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Hoshi Stars星

The stars you can see without a telescope, with names, colours and distances; the 88 constellations with their lines and boundaries; the Messier objects; and seven map projections to draw them on.

Hoshi is the Japanese word 星 for a star. About the name

Contents

Reference · Your sky: altitude and azimuth for a place and a moment

PlanetSpintype

The spin of another planet, as the IAU WGCCRE gives it: where its north pole points, and how far its prime meridian has turned.

The pole is a right ascension and declination in the ICRF (the same J2000 frame as the star positions). The prime meridian is W = w0 + rate * d, with d the days since J2000.0 (2000 January 1.5): w0 is W at J2000 in degrees and rate the degrees a day (negative for a planet that turns backwards, such as Venus). W is the angle, east, from the point where the planet's equator crosses the ICRF equator going north (the right ascension of the pole plus 90 degrees) to its prime meridian.

Import it

import type { PlanetSpin } from "@johnmorrisdotca/hoshi-stars/sky";

Definition

interface PlanetSpin {
    pole: SkyPoint;
    primeMeridian: {
        w0: number;
        rate: number;
    };
}

Members

NameTypeDescription
poleSkyPoint

The direction of the planet's north pole at J2000, in degrees.

primeMeridian{ w0: number; rate: number; }

The prime meridian: w0 degrees at J2000 and rate degrees a day.

Examples

import type { PlanetSpin } from "@johnmorrisdotca/hoshi-stars/sky";

// Mars, IAU 2015 values at J2000 (the slow drift of the pole is left out)
const mars: PlanetSpin = { pole: { rightAscension: 317.269202, declination: 54.432516 }, primeMeridian: { w0: 176.049863, rate: 350.891982443297 } };
console.log(mars.pole.declination);
54.432516

What it prints (run when this page was built)

View sourceEdit on GitHubMade from the source of @johnmorrisdotca/hoshi-stars 0.7.0.