Take-off into Mercury By: Team 6 9th D Team members: ….. Picture source: Hamilton, Calvin J. “Mercury." Views of the Solar System. 2001.

Slides:



Advertisements
Similar presentations
Solar System By Paige Hayford
Advertisements

Outline This Presentation contains slides appropriate for all the sections of the activity. – White slides are included (but hidden from the Slideshow)
The different types of stars By: Anna Peterson in partnership with Dr. Jeffrey Hall.
The Sun 6.E.1.2 Explain why Earth sustains life while other planets do not based on their properties (including types of surface, atmosphere.
The Solar System What’s out there!. Telescopes These are the kind of instruments used to discover our galaxy before satellite imaging was available. The.
Characteristics of the Atmosphere
Our Amazing Solar System
Mercury Astronomy 311 Professor Lee Carkner Lecture 10.
Present Climate Change – Inquiry Labs Lesson Global Precipitation Measurement Mission Developed by the GPM Education Team NASA Goddard Space Flight Center.
The Sun By: Tori and Caitlin. SHINNING STAR The Sun is the star at the center of the Solar System. It has a diameter of about 1,392,000 km, about 109.
Formation of the Solar System  This is a picture of the Eagle Nebula taken by the Hubble Telescope in  A nebula is a cloud of gas and dust in space.
Mercury Mercury is hard to study because it’s so close to the sun. Of all the planets, it is the second smallest. Mercury’s night temperature is the coldest.
THE SOLAR SYSTEM. By Nicholas and Dylan. The Solar System.
Name of Planet You and Your Partner’s Names Period Provide a caption for each image. Ex: This is a compilation image showing the seasons on Saturn. The.
By: Jaylen Higgins Our solar system.
Space By Rex. Table of contents Introduction………………………………………..Page 3 Chapter 1 Satellites……………………………..Page 4 Chapter 2 Stars…………………………………….page 5 Chapter.
Lecture 15. Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12 th.
The Sun. Sun Considered a medium STAR 93,000,000 miles away from Earth 1.39 million kilometers in diameter (one million Earths can fit inside the sun.
16-2 Heat Transfer. (pages 548–551) 1
4 th Grade. Sun Our Brightest Star Approximately one million Earths can fit inside the Sun. The center of the Sun, is made of helium. There are dark blotches.
Chapter 20, Section 2 The Sun Anne Marie Scrudato’s notes borrowed by Rusty Sturken.
How do colors in a spectrum help us understand stars? Image from
…..many things…. ….but what do you think is most important?
Is There Life Out There? Our Solar System (and beyond) Draw a picture of what you think life would look like on another planet, if it existed. Describe.
The Sun Chapter 3 Lesson 6 Page 122.
The person who looked through a telescope at the moon and thought he saw continents and oceans was The person who looked through a telescope at the moon.
Youth Capture the Colorful Cosmos THIS IS With Host... Your.
SU N BY: Cali Murphy. THE SUN HAS LAYERS!? WIKI-WIKI-WHATTTTTT?!?! NO! not those layers! These layers!!!
Name of Planet You and Your Partner’s Names Period Provide a caption for each image. Ex: This is a compilation image showing the seasons on Saturn. The.
By Rachel Joy Mellinger. The Sun The sun is very important. It is one of the most important parts in our solar system. The sun is one of the things that.
2 person team: The person who slams it cannot dunk it. Work together on putting response together 3-4 person team: One person slams it, another person.
Final Jeopardy Question The Sun Viewing Space 500 Galaxies Rocks And Stuff The Nine Planets The Beginning
1 Grades K-2: Introduction. 2 Did you know that our Sun is a star in the sky?
By: Phoebe Wang. What Is A Star? A star is a sphere which can produce light by Itself. Some stars have high temperature Surface, for example: THE sun.
SUN
December 7, 1631December 9, 1874 December 4, 1639December 6, 1882 June 6, 1761June 8, 2004 June 3, 1769June 6, 2012 Transits of Venus across the disk of.
Jupiter Thomas Myers.
8 th Grade Astronomy in Review Take this quiz and look at your score. Reflect. Take the quiz again as may times as you need to in order to feel good about.
ASTRONOMY 101 LECTURE SUN FACTS. A ball of hot gases Made up of 70% hydrogen 28% helium 1.5% carbon, nitrogen, and oxygen, and 0.5% all other elements.
Solar Energy Heat and Light. Energy Can take many different forms –____________ –Heat –____________.
By: Kyler Moody 9B-12 and Emily Rankin 9B-17. Location  Pluto is the usually the ninth planet from the sun, but every 248 years, it becomes the eighth.
Astronomy Big Idea: The sun is one of billions of stars in one of billions of galaxies in the universe.
Kristina Fousek May 14, 2013 Mrs.Lower  *It is the smallest planet in are solar system.
Bell Work 1/12/15 Write in agenda. Using page , identify the weather front we are currently experiencing. Think about how the weather was last week.
Sun.
Temperature Feeling hot, hot, hot….. Temperature Temperature – a measurement of how much kinetic energy the particles contain.
P What do you know about planets? L A N E T S. The Hubble Space Telescope hovers at the boundary of Earth and space in this picture,
Aim: Tools of Astronomy Do Now: List 4 tools that a chief may use DO NOW: What is this picture showing you? Notepack 21.
Our Whirling Planets 4th Grade Cherokee Elementary School.
#3 A ________ eclipse happens when the moon comes between the Earth and the sun. A. Solar B. Lunar C. Moon D. Star Trek.
Saturn By: Savannah and Christina
The Sun. Introduction sun’s gravity is most powerful force in solar system Force so strong because of Sun’s mass 99.8 % of the mass of the solar system.
Tour the Solar System. We will set up our brochures and pictures at locations spread around the room. Look for the yellow fact sheet that belongs to your.
Mercury. History Galileo had found Mercury in 1610 Galileo found Mercury because he had used a telescope to find the planets and found Mercury 1631-French.
Solar system.
Earth’s Moon Chapter 16 – 4 Part 1.
Multiwavelength Images
Earth’s Moon Chapter 16 – 4 Part 1.
The sun’s gravity holds all of the planets and comets in orbit
You and Your Partner’s Names Period
Planets Presentation Be Ready to Present in class in “Solar System Order” on Tuesday, Feb 26!! Delete this slide before turning in.
The Planets.
Earth’s Moon Chapter 16 – 4 Part 1.
MERCURY.
Mercury & The Inner Planets
Earth’s Moon Chapter 16 – 4 Part 1.
CFA #5 Space Technologies
Characteristics of the Atmosphere
Earth’s Moon Chapter 16 – 4 Part 1.
Presentation Number Title of the paper
Presentation transcript:

