Pluto and Charon. New Horizons
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- Barnard Blake
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1 Pluto and Charon New Horizons
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6 EXOPLANETS KNOWN IN 2010 Radial Velocity Transits Imaging Microlensing Other
7 Today Radial Velocity Transits 594/448/ /659/356 Imaging Microlensing Other 51/47/2 34/32/2 21/16/4
8 week month year decade
9 Planets with Radial Velocity Measurements week month year decade
10 school zone speed Planets with Radial Velocity Measurements slow walker week month year decade
11 Planets with Radial Velocity Measurements Planets with Transits? week month year decade
12 Planets with Radial Velocity Measurements Planets with Transits? week month year decade
13 Transits Radial Velocity week month year decade
14 Transits Radial Velocity Our Solar System week month year decade
15 Transits Radial Velocity school zone speed Our Solar System slow walker week month year decade
16 Transits Radial Velocity Our Solar System week month year decade
17 Discovery: Transits Radial Velocity Regular Jupiters best chance for surviving rocky planets Our Solar System Low prob of rocky planets need to look elsewhere week month Soooo many Hot Jupiters i.e. close-in Jupiter-sized planets year decade planet migration inner planets thrown into the star
18 ALMA Observes Planet Forming Disk HL Tau
19 ALMA Observes Planet Forming Disk There be planets forming! HL Tau
20 ALMA (Atacama Large mm Array) Promised to solve all the problems revealing how much more there is to learn!
21 ALMA (Atacama Large mm Array) A high-altitude desert in Chile Interferometer (many telescopes acting as one) Promised to solve all the problems revealing how much more there is to learn!
22 ALMA (Atacama Large mm Array) A high-altitude desert in Chile Interferometer (many telescopes acting as one) Promised to solve all the problems revealing how much more there is to learn!
23 MY STUDIES ON STELLAR EVOLUTION (PRETTY PICTURES TIME) RODOLFO MONTEZ JR. BRIDGE POST-DOCTORAL FELLOW VANDERBILT UNIVERSITY
24 HELIX NEBULA HUBBLE SPACE TELESCOPE
25 HELIX NEBULA HUBBLE SPACE TELESCOPE
26 CLUES OF STELLAR EVOLUTION HOW TO MEASURE CHANGES THAT TAKE BILLIONS OF YEARS +90 Declination -90 Right Ascension (50k stars within 500 ly) 0 360
27 Bright Observed Visible Magnitude Faint Blue (hot) B-V Color Red (cool)
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29 field of distant background stars nearby star sun-earth orbit
30 field of distant background stars nearby star sun-earth orbit
31 field of distant background stars nearby star sun-earth orbit
32 field of distant background stars nearby star distance to star sun-earth orbit TRIGONOMETRIC PARALLAX
33 Bright Observed Visible Magnitude Faint Blue (hot) B-V Color Red (cool)
34 Bright Absolute Magnitude (intrinsic brightness) Faint Blue (hot) B-V Color Red (cool)
35 Bright Absolute Magnitude (intrinsic brightness) main sequence white dwarfs Faint Blue (hot) B-V Color Red (cool)
36 Bright Absolute Magnitude (intrinsic brightness) end state beginning state Faint Blue (hot) B-V Color Red (cool)
37 Bright Absolute Magnitude (intrinsic brightness) Faint Blue (hot) B-V Color Red (cool)
38 Bright Absolute Magnitude (intrinsic brightness) Faint Blue (hot) B-V Color Red (cool)
39 Bright 6 5 Post Main Sequence Post AGB 7 Absolute Magnitude (intrinsic brightness) Red Giant Core Helium Ignition Horizontal Branch (He Burning) Nebula forms (fast wind?) Nebula is ionized (hot core) Fading Nebula and Core (pre-wd) Faint Blue (hot) B-V Color Red (cool) 4 Asymptotic Giant Branch (AGB)
