Observatory’s Primary Objectives

  1. Follow-up observations of Near Earth Asteroids (1,168 observations, including 150 all MPECs- as of 30 June, 2026)

  2. Finding The Rotation period of bright asteroids

  3. Multi-Band BVR Photometry of Variable Stars (4,025 observations as of 30 June, 2026)

  4. Spectroscopy of Stars

Observatory Equipment

Celestron Edge HD 8

Paramount Myt Mount MKS 6000

PrimaLuce SCT LP Focuser

Wanderer Astro Flat Panel

Player One 571 Mono 16bit, Filter Wheel 7×2”

Astrodon Filters BVI

LRGB, SHO, IR & Exoplanet Filters

Spectroscope Shelyak Alpy 600

Shelyak Guiding Module

Shelyak Calibration Module

Starlight Xpress All CCD Sky Camera

AAG CloudWatcher with Anemometer & SOLO

Beelink Mini PC

Wanderer Astro Power Box V3

Observations & Analysis at the Observatory

Three Period Analysis (3.5671 Hours) of δ Scuti Star DY Her in V Band

Photometric Determination of the Rotation Period of (20) Massalia

More than 1,000 submissions of variable stars to AAVSO

Near Earth Asteroids’ Submission report