Globular Clusters By Ryan Hood.

Slides:



Advertisements
Similar presentations
Notes 30.3 Star Groups Std 2a: Know that the solar system is located in the outer edge of the disc-shaped Milky Way galaxy Std 2b: Know galaxies are made.
Advertisements

The Milky Way. The Milky Way: Our Home Galaxy What are the different components of the Milky Way? How do we see those components? What does a map of each.
Constellations are groups of stars, sometimes in patterns of animals, or objects. Constellations are important because they can help define where in the.
Chapter 11c Surveying the Stars Star Clusters Our Goals for Learning What are the two types of star clusters? How do we measure the age of a star.
Stars, Galaxies, and the Universe.  To understand how telescopes work, its useful to understand the nature of the electromagnetic radiation. Light is.
Characteristics Of Stars Galaxy: A collection of stars, gases and dust. Universe: Contains billions of galaxies.
Galaxies & Star Systems Astronomy 2. Star Systems Our solar system only has one star (our sun); however, most are grouped together to groups of two or.
The Milky Way Galaxy.
Stars, Galaxies, and the Universe Section 3 Section 3: Star Groups Preview Key Ideas Constellations Multiple-Star Systems Star Clusters Galaxies Contents.
Ch Star Groups.
The Sun & Stars, Galaxies, & the Universe. Composition & Age of the Sun Hydrogen and helium make up over 99% of the sun’s mass. About 75% of the sun’s.
All stars form in clouds of dust and gas. Balance of pressure: outward from core and inward from gravity.
By: Tori and Michelle.  The Andromeda galaxy is a spiral galaxy approximately 2.5 million light-years away.  It is also known as Messier 31, M31, or.
The Milky Way Galaxy By: Rachel Williams & Deidre Vaughters.
When Giovanni Riccioli used a telescope like this one to observe a star in the handle of the Big Dipper, he discovered two stars that orbit each other.
Measuring the Stars Chapter Grouping of Stars Groups of stars named after animals, mythological characters, or everyday objects are called constellations.
What Am I ?  The Andromeda galaxy (Messier 31, M31 or NGC 224) is a spiral galaxy about 2.5 million light years from Earth.
Ch. 27 Stars and Galaxies Ch Characteristics of Stars.
Cluster. Star Clusters A nebula often results in a cluster of stars. A cluster of stars from the same molecular cloud: –were formed at about the same.
Binary stars and clusters Chapter 11. Review Properties of stars –apparent brightness (apparent magnitude) measure energy/area/second –luminosity (absolute.
 Students will be able to determine how distances between stars are measured.  Students will be able to distinguish between brightness and luminosity.
Stars, Galaxies, and the Universe Section 3 Section3: Star Groups Preview Objectives Constellations Multiple-Star Systems Star Clusters Galaxies Contents.
The Milky Way. The Milky Way: Our Home Galaxy What are the different components of the Milky Way? How do we see those components? What does a map of each.
Hertzsprung–Russell diagram review. Temperature Luminosity An H-R diagram plots the luminosities and temperatures of stars.
Compare the size of the earth with other planets
Earth in Space Benchmarks
Earth Science Ms. Cordaro San Marcos High School
© 2017 Pearson Education, Inc.
Simulated black hole picture
Galaxies This lesson deals with important topics relating to galaxies. Each of these topics represents a great body of knowledge and areas of interest.
Galaxies and Stars.
The different types and how they form.
Stars change over their life cycles.
Galactic Structure.
Galaxies The Galaxies 5/12/2010.
Option D Lesson 2: Astronomical Objects B.
Compare the size of the earth with other planets
Celestial Objects Solar System Objects Galactic Objects
Physical Properties Review
The Birth, Life, and Death of Stars
Section 2: Measuring the Stars
The Universe.
Galaxies This lesson deals with important topics relating to galaxies. Each of these topics represents a great body of knowledge and areas of interest.
Section 3: Star Groups Preview Key Ideas Constellations
It contains hundreds of billions of galaxies
Compare the size of the earth with other planets
The History of the Universe
What do you see in the photographs of the sky?
Characteristics of Stars
The universe and us the light version
When Giovanni Riccioli used a telescope like this one to observe a star in the handle of the Big Dipper, he discovered two stars that orbit each other.
Proxima Centauri, the red star at the center, is the closest star to the sun. A star is a large, glowing ball of gas in space, which generates energy through.
Astronomy 105 Laboratory Lab 09.
Star Clusters and their stars
Stellar Mass A star’s position on the main sequence is determined by mass. Mass and composition are set at a star’s birth.
Section 2: Measuring the Stars
Planetary Nebula Alan Iannaccone.
When Giovanni Riccioli used a telescope like this one to observe a star in the Big Dipper, he discovered two stars that orbit each other. A group of stars.
Classification of stars
Stellar Clusters are groups of stars, smaller than and contained in galaxies The open star cluster (NGC 2244) was discovered in 1690 by English astronomer.
Overview for Estimating Age of Star Clusters
Lab 9 – Ages and Distances to Clusters
Binary stars and clusters
What is a star? - body of gasses that give off “tons of” energy (light & heat) - clusters = those little specks in the sky that we see may really be more.
Compare the size of the earth with other planets
A star is a large, glowing ball of gas in space, which generates energy through nuclear fusion in its core. The closest star to Earth is the sun, which.
Chapter 30 Stars, Galaxies, and the Universe 30.3 Star Groups
The Life Cycle of a Star The Horsehead Nebula – one of the most famous pictures in astronomy.
Stellar Clusters are groups of stars, smaller than and contained in galaxies The open star cluster (NGC 2244) was discovered in 1690 by English astronomer.
Structure, Types, Known Galaxies
Presentation transcript:

