Josh Smith Zachary Blunier Michael Krauz Matt Pensa Daniel Lane Trey Keown quake rattle and roll.

Slides:



Advertisements
Similar presentations
Seismology and Earth’s Interior. Mass of the Earth Spherical masses behave as if all mass located at central point g = GMe/R 2  Me = gR 2 /G g = 9.8.
Advertisements

Fluid Mechanics 04.
ENGR 214 Chapter 16 Plane Motion of Rigid Bodies:
Summary of introductory concepts 12 February, 2007
Barry Latham Bloom High School Conceptual Physics, Hewitt, 1999.
Monday, Apr. 6, 2009PHYS , Spring 2009 Dr. Jaehoon Yu PHYS 1441 – Section 002 Lecture #16 Monday, Apr. 6, 2009 Dr. Jaehoon Yu Power Linear Momentum.
Gravitational Field Strength & Satellites. Gravitational Field Strength Gravitational force per unit mass on an object g = F g / m (units = N/Kg) g =
Circular Motion Level 1 Physics. What you need to know Objectives Explain the characteristics of uniform circular motion Derive the equation for centripetal.
Current, Ohm’s Law, Etc. The Continuity Equation for Steady State Currents Currents and current densities are constant in time – steady state. The flux.
1 Class #19 Central Force Motion Gravitational law Properties of Inverse-square forces Center of Mass motion Lagrangian for Central forces Reduced Mass.
 For circular motion: Centripetal force = gravitational force (F C = F G ) Recap: Orbital Velocity M = planet’s mass m = satellite’s mass r MG v or 
Week.  Student will: centripetal accelerationcentripetal force  Solve problems involving centripetal acceleration and centripetal force.
EULER’S EQUATION Fluid Mechanics CHAPTER 4 Dr . Ercan Kahya
Satellites What keeps them in orbit?. Satellites A satellite is any projectile given a large enough velocity so its path follows the curvature of the.
AP Physics II.A – Fluid Mechanics.
Newton reasoned that there is a force of attraction between every two objects in the universe.
-Energy Considerations in Satellite and Planetary Motion -Escape Velocity -Black Holes AP Physics C Mrs. Coyle.
What keeps them in orbit?
In order to stay in a closed orbit, an object has to be within a certain range of velocities: Too slow  Object falls back down to Earth Too fast  Object.
5 th IPPW, Bordeaux, June 25-99, 2007 Kinetic Micro-Penetrators For Exploration Of Solar System Bodies. R. Gowen & A. Smith, MSSL/UCL.
Gravitation Part II One of the very first telescopic observations ever was Galileo’s discovery of moons orbiting Jupiter. Here two moons are visible,
Physics Mrs. Coyle -Gravitational Field -Satellites -Einstein’s View of Gravity.
Planetary Environment Around a Pulsar David Dunkum, Jacob Houdyschell, Caleb Houdyschell, and Abigail Chaffins Spring Valley High School Huntington, WV.
Mullard Space Science Laboratory Planetary Micro-Penetrators Dr Rob Gowen on behalf of Glyn Collinson international - Germany, France, Austria,
Acceleration is equal to Δv/Δt. Velocity is a vector and there are two ways a vector can be changed: by changing magnitude or by changing direction.
Titan Saturn System Mission Workshop - Paris, Mar 17-19, 2008 MSSL/UCL UK Penetrators for Enceladus Titan Saturn System Mission Workshop - Paris, Mar 17-19,
AAE450 Spring 2009 Final Slide Concepts March 26, 2009 [Cory Alban] [Mission Ops] [Locomotion] 1.
Solids and Fluids Chapter 9. Phases of Matter  Solid – definite shape and volume  Liquid – definite volume but assumes the shape of its container 
Chapter 7 Rotational Motion and the Law of Gravity
المحاضرة الثالثة Circular Motion There are two types of circular motion:- 1- Uniform circular motion 2- Non uniform circular motion 1- Uniform circular.
How do you relate the angular acceleration of the object to the linear acceleration of a particular point? There are actually two perpendicular components.
Chapter 5 Circular Motion; Gravitation. 1. Use Newton's second law of motion, the universal law of gravitation, and the concept of centripetal acceleration.
Derivation of the proportionality of velocity and radius for an object in circular motion under a constant centripetal force.
Work, Energy, Power and Conservation Laws. In this week we will introduce the following concepts: o Kinetic energy of a moving object o Work done by a.
LETS Phase 3 Review 4/29/08. Agenda Team Introduction Daedalus Concept Concept of Operations Subsystem Overview Daedalus Performance Daedalus Vision Questions.
How can we study quakes on other planets? Cannot do it entirely from earth Need to send people or landers to the planet Apollo Mission sent astronauts.
Chapter 12.  Newton ’ s first law of motion - an object at rest remains at rest and an object in motion maintains its velocity unless it experiences.
Problem A shuttle is to rendezvous with a space station which is in a circular orbit at an altitude of 250 mi above the surface of the earth. The.
Laplace Meeting - Frascati, April 2008 MSSL/UCL UK Penetrators for Europa MSSL/UCL UK Professor Andrew Coates on behalf of UK Penetrator Consortium.
Proportionality between the velocity V and radius r
ATTOMIC Project Austin Tests Thermodynamics of Moon’s Inner Crust 1.
Circular Motion r v F c, a c. Centripetal acceleration – acceleration of an object in circular motion. It is directed toward the center of the circular.
Unit 6: Circular Motion Consider a Ferris wheel. ◦ The cars are in circular motion because they revolve about a single axis. ◦ The line about which the.
EGU Conference,Vienna, April15, 2008 An Update to MoonLITE Lunar Mission Rob Gowen, MSSL/UCL On behalf of the UK Penetrator Consortium + international.
Europa Penetrator Design and Survivability Testing IPPW10 Sanjay Vijendran, ESA ESTEC Marie-Claire Perkinson, Lester Waugh, Mike Williams, Astrium Tom.
How can we study quakes on other planets? Cannot do it entirely from earth Need to send people or landers to the planet Apollo Mission sent astronauts.
Measuring the Gravity and Magnetic Anomaly of a Rising Lava Plume Chris Jaeger December 3, 2015.
A LOOK AT THE NATURE OF ENERGY Force and Motion. What is Force? A force is a push or pull. A force may give energy to an object, creating motion, stopping.
Tuesday, June 10, 2008PHYS , Summer 2008 Dr. Jaehoon Yu 1 PHYS 1441 – Section 001 Lecture #8 Tuesday, June 10, 2008 Dr. Jaehoon Yu Uniform Circular.
CHINESE CIRCULAR HATCHERY
Chapter8: Conservation of Energy 8-7 Gravitational Potential Energy and Escape Velocity 8-8 Power HW6: Chapter 9: Pb. 10, Pb. 25, Pb. 35, Pb. 50, Pb. 56,
Physics. Gravitation - 2 Session Session Opener How much velocity do you need to impart a stone such that it escapes the gravitational field of the earth?
Application of the Continuity Equation Dr. Eyad Abushandi.
Newton’s Law of Universal Gravitation. Law of Universal Gravitation.
Law of Universal Gravitation Law of Universal Gravitation: gravity is a force of attraction that exists between any two objects that have mass. Force of.
Newton’s Universal Law of Gravity Every object attracts every other object with a force that is directly proportional to the masses of the objects and.
Chapter 11 - Gravity. Example 3 The International Space Station Travels in a roughly circular orbit around the earth. If it’s altitude is 385 km above.
Newton’s thought experiment: orbital velocity. Surface escape velocities Planet V escape, ft/sec Mercury13,600 Venus33,600 Earth36,700 Moon7,800 Mars16,700.
Development of an Astrobiology Penetrator and Delivery System
60 1. What is the mass M in the system as given in the
The Akon Europa Penetrator
Requirements, Alternatives, & ConOps
Payload Concept Review
Bethany, Jay, and Michael
Daedalous Payload Basic Requirements for Single Site Science Box:
The radar band is loosely taken to extend from approximately 0
Kinematics in one Dimension: Uniform motion graphs
Classroom Rocket Scientist
Class Tasks Q1: Water flows into a process unit through a 5-cm ID pipe at a rate of 4.00 m3/h. Calculate Ėk for this stream in joules/second. Q2: Water.
Sarah Shoemaker 3/20/2008 Structures, Gondola Design, Tanks, CAD Final Slides AAE 450 Spring 2008 Structures.
Presentation transcript:

