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All-Sky Meteor Camera

Nepal's first contribution to the Global Meteor Network (GMN). Wide-field camera for meteor detection, trajectory triangulation, and spectroscopy from Himalayan skies.

What it measures

Meteor detections with trajectory data, velocity, and orbital elements. Spectroscopy of brighter events for compositional analysis.

An all-sky camera for Nepal's meteor sky

An all-sky meteor camera is a fixed, upward-pointing camera with a fisheye lens that watches the entire night sky at once and automatically detects the brief streaks of meteors. Paired with a second camera some distance away, the same meteor seen from two viewpoints can be triangulated in three dimensions — recovering its speed, altitude, and the orbit it came from. This is HICS's first node for the Global Meteor Network (GMN).

~180°
all-sky field of view
a single fisheye sees the whole hemisphere
IMX291
Sony low-light sensor
sensitive enough for faint meteors
RMS
open detection software
GMN-compatible, runs on a Raspberry Pi

From a streak of light to an orbit

1 · Fisheye optics + IMX291 sensor

A wide fisheye lens images the whole sky onto a sensitive Sony IMX291 low-light sensor, capturing the night sky continuously.

2 · RMS detection software

The open-source RMS (Raspberry Pi Meteor Station) software runs on a Raspberry Pi, automatically detecting meteor streaks frame-by-frame and logging each event with a precise timestamp.

3 · Triangulation

When two or more stations record the same meteor, its three-dimensional path is triangulated from the different viewing angles — giving real height and velocity, not just a 2-D streak.

4 · Orbits and flux to the network

From the trajectory and speed, the meteoroid's original orbit around the Sun is reconstructed. Detections, orbits, and flux statistics feed back to the Global Meteor Network.

Why a grain of sand makes a streak of light

Meteoroids enter the atmosphere at 11–72 km/s. Even a sand-grain-sized particle carries enormous kinetic energy at those speeds — energy that goes into heating and ablating the grain, which excites the surrounding air to glow:

Kinetic energy of a meteoroid. Because energy scales with v², the entry speed matters far more than the mass — a tiny fast grain outshines a larger slow one.
Part of the Meteor Astronomy programme

This camera is the instrument behind HICS's Meteor Astronomy research programme — Nepal's first presence in the Global Meteor Network, from a geographic gap with near-zero coverage.

Current status

Planned. No camera is deployed yet — this page describes the design. The first station establishes Nepal's node in the network.