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=== Circumstellar discs === Based on observations between 2007 and 2012, a study found a slight excess of emissions in the 24 [[Micrometre|μm]] (mid/far-infrared) band surrounding {{nobr|α Centauri AB}}, which may be interpreted as evidence for a sparse [[circumstellar disc]] or dense [[interplanetary dust cloud|interplanetary dust]].<ref name="Wiegart2014"/> The total mass was estimated to be between {{10^|-7}} to {{10^|-6}} the mass of the [[Moon]], or 10–100 times the mass of the Solar System's [[zodiacal cloud]].<ref name=Wiegart2014/> If such a disc existed around both stars, {{nobr|α Centauri A's}} disc would likely be stable to {{nobr|2.8 AU,}} and {{nobr|α Centauri B's}} would likely be stable to {{nobr|2.5 AU }}<ref name=Wiegart2014/> This would put A's disc entirely within the [[frost line (astrophysics)|frost line]], and a small part of B's outer disc just outside.<ref name=Wiegart2014> {{cite journal |last1 = Wiegert |first1 = J. |last2 = Liseau |first2 = R. |last3 = Thébault |first3 = P. |last4 = Olofsson |first4 = G. |last5 = Mora |first5 = A. |last6 = Bryden |first6 = G. |last7 = Marshall |first7 = J.P. |last8 = Eiroa |first8 = C. |last9 = Montesinos |first9 = B. |last10 = Ardila |first10 = D. |last11 = Augereau |first11 = J.C. |last12 = Bayo Aran |first12 = A. |last13 = Danchi |first13 = W.C. |last14 = del Burgo |first14 = C. |last15 = Ertel |first15 = S. |last16 = Fridlund |first16 = M.C.W. |last17 = Hajigholi |first17 = M. |last18 = Krivov |first18 = A.V. |last19 = Pilbratt |first19 = G.L. |last20 = Roberge |first20 = A. |last21 = White |first21 = G.J. |last22 = Wolf |first22 = S. |display-authors = 6 |date = March 2014 |title = How dusty is {{nobr|α Centauri?}} Excess or non-excess over the infrared photospheres of main-sequence stars |journal = [[Astronomy & Astrophysics]] |volume = 563 |page = A102 |doi = 10.1051/0004-6361/201321887 |bibcode = 2014A&A...563A.102W |arxiv = 1401.6896 |s2cid = 119198201 }} </ref>
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