Loading…

Exoplanet Predictions Based on the Generalised Titius-Bode Relation

We evaluate the extent to which newly detected exoplanetary systems containing at least four planets adhere to a generalized Titius-Bode (TB) relation. We find that the majority of exoplanet systems in our sample adhere to the TB relation to a greater extent than the Solar System does, particularly...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2013-08
Main Authors: Bovaird, Timothy, Lineweaver, Charles H
Format: Article
Language:English
Subjects:
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Bovaird, Timothy
Lineweaver, Charles H
description We evaluate the extent to which newly detected exoplanetary systems containing at least four planets adhere to a generalized Titius-Bode (TB) relation. We find that the majority of exoplanet systems in our sample adhere to the TB relation to a greater extent than the Solar System does, particularly those detected by the Kepler mission. We use a generalized TB relation to make a list of predictions for the existence of 141 additional exoplanets in 68 multiple-exoplanet systems: 73 candidates from interpolation, 68 candidates from extrapolation. We predict the existence of a low-radius (R < 2.5 Earth Radii) exoplanet within the habitable zone of KOI-812 and that the average number of planets in the habitable zone of a star is 1-2. The usefulness of the TB relation and its validation as a tool for predicting planets will be partially tested by upcoming Kepler data releases.
doi_str_mv 10.48550/arxiv.1304.3341
format article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2082830266</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2082830266</sourcerecordid><originalsourceid>FETCH-LOGICAL-a516-7aaac8b6a90bdb50639765b7969475fc7eca152d7b4d32e47869ea6972fbe80b3</originalsourceid><addsrcrecordid>eNotj0tLw0AUhQdBsNTuXQ64Tpz3Y2lLrUJBkezLncwNTgmZmkmkP98WXR04fJyPQ8gDZ7VyWrMnGM_pp-aSqVpKxW_IQkjJK6eEuCOrUo6MMWGs0FouyGZ7zqceBpzox4gxtVPKQ6FrKBhpHuj0hXSHA47Qp2vVpCnNpVrniPQTe7ji9-S2g77g6j-XpHnZNpvXav--e9s87yvQ3FQWAFoXDHgWYtDMSG-NDtYbr6zuWostcC2iDSpKgco64xGMt6IL6FiQS_L4N3sa8_eMZToc8zwOF-NBMCecvLwy8hceoEuB</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2082830266</pqid></control><display><type>article</type><title>Exoplanet Predictions Based on the Generalised Titius-Bode Relation</title><source>Publicly Available Content Database</source><creator>Bovaird, Timothy ; Lineweaver, Charles H</creator><creatorcontrib>Bovaird, Timothy ; Lineweaver, Charles H</creatorcontrib><description>We evaluate the extent to which newly detected exoplanetary systems containing at least four planets adhere to a generalized Titius-Bode (TB) relation. We find that the majority of exoplanet systems in our sample adhere to the TB relation to a greater extent than the Solar System does, particularly those detected by the Kepler mission. We use a generalized TB relation to make a list of predictions for the existence of 141 additional exoplanets in 68 multiple-exoplanet systems: 73 candidates from interpolation, 68 candidates from extrapolation. We predict the existence of a low-radius (R &lt; 2.5 Earth Radii) exoplanet within the habitable zone of KOI-812 and that the average number of planets in the habitable zone of a star is 1-2. The usefulness of the TB relation and its validation as a tool for predicting planets will be partially tested by upcoming Kepler data releases.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1304.3341</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Circumstellar habitable zone ; Extrasolar planets ; Interpolation ; Kepler mission (NASA) ; Planet detection ; Planetary systems ; Predictions ; Solar system</subject><ispartof>arXiv.org, 2013-08</ispartof><rights>2013. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2082830266?