⭐ Stellar Distance Laboratory

🌌 Night Sky Observer

Explore the night sky in 3D. Adjust time and date to see how the sky changes.

Loading star database...
Facing: N | Alt: 45Β° | FOV: 90Β°
21:00
Toronto time
Nov 28, 2025
β˜€οΈ Sun: -15Β° below horizon
Moon: --
Loading...
πŸ–±οΈ Drag to look around (any direction) β€’ Click star to select β€’ Scroll to zoom
12 3 6 9 β˜€οΈ πŸŒ™
Click time to type Β· spin past midnight to change date

Selected Star

Click on a star to select it

πŸ”₯ Blackbody Spectrum Simulator

Adjust the temperature to match your star's color. This determines the surface temperature.

Blackbody Temperature

K
2,000 K 40,000 K

πŸ”¬ Absorption Spectrum Analysis

Analyze the star's absorption spectrum to determine its spectral class. Compare with reference spectra.

πŸ“‹ From Previous Steps
Star: --
Temperature: --
Temp Class: --
--
Temperature Class: --

Determine Spectral Type

Select the spectral type that best matches the star's spectrum.

Normal 1.0x 3x Zoom
Click and drag to pan when zoomed

πŸ“Š Hertzsprung-Russell Diagram

Drag the star, use sliders, or type a temperature to position your star on the H-R diagram.

K

πŸ“‹ From Previous Steps

Selected Star --
Apparent Mag --
Observed Color --
Your Temp Estimate --

Derived Properties

Temperature --
Luminosity --
Absolute Mag --
Radius --
Spectral Type --

πŸ““ Observation Notebook

Name -- --
ID -- --
Constellation -- --
Apparent Magnitude -- --
Temperature (K) -- --
Spectral Class -- --
Luminosity Class -- --
H-R Diagram Position -- --
Luminosity (Lβ˜‰) -- --
Radius (Rβ˜‰) -- --
Absolute Magnitude -- --
Distance (Light Years) -- --

⚠️ Please record the distance in your notebook before proceeding.

πŸ“ Distance Calculator

Compare apparent and absolute magnitude to calculate the distance to your star.

Apparent Magnitude (m)

How bright the star appears from Earth

Enter value from your notebook

Absolute Magnitude (M)

Brightness at 10 parsecs (32.6 ly)

Enter value from your notebook

Distance Modulus

m - M = 5Β·log₁₀(d/10)

--
ΞΌ = m - M

🎯 Calculated Distance to Star

-- light years
d = 10^((m - M + 5) / 5) Γ— 3.262 light years

πŸ““ Results Comparison

Observations Actual Values Error Analysis
Name -- --
ID -- --
Constellation -- --
Apparent Magnitude -- --
Temperature (K) -- --
Spectral Class -- --
Luminosity Class -- --
H-R Diagram Position -- --
Luminosity (Lβ˜‰) -- --
Radius (Rβ˜‰) -- --
Absolute Magnitude -- --
Distance (Light Years) -- --

πŸ“Š Results & Accuracy

Compare your measurements and classifications with the actual star data.

Overall Accuracy Score

--
--

πŸ“ H-R Diagram Comparison

Your estimated position (gold ring) vs. the star's actual position (solid circle)

Your Estimate
Actual Position