(386723) 2009 YE7: Diferenzas entre revisións
Contido eliminado Contido engadido
Liña 101:
{{Imaxe-Mapa TNOs}}
[[Michael E. Brown|Mike Brown]] believes that {{mp|2009 YE|7}} may be a [[Haumea family]] fragment due to the Haumea-like inclination of the orbit.<ref name="Brown2009"/> If this is the case, {{mp|2009 YE|7}} could have an albedo of up to 0.7, resulting in a smaller size closer to the 200km estimate. If [[infrared spectrum]]s show that {{mp|2009 YE|7}} has evidence of deep water ice absorption features, it would link {{mp|2009 YE|7}} to the Haumea family.<ref name="Brown2009"/>
Any icy body with a diameter greater than 400 km is likely spherical.<ref name=Brown> {{
|url=http://web.gps.caltech.edu/~mbrown/dwarfplanets/
|
|
|
== Referencias ==
|