Few Comments on the Relation Between the Initial Proto-planetary Disc Model and the Oort Cloud Formation View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2009-03-17

AUTHORS

Tomáš Paulech, Marián Jakubík, Luboš Neslušan, Piotr A. Dybczyński, Giuseppe Leto

ABSTRACT

A fraction of small bodies from the once existing proto-planetary disc was ejected, by the giant planets, to large heliocentric distances and start to build the comet Oort cloud. Considering four models of initial proto-planetary disc, we attempt to roughly map a dependence between the initial disc’s structure and some properties of the Oort cloud. We find that it is difficult to construct the proto-planetary disc if (i) the amount of heavy chemical elements in Jupiter and Saturn is as high as currently accepted and (ii) the total mass of the minimum-mass solar nebula is assumed to be lower than \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\approx0.05\,\hbox{M}_{\odot}.$$\end{document} The behaviour of the Oort cloud formation does not crucially depend on the initial disc model. Some differences in its structure are obvious: since the cloud is known to be filled mainly by Uranus and Neptune, the efficiency of its formation is higher when the initial amount of particles in the Uranus-Neptune region is relatively higher. A significantly large number of Jupiter Trojans in our simulation appears, however, only in the case of the initially non-gapped disc, with the particles situated also close to the Jupiter’s orbit. More... »

PAGES

367-371

References to SciGraph publications

  • 1977-09. The distribution of mass in the planetary system and solar nebula in ASTROPHYSICS AND SPACE SCIENCE
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/s11038-009-9299-6

    DOI

    http://dx.doi.org/10.1007/s11038-009-9299-6

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1016968476


    Indexing Status Check whether this publication has been indexed by Scopus and Web Of Science using the SN Indexing Status Tool
    Incoming Citations Browse incoming citations for this publication using opencitations.net

    JSON-LD is the canonical representation for SciGraph data.

    TIP: You can open this SciGraph record using an external JSON-LD service: JSON-LD Playground Google SDTT

