Shape models and spin states of Jupiter Trojans: Testing the streaming instability formation Article Swipe
J. Hanuš
,
David Vokrouhlický
,
David Nesvorný
,
Josef Ďurech
,
Robert D. Stephens
,
Ondřej Pejcha
,
Vladimir Benishek
,
Julian Oey
·
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.5194/epsc2022-396
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.5194/epsc2022-396
<div class="ui-layout-east ui-layout-pane ui-layout-pane-east ui-layout-pane-hover ui-layout-pane-east-hover ui-layout-pane-open-hover ui-layout-pane-east-open-hover"> <div class="ng-scope"> <div class="pdf full-size"> <div class="pdf-viewer"> <div class="pdfjs-viewer pdfjs-viewer-outer"> <div class="pdfjs-viewer-inner" tabindex="0" role="tabpanel"> <div class="pdfViewer"> <div class="page" role="region" data-page-number="1" aria-label="Page 1" data-loaded="true"> <div class="textLayer"><span dir="ltr" role="presentation">The origin of Jupiter Trojans (JTs) remains an open problem.</span><span dir="ltr" role="presentation"> The currently leading theory assumes that JTs were captured </span><span dir="ltr" role="presentation">to their orbits near the Lagrangian points during the early </span><span dir="ltr" role="presentation">reconfiguration of the giant planets (Morbidelli et al. 2005;</span><span dir="ltr" role="presentation"> Nesvorný et al. 2013). The natural source region for the majority </span><span dir="ltr" role="presentation">of JTs would then be the population of planetesimals born in </span><span dir="ltr" role="presentation">a massive trans-Neptunian disk. As a result, JTs should share </span><span dir="ltr" role="presentation">the physical properties of currently observed trans-Neptunian</span><span dir="ltr" role="presentation"> objects (TNOs), as well as comets and irregular satellites of</span><span dir="ltr" role="presentation"> giant planets.</span> <span dir="ltr" role="presentation">Other theories avoid involving the planetary </span><span dir="ltr" role="presentation">reconfiguration event and postulate that JTs formed at their</span><span dir="ltr" role="presentation"> current location together with Jupiter (see reviews in Marzari</span><span dir="ltr" role="presentation"> et al. 2002; Emery et al. 2015), or were born in the Jupiter</span><span dir="ltr" role="presentation"> coorbital zone and accompanied its early inward migration </span><span dir="ltr" role="presentation">(Pirani et al. 2019). In this work, we adopt the capture model</span><span dir="ltr" role="presentation"> for JTs as a baseline hypothesis, because several other pieces</span><span dir="ltr" role="presentation"> of evidence support the view that giant planets underwent a </span><span dir="ltr" role="presentation">violent instability at some early moment of the Solar System</span><span dir="ltr" role="presentation"> evolution (see, e.g., Nesvorný 2018).</span></div> <div class="textLayer"><span dir="ltr" role="presentation">In our contribution, we compile photometric datasets for </span><span dir="ltr" role="presentation">about 900 JTs and apply the convex inversion technique in </span><span dir="ltr" role="presentation">order to derive their shapes and spin states. We obtained full</span><span dir="ltr" role="presentation"> solutions for</span> <span dir="ltr" role="presentation">71</span> <span dir="ltr" role="presentation">JTs, and partial solutions (of a little less sta</span><span dir="ltr" role="presentation">tistical significance) for additional</span> <span dir="ltr" role="presentation">15</span> <span dir="ltr" role="presentation">JTs. This represents an </span><span dir="ltr" role="presentation">increase in the sample of known spin state and shape solu</span><span dir="ltr" role="presentation">tions for JTs by a factor of</span> <span dir="ltr" role="presentation">∼</span><span dir="ltr" role="presentation">3. JTs librating about L</span><span dir="ltr" role="presentation">4</span> <span dir="ltr" role="presentation">and L</span><span dir="ltr" role="presentation">5</span><span dir="ltr" role="presentation"> points contribute roughly equally to our solutions. We found a factor of ~1.5 between the number of prograde and retrograde populations, or ~60% abundance of prograde rotators in the overall JT population.</span></div> <div class="textLayer"><span dir="ltr" role="presentation">We found evidence that the observed distribution of the ro</span><span dir="ltr" role="presentation">tation pole obliquities/latitudes of JTs qualitatively resembles </span><span dir="ltr" role="presentation">expectations from a numerical simulation of the streaming in</span><span dir="ltr" role="presentation">stability, the leading mechanism for the formation of planetes</span><span dir="ltr" role="presentation">imals in the trans-Neptunian disk. JTs pole distribution has a </span><span dir="ltr" role="presentation">slightly smaller north/south asymmetry, but this can be plau</span><span dir="ltr" role="presentation">sibly reconciled by the effects of a brief period of post-formation </span><span dir="ltr" role="presentation">collisional activity.