We Can Recognize Solstices and Equinoxes by Sun's Path Across Sky: If You Are Located in the Continental U.S. on the First
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Planet Positions: 1 Planet Positions
Planet Positions: 1 Planet Positions As the planets orbit the Sun, they move around the celestial sphere, staying close to the plane of the ecliptic. As seen from the Earth, the angle between the Sun and a planet -- called the elongation -- constantly changes. We can identify a few special configurations of the planets -- those positions where the elongation is particularly noteworthy. The inferior planets -- those which orbit closer INFERIOR PLANETS to the Sun than Earth does -- have configurations as shown: SC At both superior conjunction (SC) and inferior conjunction (IC), the planet is in line with the Earth and Sun and has an elongation of 0°. At greatest elongation, the planet reaches its IC maximum separation from the Sun, a value GEE GWE dependent on the size of the planet's orbit. At greatest eastern elongation (GEE), the planet lies east of the Sun and trails it across the sky, while at greatest western elongation (GWE), the planet lies west of the Sun, leading it across the sky. Best viewing for inferior planets is generally at greatest elongation, when the planet is as far from SUPERIOR PLANETS the Sun as it can get and thus in the darkest sky possible. C The superior planets -- those orbiting outside of Earth's orbit -- have configurations as shown: A planet at conjunction (C) is lined up with the Sun and has an elongation of 0°, while a planet at opposition (O) lies in the opposite direction from the Sun, at an elongation of 180°. EQ WQ Planets at quadrature have elongations of 90°. -
Sun Tool Options
Sun Study Tools Sophomore Architecture Studio: Lighting Lecture 1: • Introduction to Daylight (part 1) • Survey of the Color Spectrum • Making Light • Controlling Light Lecture 2: • Daylight (part 2) • Design Tools to study Solar Design • Architectural Applications Lecture 3: • Light in Architecture • Lighting Design Strategies Sun Tool Options 1. Paper and Pencil 2. Build a Model 3. Use a Computer The first step to any of these options is to define…. Where is the site? 1 2 Sun Study Tools North Latitude and Longitude South Longitude Latitude Longitude Sun Study Tools North America Latitude 3 United States e ud tit La Sun Study Tools New York 72w 44n 42n Site Location The site location is specified by a latitude l and a longitude L. Latitudes and longitudes may be found in any standard atlas or almanac. Chart shows the latitudes and longitudes of some North American cities. Conventions used in expressing latitudes are: Positive = northern hemisphere Negative = southern hemisphere Conventions used in expressing longitudes are: Positive = west of prime meridian (Greenwich, United Kingdom) Latitude and Longitude of Some North American Cities Negative = east of prime meridian 4 Sun Study Tools Solar Path Suns Position The position of the sun is specified by the solar altitude and solar azimuth and is a function of site latitude, solar time, and solar declination. 5 Sun Study Tools Suns Position The rotation of the earth about its axis, as well as its revolution about the sun, produces an apparent motion of the sun with respect to any point on the altitude earth's surface. The position of the sun with respect to such a point is expressed in terms of two angles: azimuth The sun's position in terms of solar altitude (a ) and azimuth (a ) solar azimuth, which is the t s with respect to the cardinal points of the compass. -
Equatorial and Cartesian Coordinates • Consider the Unit Sphere (“Unit”: I.E
Coordinate Transforms Equatorial and Cartesian Coordinates • Consider the unit sphere (“unit”: i.e. declination the distance from the center of the (δ) sphere to its surface is r = 1) • Then the equatorial coordinates Equator can be transformed into Cartesian coordinates: right ascension (α) – x = cos(α) cos(δ) – y = sin(α) cos(δ) z x – z = sin(δ) y • It can be much easier to use Cartesian coordinates for some manipulations of geometry in the sky Equatorial and Cartesian Coordinates • Consider the unit sphere (“unit”: i.e. the distance y x = Rcosα from the center of the y = Rsinα α R sphere to its surface is r = 1) x Right • Then the equatorial Ascension (α) coordinates can be transformed into Cartesian coordinates: declination (δ) – x = cos(α)cos(δ) z r = 1 – y = sin(α)cos(δ) δ R = rcosδ R – z = sin(δ) z = rsinδ Precession • Because the Earth is not a perfect sphere, it wobbles as it spins around its axis • This effect is known as precession • The equatorial coordinate system relies on the idea that the Earth rotates such that only Right Ascension, and not declination, is a time-dependent coordinate The effects of Precession • Currently, the star Polaris is the North Star (it lies roughly above the Earth’s North Pole at δ = 90oN) • But, over the course of about 26,000 years a variety of different points in the sky will truly be at δ = 90oN • The declination coordinate is time-dependent albeit on very long timescales • A precise astronomical coordinate system must account for this effect Equatorial coordinates and equinoxes • To account -