    [
      {
        "@context": "https://springernature.github.io/scigraph/jsonld/sgcontext.json", 
        "about": [
          {
            "id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/02", 
            "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
            "name": "Physical Sciences", 
            "type": "DefinedTerm"
          }, 
          {
            "id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/0299", 
            "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
            "name": "Other Physical Sciences", 
            "type": "DefinedTerm"
          }
        ], 
        "author": [
          {
            "affiliation": {
              "alternateName": "Astronomical Institute, Slovak Academy of Sciences, D\u00fabravsk\u00e1 9, 84504, Bratislava, Slovakia", 
              "id": "http://www.grid.ac/institutes/grid.419303.c", 
              "name": [
                "Astronomical Institute, Slovak Academy of Sciences, D\u00fabravsk\u00e1 9, 84504, Bratislava, Slovakia"
              ], 
              "type": "Organization"
            }, 
            "familyName": "Paulech", 
            "givenName": "Tom\u00e1\u0161", 
            "id": "sg:person.010030032535.76", 
            "sameAs": [
              "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.010030032535.76"
            ], 
            "type": "Person"
          }, 
          {
            "affiliation": {
              "alternateName": "Astronomical Institute, Slovak Academy of Sciences, 05960, Tatransk\u00e1 Lomnica, Slovakia", 
              "id": "http://www.grid.ac/institutes/grid.493212.f", 
              "name": [
                "Astronomical Institute, Slovak Academy of Sciences, 05960, Tatransk\u00e1 Lomnica, Slovakia"
              ], 
              "type": "Organization"
            }, 
            "familyName": "Jakub\u00edk", 
            "givenName": "Mari\u00e1n", 
            "id": "sg:person.01270443205.36", 
            "sameAs": [
              "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.01270443205.36"
            ], 
            "type": "Person"
          }, 
          {
            "affiliation": {
              "alternateName": "Astronomical Institute, Slovak Academy of Sciences, 05960, Tatransk\u00e1 Lomnica, Slovakia", 
              "id": "http://www.grid.ac/institutes/grid.493212.f", 
              "name": [
                "Astronomical Institute, Slovak Academy of Sciences, 05960, Tatransk\u00e1 Lomnica, Slovakia"
              ], 
              "type": "Organization"
            }, 
            "familyName": "Neslu\u0161an", 
            "givenName": "Lubo\u0161", 
            "id": "sg:person.012152240735.08", 
            "sameAs": [
              "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.012152240735.08"
            ], 
            "type": "Person"
          }, 
          {
            "affiliation": {
              "alternateName": "Astronomical Observatory, A. Mickiewicz University, S\u0142oneczna 36, 60-286, Pozna\u0144, Poland", 
              "id": "http://www.grid.ac/institutes/grid.5633.3", 
              "name": [
                "Astronomical Observatory, A. Mickiewicz University, S\u0142oneczna 36, 60-286, Pozna\u0144, Poland"
              ], 
              "type": "Organization"
            }, 
            "familyName": "Dybczy\u0144ski", 
            "givenName": "Piotr A.", 
            "id": "sg:person.013652577302.24", 
            "sameAs": [
              "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.013652577302.24"
            ], 
            "type": "Person"
          }, 
          {
            "affiliation": {
              "alternateName": "Catania Astrophysical Observatory, Via Santa Sofia 78, I-95123, Catania, Italy", 
              "id": "http://www.grid.ac/institutes/grid.450009.8", 
              "name": [
                "Catania Astrophysical Observatory, Via Santa Sofia 78, I-95123, Catania, Italy"
              ], 
              "type": "Organization"
            }, 
            "familyName": "Leto", 
            "givenName": "Giuseppe", 
            "id": "sg:person.010354272373.07", 
            "sameAs": [
              "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.010354272373.07"
            ], 
            "type": "Person"
          }
        ], 
        "citation": [
          {
            "id": "sg:pub.10.1007/bf00642464", 
            "sameAs": [
              "https://app.dimensions.ai/details/publication/pub.1049693737", 
              "https://doi.org/10.1007/bf00642464"
            ], 
            "type": "CreativeWork"
          }
        ], 
        "datePublished": "2009-03-17", 
        "datePublishedReg": "2009-03-17", 