</span> <span dir="ltr" role="presentation">Our numerical simulations of the post-</span><span dir="ltr" role="presentation">capture spin evolution indicate the JTs pole distribution is not</span><span dir="ltr" role="presentation"> significantly affected by dynamical processes.</span></div> <div class="textLayer"><strong><span dir="ltr" role="presentation">Acknowledgments</span></strong><br role="presentation" /><span dir="ltr" role="presentation">The work of JH and JD has been supported by the Czech</span><span dir="ltr" role="presentation"> Science Foundation through grant 20-08218S. The work </span><span dir="ltr" role="presentation">of DV has been supported by the Czech Science Founda</span><span dir="ltr" role="presentation">tion through grant 21-11058S. The work of OP has been</span><span dir="ltr" role="presentation"> supported by INTER-EXCELLENCE grant LTAUSA18093</span><span dir="ltr" role="presentation"> from the Ministry of Education, Youth, and Sports.</span></div> <div class="textLayer"><span dir="ltr" role="present
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Shape models and spin states of Jupiter Trojans: Testing the streaming instability formationWork title
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preprintOpenAlex work type
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enPrimary language
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2022Year of publication
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2022-09-23Full publication date if available
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J. Hanuš, David Vokrouhlický, David Nesvorný, Josef Ďurech, Robert D. Stephens, Ondřej Pejcha, Vladimir Benishek, Julian OeyList of authors in order
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https://doi.org/10.5194/epsc2022-396Publisher landing page
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goldOpen access status per OpenAlex
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| abstract_inverted_index.period | 466 |
| abstract_inverted_index.points | 63, 361 |
| abstract_inverted_index.region | 87 |
| abstract_inverted_index.sample | 326 |
| abstract_inverted_index.shapes | 282 |
| abstract_inverted_index.should | 114 |
| abstract_inverted_index.source | 86 |
| abstract_inverted_index.theory | 49 |
| abstract_inverted_index.(TNOs), | 128 |
| abstract_inverted_index.Jupiter | 37, 166 |
| abstract_inverted_index.Science | 520, 537 |
| abstract_inverted_index.Trojans | 38 |
| abstract_inverted_index.assumes | 50 |
| abstract_inverted_index.because | 218 |
| abstract_inverted_index.between | 374 |
| abstract_inverted_index.capture | 208 |
| abstract_inverted_index.compile | 260 |
| abstract_inverted_index.current | 162 |
| abstract_inverted_index.effects | 462 |
| abstract_inverted_index.equally | 364 |
| abstract_inverted_index.leading | 48, 428 |
| abstract_inverted_index.massive | 107 |
| abstract_inverted_index.natural | 85 |
| abstract_inverted_index.objects | 127 |
| abstract_inverted_index.overall | 390 |
| abstract_inverted_index.partial | 300 |
| abstract_inverted_index.planets | 73, 231 |
| abstract_inverted_index.remains | 40 |
| abstract_inverted_index.result, | 112 |
| abstract_inverted_index.reviews | 168 |
| abstract_inverted_index.roughly | 363 |
| abstract_inverted_index.several | 219 |
| abstract_inverted_index.smaller | 449 |
| abstract_inverted_index.states. | 285 |
| abstract_inverted_index.support | 226 |
| abstract_inverted_index.through | 522, 541 |
| abstract_inverted_index.Ministry | 561 |
| abstract_inverted_index.affected | 495 |
| abstract_inverted_index.baseline | 216 |
| abstract_inverted_index.captured | 54 |
| abstract_inverted_index.datasets | 262 |
| abstract_inverted_index.evidence | 225, 398 |
| abstract_inverted_index.indicate | 485 |
| abstract_inverted_index.location | 163 |
| abstract_inverted_index.majority | 90 |
| abstract_inverted_index.observed | 123, 401 |
| abstract_inverted_index.obtained | 287 |
| abstract_inverted_index.physical | 119 |
| abstract_inverted_index.prograde | 378, 386 |
| abstract_inverted_index.rotators | 387 |
| abstract_inverted_index.theories | 144 |
| abstract_inverted_index.together | 164 |
| abstract_inverted_index.abundance | 384 |
| abstract_inverted_index.coorbital | 188 |
| abstract_inverted_index.currently | 47, 122 |
| abstract_inverted_index.dynamical | 497 |
| abstract_inverted_index.evolution | 248, 484 |