Globular Clusters By Ryan Hood

Definition and Significance They are Densely packed collections of stars (hundreds of thousands, sometimes millions per cluster) Used to estimate age of universe. 150 known globular clusters in the Milky May All stars in a cluster tend to be very similar in age.

How do they form? They start as a large accumulation of gas and dust These gasses and dust start to collect into clumps. All the stars orbit the clusters center of mass.

Metallicity Metallicity: The abundance of elements in a cluster that are heaver than hydrogen and helium. Metals (astronomer definition): all elements except hydrogen and helium

How do they estimate age? Globular clusters are chemically homogenous and the stars very close in time to each-other. We Examine the mass of the of the stars that exceed the main sequence turn off point. The cluster age is relatively equivalent to the main sequence lifetime of the turnoff stars. All globular clusters have low metallicity, which follows the characteristics of the early universe, therefore these formed early in the universes existence.

Messier 2 Sketch and Photograph 0.34 arcminutes 240X

Details of M2 Apparent magnitude: 13.1 Position: Within the Aquarius constellation, roughly 37000 light years away from earth. Diameter: 175 light years 13 billion years old 150,000 stars.

How to observe? In some conditions it is visible with the naked eye. Low power telescopes will show M2 as non-stellar. Higher power will help distinguish individual stars. (150x or greater)

Messier 13 Sketch and Photograph 20 arcminutes 200X

Details of M13 Apparent magnitude: 5.8 Position: Within the Hercules constellation, roughly 22200 light years away from earth. Diameter: 145 light years 11.7 billion years old Contains approximately 300,000 stars

How to observe? Look for the 4 stars that make up the Keystone of Hercules, should be on the western side. It can be seen with low power visual aid, such as binoculars. Higher power will show individual stars in the cluster.

Messier 22 Sketch and Photograph 32 arcminutes 120X

Details of M22 Apparent magnitude: 5.1 Position: Within the Sagittarius constellation, roughly 10600 light years away from earth. Diameter: 100 light years 12 billion years old Contains approximately 83,000 stars

How to observe? Sagittarius constellation Visible with the naked eye only in very dark skies. High power telescopes will be best viewing experience

Messier 56 Sketch and Photograph 8.8 arcminutes 196x

Details of M56 Apparent magnitude: 8.3 Position: Within the Lyra constellation, roughly 32900 light years away from earth. Diameter: 84 light years 13.7 billion years old Contains approximately 80,000 stars

How to observe? Lyra constellation Not easily visible to naked eye or lower power telescopes, its very dim. Higher power needed.

Sources: https://www.space.com/29717-globular-clusters.html http://www.deepskywatch.com/Astrosketches/messier-2-sketch.html http://www.deepskywatch.com/Astrosketches/messier-13-sketch.html http://www.messier-objects.com/messier-2/ https://en.wikipedia.org/wiki/Messier_2