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>780,784,25753,27925,37012,44590</link.rule.ids></links><search><creatorcontrib>Bovaird, Timothy</creatorcontrib><creatorcontrib>Lineweaver, Charles H</creatorcontrib><title>Exoplanet Predictions Based on the Generalised Titius-Bode Relation</title><title>arXiv.org</title><description>We evaluate the extent to which newly detected exoplanetary systems containing at least four planets adhere to a generalized Titius-Bode (TB) relation. We find that the majority of exoplanet systems in our sample adhere to the TB relation to a greater extent than the Solar System does, particularly those detected by the Kepler mission. We use a generalized TB relation to make a list of predictions for the existence of 141 additional exoplanets in 68 multiple-exoplanet systems: 73 candidates from interpolation, 68 candidates from extrapolation. We predict the existence of a low-radius (R &lt; 2.5 Earth Radii) exoplanet within the habitable zone of KOI-812 and that the average number of planets in the habitable zone of a star is 1-2. The usefulness of the TB relation and its validation as a tool for predicting planets will be partially tested by upcoming Kepler data releases.</description><subject>Circumstellar habitable zone</subject><subject>Extrasolar planets</subject><subject>Interpolation</subject><subject>Kepler mission (NASA)</subject><subject>Planet detection</subject><subject>Planetary systems</subject><subject>Predictions</subject><subject>Solar system</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotj0tLw0AUhQdBsNTuXQ64Tpz3Y2lLrUJBkezLncwNTgmZmkmkP98WXR04fJyPQ8gDZ7VyWrMnGM_pp-aSqVpKxW_IQkjJK6eEuCOrUo6MMWGs0FouyGZ7zqceBpzox4gxtVPKQ6FrKBhpHuj0hXSHA47Qp2vVpCnNpVrniPQTe7ji9-S2g77g6j-XpHnZNpvXav--e9s87yvQ3FQWAFoXDHgWYtDMSG-NDtYbr6zuWostcC2iDSpKgco64xGMt6IL6FiQS_L4N3sa8_eMZToc8zwOF-NBMCecvLwy8hceoEuB</recordid><startdate>20130801</startdate><enddate>20130801</enddate><creator>Bovaird, Timothy</creator><creator>Lineweaver, Charles H</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20130801</creationdate><title>Exoplanet Predictions Based on the Generalised Titius-Bode Relation</title><author>Bovaird, Timothy ; Lineweaver, Charles H</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a516-7aaac8b6a90bdb50639765b7969475fc7eca152d7b4d32e47869ea6972fbe80b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Circumstellar habitable zone</topic><topic>Extrasolar planets</topic><topic>Interpolation</topic><topic>Kepler mission (NASA)</topic><topic>Planet detection</topic><topic>Planetary systems</topic><topic>Predictions</topic><topic>Solar system</topic><toplevel>online_resources</toplevel><creatorcontrib>Bovaird, Timothy</creatorcontrib><creatorcontrib>Lineweaver, Charles H</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bovaird, Timothy</au><au>Lineweaver, Charles H</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Exoplanet Predictions Based on the Generalised Titius-Bode Relation</atitle><jtitle>arXiv.org</jtitle><date>2013-08-01</date><risdate>2013</risdate><eissn>2331-8422</eissn><abstract>We evaluate the extent to which newly detected exoplanetary systems containing at least four planets adhere to a generalized Titius-Bode (TB) relation. We find that the majority of exoplanet systems in our sample adhere to the TB relation to a greater extent than the Solar System does, particularly those detected by the Kepler mission. We use a generalized TB relation to make a list of predictions for the existence of 141 additional exoplanets in 68 multiple-exoplanet systems: 73 candidates from interpolation, 68 candidates from extrapolation. We predict the existence of a low-radius (R &lt; 2.5 Earth Radii) exoplanet within the habitable zone of KOI-812 and that the average number of planets in the habitable zone of a star is 1-2. The usefulness of the TB relation and its validation as a tool for predicting planets will be partially tested by upcoming Kepler data releases.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1304.3341</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2013-08
issn 2331-8422
language eng
recordid cdi_proquest_journals_2082830266
source Publicly Available Content Database
subjects Circumstellar habitable zone
Extrasolar planets
Interpolation
Kepler mission (NASA)
Planet detection
Planetary systems
Predictions
Solar system
title Exoplanet Predictions Based on the Generalised Titius-Bode Relation
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-29T20%3A02%3A23IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Exoplanet%20Predictions%20Based%20on%20the%20Generalised%20Titius-Bode%20Relation&rft.jtitle=arXiv.org&rft.au=Bovaird,%20Timothy&rft.date=2013-08-01&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1304.3341&rft_dat=%3Cproquest%3E2082830266%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a516-7aaac8b6a90bdb50639765b7969475fc7eca152d7b4d32e47869ea6972fbe80b3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2082830266&rft_id=info:pmid/&rfr_iscdi=true