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Quark Planet?

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A quark planet? Really? I'm afraid I'm skeptical on that count.

In order for quark degeneracy (which is still a theoretical concept) to occur, you require an extremely high density. I don't believe any planetary mass object would be capable of attaining and maintaining such a density. It's still quite likely that this planets composition may be very different to those known to us, but this would be due to it being born in a supernova.

Any thoughts? --InvaderXan (talk) 10:52, 17 March 2010 (UTC)[reply]


Requested move 02 July 2014

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The following discussion is an archived discussion of a requested move. Please do not modify it. Subsequent comments should be made in a new section on the talk page. Editors desiring to contest the closing decision should consider a move review. No further edits should be made to this section.

The result of the move request was: moved. Jenks24 (talk) 07:45, 9 July 2014 (UTC)[reply]



PSR B1828-10PSR B1828-11 – The list of articles in SIMBAD [1] shows that the designation PSR B1828-11 is more frequently-used than the PSR B1828-10 designation. 77.57.25.250 (talk) 22:09, 2 July 2014 (UTC)[reply]

Survey

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Feel free to state your position on the renaming proposal by beginning a new line in this section with *'''Support''' or *'''Oppose''', then sign your comment with ~~~~. Since polling is not a substitute for discussion, please explain your reasons, taking into account Wikipedia's policy on article titles.

Discussion

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Any additional comments:

The above discussion is preserved as an archive of a requested move. Please do not modify it. Subsequent comments should be made in a new section on this talk page or in a move review. No further edits should be made to this section.

Orbitbox

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The PSR B1828−11 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
A (unconfirmed) 3 M🜨 0.93 384.3649 0
B (unconfirmed) 12 M🜨 1.32 493.077375
C (unconfirmed) 8 M🜨
The PSR B1828−11 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b (unconfirmed) ≥0.0019 M🜨 ? ? ?

Why have the above orbitboxes above been removed? 🪐Kepler-1229b | talk | contribs🪐 19:33, 29 January 2021 (UTC)[reply]

The first because the planets were disproven, as the article states; the second I don't know. SevenSpheresCelestia (talk) 20:16, 29 January 2021 (UTC)[reply]