Frontiers Briefing Template Slides Mission: [Enter Topic Name Here]
Physics Frontiers Research Briefing
Agent: [Student 1] Agent: [Student 2]
Word Count: 6 / 10
01
The Hook
Capture attention with one bold statement or a question.
Template Tip: Use a high-quality, full-screen image background here.
Word Count: 9 / 10
Key Concepts
[Term 1]
[Term 2]
Explain these definitions out loud. Don't write them here!
Word Count: 4 / 10
Mathematical Model
F = m · a
Explain the relationship between force, mass, and acceleration.
Word Count: 7 / 10
Breaking It Down
F
Force
(Newtons)
m
Mass
(Kilograms)
a
Accel.
(m/s²)
Use this space to explain units and meaning.
Word Count: 9 / 10
Visual Analysis
Insert a graph, diagram, or experimental data image.
Place Diagram Here
Word Count: 8 / 10
Physics in Action
How does this concept impact the real world?
Word Count: 9 / 10
Mission Summary
"One final takeaway you want the class to remember."
Word Count: 9 / 10
Intelligence Log
Reputable Source URL or Citation 01
Reputable Source URL or Citation 02
End of Briefing
Mission Complete
Frontiers Concept Master Guide Internal Use Only REF_ID: PHY-FRONTIER-MG-2026
Frontiers Master Guide
Essential equations, vocabulary, and conceptual standards for the Physics Frontiers Research Project. Use this guide to verify student accuracy during presentations and for final exam alignment.
01. Meteors, Orbits & Gravity
Essential Equation
\[ F_g = G \frac{m_1 m_2}{r^2} \]
Function: Calculates gravitational pull between two masses; models orbital paths and impact forces.
Fg: Gravity (N) | G: Constant | m: Mass | r: Distance
Conceptual Look-Fors
Inverse Square Law: If distance doubles, force drops to 1/4th.
Energy Trade-off: Kinetic vs. Potential in elliptical orbits.
Key Vocabulary
Universal Gravitation
Every particle with mass attracts every other particle with mass.
Elliptical Orbit
Oval-shaped path of a celestial body; gravity acts as centripetal force.
Orbital Velocity
The specific speed required to maintain a stable, constant orbit.
02. Electromagnetic Radiation
Essential Equation
\[ c = f \lambda \]
Function: Relates wave speed to frequency and wavelength; identifies EM spectrum types.
c: Light speed | f: Freq (Hz) | λ: Wavelength (m)
Conceptual Look-Fors
High frequency (short wavelength) = High energy radiation.
Duality: Light behaving as discrete photons and continuous waves.
Key Vocabulary
EM Spectrum
The full range of light waves, from Radio to Gamma rays.
Photon
A quantum packet of light energy; massless but carries momentum.
Ionizing Radiation
Radiation with energy to knock electrons off atoms (UV, X-ray, Gamma).
03. Stellar Lifecycles
Essential Equation
\[ E = mc^2 \]
Function: Calculates energy from mass conversion; explains the massive power of nuclear fusion.
E: Energy (J) | m: Mass lost | c: Speed of light
Conceptual Look-Fors
Equilibrium: Balance between gravity and fusion pressure.
Nucleosynthesis: Forging heavy elements in massive star deaths.
Key Vocabulary
Nuclear Fusion
Combining light atomic nuclei to form heavier ones, releasing energy.
Main Sequence
Stable stage where a star fuses hydrogen into helium.
Supernova
Catastrophic explosion of a massive star at the end of its life.
04. Radioactive Decay
Essential Equation
\[ N(t) = N_0 \left(\frac{1}{2}\right)^n \]
Function: Predicts remaining material after time passes; used for dating and safety modeling.
N(t): Final | N0: Initial | n: Half-lives elapsed
Conceptual Look-Fors
Decay Types: Alpha (part.), Beta (elec.), Gamma (energy).
Stability: Balance of Strong Nuclear force vs. EM repulsion.
Key Vocabulary
Isotope
Atoms of the same element with different neutron numbers.
Half-Life
Time required for half of a radioactive sample to decay.
Binding Energy
The energy required to disassemble a nucleus into components.
05. Physics of Sound
Essential Equation
\[ v = f \lambda \]
Function: Relates sound speed to pitch and wavelength; models resonance and harmonics.
v: Speed (m/s) | f: Frequency | λ: Wavelength
Conceptual Look-Fors
Medium: Speed increases in denser, more elastic materials.
