star Quiz Angular Measurement Lab

Agenda. LAB (Inst. Dickinson): Lab Constellation/Star Quiz Angular Measurement Lab LAB (Inst. Dickinson): Lab Constellation/Star Quiz Angular Measurement Lab Agenda LECTURE (Prof. Canales): Discuss Formal Lab Report on FOV- Due Tues 2/15 LAB PREP: Unit Conversion Review Dec. & RA and

More information

1.5 Quarter Assessment Study Guide. 1. What branch of earth science deals with studying the objects in space?

1.5 Quarter Assessment Study Guide. 1. What branch of earth science deals with studying the objects in space? Name: # Study Guide is due WEDNESDAY November 2 nd 1.5 Quarter Assessment Test is FRIDAY Nov. 4 th 1.5 Quarter Assessment Study Guide 1. What branch of earth science deals with studying the objects in

More information

Astronomy 1 Introductory Astronomy Spring 2014

Astronomy 1 Introductory Astronomy Spring 2014 Astronomy 1 Introductory Astronomy Spring 2014 Lab 5: Observing the Sky pt. 2 Quick overview Meet at 8 p.m. in Science Center Room 187. We will go up to the roof from there, and make several different

More information

5-ESS1-1 Earth's Place in the Universe

5-ESS1-1 Earth's Place in the Universe 5-ESS1-1 Earth's Place in the Universe 5-ESS1-1. Support an argument that the apparent brightness of the sun and stars is due to their relative distances from the Earth. [Assessment Boundary: Assessment

More information

Why Don t We See Stars in the Daytime?

Why Don t We See Stars in the Daytime? Why Don t We See Stars in the Daytime? Photo Credit: ESA Hubble NASA At night, we see many stars in the sky. Those stars are made of burning gases. They are hot, and they shine. But stars are in the sky

More information

Equatorial Telescope Mounting

Equatorial Telescope Mounting Equatorial Telescope Mounting Star Catalogs simbad IRSA The Meridian Every line of celestial longitude is a meridian of longitude, but we recognize the line of longitude, or simply the great circle line,

More information

LIGHT POLLUTION IN LAZIO A measure by high-school students

LIGHT POLLUTION IN LAZIO A measure by high-school students LIGHT POLLUTION IN LAZIO A measure by high-school students Roberto Nesci Department of Physics, University La Sapienza, P.le Aldo Moro 2, 00185, Roma, Italy roberto.nesci@uniroma1.it Keywords: Abstract:

More information

The sun then falls below the horizon, and it is nighttime for our little person:

The sun then falls below the horizon, and it is nighttime for our little person: Venus Update! Problem 6 on Homework 1 in Physics 2A last September asked you to find the distance from Earth to Venus at that time. I gave you the angle between the sun and Venus at that time; you drew

More information

Steps: A Windows to the Universe Citizen Science Event. October 1-15, 2007

Steps: A Windows to the Universe Citizen Science Event.  October 1-15, 2007 Steps: WHAT do I need? Pen or pencil Red-light or night-vision flashlight GPS unit, access to the Internet or topographic map Printed Activity Guide with report form HOW do I make a nightvision flashlight?

More information

LIGHT POLLUTION, AN INTRODUTION TO ASTRONOMY/ENVIRONMENTAL EDUCATION

LIGHT POLLUTION, AN INTRODUTION TO ASTRONOMY/ENVIRONMENTAL EDUCATION LIGHT POLLUTION, AN INTRODUTION TO ASTRONOMY/ENVIRONMENTAL EDUCATION Dr.M.Metaxa IDA Education Outreach Working Group IAU Com.50 wg m-metaxa@otenet.gr Abstract The problem of Light Pollution exists most

More information

L ight color influence on obstacle recognition in road lighting. 1. Introduction

L ight color influence on obstacle recognition in road lighting. 1. Introduction Computer Applications in Electrical Engineering L ight color influence on obstacle recognition in road lighting Małgorzata Górczewska, Sandra Mroczkowska, Przemysław Skrzypczak Poznań University of Technology

More information

Astronomy 4 Test #2 PRACTICE VERSION

Astronomy 4 Test #2 PRACTICE VERSION Given (a.k.a. `First ) Name(s): Family (a.k.a. `Last ) name: ON YOUR PARSCORE: Write your name, and `bubble your I.D. number, your test version, and your multiple-choice answers. I will keep the Parscore

