Open%20Clusters - PowerPoint PPT Presentation

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Open%20Clusters

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3 different filters allow us to see color (red, green, and blue) ... Emily Freeland. Elinor Gate. John Martin. Hilary O'Bryan. Jay Strader. Gene Switkes. Vay Hoang ... – PowerPoint PPT presentation

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Title: Open%20Clusters


1
Open Clusters
  • Allan Harrell
  • Edgar Toledo
  • Tenaya Pusley
  • Carmen De Martis

2
What is a star?
  • A giant ball of gas
  • Hydrogen
  • Emits light
  • Different colors and sizes

3
How do stars form?
  • Form from clouds of dust and molecular hydrogen
  • Gravity collapse

4
Why doesnt a star continue collapsing?
  • Hydrostatic Equilibrium
  • Gravity pushes in.
  • Pressure pushes out
  • Create an equilibrium

5
What are open clusters?
  • Young stars
  • Same chemical composition
  • Same Age
  • Distance
  • Bound by gravity
  • Form in spiral and irregular galaxies

6
The Main Sequence
7
About Main Sequence Stars
  • Stars spend most of their life in the main
    sequence, about 90
  • Our sun is 5 billion years into its main sequence
  • The larger the star, the less time it will spend
    on the main sequence
  • Main sequence stars maintain brightness and
    energy through fusion

8
Photosphere
9
?
?
10
Fusion is important!!
  1. Fusion creates energy
  2. Energy raises temperature
  3. Temperature makes atoms move faster
  4. Faster moving atoms increase pressure
  5. Pressure fights against gravity

11
(No Transcript)
12
http//www.star.ucl.ac.uk/groups/hotstar/images/li
fe_cycle.jpg
13
What happens in a high mass star?
  • Shorter lifetimes
  • Consumes fuel faster
  • Fuses more elements.
  • Fusion of iron consumes energy instead of giving
    off energy.

14
Fuel fusion
http//physics.uoregon.edu/jimbrau/BrauImNew/Chap
21/FG21_05.jpg
15
Supernova explosion
http//imgsrc.hubblesite.org/hu/db/2004/29/videos
/d/stills/3/image.jpg
16
What happens after death
  • It either becomes a
  • Black hole
  • or a
  • Neutron star.

17
http//dante.physics.montana.edu/ns_interior.jpg
18
Black Hole
http//www.wvp-consulting.com/astronomy/images/bla
ckhole.jpg
19
Observations
  • Used the Lick Nickel 40 inch telescope
  • Observed remotely with the help of Elinor Gates
  • Took images of 4 open clusters

http//www.ucolick.org/graphics/nickel_lg.jpg
20
CCDs
  • Basic tools of astronomical imaging
  • Grids of light buckets
  • Colorblind
  • 3 different filters allow us to see color (red,
    green, and blue)
  • Same as the digital cameras that you may own

21
Isochrones
  • Freeze frame of a cluster
  • Reveals age of cluster
  • Made by computer

Ybrightness
Xcolor and temp.
22
Which Isochrone Matches the CMD?
A.
B.
This one! Correct! )
23
(CMD)
(ISOCHRONE)
24
d100.2 ( m-M5-Ar )
How to calculate the distance
Due to dust
Apparent Mag.
(from CMD)
Absolute Mag.
Distance
(from isochrone)
25
M11, The Wild Duck Cluster
i
hh
26
M11
27
Color Magnitude Diagram
  • y-axis brightness
  • x-axis color
  • M11
  • Around 2000 parsecs
  • Around 6000 light years
  • Mostly main sequence
  • stars
  • 200 million years old

28
NGC6939
  • What I found out
  • 5095 light years from the earth
  • 1.6 billion years old

29
My Color Magnitude Diagram
30
Open Cluster NGC6939
31
NGC 6819Apparent Diameter 5 arc min.
32
NGC 6819Open star cluster
According to my results -It is about 3/4 of
the Earths lifetime old. -It is about 7,603
light years away from us. -Has a metallicity of
about 2---like Sun
33
Isochrone CMD
for NGC 6819
34
NGC 6791
  • Observed and recorded data for NGC 6791
  • 7.6 billion years old
  • Looking at isochrones
  • 4972 parsecs (3.26 light years 1 parsec)

35
Isochrones
36
Puzzles from NGC 6791
  • Its really old
  • Metal rich

37
NGC 6705
NGC 6791
NGC 6819
Sun
NGC 6939
38
We would like to thank
  • CFAO
  • Laura Chomiuk
  • Kathy Cooksey
  • Daisy Corral
  • Liz Espinoza
  • Emily Freeland
  • Elinor Gate
  • John Martin
  • Hilary OBryan
  • Jay Strader
  • Gene Switkes
  • Vay Hoang
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