Initial attempts to produce orbit for Uranus unsuccessful 1821: Bouvard produces orbit based on contemporary observations includes gravitational influences.

Slides:



Advertisements
Similar presentations
Downs 4 th Grade Science Solar System Review The Planets & Other Objects in Space.
Advertisements

A presentation by Ann-Kathrin Rink. introduction facts about pluto a dwarf among giants the discovery sources.
The Solar System What is a solar system and what does it entail?
Dwarf Planets And TNOs. The Problem of Pluto Pluto was discovered in Named after the god of the dead. Its position was predicted by perturbations.
Dwarf Planets.
How Many Planets… In Our Solar System? With the advent of powerful new telescopes on the ground and in space, recent new discoveries have been made of.
Our Solar System. Your Parents Solar System 21 st Century Solar System.
Solar System Geocentric = Earth (geo) is center of universe Heliocentric = Sun (helio) is center of universe Which is correct? Heliocentric… proved by.
Honey, I Shrunk the Solar System or Pluto We Barely Knew Ye as a Planet Image credit JPL.
What Is a Planet? Pluto and Its Place in the Solar System Dr. Matthew Tiscareno, Cornell University.
Towards an Initial Understanding of Science Russell McNeil, PhD Malaspina Great Books Lecture Series Malaspina Great Books 2006.
Trans-Neptunian Objects and Pluto Astronomy 311 Professor Lee Carkner Lecture 21.
The Formed Solar System Now we will begin our investigation of the Solar System as it is now. After we finish this, we will discuss the binding forces.
 The solar system has 8 planets.  The solar system has 1dwarf planet named Pluto.
Astronomy: Solar System
Solar System What you need to know Where we live in Space.
The Dwarf Planet Pluto & New Horizon Dr. Harold Williams Montgomery College Planetarium.
Chapter 8, Astronomy. Identify planets by observing their movement against background stars. Explain that the solar system consists of many bodies held.
Honey, I Shrunk the Solar System or Pluto We Barely Knew Ye as a Planet Image credit JPL.
THE SOLAR SYSTEM. Solar System Solar System- a star and all the objects orbiting it. Our solar system includes the Sun and all of the planets, dwarf planets,
Not Your Parents’ Solar System! Dr. Frank Summers Space Telescope Science Institute March 28, 2008 It’s.
Lecture 2 The Solar System The Universal Gravitation Chapter 1.3  1.11 Homework: On-line quiz for Chapter 1 (due August 27th) Outline What we see in the.
Our Solar System Cornell Notes Pg. 77. Our Solar System 8 planets revolve around our sun, as well as many other celestial bodies Heliocentric.
 If it has mass, it has gravity!  What does it cause to happen?  Attraction, orbiting  Laws - Newton  More mass = more gravity  Closer together =
14b. Pluto, Kuiper Belt & Oort Cloud
Not Your Parents’ Solar System! Original ideas from Frank Summers Space Telescope Science Institute NSTA Institute Symposium November 15, 2003.
Halfway Around the World for 5 Minutes of data
Solar System – Odds & Ends. So what was that “retrograde motion” stuff all about? Why do the planets appear to move backwards sometimes?
Europa Clipper. Kuiper Belt, Dwarf Planets & the Oort Cloud.
Chapter 11: Part 1 Pluto and the Dwarf Planets. Pluto was discovered by Clyde Tombaugh in 1930 by comparing one image of the sky taken one night with.
The Solar System The Sun’s Family - the Giants The Sun’s Family - the Dwarfs Earth Venus Mars GanymedeTitanMercury Callisto Io Moon EuropaTriton Pluto.
Stars, Planets, and Moons Cornell Notes Page 81. Stars a massive sphere of gas so much pressure (from its own gravity), nuclear fusion takes place- this.
Unit 3 Lesson 6 Small Bodies in the Solar System
Pluto Scientists calculated that Neptune’s gravity was not enough to cause all of the irregularities of Uranus’ orbit.
Earth and the solar system Chapter 9 Video Video.
Voyagers (1970s) 1800 lbs, dish >12 ft diameter data rates ~115,000 bits/sec (twice dial-up!) Radioisotope Power Generators.
Uranus and Neptune – gas giant twins Uranus 19.2 AU from Sun Diameter 4 x Earth Mass 14.5 x Earth Density 1.3 gm/cm 3 Neptune 30 AU from Sun Diameter 3.9.
5 The Solar System A planet by any other name …..
With the advent of powerful new telescopes on the ground and in space, recent new discoveries have been made of objects in the outer regions of our Solar.
The Solar System. The solar system A solar system is a group of planets orbiting a central star. The solar system contains a sun, 8 planets, 3 dwarf planets,
The Solar System The Planets. Celestial Bodies Is an old term that means the sun, moon and stars Is an old term that means the sun, moon and stars Thousands.
The Solar System. According to Aug 24, 06 Resolution the Solar System is composed of: – Eight planets with their moons – Three dwarf planets with their.
Against the milky way, we are just a speck of dust in the wind on the Orion arm. The Milky way galaxy has rotated about 50 times.
The Solar System. The Solar System Contains: One star (the sun). Nine planets (well now there’s eight planets and 3 dwarf planets). 157 moons (at last.
The Sun and all the planets that orbit it form the Solar System. The Solar System contains eight planets and their satellites, and a large number of comets.
Uranus.
The known Universe consists of only 8 bodies: Earth, Sun, Moon, Mercury, Venus, Mars, Jupiter, Saturn. Earth is thought to be the centre of the Universe.
The Sun The Sun is a star. The Sun is a star. It is 4,500 million years old It is 4,500 million years old It takes 8 minutes for its light to reach.
Kepler’s Laws of Planetary Motion - 3 Laws -. Elliptical Orbits Planets travel in elliptical orbits with the sun at one focus. Furthest point = Aphelion.
Other Objects in the Solar System
Solar System Distance Model The planets nearest the Sun are very different from the planets farther out in composition and structure.
Trans-Neptunian objects = celestial objects beyond Neptune.
Know about Pluto Know about the Asteroids Know about Comets Comprehend the Oort Cloud and Kuiper Belt Asteroids and Kuiper Belt Objects.
THE SOLAR SYSTEM. BODIES IN THE SOLAR SYSTEM Our planet, Earth, is part of a system of planets that orbit a star, the sun. The solar system is comprised.
The 8 Planets in our Solar System. **A revolution is the time it takes for a planet to orbit the sun. It defines the length of 1 year. **Rotation is how.
Other Solar System Objects. A moon is a natural satellite Solar systems Moons All are composed of rock & metal Most orbit the outer planets Mercury &
The Planets SPACE. Learning Goals  To be able to describe the planets of our solar system.
Asteroids, Comets, and Pluto (Most of) The Rest of the Solar System.
Introducing The Solar System WHAT’S IN IT? HOW DID IT FORM?
Dwarf Planets And TNOs.
The Dwarf Planet Pluto Dr. Harold Williams Montgomery College Planetarium
Solar System Inventory
Understand the movement of planetary bodies.
How we came about the knowledge of what is out there in space.
The Pluto Controversy
The “New” Solar System.
Chapter 28 Notes Our Solar System.
Dwarf Planets And TNOs.
Unit 4: Astronomy Lesson 4: The Solar System
Presentation transcript:

