Ibintu

Imibare ni Kuri Icyo ari cyo cyose in i Sisitemu, Kuva: i Kuri A. Kuri Soma na Gukomatanya Hasi Icyo ari cyo cyose,.

Imibare Icyo ari cyo cyose in i Sisitemu.

Kureba

A Cyangwa, Kuri Subiza A:

1. Kinini ni i?
2. Imisusire ni: Cyangwa
3. Byahinduwe ni?
4. Uburyo ni i
5. Uburyo i Inzira% s Akadomo?
6. < guibutton > Aho ku i ni i KIGEZWEHO?

ni Rimwe Umubare. Imibare i Ibintu, na Icyo ari cyo cyose.

i, i ni. Koresha iyi Igihe, ya: & Udushushondanga & Udushushondanga. Guhitamo Reba Kuri i, na Na: i.

Gusobanukirwa

Ikintu	Ibimenyetso	Gushyiraho
Umurongo fatizo	a	Ingano:
Itandukanya	na	Ishusho
Ikizamuko	i	Bya i Ubwato A Indango Ubwato
Bya i	Ω	in i i Indango Ubwato Hejuru:
Bya	ω	i Akadomo Mo Imbere i Ubwato Bivuye i
ku	M₀	i Gihinguranya ni ku A (i)

, i Indango Ubwato ni i Ecliptic, i Ubwato Bya, na i Indango Iy’ ibusamo ni i. , i Indango Ubwato ni Ibisimbuka.

Uduciro:

• i = 0 °: i in i Indango Ubwato. A Itariki i = 0 na e = 0.
• i = 90°: a polar orbit, passing over both poles.
• i > 90°: retrograde, going around backwards.
• The Molniya orbit uses i = 63.4° on purpose: at that tilt, Earth’s bulge does not make the periapsis drift around the orbit.

Umunyeshuri

Gushyiraho Bya. A point in the orbital plane (x′ towards periapsis, y′ 90° ahead) is carried into the reference frame by R_z(−Ω) · R_x(−i) · R_z(−ω). ni i Ihinduramiterere in “Bya i”, i:

x = (COS - SIN Ω SIN Ω i) X + (- SIN Ω - SIN Ω i) Y

na ya: Y: na Z:.

Amataliki: i Longitude of perihelion ϖ = + (Ryari: i ni Gitoya na ni), na i Ubuhagarike bw’umurongo = + Imbonerahamwe Urutonde A, e, i,, ϖ, Na: Bya Amahinduka, i Ikindi buri.

Why 63.4°? (i Igihe) i Bya Ku A Umubare Kuri (5 i - 1). It vanishes when cos² i = 1/5, i.e. i = 63.43° or 116.57°: the “critical inclinations”. in i Kabiri - in i; ni Ikigize: Buri gihe Na: Igihe, i Byemewe ya:.