        "description": "A fraction of small bodies from the once existing proto-planetary disc was ejected, by the giant planets, to large heliocentric distances and start to build the comet Oort cloud. Considering four models of initial proto-planetary disc, we attempt to roughly map a dependence between the initial disc\u2019s structure and some properties of the Oort cloud. We find that it is difficult to construct the proto-planetary disc if (i) the amount of heavy chemical elements in Jupiter and Saturn is as high as currently accepted and (ii) the total mass of the minimum-mass solar nebula is assumed to be lower than \\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$\\approx0.05\\,\\hbox{M}_{\\odot}.$$\\end{document} The behaviour of the Oort cloud formation does not crucially depend on the initial disc model. Some differences in its structure are obvious: since the cloud is known to be filled mainly by Uranus and Neptune, the efficiency of its formation is higher when the initial amount of particles in the Uranus-Neptune region is relatively higher. A significantly large number of Jupiter Trojans in our simulation appears, however, only in the case of the initially non-gapped disc, with the particles situated also close to the Jupiter\u2019s orbit.", 
        "genre": "article", 
        "id": "sg:pub.10.1007/s11038-009-9299-6", 
        "inLanguage": "en", 
        "isAccessibleForFree": false, 
        "isPartOf": [
          {
            "id": "sg:journal.1026186", 
            "issn": [
              "0167-9295", 
              "1573-0794"
            ], 
            "name": "Earth, Moon, and Planets", 
            "publisher": "Springer Nature", 
            "type": "Periodical"
          }, 
          {
            "issueNumber": "2-4", 
            "type": "PublicationIssue"
          }, 
          {
            "type": "PublicationVolume", 
            "volumeNumber": "105"
          }
        ], 
        "keywords": [
          "proto-planetary disks", 
          "Oort cloud formation", 
          "Oort cloud", 
          "initial disc model", 
          "heavy chemical elements", 
          "disk model", 
          "minimum-mass solar nebula", 
          "Uranus-Neptune region", 
          "large heliocentric distances", 
          "giant planets", 
          "Jupiter's orbit", 
          "heliocentric distance", 
          "cloud formation", 
          "disk structure", 
          "total mass", 
          "Jupiter Trojans", 
          "solar nebula", 
          "chemical elements", 
          "orbit", 
          "cloud", 
          "disk", 
          "Jupiter", 
          "particles", 
          "nebula", 
          "Saturn", 
          "Uranus", 
          "Neptune", 
          "planets", 
          "small bodies", 
          "structure", 
          "dependence", 
          "formation", 
          "mass", 
          "distance", 
          "properties", 
          "simulations", 
          "model", 
          "region", 
          "large number", 
          "efficiency", 
          "fraction", 
          "elements", 
          "behavior", 
          "initial amount", 
          "relation", 
          "Trojans", 
          "amount", 
          "cases", 
          "number", 
          "comments", 
          "differences", 
          "body", 
          "comet Oort cloud", 
          "initial proto-planetary disc", 
          "initial disc\u2019s structure", 
          "non-gapped disc", 
          "Initial Proto-planetary Disc Model", 
          "Proto-planetary Disc Model"
        ], 
        "name": "Few Comments on the Relation Between the Initial Proto-planetary Disc Model and the Oort Cloud Formation", 
        "pagination": "367-371", 
        "productId": [
          {
            "name": "dimensions_id", 
            "type": "PropertyValue", 
            "value": [
              "pub.1016968476"
            ]
          }, 
          {
            "name": "doi", 
            "type": "PropertyValue", 
            "value": [
              "10.1007/s11038-009-9299-6"
            ]
          }
        ], 
        "sameAs": [
          "https://doi.org/10.1007/s11038-009-9299-6", 
          "https://app.dimensions.ai/details/publication/pub.1016968476"
        ], 
        "sdDataset": "articles", 
        "sdDatePublished": "2021-11-01T18:14", 
        "sdLicense": "https://scigraph.springernature.com/explorer/license/", 
        "sdPublisher": {
          "name": "Springer Nature - SN SciGraph project", 
          "type": "Organization"
        }, 
        "sdSource": "s3://com-springernature-scigraph/baseset/20211101/entities/gbq_results/article/article_500.jsonl", 
        "type": "ScholarlyArticle", 
        "url": "https://doi.org/10.1007/s11038-009-9299-6"
      }
    ]
     