More information

Sky, Celestial Sphere and Constellations

Sky, Celestial Sphere and Constellations Sky, Celestial Sphere and Constellations Last lecture Galaxies are the main building blocks of the universe. Consists of few billions to hundreds of billions of stars, gas clouds (nebulae), star clusters,

More information

The full, blue supermoon is coming to the night sky near you

The full, blue supermoon is coming to the night sky near you The full, blue supermoon is coming to the night sky near you By Shannon Schmoll, The Conversation, adapted by Newsela staff on 01.30.18 Word Count 872 Level 980L Image 1. A picture of the moon. It shows

More information

Dark Sky Observing Preview. BSA Troop 4 Pasadena, CA

Dark Sky Observing Preview. BSA Troop 4 Pasadena, CA Dark Sky Observing Preview BSA Troop 4 Pasadena, CA Topics Finding Dark sky Observing etiquette Observing basics Things to see Resources Finding Dark Sky To see faint objects, you want the darkest sky

More information

NSF-MARGINS Expedition to Anatahan Volcano March 2005

NSF-MARGINS Expedition to Anatahan Volcano March 2005 1 NSF-MARGINS Expedition to Anatahan Volcano March 2005 According to the Emergency Management Office (EMO) report distributed in February 2005, the third historical eruption of Anatahan began on January

More information

Seasons. What causes the seasons?

Seasons. What causes the seasons? Questions: Seasons What causes the seasons? How do we mark the progression of the seasons? What is the seasonal motion of the sun in the sky? What could cause the seasonal motion of the sun to change over

More information

Science Test Prep, Chapter 11

Science Test Prep, Chapter 11 Answers to Page 79 Science Test Prep, Chapter 11 1 The correct answer is A (the Sun). Florida Science GLE: SC.E.2.1.1.1.1 knows and differentiates objects seen in the day and night sky (for example, clouds,

More information

Test ABCDE. 1. What is the oldest era on the geological timescale? A. Precambrian B. Paleozoic C. Mesozoic D. Cenozoic

Test ABCDE. 1. What is the oldest era on the geological timescale? A. Precambrian B. Paleozoic C. Mesozoic D. Cenozoic Test - 8.8 ABCDE 1. What is the oldest era on the geological timescale? A. Precambrian B. Paleozoic C. Mesozoic D. Cenozoic 2. A light-year is defined as- F. the distance from Earth to the Sun. G. the

More information

COLOR MAGNITUDE DIAGRAMS

COLOR MAGNITUDE DIAGRAMS COLOR MAGNITUDE DIAGRAMS What will you learn in this Lab? This lab will introduce you to Color-Magnitude, or Hertzsprung-Russell, Diagrams: one of the most useful diagnostic tools developed in 20 th century

More information

Astronomy Club of Asheville November 2017 Sky Events

Astronomy Club of Asheville November 2017 Sky Events November 2017 Sky Events The Planets this Month page 2 Close Conjunction of Venus and Jupiter page 7 Conjunction of Crescent Moon, Saturn & Mercury page 8 Planet Highlights page 9 Moon Phases page 12 November

More information

What Objects Are Part of the Solar System?

What Objects Are Part of the Solar System? What Objects Are Part of the Solar System? Lesson 1 Quiz Josleen divided some of the planets into two main groups. The table below shows how she grouped them. Paul created a poster showing the solar system.

More information

STUDENT NAME. Science Grade 4. Read each question and choose the best answer. Be sure to mark all of your answers. Switch Lightbulb Battery

STUDENT NAME. Science Grade 4. Read each question and choose the best answer. Be sure to mark all of your answers. Switch Lightbulb Battery FORMATIVE MINI ASSESSMENTS Third Grading Period 2009-10 February 1-5 STUDENT NAME DATE Science Grade 4 Read each question and choose the best answer. Be sure to mark all of your answers. + Switch Lightbulb

More information

LESSON PLAN - Optimum Orientation of Solar Panels Using Soltrex Data

LESSON PLAN - Optimum Orientation of Solar Panels Using Soltrex Data LESSON PLAN - Optimum Orientation of Solar Panels Using Soltrex Data Title of Lesson: Optimum Orientation of Solar Panels Using Soltrex Data Description of class: High School physics, astronomy, or environmental

More information

Astronomy Club of Asheville January 2016 Sky Events

Astronomy Club of Asheville January 2016 Sky Events January 2016 Sky Events The Planets this Month - page 2 Planet Highlights - page 7 All 5 Naked-Eye Planets in the Dawn Sky - page 10 Moon Phases - page 11 Earth Reaches Perihelion on Jan. 4 - page 12 Quadrantid

More information

A blue flame is hotter than a yellow one.