Sarah Provancher Jeanne Hilt (502) 439-7138 (502) 614-4122 [email protected] [email protected]
FOR IMMEDIATE RELEASE: Tuesday, June 5, 2018 CONTACT: Sarah Provancher Jeanne Hilt (502) 439-7138 (502) 614-4122 [email protected] [email protected] DOWNTOWN TO SHOWCASE FÊTE DE LA MUSIQUE LOUISVILLE ON JUNE 21 ST Downtown Louisville to celebrate the Summer Solstice with live music and more than 30 street performers for a day-long celebration of French culture Louisville, KY – A little taste of France is coming to Downtown Louisville on the summer solstice, Thursday, June 21st, with Fête de la Musique Louisville (pronounced fet de la myzic). The event, which means “celebration of music” in French, has been taking place in Paris on the summer solstice since 1982. Downtown Louisville’s “celebration of music” is presented by Alliance Francaise de Louisville in conjunction with the Louisville Downtown Partnership (LDP). Music will literally fill the downtown streets all day on the 21st with dozens of free live performances over the lunchtime hour and during a special Happy Hour showcase on the front steps of the Kentucky Center from 5:30-7:30pm. A list of performance venues with scheduled performers from 11am-1pm are: Fourth Street Live! – Classical musicians including The NouLou Chamber Players, 90.5 WUOL Young Musicians and Harin Oh, GFA Youth Guitar Summit Kindred Plaza – Hewn From The Mountain, a local Irish band 400 W. Market Plaza – FrenchAxe, a French band from Cincinnati Old Forester Distillery – A local jug band The salsa band Milenio is the scheduled performance group for the Happy Hour also at Fourth Street Live! from 5 – 7 pm. "In Paris and throughout France, the Fête de la Musique is literally 24 hours filled with music by all types of musicians of all skill levels. -
Regents and Midterm Prep Answers
Name__________________________________!Regents and Mid Term Preparation The Seasons Description Position Description Position March 21st B South Pole-24 Hrs of Dark C June 21st C High Kinetic Energy A December 21st A Low Kinetic Energy C September 23rd D Earth Close to Sun A Northern Hemisphere Winter A Earth Far from Sun C Northern Hemisphere Spring B Southern Hemisphere Spring D North Hemisphere Summer C Southern Hemisphere Fall B Northern Hemisphere Fall D Southern Hemisphere Winter C Greatest Orbital Velocity A South Hemisphere Summer A Least Orbital Velocity C 9 Hrs of Day in NYS A 23 1/2 N-Zenith C 12 Hrs of Day in NYS D,B 0 (Equator)-Zenith D,B 15 Hrs of Day in NYS C 23 1/2 S-Zenith A Winter Solstice A North Pole-24 Hrs Day C Vernal Equinox B South Pole-24 Hrs Day A Autumnal Equinox D North Pole-24 Hrs Dark A Summer Solstice C Name__________________________________!Regents and Mid Term Preparation Sunʼs Path in NYS 1. What direction does the sun rise in summer? _____NE___________________ 2. What direction does the sun rise in winter? _________SE_________________ 3. What direction does the sun rise in fall/spring? ________E_______________ 4. How long is the sun out in fall/spring? ____12________ 5. How long is the sun out in winter? _________9______ 6. How long is the sun out in summer? ________15_______ 7. What direction do you look to see the noon time sun? _____S________ 8. What direction do you look to see polaris? _______N_________ 9. From sunrise to noon, what happens to the length of a shadow? ___SMALLER___ 10. -
Summer Solstice
A FREE RESOURCE PACK FROM EDMENTUM Summer Solstice PreK–6th Topical Teaching Grade Range Resources Free school resources by Edmentum. This may be reproduced for class use. Summer Solstice Topical Teaching Resources What Does This Pack Include? This pack has been created by teachers, for teachers. In it you’ll find high quality teaching resources to help your students understand the background of Summer Solstice and why the days feel longer in the summer. To go directly to the content, simply click on the title in the index below: FACT SHEETS: Pre-K – Grade 3 Grades 3-6 Grades 3-6 Discover why the Sun rises earlier in the day Understand how Earth moves and how it Discover how other countries celebrate and sets later every night. revolves around the Sun. Summer Solstice. CRITICAL THINKING QUESTIONS: Pre-K – Grade 2 Grades 3-6 Discuss what shadows are and how you can create them. Discuss how Earth’s tilt cause the seasons to change. ACTIVITY SHEETS AND ANSWERS: Pre-K – Grade 3 Grades 3-6 Students are to work in pairs to explain what happens during Follow the directions to create a diagram that describes the Summer Solstice. Summer Solstice. POSTER: Pre-K – Grade 6 Enjoyed these resources? Learn more about how Edmentum can support your elementary students! Email us at www.edmentum.com or call us on 800.447.5286 Summer Solstice Fact Sheet • Have you ever noticed in the summer that the days feel longer? This is because there are more hours of daylight in the summer. • In the summer, the Sun rises earlier in the day and sets later every night. -