    Download the RDF metadata as:  json-ld nt turtle xml License info

    HOW TO GET THIS DATA PROGRAMMATICALLY:

    JSON-LD is a popular format for linked data which is fully compatible with JSON.

    curl -H 'Accept: application/ld+json' 'https://scigraph.springernature.com/pub.10.1007/s11038-009-9299-6'

    N-Triples is a line-based linked data format ideal for batch operations.

    curl -H 'Accept: application/n-triples' 'https://scigraph.springernature.com/pub.10.1007/s11038-009-9299-6'

    Turtle is a human-readable linked data format.

    curl -H 'Accept: text/turtle' 'https://scigraph.springernature.com/pub.10.1007/s11038-009-9299-6'

    RDF/XML is a standard XML format for linked data.

    curl -H 'Accept: application/rdf+xml' 'https://scigraph.springernature.com/pub.10.1007/s11038-009-9299-6'


     

    This table displays all metadata directly associated to this object as RDF triples.

    157 TRIPLES      22 PREDICATES      84 URIs      75 LITERALS      6 BLANK NODES

    Subject Predicate Object
    1 sg:pub.10.1007/s11038-009-9299-6 schema:about anzsrc-for:02
    2 anzsrc-for:0299
    3 schema:author N8cb19e18b86749db95c98762e7649c2c
    4 schema:citation sg:pub.10.1007/bf00642464
    5 schema:datePublished 2009-03-17
    6 schema:datePublishedReg 2009-03-17
    7 schema:description A fraction of small bodies from the once existing proto-planetary disc was ejected, by the giant planets, to large heliocentric distances and start to build the comet Oort cloud. Considering four models of initial proto-planetary disc, we attempt to roughly map a dependence between the initial disc’s structure and some properties of the Oort cloud. We find that it is difficult to construct the proto-planetary disc if (i) the amount of heavy chemical elements in Jupiter and Saturn is as high as currently accepted and (ii) the total mass of the minimum-mass solar nebula is assumed to be lower than \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\approx0.05\,\hbox{M}_{\odot}.$$\end{document} The behaviour of the Oort cloud formation does not crucially depend on the initial disc model. Some differences in its structure are obvious: since the cloud is known to be filled mainly by Uranus and Neptune, the efficiency of its formation is higher when the initial amount of particles in the Uranus-Neptune region is relatively higher. A significantly large number of Jupiter Trojans in our simulation appears, however, only in the case of the initially non-gapped disc, with the particles situated also close to the Jupiter’s orbit.
    8 schema:genre article
    9 schema:inLanguage en
    10 schema:isAccessibleForFree false
    11 schema:isPartOf N1dba94ca93a945b1b922c03332b1dfc7
    12 N8767ed5f0c094bf5a90330e2cf4a2b9b
    13 sg:journal.1026186
    14 schema:keywords Initial Proto-planetary Disc Model
    15 Jupiter
    16 Jupiter Trojans
    17 Jupiter's orbit
    18 Neptune
    19 Oort cloud
    20 Oort cloud formation
    21 Proto-planetary Disc Model
    22 Saturn
    23 Trojans
    24 Uranus
    25 Uranus-Neptune region
    26 amount
    27 behavior
    28 body
    29 cases
    30 chemical elements
    31 cloud
    32 cloud formation
    33 comet Oort cloud
    34 comments
    35 dependence
    36 differences
    37 disk
    38 disk model
    39 disk structure
    40 distance
    41 efficiency
    42 elements
    43 formation
    44 fraction
    45 giant planets
    46 heavy chemical elements
    47 heliocentric distance
    48 initial amount
    49 initial disc model
    50 initial disc’s structure
    51 initial proto-planetary disc
    52 large heliocentric distances
    53 large number
    54 mass
    55 minimum-mass solar nebula
    56 model
    57 nebula
    58 non-gapped disc
    59 number
    60 orbit
    61 particles
    62 planets
    63 properties
    64 proto-planetary disks
    65 region
    66 relation
    67 simulations
    68 small bodies
    69 solar nebula
    70 structure
    71 total mass
    72 schema:name Few Comments on the Relation Between the Initial Proto-planetary Disc Model and the Oort Cloud Formation
    73 schema:pagination 367-371
    74 schema:productId N0edbe2bfa0bf419b89de7f2aebb93f72
    75 Nb68dffa84df54e65be347029a8cd708f
    76 schema:sameAs https://app.dimensions.ai/details/publication/pub.1016968476
    77 https://doi.org/10.1007/s11038-009-9299-6
    78 schema:sdDatePublished 2021-11-01T18:14
    79 schema:sdLicense https://scigraph.springernature.com/explorer/license/
    80 schema:sdPublisher Ncf3e71405bf543e5a191860d4920de5d