| abstract_inverted_index.formation | 432 |
| abstract_inverted_index.inversion | 273 |
| abstract_inverted_index.involving | 146 |
| abstract_inverted_index.irregular | 134 |
| abstract_inverted_index.librating | 348 |
| abstract_inverted_index.mechanism | 429 |
| abstract_inverted_index.migration | 195 |
| abstract_inverted_index.numerical | 419, 476 |
| abstract_inverted_index.planetary | 148 |
| abstract_inverted_index.postulate | 154 |
| abstract_inverted_index.resembles | 413 |
| abstract_inverted_index.solutions | 291, 301 |
| abstract_inverted_index.streaming | 423 |
| abstract_inverted_index.supported | 514, 533, 552 |
| abstract_inverted_index.technique | 274 |
| abstract_inverted_index.underwent | 232 |
| abstract_inverted_index.20-08218S. | 524 |
| abstract_inverted_index.21-11058S. | 543 |
| abstract_inverted_index.Education, | 563 |
| abstract_inverted_index.Foundation | 521 |
| abstract_inverted_index.Lagrangian | 62 |
| abstract_inverted_index.asymmetry, | 451 |
| abstract_inverted_index.contribute | 362 |
| abstract_inverted_index.population | 99 |
| abstract_inverted_index.properties | 120 |
| abstract_inverted_index.reconciled | 459 |
| abstract_inverted_index.represents | 319 |
| abstract_inverted_index.retrograde | 380 |
| abstract_inverted_index.satellites | 135 |
| abstract_inverted_index.simulation | 420 |
| abstract_inverted_index.solutions. | 367 |
| abstract_inverted_index.&lt;div | 0, 8, 10, 13, 15, 18, 22, 24, 31, 253, 393, 499, 567 |
| abstract_inverted_index.(Morbidelli | 74 |
| abstract_inverted_index.1&quot; | 29 |
| abstract_inverted_index.accompanied | 191 |
| abstract_inverted_index.hypothesis, | 217 |
| abstract_inverted_index.instability | 237 |
| abstract_inverted_index.north/south | 450 |
| abstract_inverted_index.photometric | 261 |
| abstract_inverted_index.simulations | 477 |
| abstract_inverted_index.&lt;span | 141, 293, 296, 312, 315, 342, 353, 473 |
| abstract_inverted_index.distribution | 402, 443, 489 |
| abstract_inverted_index.populations, | 381 |
| abstract_inverted_index.contribution, | 258 |
| abstract_inverted_index.planetesimals | 101 |
| abstract_inverted_index.qualitatively | 412 |
| abstract_inverted_index.significance) | 309 |
| abstract_inverted_index.significantly | 494 |
| abstract_inverted_index.post-formation | 468 |
| abstract_inverted_index.ui-layout-pane | 2 |
| abstract_inverted_index.trans-Neptunian | 108, 439 |
| abstract_inverted_index.INTER-EXCELLENCE | 554 |
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| abstract_inverted_index./&gt;&lt;span | 504 |
| abstract_inverted_index.Nesvorn&amp;#253; | 80, 251 |
| abstract_inverted_index.obliquities/latitudes | 409 |
| abstract_inverted_index.role=&quot;present | 570 |
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| abstract_inverted_index.ui-layout-pane-east-hover | 5 |
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| abstract_inverted_index.planetes&lt;/span&gt;&lt;span | 434 |
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| abstract_inverted_index.role=&quot;presentation&quot;&gt;In | 256 |
| abstract_inverted_index.role=&quot;presentation&quot;&gt;We | 396 |
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| abstract_inverted_index.role=&quot;presentation&quot;&gt;to | 57 |
| abstract_inverted_index.Sports.&lt;/span&gt;&lt;/div&gt; | 566 |
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| abstract_inverted_index.role=&quot;presentation&quot;&gt;The | 34, 506 |
| abstract_inverted_index.role=&quot;presentation&quot;&gt;and | 355 |
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| abstract_inverted_index.role=&quot;presentation&quot;&gt;tion | 540 |
| abstract_inverted_index.role=&quot;presentation&quot;&gt;Other | 143 |
| abstract_inverted_index.role=&quot;presentation&quot;&gt;about | 266 |
| abstract_inverted_index.role=&quot;presentation&quot;&gt;imals | 436 |
| abstract_inverted_index.role=&quot;presentation&quot;&gt;order | 278 |
| abstract_inverted_index.role=&quot;presentation&quot;&gt;sibly | 458 |
| abstract_inverted_index.role=&quot;presentation&quot;&gt;tions | 335 |
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| abstract_inverted_index.role=&quot;presentation&quot;&gt;(Pirani | 198 |
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| abstract_inverted_index.role=&quot;presentation&quot;&gt;reconfiguration | 69, 151 |
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| abstract_inverted_index.role=&quot;presentation&quot;&gt;Acknowledgments&lt;/span&gt;&lt;/strong&gt;&lt;br | 502 |
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| institutions_distinct_count | 8 |
| citation_normalized_percentile.value | 0.12798087 |
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