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Low-activity Main-belt Comet 133P/Elst-Pizarro: New Constraints on Its Albedo, Temperature, and Active Mechanism from a Thermophysical Perspective

机译:低活动主带彗星133p / elst-pizarro:来自热物理视角的新约束,温度和活性机制

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133P/Elst-Pizarro is the first recognized main-belt comet, but we still know little about its nucleus.First we use mid-infrared data of Spitzer MIPS, Spitzer IRS, and the Wide-field Infrared Survey Explorer to estimate its effective diameter, ${D}_{mathrm{eff}}={3.9}_{-0.3}^{+0.4}$ km, geometric albedo, ${p}_{{m{v}}}=0.074pm 0.013$, and mean Bond albedo ${A}_{mathrm{eff},{m{B}}}=0.024pm 0.004$.The albedo is used to compute 133P's temperature distribution, which shows significant seasonal variation, especially polar regions, ranging from ~40 to ~200 K.Based on current activity observations, the maximum water gas production rate is estimated to be $sim 1.4imes {10}^{23},{{m{s}}}^{-1}$, being far weaker than $sim {10}^{26},{{m{s}}}^{-1}$ of JFC 67P at a similar heliocentric distance of ~2.7 au, indicating a thick dust mantle on the surface to lower down the gas production rate.The diameter of the sublimation area may be 100 Myr, indicating that 133P may be more likely to be a relatively old planetesimals or a member of an old family than a recently formed fragment of some young family.
机译:133P / ELST-PIZARRO是第一个公认的主腰带彗星,但我们仍然涉及其核心。首先,我们使用SPITZER MIPS,SPITZER IRS的中红外数据和广泛的红外测量探险家来估算其有效直径,$ {d} _ { mathrm {upm}} = {3.9} _ { - 0.3} ^ { - 0.3} ^ {+ 0.4} $ ick,几何albedo,$ {p} _ {{ rm {v}}} = 0.074 PM 0.013 $,均值键入Albedo $ {a} _ { mathrm {eff},{ rm {b}}} = 0.024 pm 0.004 $。Albedo用于计算133p的温度分布,这显示出显着的季节变化,特别是极地区域,范围从〜40到〜200 k。基于当前的活动观察,估计最大水源生产率为$ sim 1.4 times {10} ^ {23} ,{{ rm { }}}}}}}}} ^ { - 1} $,远远弱于$ sim {10} ^ {26} ,{{ rm {s}} ^ {{ rm {s}} ^ { - 1} $ of JFC 67p,在类似的天真距离〜2.7 Au,表示表面上的厚尘套,降低气体生产率。升华区域的直径可以是100 myR,表明133p可能更有可能是一个比较旧的星球或旧家庭的成员,而不是一些年轻家庭的最近形成的片段。

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