Wẹkẹ
Appearance
Wẹkẹ
| Part of | |
|---|---|
| Name in kana | うちゅう |
| Named by | Philipp von Zesen |
| Start time | 13798 million years BCE |
| Has cause | Big Bang |
| Studied by | cosmology, Q12771345 |
| Described at URL | https://baike.sogou.com/v47966.htm |
| Contains | baryonic matter, dark matter, dark energy |
| Has characteristic | gravity, fundamental interaction |
| History of topic | chronology of the universe |
| Shape | unknown value, flatness |
| Stack Exchange tag | https://physics.stackexchange.com/tags/universe, https://astronomy.stackexchange.com/tags/universe, https://philosophy.stackexchange.com/tags/universe |
| Opposite of | antiverse |
Wẹkẹ yin dopo to nudida lẹ mẹ sọn Jiwheyẹwhe de he ko yin didá sọn bẹjẹeji na gbẹtọvi lẹ nado nọ nọ e mẹ.
Tito wẹkẹ lọ tọn
[jlado | jla asisado]Sunwhlẹvu lẹ yin tito tẹnwin-lẹnwin tọn de to agahomẹ, linlinwe lọ Astronomy dọ dọ didẹn de ye dẹn do yede ma yin gbọn kosọ dali. Gbọnna? Dodinnanutọ lẹ dọ dọ nuhe nukun ma sọgan mọ de he nọ yin yiylọdọ matiere noire wẹ nọ hẹn ye dote. Ehe nọ deanana bẹplidopọ sunwhlẹvu lẹ tọn, pẹvi, daho po daho blibata lẹ po.