Josh Smith Zachary Blunier Michael Krauz Matt Pensa Daniel Lane Trey Keown quake rattle and roll

Determine the inner structure of EuropaDetermine the inner structure of Europa Rough surface suggests inner geological activityRough surface suggests inner geological activity Caused by either strong tremors or a flowing subsurface oceanCaused by either strong tremors or a flowing subsurface ocean Very interesting candidate for extraterrestrial lifeVery interesting candidate for extraterrestrial life scienceobjectives

operationalstrategy Deploy Seismometer Measurement Mechanisms (SMM) at predetermined locationsDeploy Seismometer Measurement Mechanisms (SMM) at predetermined locations Transfer seismic data back to orbiter as it orbits aboveTransfer seismic data back to orbiter as it orbits above

payloadspecs Two components: EDID and SMMTwo components: EDID and SMM EDID is launcher (double-barreled shotgun)EDID is launcher (double-barreled shotgun) SMMs are ammoSMMs are ammo SMMEDID Dimensions8 cm x 8 cm x 8 cm 4 cm radius Shell Thickness0.5 cm Weight0.5 kg PowerInternal battery Dimensions29cm x 18cm x 46cm Weight5 kg PowerPassive; powered by excess helium in propulsion tank michael’s previousdesigns zach’s

payload technology SMMs has a battery, microprocessor, a seismometer, and a UHF transmitterSMMs has a battery, microprocessor, a seismometer, and a UHF transmitter Continuously collect data and beam back when orbiter passes overheadContinuously collect data and beam back when orbiter passes overhead 16 samples/second, 720 bits/second, 50 mb/week16 samples/second, 720 bits/second, 50 mb/week

physics breakdown Solved for tangential velocitySolved for tangential velocity Found impact velocity from tangental velocityFound impact velocity from tangental velocity From impact velocity, found the penetration depth and decelerationFrom impact velocity, found the penetration depth and deceleration From deceleration and Europa’s gravitational constant, found g-force SMM must sustainFrom deceleration and Europa’s gravitational constant, found g-force SMM must sustain

thank you. questions or comments?