A blue flame is hotter than a yellow one. CHAPTER 19 1 Stars SECTION Stars, Galaxies, and the Universe BEFORE YOU READ After you read this section, you should be able to answer these questions: Why are stars different colors? How can scientists

More information

INDEPENDENT PROJECT: The Summer Night Sky

INDEPENDENT PROJECT: The Summer Night Sky INDEPENDENT PROJECT: The Summer Night Sky What is the difference between observing and looking? As John Rummel said to the Madison Astronomical Society, January 11, 2002: Looking implies a passive exercise

More information

Name Date Per Teacher. Packet #4 The Sun

Name Date Per Teacher. Packet #4 The Sun Packet #4 The Sun Reading Guide: Chapter 29.1 (read text pages 755 760) STRUCTURE OF THE SUN 1e Students know the Sun is a typical star and is powered by nuclear reactions, primarily the fusion of hydrogen

More information

Total Eclipse of the Sun. 29th March Peter Meadows

Total Eclipse of the Sun. 29th March Peter Meadows Total Eclipse of the Sun 29th March 2006 Peter Meadows AWT Turkey Tour 1 1 Introduction "A total eclipse of the Sun is the most sublime and awe-inspiring of all celestial events. As the Moon's black disk

More information

PHYS 160 Astronomy Test #1 Name Answer Key Test Version A

PHYS 160 Astronomy Test #1 Name Answer Key Test Version A PHYS 160 Astronomy Test #1 Name Answer Key Test Version A True False Multiple Choice 1. T 1. C 2. F 2. B 3. T 3. A 4. T 4. E 5. T 5. B 6. F 6. A 7. F 7. A 8. T 8. D 9. F 9. D 10. F 10. B 11. B 12. D Definitions

More information

Practice Questions: Seasons #1

Practice Questions: Seasons #1 1. Seasonal changes on Earth are primarily caused by the A) parallelism of the Sun's axis as the Sun revolves around Earth B) changes in distance between Earth and the Sun C) elliptical shape of Earth's

More information

This work is partly supported by Grant-in-Aid for Scientific Research from the Japan Society for the Promotion of Science.

This work is partly supported by Grant-in-Aid for Scientific Research from the Japan Society for the Promotion of Science. Nobuaki OCHI Yonago National College of Technology, Japan IDA Education Committee and the GaN team This work is partly supported by Grant-in-Aid for Scientific Research from the Japan Society for the Promotion

More information

CHAPTER 2 A USER'S GUIDE TO THE SKY

CHAPTER 2 A USER'S GUIDE TO THE SKY CHAPTER 2 A USER'S GUIDE TO THE SKY MULTIPLE CHOICE 1. Seen from the northern latitudes (mid-northern hemisphere), the star Polaris a. is never above the horizon during the day. b. always sets directly

More information

Instruction Manual. Polar finder scope for BRESSER EXOS-I Mount

Instruction Manual. Polar finder scope for BRESSER EXOS-I Mount Instruction Manual Polar finder scope for BRESSER EXOS-I Mount Art.No. 49-64210 Scope of delivery: Polar finder scope with illuminated recticle Rubber ring Necessary tools (have to be purchased seperately):

More information

Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? Constellations. 2.1 Patterns in the Night Sky

Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? Constellations. 2.1 Patterns in the Night Sky Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we

More information

Night Sky Brightness Monitoring Network in Hong Kong

Night Sky Brightness Monitoring Network in Hong Kong 11th European Symposium for the Protection of the Night Sky Osnabrück, Germany Night Sky Brightness Monitoring Network in Hong Kong Dr Jason C. S. Pun, Mr Chu-wing SO, Mr Terry C. F. Wong Department of

More information

Astrochart Links: Pennsic 43: coming July 25

Astrochart Links: Pennsic 43: coming July 25 Astrochart Links: Pennsic 43: coming July 25 Here are the views of the sky each night of Pennsic XLIII, July & August 2014. Stars begin to come out half an hour after sunset, around 9 o'clock to half past,

More information

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we

More information

Heat Transfer. Energy from the Sun. Introduction

Heat Transfer. Energy from the Sun. Introduction Heat Transfer Energy from the Sun Introduction The sun rises in the east and sets in the west, but its exact path changes over the course of the year, which causes the seasons. In order to use the sun

More information