40 Bright 6 5 Post Main Sequence Post AGB 7 Absolute Magnitude (intrinsic brightness) Red Giant Core Helium Ignition Horizontal Branch (He Burning) Nebula forms (fast wind?) Nebula is ionized (hot core) Fading Nebula and Core (pre-wd) Faint Blue (hot) B-V Color Red (cool) 4 Asymptotic Giant Branch (AGB) Brightness t MS ~10 9 yr t RG->AGB ~10 7 yr t PN <10 5 yr 7 t WD >10 9 yr Elapsed Time (years)
41 Bright 6 5 Post Main Sequence Post AGB 7 Absolute Magnitude (intrinsic brightness) Red Giant Core Helium Ignition Horizontal Branch (He Burning) Nebula forms (fast wind?) Nebula is ionized (hot core) Fading Nebula and Core (pre-wd) Faint Blue (hot) B-V Color Red (cool) 4 Asymptotic Giant Branch (AGB) Brightness Mass t MS 1 ~10 9 yr 2 3 t RG->AGB ~10 7 yr t PN <10 5 yr 7 t WD >10 9 yr Elapsed Time (years)
42 Bright 6 5 Post Main Sequence Post AGB 7 Absolute Magnitude (intrinsic brightness) Red Giant Core Helium Ignition Horizontal Branch (He Burning) Nebula forms (fast wind?) Nebula is ionized (hot core) Fading Nebula and Core (pre-wd) Faint Blue (hot) B-V Color Red (cool) 4 Asymptotic Giant Branch (AGB) t MS Mass ~10 9 yr 1 2 t RG->AGB ~10 7 yr t PN <10 5 yr 6 7 t WD >10 9 yr Elapsed Time (years)
43 Bright 6 5 Post Main Sequence Post AGB 7 Absolute Magnitude (intrinsic brightness) Red Giant Core Helium Ignition Horizontal Branch (He Burning) Nebula forms (fast wind?) Nebula is ionized (hot core) Fading Nebula and Core (pre-wd) Faint Blue (hot) B-V Color Red (cool) 4 Asymptotic Giant Branch (AGB) t MS Mass ~10 9 yr 1 2 t RG->AGB ~10 7 yr t PN <10 5 yr 6 7 MASS LOSS t WD >10 9 yr Elapsed Time (years)
44 SPIROGRAPH NEBULA HUBBLE SPACE TELESCOPE
45 BLINKING NEBULA HUBBLE SPACE TELESCOPE
46 ESKIMO NEBULA HUBBLE SPACE TELESCOPE
47 RING NEBULA HUBBLE SPACE TELESCOPE
48 LITTLE GHOST NEBULA HUBBLE SPACE TELESCOPE
49 HUBBLE 5 NEBULA HUBBLE SPACE TELESCOPE
50 CAT S EYE NEBULA HUBBLE SPACE TELESCOPE
51 ERA OF SPACE TELESCOPES WHAT DOES HUBBLE SPY WITH ITS ORBITING EYE? VARIETY OF MORPHOLOGICAL DETAILS MOSTLY ELLIPTICAL OR ELONGATED VERY FEW ROUND/SPHERICAL NEBULA JET-LIKE AND BIPOLAR STRUCTURES
52 ERA OF SPACE TELESCOPES WHAT DOES HUBBLE SPY WITH ITS ORBITING EYE? VARIETY OF MORPHOLOGICAL DETAILS MOSTLY ELLIPTICAL OR ELONGATED VERY FEW ROUND/SPHERICAL NEBULA JET-LIKE AND BIPOLAR STRUCTURES
53 MORPHOLOGICAL CONFUSION WHY SO ASYMMETRICAL? round/elliptical hourglass/bipolar multipolar
54 MORPHOLOGICAL CONFUSION WHY SO ASYMMETRICAL? round/elliptical hourglass/bipolar multipolar
55 MORPHOLOGICAL CONFUSION WHY SO ASYMMETRICAL? pinched waist two lobes hourglass/bipolar
56 MORPHOLOGICAL CONFUSION WHY SO ASYMMETRICAL? pinched waist two lobes hourglass/bipolar
57 MORPHOLOGICAL CONFUSION WHY SO ASYMMETRICAL? pinched waist torus two lobes hourglass/bipolar
58 MORPHOLOGICAL CONFUSION WHY SO ASYMMETRICAL? pinched waist torus two lobes hourglass/bipolar
59 MORPHOLOGICAL CONFUSION WHY SO ASYMMETRICAL? pinched waist torus two lobes hourglass/bipolar
60 MORPHOLOGICAL CONFUSION WHY SO ASYMMETRICAL? pinched waist torus two lobes? hourglass/bipolar
61 MORPHOLOGICAL CONFUSION WHY SO ASYMMETRICAL? pinched waist torus two lobes? hourglass/bipolar
62 MORPHOLOGICAL CONFUSION WHY SO ASYMMETRICAL? pinched waist torus binary two lobes? hourglass/bipolar
63 BINARY HYPOTHESIS RELATIONSHIPS ARE HARD pinched waist torus binary two lobes hourglass/bipolar
64 BINARY HYPOTHESIS RELATIONSHIPS ARE HARD envelope ejection merger ejection
65 BINARY HYPOTHESIS RELATIONSHIPS ARE HARD envelope ejection merger ejection TESTING THE HYPOTHESIS EVIDENCE FOR COMPANIONS
66 TESTING THE HYPOTHESIS EVIDENCE FOR COMPANIONS (PAST AND PRESENT) Bright Absolute Magnitude (intrinsic brightness) Faint Blue (hot) B-V Color Red (cool)
67 X-RAY SURVEY OF DYING STARS HOT STARS AND HOT BUBBLES
68 X-RAY SURVEY OF DYING STARS HOT STARS AND HOT BUBBLES
69 BUT THE SUN IS NOT A BINARY NO BEAUTIFUL SWAN SONG FOR THE SUN?
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