Resonance: Matching natural frequencies to boost amplitude.
Key Vocabulary
Longitudinal Wave
Wave where vibration is parallel to travel direction.
Doppler Effect
Frequency shift caused by relative motion of source/observer.
Pitch
The perceived highness or lowness of a sound frequency.
06. Newton in Motion
Essential Equations
\[ F = ma \quad p = mv \]
Function: F=ma models motion changes; p=mv measures momentum and quantity of motion.
F: Force | a: Accel | p: Momentum | v: Vel
Conceptual Look-Fors
Impulse-Momentum: Extending impact time reduces force.
Rotational Inertia: Mass distribution's effect on angular speed.
Key Vocabulary
Inertia
The tendency of an object to resist changes in its motion.
Center of Mass
Point at which all mass of an object is considered concentrated.
Normal Force
The support force exerted by a surface against weight.
Project Milestone Tracker Milestone Tracker
Physics Frontiers Research Expedition
Mission Deadline 4th: May 15 1st/2nd: May 18 Dance: May 20
1
Discovery
Pair up and select your core physics topic.
Discuss research roles within your partnership.
2
Evidence Acquisition
Complete: Reliable Sources Log
2 reputable sources verified with reliability reasoning.
TEACHER GATEKEEP: SOURCE APPROVAL
3
Physics Synthesis
Complete: Vocab Connection Map
4+ terms defined and conceptually linked.
Complete: Frontier Formula Sheet
1-2 equations with examples and revelations.
TEACHER GATEKEEP: CONTENT VERIFICATION
4
Polishing & Performance
Finalize slides: 10-word limit per slide. High visual impact.
Practice Recording: Submit full run-through video + reflection notes to Canvas.
Must show complete transition between partners and use of all visual aids.
Rehearsal: Practice without reading off notes/cards.
Must meet 6-8 min window with balanced partner speaking time.
MISSION LAUNCH: LIVE PRESENTATION DELIVERED
Mandatory Instructor Checkpoints required for presentation eligibility
Mission Scoring Rubric Mission Scoring Rubric
Physics Frontiers Live Presentation (30 Points Total)
4th: May 15
1/2: May 18
Dance: May 20
Criterion Exceptional (5 pts) Proficient (4 pts) Developing (2 pts) Public Speaking
Eyes, Volume, Familiarity
| Consistent eye contact; no reading cards; familiarity obvious; audible volume. | Frequent eye contact; occasional note checking; audible and mostly comfortable. | Reads directly off cards; little eye contact; volume too low for room. |
|
Content Description
Accuracy & Detail
| Deep, accurate explanation of physics concepts. Answers "why" and "how". | Accurate description of concepts. Covers major points in mission brief. | Surface-level description. Significant inaccuracies or missing components. |
|
Vocabulary Usage
4+ Terms in Flow
| 4+ key terms used naturally and defined accurately within talk flow. | 4 key terms included and defined, but usage may feel forced. | Fewer than 4 terms used; definitions missing or conceptually incorrect. |
|
Equation Analysis
Variables & Revelation
| Equation presented; variables defined; physical meaning perfectly explained. | Equation presented and defined; basic explanation of how formula applies. | Equation missing/incorrect; variables undefined; no meaning explained. |
|
10-Word Rule
Visual impact
| Every slide strictly follows the 10-word limit. High visual impact visuals. | Most slides follow the limit. Minimal clutter. Visuals support content. | Excessive text on slides; 10-word limit ignored. Cluttered layout. |
|
Teamwork & Time
6-8 Mins / Partners
| 6-8 mins. Equal speaking time for all partners; smooth transitions. | 5-9 mins. All partners speak, though time may be unbalanced. | Significant timing issues. One partner dominates speaking time. |
Instructor Feedback
Presentation Total
/ 30
Grade: __________
Note: Research Verification, Vocab Maps, and Formula Sheets are graded as separate checkpoints and are not included in this presentation score.
Impact Dynamics Example Slides Mission: Impact Dynamics
Collisions and Momentum Intelligence Briefing
Agent: Lenny Agent: Physics Pro
Word Count: 6 / 10
01
The Hook
How do massive semi-trucks stop without causing total destruction?