Chapter Outline Thinking Ahead 4 EARTH, MOON, AND
Chapter 4 Earth, Moon, and Sky 103 4 EARTH, MOON, AND SKY Figure 4.1 Southern Summer. As captured with a fish-eye lens aboard the Atlantis Space Shuttle on December 9, 1993, Earth hangs above the Hubble Space Telescope as it is repaired. The reddish continent is Australia, its size and shape distorted by the special lens. Because the seasons in the Southern Hemisphere are opposite those in the Northern Hemisphere, it is summer in Australia on this December day. (credit: modification of work by NASA) Chapter Outline 4.1 Earth and Sky 4.2 The Seasons 4.3 Keeping Time 4.4 The Calendar 4.5 Phases and Motions of the Moon 4.6 Ocean Tides and the Moon 4.7 Eclipses of the Sun and Moon Thinking Ahead If Earth’s orbit is nearly a perfect circle (as we saw in earlier chapters), why is it hotter in summer and colder in winter in many places around the globe? And why are the seasons in Australia or Peru the opposite of those in the United States or Europe? The story is told that Galileo, as he left the Hall of the Inquisition following his retraction of the doctrine that Earth rotates and revolves about the Sun, said under his breath, “But nevertheless it moves.” Historians are not sure whether the story is true, but certainly Galileo knew that Earth was in motion, whatever church authorities said. It is the motions of Earth that produce the seasons and give us our measures of time and date. The Moon’s motions around us provide the concept of the month and the cycle of lunar phases. -
How Does Solar Altitude, Diameter, and Day Length Change Daily and Throughout the Year?
How does solar altitude, diameter, and day length change daily and throughout the year? Let’s prove distance doesn’t matter in seasons by investigating SOLAR ALTITUDE, DAY LENGTH and SOLAR DISTANCE… Would the sun have the same appearance if you observed it from other planets? Why do we see the sun at different altitudes throughout the day? We use the altitude of the sun at a time called solar “noon” because of daily solar altitude changes from the horizon at sunrise and sunset to it’s maximum daily altitude at noon. If you think solar noon is at 12:00:00, you’re mistaken! Solar “noon” doesn’t usually happen at clock-noon at your longitude for lots of reasons! SOLAR INTENSITY and ALTITUDE - Maybe a FLASHLIGHT will help us see this relationship! Draw the beam shape for 3 solar altitudes in your notebooks! How would knowing solar altitude daily and seasonally help make solar panels (collectors)work best? Where would the sun have to be located to capture the maximum amount of sunlight energy? Draw the sun in the right position to maximize the light it receives on panel For the northern hemisphere, in which general direction would they be pointed? For the southern hemisphere, in which direction would they be pointed? SOLAR PANELS at different ANGLES ON GROUND How do shadows show us solar altitude? You used a FLASHLIGHT and MODELING CLAY to show you how SOLAR INTENSITY, ALTITUDE, and SHADOW LENGTH are related! Using at least three solar altitudes and locations, draw your conceptual model of this relationship in your notebooks… Label: Sun compass direction Shadow compass direction Solar altitude Shadow length (long/short) Sun intensity What did the lab show us about how SOLAR ALTITUDE, DIAMETER, & DAY LENGTH relate to each other? YOUR GRAPHS are PROBABLY the easiest way to SEE the RELATIONSHIPS. -
Earth-Moon-Sun-System EQUINOX Presentation V2.Pdf
The Sun http://c.tadst.com/gfx/750x500/sunrise.jpg?1 The sun dominates activity on Earth: living and nonliving. It'd be hard to imagine a day without it. The daily pattern of the sun rising in the East and setting in the West is how we measure time...marking off the days of our lives. 6 The Sun http://c.tadst.com/gfx/750x500/sunrise.jpg?1 Virtually all life on Earth is aware of, and responds to, the sun's movements. Well before there was written history, humankind had studied those patterns. 7 Daily Patterns of the Sun • The sun rises in the east and sets in the west. • The time between sunrises is always the same: that amount of time is called a "day," which we divide into 24 hours. Note: The term "day" can be confusing since it is used in two ways: • The time between sunrises (always 24 hours). • To contrast "day" to "night," in which case day means the time during which there is daylight (varies in length). For instance, when we refer to the summer solstice as being the longest day of the year, we mean that it has the most daylight hours of any day. 8 Explaining the Sun What would be the simplest explanation of these two patterns? • The sun rises in the east and sets in the west. • The time between sunrises is always the same: that amount of time is called a "day." We now divide the day into 24 hours. Discuss some ideas to explain these patterns. -
Lecture 6: Where Is the Sun?
