Astronomy Distance Converters
Convert astronomical and space-scale distances across AU, light-years, parsecs, lunar distance, and standard metric or imperial units.
Scope & Verification
This hub groups related converter families so you can move from the category level to exact routes with one clear basis per page.
- Families are split so exact-factor, profile-based, density-based, and estimate-style pages do not collapse into one generic answer.
- Leaf pages keep calculator, common values, FAQ, and reverse routes aligned to the same assumption.
- Methodology and verification pages document how those assumptions are chosen and checked.
Public interfaces
Machine access
Conversions in this hub are represented by the canonical astronomy-distance family and its registered source and target units.
Its 210 published directions use the same canonical engine through the website, JSON API, OpenAPI and WebMCP.
API & Agent documentationExplanation
This hub groups astronomy distance conversions used for educational, observational, and astrophysical scale comparisons. Unit relationships are normalized through fixed meter-based constants, including the exact astronomical unit definition and standard light-time/parsec relationships used in scientific references.
Astronomy Distance pages are organized by conversion direction so mirror leaves remain aligned and comparable.
Open a family hub to reach leaf pages with direct answers, calculator output, and reverse links built on the same constants.
Questions & answers
Frequently Asked Questions
What units are included in this astronomy distance hub?
It includes AU, light-seconds, light-years, parsecs (pc, kpc, Mpc, Gpc), lunar distance, Earth/Solar radii and diameters, plus km, meters, and miles.
Are these conversion factors fixed constants?
Yes. Every factor is derived from fixed meter-based constants so mirror conversions remain consistent and reversible.
Can I use decimal inputs for very large distances?
Yes. Decimal values are supported for both near-Earth and deep-space scale conversions.