It all comes down to the physics of momentum.
Word Count: 9 / 10
Key Concepts
Momentum
Impulse
Inertia in motion vs. the change in that motion.
Word Count: 8 / 10
Conservation Law
p_i = p_f
Initial momentum equals final momentum in a closed system.
Word Count: 9 / 10
Breaking It Down
m
Mass
(kg)
v
Velocity
(m/s)
Momentum is the product of mass and velocity.
Word Count: 7 / 10
Collision Types
Bouncing vs. Sticking: Elastic and Inelastic interactions.
Elastic
Inelastic
Word Count: 7 / 10
Safety Engineering
Crumple zones increase impact time to decrease force.
Word Count: 8 / 10
Mission Summary
"Momentum is never lost, only transferred between objects."
Word Count: 8 / 10
Intelligence Log
IIHS: Crash Test Safety Ratings Database
Physics Classroom: Momentum and Its Conservation
Briefing Complete
Mission Success
Physics Frontiers Project Brief Physics Frontiers
Research Presentation Assignment
Name: __________________________
Partner: __________________________
Mission Objective
Become an expert on a specific niche of physics. Deliver a 6-8 minute briefing supported by reputable evidence, mathematical modeling, and precise terminology. Slides must follow the 10-word limit rule —let your visuals and your voice do the teaching.
Visual Guidelines
Max 10 words per slide.
Include diagrams, graphs, and high-quality visuals.
Equal partner speaking time (6-8 mins total).
Mandatory Checkpoints
Verify with instructor before presenting
Sources: 2 Reputable (verified with log).Vocabulary: Connection Map for 4+ terms.Equation: Formula Sheet with solved example.
Presentation Standards & Scoring (30 Points)
Performance (15)
Public Speaking: Eye contact, no reading cards, audible volume.10-Word Rule: Strict limit per slide.Teamwork: Balanced time.
Physics (10)
Description: Accurate explanation of concepts.Vocabulary: 4+ terms defined naturally in talk.
Math (5)
Equation: Formula meaning and variables revealed.
*Presentation Field Notes (Graded Separately): 10 pts
Submit via LMS Portal
Launch Window
4th Period
MAY 15
1st & 2nd
MAY 18
Dancers
MAY 20
Presentation Live Scoring Sheet Frontiers Live Scoring Sheet
Teacher Resource • Presentation Day Workflow
Target Score
30 PTS
Scale:
Exceptional: 5 pts
Proficient: 4 pts
Developing: 2 pts
01
Presenters / Topic
________________________________
Start / End
_______ / _______
Performance (15 pts)
Public SpeakingEyes up, volume
/5
10-Word RuleStrict limit
/5
Teamwork & Timing6-8 min window
/5
Observational notes...
Physics Content (15 pts)
Content DescriptionDeep/Accurate
/5
Vocabulary UsageDefined in talk
/5
Equation AnalysisMeaning revealed
/5
One-Word Takeaway:
________________________
02
Presenters / Topic
________________________________
Start / End
_______ / _______
Performance (15 pts)
Public SpeakingEyes up, volume
/5
10-Word RuleStrict limit
/5
Teamwork & Timing6-8 min window
/5
Observational notes...
Physics Content (15 pts)
Content DescriptionDeep/Accurate
/5
Vocabulary UsageDefined in talk
/5
Equation AnalysisMeaning revealed
/5
One-Word Takeaway:
________________________
Presentation-only score (30 pts). Checkpoints are graded separately.
PHYS-9_FRONTIERS_LIVE_V3
Frontiers Project Launch Slides Physics Frontiers
Project Launch Briefing
THE 10-WORD RULE
NO MORE THAN 10 WORDS ON ANY SLIDE.
Strictly Enforced Scoring
Source Verification
Phase 1:
TWO REPUTABLE SOURCES LOGGED
Mandatory Checkpoint
Teacher approval required before slides begin.
Content Verification
Phase 2:
VOCAB MAP & FORMULA SHEET
Mandatory Checkpoint
Accuracy check must be complete before rehearsal.
