Astrophyzix Observatory
Evidence-First Publication

Astrophyzix.com is an independent digital observatory publication offering unpaywalled, evidence‑driven analysis and real‑time monitoring of PHAs and NEOs. Our tracking consoles and reporting systems use and provide access to official NASA CNEOS Scout, JPL CAD, NeoWs, JPL SBDB, Horizons and NOAA observational datasets, peer‑reviewed sources, and high‑precision numerical methods (IEEE‑754 Float64, RKN4). Designed for students, educators, researchers, and the public, every console is uniquely designed and engineered by the Astrophyzix Digital Observatory. Our research notes and papers can be found at Astrophyzix.Academia.Edu

Showing posts with label Exoplanets. Show all posts
Showing posts with label Exoplanets. Show all posts

Friday, 1 May 2026

Astrophyzix Launches SolarForm — A Real‑Time Solar System Formation Simulation Engine

A One of a Kind, Unique, Real‑Time Solar System Formation Simulation Engine


Written by: Astrophyzix Digital Observatory

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Platform Update Astrophysics Simulation Educational Module

Introduction

Astrophyzix is proud to announce the release of SolarForm, a scientifically rigorous, real‑time simulation engine that models the birth and evolution of a planetary system from the collapse of a protoplanetary nebula to the emergence of planetesimals, proto‑planets, and gas giants.

SolarForm is designed as an educational scientific module, providing the public, students, and astronomy enthusiasts with a clear, interactive way to explore the physics that shaped our Solar System. The module is powered by real astrophysical equations, peer‑reviewed models, and a direct N‑body gravitational integrator.

A Real‑Time Window Into Planetary Formation

SolarForm simulates the early stages of solar system formation using physically grounded models drawn from astrophysics, celestial mechanics, and planetary science. Users can watch a nebular disk evolve dynamically as bodies collide, merge, accrete, and migrate under gravity.

Key features include:

  • N‑body gravitational physics using a velocity‑Verlet symplectic integrator.
  • Planetesimal growth and accretion through inelastic collisions with gravitational focusing.
  • Protoplanetary disk density profiles based on the Minimum Mass Solar Nebula (MMSN).
  • Keplerian orbital initialization scaled by nebula mass and angular momentum.
  • Snowline physics determining where ice bodies and gas giant cores can form.
  • Real‑time classification of bodies into planetesimals, proto‑planets, rocky planets, and gas giants.

The simulation updates continuously, allowing users to observe the chaotic, emergent behaviour of early planetary systems as they stabilize over time.


Saturday, 28 February 2026

Exoplanets: A Comprehensive Scientific Review

Astrophyzix Digital Observatory Research Dossier

Subject: Exoplanetary Science
Classification: Evidence-First, Peer‑Reviewed Sourced Review
Data Sources: NASA, ESA, ESO, STScI, Nature, PNAS, Annual Reviews

Exoplanets

Exoplanets — A Comprehensive Scientific Review

The detection of planets orbiting stars beyond our Solar System — known as exoplanets — has reshaped astronomy over the past three decades. Prior to 1992, only indirect speculation existed about planets around other stars. Today, nearly 6,000 exoplanets have been confirmed through a variety of observation techniques, revealing planetary systems that challenge traditional theories of formation and habitability. (NASA Exoplanet Archive)

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