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MOTIVATION context setup results synthesis. Prettyman et al. (2012); McCord et al. (2012); Goodrich et al. (2015); meteorite image by Peter Jenniskens. 20 km ...
Bridging the Gap III September 2015
Experiments & numerical models provide complementary information about projectile survival & delivery R. Terik Daly 1 , Megan Bruck Syal 2 & Peter H. Schultz 1 1 Brown University, 2 Lawrence Livermore National Lab
OUTLINE 1. Context and driving questions 2. Setup: experiments and models
3. Results 4. Synthesis
context
setup
results
synthesis
MOTIVATION
20 km Prettyman et al. (2012); McCord et al. (2012); Goodrich et al. (2015); meteorite image by Peter Jenniskens
context
setup
results
synthesis
DRIVING QUESTIONS How much of the projectile remains? What is its spatial distribution? What is its physical state?
What do experiments and shock physics codes each contribute?
context
setup
results
synthesis
DRIVING QUESTIONS How much of the projectile remains? What is its spatial distribution? What is its physical state? What do experiments and shock physics codes each contribute? Strategy: direct comparisons
context
setup
results
synthesis
EXPERIMENTS AT NASA AVGR Projectile: ¼” Al, basalt Targets: pumice, snow Speeds: 4.5 – 5 km s-1 Angle: 30° to 90°
Image credit: Wired magazine
context
setup
results
synthesis
AVGR EXPERIMENTS (CONT.) PUMICE TARGETS
SNOW TARGETS
Recover breccias
Melt
Composition
Sieve
Mixing model
Sort
Mass retained
Weigh
context
setup
results
synthesis
CTH MODELS Projectiles: ¼” ANEOS Al and ANEOS basalt
Targets: ANEOS SiO2 and ANEOS water ice (density reduced using p-α porosity) Impact speed: 5 km s-1 Angle: 30° to 90°
Track mass remaining below escape speed
context
setup
results
synthesis
DRIVING QUESTIONS How much of the projectile remains? What is its spatial distribution? What is its physical state?
context
Delivered Fraction
100%
setup
results
synthesis
Porous ice
80%
Porous SiO 2
60% 40%
20% 0% 0
30 60 Impact Angle (°)
90
context
setup
results
synthesis
Fraction Delivered Retained Fraction
100%
A→P
80%
A→S
60% 40%
B→P
20%
B→S
0% 0
30 60 Impact Angle (°)
90
context
setup
results
synthesis
DRIVING QUESTIONS How much of the projectile remains? What is its spatial distribution? What is its physical state?
context
setup
results
synthesis
Fraction Retention DeliveredEfficiency
Linked to fraction deposited far away? Ceres 100% 80% 80% 60% 60% 40% 40% 20% 20% 0% 0% 0 0
30 60 Impact 30 Angle 60(°)
Impact Angle (°)
90
90
context
Beyond Rim
Inside Crater
90°
setup
results
synthesis
45°
Increasing amounts of projectile retained downrange
Scale bars = 5 mm
context
setup
results
synthesis
DRIVING QUESTIONS How much of the projectile remains? What is its spatial distribution? What is its physical state?
Greatly strengthens case for impactor contamination (in melts and as relics) on asteroids/dwarf planets Larger-scale CTH calculations support For impacts at 5 km s-1 and below, impactor retention is the expectation, not the exception Daly and Schultz (2015a, 2015b)
Bridging the Gap III September 2015
Experiments & numerical models provide complementary information about projectile survival & delivery With gratitude toward: the Barringer Crater Company, Paul. G. Benedum Graduate Travel & Research Fund for Geological Sciences, and the crew of the NASA AVGR.
context
setup
results
synthesis
PRIOR WORK Experiments: Schultz & Gault (1990); Burchell & Wickham-Eade (this session); Ebert et al. (2013); Daly and Schultz (2013, 2014, 2015)
Numerical models: Pierazzo and Melosh (2000); Pierazzo and Chyba (2002); Bland et al. (2008); Svetsov (2011); Yue et al. (2013); Bruck Syal et al. (2015)