Plutoide: differenze tra le versioni

Versione delle 02:09, 1 nov 2011

Versione delle 02:12, 1 nov 2011

Riga 89:

| '''[[Eris (astronomia)|Eris]]'''

| {{uakm|ua=68.071}}

| {{M|2326|pm=12|k|m}}<ref name="sicardy" />

{{cite journal

| title = Size, density, albedo and atmosphere limit of dwarf planet Eris from a stellar occultation

| journal = European Planetary Science Congress Abstracts

| volume = 6

| year = 2011

| url = http://meetingorganizer.copernicus.org/EPSC-DPS2011/EPSC-DPS2011-137-8.pdf

| accessdate = 2011-09-14

}}

</ref>

| ~{{M|1,6|e=22|k|g}}<ref>Brown, M.E. et al. 2006. Satellites of the Largest Kuiper Belt Objects. Astrophysical Journal, 639:L43-L46 More accurate work based on Dysnomia's orbit in preparation.</ref>

| -1,19

Riga 367 ⟶ 376:

== Note ==

<span style="display:none">

<ref name="sicardy">

{{cite journal

| title = Size, density, albedo and atmosphere limit of dwarf planet Eris from a stellar occultation

| journal = European Planetary Science Congress Abstracts

| volume = 6

| year = 2011

| url = http://meetingorganizer.copernicus.org/EPSC-DPS2011/EPSC-DPS2011-137-8.pdf

| accessdate = 2011-09-14

}}

</ref>

</span>

<references />