Quantum redactiones paginae "Classis spectralis" differant
Content deleted Content added
mNo edit summary |
|||
Linea 1:
{{Vicificanda}}{{latinitas|-
== Classificatio Harvardiana ==
[[Imago:Morgan-Keenan spectral classification.png|500px|right|thumb|Classificatio Harvardiana]]
Classificatione Harvardiana, stellae dividuntur in classes O—B—A—F—G—K—M—C—S. Plerumque communes sunt stellae classium O—B—A—F—G—K—M, quae appellantur "stellae normales," sed stellae classium C—S (atque R, N, T, L) sunt "stellae peculiares," hoc est stellae quae spectrum "peculiare" habent.
Line 57 ⟶ 58:
|style="background:#f8f7ff;"| albus
| 1.7 [[Massa solaris |M<sub>☉</sub>]]
| 1.3 [[
| 6 [[Luminocitas solaris|L<sub>☉</sub>]]
| medii
| 3%
|- style="background:#fff4ea;"
!style="background:#fff4ea;"| [[#
| 5,000–6,000 K
|style="background:#fff2a1;"| flavus
Line 72 ⟶ 73:
| 8%
|- style="background:#ffd2a1;"
!style="background:#ffd2a1;"| [[#
| 3,500–5,000 K
|style="background:#ffc46f;"| aurantinus
Line 82 ⟶ 83:
| 13%
|- style="background:#ffcc6f;"
!style="background:#ffcc6f;"| [[#
| 2,000–3,500 K
|style="background:#ff6060;"| Ruber
Line 94 ⟶ 95:
== Classificatio Yerkes ==
Factor supplementaruis afficiens in characterem spectri est densitas stratorum exteriorum stellae, dependens a massa et densitate stellae, hoc est a luminositate. Admodum a lumnositate
Ha clssificatione stella habet classem luminocitatis:
| |||