Take-off into Mercury By: Team 6 9th D Team members: ….. Picture source: Hamilton, Calvin J. “Mercury." Views of the Solar System (10 Oct. 2002).

Table of Contents ► Introduction ………………………………… Slide 3 ► Mercury Video ……………………………... Slide 4 ► Risk Analysis ……………………………….. Slide 5 ► Geology ………………………………………. Slide 10 ► Climate …… ► Mercury News …… ► Mercury Facts …… ► Trip Outline …… ► Conclusion …… Picture source: Hamilton, Calvin J. “Mercury." Views of the Solar System (10 Oct. 2002).

Video This is a slow gif animation based on images recorded by a satellite. The false color were made in ultraviolet light and tend to show the hot gas just above the Sun’s visible surface. Mercury’s disk is silhouetted against the seething plasma as it follows a trajectory near the edge of the Sun. It is a transit of Mercury that occurred in Nov. 15’1999 when the planet crossed the face of the Sun. The next Mercury transit will occur in If you want to enjoy a mercurial transit, you just require an appropriately filtered telescope. Gif source: Nemiroff, Robert & Bonnell, Jerry. "Astronomy Picture of the Day." Laboratory for High Energy Astrophysics (10 Oct. 2002).

Risk Analysis By: abcd abcd Image source: Nemiroff, Robert & Bonnell, Jerry. "Astronomy Picture of the Day." Laboratory for High Energy Astrophysics (10 Oct. 2002).

Risk Analysis Talking about temperature, on the surface of planet Mercury, we can feel from 467 degrees Celsius (872 degrees Fahrenheit) up to a bone-chilling -183 degrees Celsius (-300 degrees Fahrenheit). We have to be prepared for it! Image source: Nemiroff, Robert & Bonnell, Jerry. "Astronomy Picture of the Day." Laboratory for High Energy Astrophysics (10 Oct. 2002).