139 asteroids are passing through Earth's neighborhood this month.

neoradar.space · 2026-07-22 · by Long Nguyen ·generic
Real orbital-mechanics engine for tracking Near-Earth Objects. Heliocentric N-body simulation with Newton-Raphson Kepler solver, RK4 adaptive integrator, and live perturbation from Jupiter and Saturn.

139 asteroids are passing through

Earth's neighborhood this month.

Open Radar

Data · JPL Horizons MAY · 2026

139 asteroids are passing through

Earth's neighborhood this month.

NEO Radar is a real orbital-mechanics engine for tracking Near-Earth Objects. 47 high-fidelity objects with full RK4 N-body dynamics, plus 41,812 MPC catalog asteroids with real positions — all 8 planets simulated. Click any asteroid for a complete physical dossier.

Open Radar How it works

Next Close Approach

0.71lunar distances

2025 PT5 · in 2 d 14 h 22 m

2024 YR4

a=1.18 AU · e=0.66

Monitor 0.94 LD

Apophis

99942 · NEA, Aten

Caution 31,800 km

2025 QV1

a=0.93 AU · e=0.41

Safe 2.4 LD

View All 41,859 Tracked

Engineering

Real physics. Not approximations.

Every trajectory in NEO Radar is integrated from JPL Horizons ephemeris with full gravitational perturbation from the outer planets. The numbers you see are the numbers a mission planner would see.

E₀ → E₁ → E₂ → E₃ ε < 1e-12

01 / Kepler

Solves Kepler's equation, not lookup tables.

Mean anomaly to eccentric anomaly via Newton-Raphson with adaptive seed, converging to 1×10⁻¹² in under four iterations even for high-eccentricity orbits.

M → E → ν e < 0.99 ε = 1e-12

\+ Δv

02 / Perturbation

Jupiter and Saturn pulled, and you see the pull.

Toggle outer-planet gravity on or off. The uncertainty cone widens visibly on Jupiter-flyby trajectories — what mission planners call the keyhole problem.

N-body RK4 Adaptive Δt All 8 planets

1999 2025 2050 26 yr arc σ = 412 km

03 / Data

JPL Horizons ephemeris, locally cached.

Pulled directly from JPL Horizons and pinned to disk for instant access. Observation arcs and uncertainty parameters travel with every object — no approximations, no drift.

NASA NeoWs SPICE kernels Local cache

Trust

How accurate is it?

We benchmark every NEO Radar trajectory against JPL Horizons ephemeris over a 50-year window. Where simplified two-body models drift by tens of thousands of kilometers, NEO Radar stays inside the actual uncertainty cone.

Position accuracy is computed as RMS deviation from JPL ground truth across the same 50-year window for the 47 high-fidelity objects.

NEO Radar 412 km

Kepler-only 18,400 km

2-body sim 112,000 km

Position RMS · 50 yr

412 km

Catalog Objects

41,859

Integrator Order

RK4

Adaptive Δt

10⁻³–10⁰ d

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