MISSION 001Astrophysics
Why Stars Shine
Proton–proton fusion, quantum tunnelling, and the hundred-thousand-year journey a photon takes from the solar core to the surface.
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A Cosmic Journey
Hi, I'm Hestia Quinna
Exploring Physics, Astronomy and Artificial Intelligence.
Exploring the Universe, One Question at a Time.
🌍 Earth
It begins at home.
A pale blue dot suspended in a sunbeam — the only world we have ever known to hold curiosity. Every question I ask starts from this fragile, luminous ground.
🌙 Moon
Our first step outward.
The Moon taught humanity that the sky is a place, not a ceiling. Tides, eclipses, and libration — my earliest notebooks are full of its quiet arithmetic.
☀️ Solar System
A family of worlds.
Eight planets locked in Kepler's elegant dance. Studying their orbits is where physics stopped being equations on a page and became the machinery of the cosmos.
🌌 Milky Way
Two hundred billion suns.
A barred spiral we live inside and can never photograph from without. Between its arms lie the questions I want to spend a lifetime answering.
Choose a world. Open the research.
Each planet holds a working investigation — from a physics simulation down to the paper and the reproducible notebook behind it.
Mars
Modelling dust-storm dynamics and thin-atmosphere heat transfer.
- 1
Physics Simulation
A 1-D radiative–convective model of the Martian boundary layer, exploring how suspended dust reshapes the daytime temperature profile.
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Python Code
NumPy + SciPy integrator with a Monte-Carlo scattering kernel; results plotted against Viking lander telemetry for validation.
- 3
Paper
“Thermal Response of the Martian Lower Atmosphere to Dust Loading” — draft manuscript, methods and figures complete.
- 4
Notebook
Fully reproducible Jupyter notebook: derivation, code, and every figure regenerated from raw data in one run.
Mission Log
Not a blog — a record of expeditions into ideas. Each entry is logged like a transmission from the field.
MISSION 002Physics
Understanding Gravity
From Newton's inverse square to Einstein's curved spacetime — how the weakest force ends up shaping the largest structures.
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MISSION 003Relativity
Black Holes
Event horizons, Hawking radiation, and why an object with no surface can still be the loudest thing in a galaxy.
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MISSION 004Spectroscopy
The Language of Light
Every element signs its name in spectral lines. How we read the temperature, motion, and chemistry of a star we can never touch.
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MISSION 005AI + Astronomy
Teaching Machines to See Galaxies
Training a convolutional network to classify galaxy morphology — where artificial intelligence meets the deep sky.
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MISSION 006Celestial Mechanics
The Shape of an Orbit
Conic sections, escape velocity, and Kepler's second law — a hands-on derivation of why planets sweep equal areas in equal times.
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The Space Station
Every achievement is a satellite in orbit. The more we accomplish, the busier the sky above the station becomes.
🛰️
Tap a satellite to inspect the achievement it carries.
A Rocket Launch, not a straight line
The plan reads from the ground up — ignition first, deep space last.
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2035+
Research
Toward original contributions in astrophysics and AI — the questions I don't yet know how to ask.
2030
MIT / Caltech
Undergraduate physics & astronomy — the observatory doors open wider.
2028
IOAA
Target: represent the national team at the International Olympiad on Astronomy and Astrophysics.
2027
Ascent
National olympiad campaigns in physics and astronomy; first peer-reviewed submission drafted.
2026
Ignition
Launch of this scientific identity. First research notebooks and the science journal go public.
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🔭 About
A scientist in the making.
I'm Hestia Quinna — a student captivated by the physics of the very large and the very small, by the choreography of the planets, and by the machines we are teaching to help us see farther.
This site is not a blog. It is a digital scientific identity — a growing record of research, olympiads, and questions, meant to evolve alongside a career from the classroom to the observatory.
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