Title: The Greatest Explosions since the Big Bang:
1The Greatest Explosions since the Big Bang
Supernovae!
2Up for discussion
- Why are they so important?
- How do we find them?
- How do we classify them?
- What is it that explodes?
- Major discoveries using supernovae
3The importance of Supernovae
- Nucleosynthesis of chemical elements
- Star formation histories
- Chemical evolution
- Distance measurement
- Peculiar velocity studies
- Cosmological models
- The nature of Gamma Ray Bursts
4Can you spot the new SN?
Photographic Plates UKS 6.6ox6.6o Wide
Field Imagers MaCHO 45x45 Mosaic II
36x36 ESO WFI 34x33 OmegaCam 1ox1o
5Searching for Supernovae
Construct a Template
6Searching for Supernovae - 2
New Image with SN
Shifted to Template
7Searching for Supernovae - 3
Adjusted for Seeing and transparency
Subtracted
8Searching for Supernovae - 4
Red Image
Blue Image
Red Subtraction
Blue Subtraction
Red Template
Blue Template
9Searching for Supernovae - 5
- Cosmic Ray
- Rare to have coincident CRs in 2 images
- Asteroid
- Only if observing close to the ecliptic
- Generally not associated with a galaxy in the
template - Variable Star
- Associated with a star in the template
- Recurrent over many observations
- AGN
- Located in the centre of the galaxy
10How many supernovae do we find?
11And the winner is --- KAIT!
- 76cm telescope _at_ Lick
- Robotic telescope to search for SNe and monitor
other events (e.g. GRBs/Novae)
12Classification
Type Ic
t 1 week
13SN Progenitors
14Type II, Type Ib, Type Ic Progenitors
15Type Ia Progenitors
16Its all good!
17Or is it?
(Type Ia)
18Type IIn
vs
Type II
19Type Ia
Type IIn
20SN 1997cy
21SN 1999E
22Confused?
Type Ic
Type Ia
Type II
Type IIn
core-collapse
Type Ib
23Supernova classification tree
24Nucleosynthesis
Type Ia (white dwarf binary)
Core-collapse (massive stars)
Ni, Co, Mn, Fe gt Fe
C, O, N gtFe
25Late-time spectra of SNe
26Light Curves of Supernovae
27Light Curves of Type Ia SNe
28Brighter SlowerFainter Faster
29Luminosity-Decline Rate Relation
30Template Fitting MCLS ?m15
31Template Fitting - Stretch
32Template Fitting - how good is it?
- But why does this work at all
33Measuring Distances with SNIa
- Have absolute magnitude of the SN through
template fitting methods - Have apparent brightness of the SN through
photometry
DISTANCES accurate to 7
34What have we learned from Type Ia Supernovae?
35The Universe is Accelerating!
- SNe at high-Z are fainter than expected
- Acceleration started sometime in the last 10
billion years
36The Universe is Accelerating!
- Best cosmological model
- ?M 0.28
- ?? 0.72
37What Does this Mean?
- The Mundane Astronomers have been fooled by
supernovae into believing the Universe is
accelerating. Perhaps supernovae were
intrinsically fainter in the past and therefore
look further away?
38Probably not )
- CMB data alone suggests a flat universe with ?gt0
- Any 2 of CMB/SN/LSS taken together indicate an
accelerating Universe with a dark energy
component of 70
39What Does this Mean?
- The Heretical General Relativity (though sacred
in Physics) may be wrong. Since the observations
are interpreted through the predictions of
General Relativity, the conclusion that the
Universe is accelerating may also be wrong -/
40What Does this Mean?
- The Exciting The Universe is being accelerated
by some unknown type of energy that is spread
throughout the cosmos!
41Where do we go from here?
- SNAP - SN acceleration probe
- 2000 SNe/year for 3 years
- Expansion history to 1
42What have we learned from core-collapse
Supernovae?
43Hypernovae long duration GRBs
44Summary
VERY
- Nucleosynthesis of chemical elements
- Measuring Distances/Cosmology
- Understanding GRBs
45Summary
Thank goodness for computers!
- Initially by eye (I cant bear to think of it!)
- Now by fully automatic, robotic telescopes
46Summary
- Classification Progenitors
Very messy!
- Basically 2 types
- Type Ia explosion of a white dwarf binary
- Core-collapse explosion of a massive star
47Summary
Very EXCITING!
- Type Ia revealed the accelerating Universe and
the existence of dark energy - Core-collapse are associated with GRBs
48Who is next to explode?
49Best Candidate?
- Bright as a half moon but a point of light, not a
disk - Visible to the naked eye for many months
- Could be tomorrow, could be in 10,000 years.
Betelgeuse
50Or perhaps?
51Interested in Learning More?
http//astronomy.swin.edu.au/lgermany/