4.430 Daylighting Massachusetts Institute of Technology Christoph Reinhart Department of Architecture 4.430 Where is the sun? Building Technology Program Goals for This Week Where is the sun? Designing Static Shading Systems MIT 4.430 Daylighting, Instructor C Reinhart 1 1 MISC Meeting on group projects Reduce HDR image size via pfilt –x 800 –y 550 filne_name_large.pic > filename_small>.pic Note: pfilt is a Radiance program. You can find further info on pfilt by googeling: “pfilt Radiance” MIT 4.430 Daylighting, Instructor C Reinhart 2 2 Daylight Factor Hand Calculation Mean Daylight Factor according to Lynes Reinhart & LoVerso, Lighting Research & Technology (2010) Move into the building, design the facade openings, room dimensions and depth of the daylit area. Determine the required glazing area using the Lynes formula. A glazing = required glazing area A total = overall interior surface area (not floor area!) R mean = area-weighted mean surface reflectance vis = visual transmittance of glazing units = sun angle 3 ‘Validation’ of Daylight Factor Formula Reinhart & LoVerso, Lighting Research & Technology (2010) Graph of mean daylighting factor according to Lynes formula v. Radiance removed due to copyright restrictions. Source: Figure 5 in Reinhart, C. F., and V. R. M. LoVerso. "A Rules of Thumb Based Design Sequence for Diffuse Daylight." Lighting Research and Technology 42, no. 1 (2010): 7-32. Comparison to Radiance simulations for 2304 spaces. Quality control for simulations. LEED 2.2 Glazing Factor Formula Graph of mean daylighting factor according to LEED 2.2 v. Radiance removed due to copyright restrictions. Source: Figure 11 in Reinhart, C. F., and V. -
The Application of Precision Measurement in Historic Building
The Application of Precision Measurement in Historic Building Conservation: Taking Guanxing Tai, a historic Chinese Observatory, as an Example Xiao Jinliang 1 1Beijing Tsinghua Urban Planning & Design Institute, Department of Architecture & Urban Heritage Beijing, P. R. China [email protected] Keywords : Guanxing Tai, Precision Measurement, Total Station, Historic Building Conservation Abstract: Guanxing Tai, the ancient Observatory in central China, built in the 13th century as a national facility for astronomical observations, served the dual purposes of an astronomical building and an astronomical instrument as well. For a long time, many historians and astronomers attribute the Observatory’s somewhat peculiar design to special astronomical numeric values like the solar elevation angle. Besides, the askew brick joints in this old brick-made building make heritage conservation experts doubt the stability of its foundations. By means of total station survey system, close-range photogrammetry and geophysical survey, we have collected precise information about its exterior and inner structure, and gradually unraveled the mysteries about the ancient building through GIS analysis and computer simulation. Our tests rule out the connection between its design and astronomical numeric values, enable us to propose a new view, i.e. the peculiar architectural style may be the result of ancient craftsmen’s unconscious brick-laying acts in two directions, and invalidate the conclusion of the seemingly unstable foundations. Our new findings also provide us with more clues as to the brick processing techniques in ancient China. 1. Overview, History and Value The Guanxing Tai Observatory is the earliest one of its kind so far extant in China, and is also one of the earliest buildings for astronomical observation in the world. -
PRIME MERIDIAN a Place Is
Lines of Latitude and Longitude help us to answer a key geographical question: “Where am I?” What are Lines of Latitude and Longitude? Lines of Latitude and Longitude refer to the grid system of imaginary lines you will find on a map or globe. PARALLELS of Latitude and MERIDIANS of Longitude form an invisible grid over the earth’s surface and assist in pinpointing any location on Earth with great accuracy; everywhere has its own unique grid location, and this is expressed in terms of LATITUDE and LONGITUDE COORDINATES. Lines of LATITUDE are the ‘horizontal’ lines. They tell us whether a place is located in the NORTHERN or the SOUTHERN HEMISPHERE as well as how far North or South from the EQUATOR it is. Lines of LONGITUDE are the ‘vertical’ lines. They indicate how far East or West of the PRIME MERIDIAN a place is. • The EQUATOR is the 0° LATITUDE LINE. o North of the EQUATOR is the NORTHERN HEMISPHERE. o South of the EQUATOR is the SOUTHERN HEMISPHERE. • Lines of Latitude cross the PRIME MERIDIAN (longitude line) at right angles (90°). • Lines of Latitude circle the globe/world in an east- west direction. • Lines of Latitude are also known as PARALLELS. o As they are parallel to the Equator and apart always at the same distance. • Lines of Latitude measure distance north or south from the equator i.e. how far north or south a point lies from the Equator. • The distance between degree lines is about 69 miles (or about 110km). o A DEGREE (°) equals 60 minutes - 60’.