The Live Briefing
Eyes Up, No Reading
Speak with Authority
Balanced Partnership
30 Point Rubric
Performance 15 pts
Physics Content 10 pts
Math Analysis 5 pts
DEADLINES
4th
MAY 15
1st / 2nd
MAY 18
Dancers
MAY 20
Reliable Sources Log Reliable Sources Log
Frontier Mission 02: Evidence Acquisition
DUE DATES:
4th: May 15
1/2: May 18
Dance: May 20
Reliability Check
Justify reliability using Authority (expertise), Accuracy (verified info), and Purpose (educational intent).
Name: ________________
Topic: ________________
1
Primary Source
Title / Author / Organization
URL / Publication Detail
Reliability Justification
2
Secondary Source
Title / Author / Organization
URL / Publication Detail
Reliability Justification
SOURCE VERIFICATION
Instructor initials required before synthesis
Vocab Connection Map Vocab Connection Map
Mission 03: Conceptual Mapping
DUE DATES:
4th: May 15 | 1/2: May 18 | Dancers: May 20
Key Term 01
Definition
Key Term 02
Definition
Key Term 03
Definition
Key Term 04
Definition
The Web: Term Connections
How do these terms relate to each other in a logical narrative?
Big Picture: Frontier Connection
How do these terms explain your main Frontier topic?
Mission_Synthesizer_v2.0
Student Name: ____________________
Frontier Formula Sheet Frontier Formula Sheet
Mission 03: Mathematical Modeling
DUE DATES:
4th: May 15 | 1/2: May 18 | Dancers: May 20
1
Primary Equation
Formula Here
Variable Key (Symbol = Unit)
Example Calculation
Mathematical Revelation (What does this prove?)
2
Secondary Equation
Formula Here
Variable Key
Example Calculation
Mathematical Revelation
Physics_Frontier_Model_v2
Name: ____________________
Topic Explorer Guide Topic Sector 01
Meteors, Orbits & Gravity
The Mission Brief
Why do planets stay in orbit? Why don't meteors just fly off into space? This research area dives into the invisible strings that hold the universe together. You'll explore how energy transfers during cosmic collisions and the mathematical laws that govern every move in the solar system.
Core Concepts
Newton's Universal Law of Gravitation
Kepler's Three Laws of Planetary Motion
Kinetic vs. Potential Energy in Orbits
Forces at a Distance
Why choose this?
"If you want to understand how the giant clockwork of the universe ticks, this is your topic. You'll explain everything from falling stars to why the Moon doesn't crash into Earth."
Explain the "invisible force"
Model elliptical paths
Analyze meteor impacts
Topic Sector 02
Electromagnetic Radiation
The Mission Brief
From the WiFi signals in your pocket to the light from distant galaxies, EM radiation is how the universe communicates. This topic explores the weird duality of light—how it acts like both a wave and a particle—and how different frequencies of light affect the matter they hit.
Core Concepts
The EM Spectrum (Radio to Gamma)
Wave Properties (Frequency, Wavelength)
Wave-Particle Duality (Photons)
Absorption, Reflection, and Transmission
Why choose this?
"Explore the invisible world. You'll explain how we use invisible waves to see through skin (X-rays), cook food (Microwaves), and send messages across the globe."
Decode the spectrum
Explain energy vs frequency
Analyze modern technology
Topic Sector 03
Stellar Lifecycles
The Mission Brief
Stars are the ultimate nuclear laboratories. This topic follows the journey from a collapsing cloud of gas to a spectacular death as a supernova, black hole, or white dwarf. You'll look at the incredible pressure and heat that forces atoms together to create new elements.
Core Concepts
Nuclear Fusion (Hydrogen to Helium)
The Life Cycle (Main Sequence to Remnants)
Supernovae & Element Creation
Stellar Equilibrium (Gravity vs Pressure)
Why choose this?
"We are literally made of star-stuff. Choose this to learn how every atom in your body was once inside a star, and what happens when the most massive objects in the universe run out of fuel."
Frontiers Field Notes Sheet Frontiers Field Notes
10 PTS
Presenter(s)
Frontier Topic
Key Vocabulary Terms
Physics Equation(s)
Main Discovery / "Aha!" Moment
What was the most surprising thing you learned?
MISSION_LOG_OBS_1 Peer Review Participation
Frontiers Field Notes
10 PTS
Presenter(s)
Frontier Topic
Key Vocabulary Terms
Physics Equation(s)
Main Discovery / "Aha!" Moment
What was the most surprising thing you learned?
MISSION_LOG_OBS_2 Peer Review Participation