    81 schema:url https://doi.org/10.1007/s11038-009-9299-6
    82 sgo:license sg:explorer/license/
    83 sgo:sdDataset articles
    84 rdf:type schema:ScholarlyArticle
    85 N0ac21c9453ac4b09ae8e28860e5b3922 rdf:first sg:person.012152240735.08
    86 rdf:rest N2ee298999ad44f169242171b8c7f34ce
    87 N0edbe2bfa0bf419b89de7f2aebb93f72 schema:name doi
    88 schema:value 10.1007/s11038-009-9299-6
    89 rdf:type schema:PropertyValue
    90 N1dba94ca93a945b1b922c03332b1dfc7 schema:volumeNumber 105
    91 rdf:type schema:PublicationVolume
    92 N2ee298999ad44f169242171b8c7f34ce rdf:first sg:person.013652577302.24
    93 rdf:rest Ne3a810c0783d4e05b6748474646ad199
    94 N8767ed5f0c094bf5a90330e2cf4a2b9b schema:issueNumber 2-4
    95 rdf:type schema:PublicationIssue
    96 N8cb19e18b86749db95c98762e7649c2c rdf:first sg:person.010030032535.76
    97 rdf:rest Nbb8fa2afe252460aa75eb98bdc609498
    98 Nb68dffa84df54e65be347029a8cd708f schema:name dimensions_id
    99 schema:value pub.1016968476
    100 rdf:type schema:PropertyValue
    101 Nbb8fa2afe252460aa75eb98bdc609498 rdf:first sg:person.01270443205.36
    102 rdf:rest N0ac21c9453ac4b09ae8e28860e5b3922
    103 Ncf3e71405bf543e5a191860d4920de5d schema:name Springer Nature - SN SciGraph project
    104 rdf:type schema:Organization
    105 Ne3a810c0783d4e05b6748474646ad199 rdf:first sg:person.010354272373.07
    106 rdf:rest rdf:nil
    107 anzsrc-for:02 schema:inDefinedTermSet anzsrc-for:
    108 schema:name Physical Sciences
    109 rdf:type schema:DefinedTerm
    110 anzsrc-for:0299 schema:inDefinedTermSet anzsrc-for:
    111 schema:name Other Physical Sciences
    112 rdf:type schema:DefinedTerm
    113 sg:journal.1026186 schema:issn 0167-9295
    114 1573-0794
    115 schema:name Earth, Moon, and Planets
    116 schema:publisher Springer Nature
    117 rdf:type schema:Periodical
    118 sg:person.010030032535.76 schema:affiliation grid-institutes:grid.419303.c
    119 schema:familyName Paulech
    120 schema:givenName Tomáš
    121 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.010030032535.76
    122 rdf:type schema:Person
    123 sg:person.010354272373.07 schema:affiliation grid-institutes:grid.450009.8
    124 schema:familyName Leto
    125 schema:givenName Giuseppe
    126 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.010354272373.07
    127 rdf:type schema:Person
    128 sg:person.012152240735.08 schema:affiliation grid-institutes:grid.493212.f
    129 schema:familyName Neslušan
    130 schema:givenName Luboš
    131 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.012152240735.08
    132 rdf:type schema:Person
    133 sg:person.01270443205.36 schema:affiliation grid-institutes:grid.493212.f
    134 schema:familyName Jakubík
    135 schema:givenName Marián
    136 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.01270443205.36
    137 rdf:type schema:Person
    138 sg:person.013652577302.24 schema:affiliation grid-institutes:grid.5633.3
    139 schema:familyName Dybczyński
    140 schema:givenName Piotr A.
    141 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.013652577302.24
    142 rdf:type schema:Person
    143 sg:pub.10.1007/bf00642464 schema:sameAs https://app.dimensions.ai/details/publication/pub.1049693737
    144 https://doi.org/10.1007/bf00642464
    145 rdf:type schema:CreativeWork
    146 grid-institutes:grid.419303.c schema:alternateName Astronomical Institute, Slovak Academy of Sciences, Dúbravská 9, 84504, Bratislava, Slovakia
    147 schema:name Astronomical Institute, Slovak Academy of Sciences, Dúbravská 9, 84504, Bratislava, Slovakia
    148 rdf:type schema:Organization
    149 grid-institutes:grid.450009.8 schema:alternateName Catania Astrophysical Observatory, Via Santa Sofia 78, I-95123, Catania, Italy
    150 schema:name Catania Astrophysical Observatory, Via Santa Sofia 78, I-95123, Catania, Italy
    151 rdf:type schema:Organization
    152 grid-institutes:grid.493212.f schema:alternateName Astronomical Institute, Slovak Academy of Sciences, 05960, Tatranská Lomnica, Slovakia
    153 schema:name Astronomical Institute, Slovak Academy of Sciences, 05960, Tatranská Lomnica, Slovakia
    154 rdf:type schema:Organization
    155 grid-institutes:grid.5633.3 schema:alternateName Astronomical Observatory, A. Mickiewicz University, Słoneczna 36, 60-286, Poznań, Poland
    156 schema:name Astronomical Observatory, A. Mickiewicz University, Słoneczna 36, 60-286, Poznań, Poland
    157 rdf:type schema:Organization
     




    Preview window. Press ESC to close (or click here)


    ...