initial attempts to produce orbit for Uranus unsuccessful 1821: Bouvard produces orbit based on contemporary observations includes gravitational influences of Jupiter and Saturn discrepancy possibly due to gravitational perturbations of an unknown planet deviations between prediction and observations (perturbations) increase with time Problem: use the observed perturbations to predict location of the unknown NEPTUNE

Adams (English) approximate method to determine location and mass (1843) used Newton's laws of Mechanics and Gravitation assumed circular orbit, twice the radius of Uranus' dropped assumptions when more accurate data obtained calculated orbit and mass of the unknown (1845) orbit presented to Challis and Airy at Cambridge Observatory search delayed due to concerns of Challis and Airy LeVerrier (French) determined size of perturbations very precisely by examining effects of Jupiter and Saturn assumed orbit fit T-B law (38.8 AU) also used Newton's Laws produced ephemeris (August, 1846)

The Race Adams becomes aware of Leverrier's work, requests Challis begin search for object Challis begins observing (July 1846) Cambridge lacked detailed sky maps of region necessitates large amount of data analysis, Challis reluctant uses new Star Map of the Berlin Academy (created in response to discovery of asteroids) locates a new object within 52' of prediction Galle and Enke confirm object moves Leverrier's ephemeris sent to Galle at Berlin Observatory (Sept. 23, 1846) must be planet - Neptune

The Aftermath British had observed Neptune on Aug. 4 and 12 didn't analyse the observations until after discovery at Berlin controversy over credit Galileo may have observed it in Neptune's orbit has radius of 30.1 AU, period 164 years T-B law discredited discovery added credence to Newton's theories LeVerrier examines Mercury's orbit perihelion advance (1.5° per century) gravitational perturbations account for all but 40" of the advance suggested existence of another planet (Vulcan)- never found Mercury

PLUTO Uranus' orbit apparently still had unaccounted perturbations Lowell predicts position of another unknown object Clyde Tombaugh searches for planet at Lowell Observatory uses blink comparator Feb. 1930: discovers object within 6° of Lowell's prediction – Pluto perturbations of Uranus were not produced by Pluto Pluto and Charon orbit: 39.5 AU, period 248 years

MOONS AND MINOR BODIES many new moons discovered as telescope resolution improves moons of Mars Jupiter - 63, Saturn Pluto's moon Charon more moons for Pluto (discovered with HST) Phobos Deimos

collection of rocky/icy bodies out to 50,000 AU home of long-period comets Kuiper Belt (1951) rocky objects beyond Pluto, out to 500 AU home of short-period comets Quaoar, Sedna - similar to Pluto Sedna Quaoar’s orbit Eris (2006) - larger than Pluto Oort Cloud (1950)

round due to gravity not heavy enough to clean majority of nearby space Pluto, Ceres Trans-Neptunian Objects Dwarf Planets (August 2006)