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Open Clusters

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Stars spend most of their life in the main sequence, about 90% Our sun is 5 billion years ... The larger the star, the less time it will spend on the main sequence ... – PowerPoint PPT presentation

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Title: Open Clusters


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!!
  • Fusion creates energy
  • Energy raises temperature
  • Temperature makes atoms move faster
  • Faster moving atoms increase pressure
  • 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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