{"id":{"repo_id":"mit","oai_identifier":"oai:dspace.mit.edu:1721.1/37279"},"canonical_url":"https://search.dev.ndltd.org/etd/mit/oai:dspace.mit.edu:1721.1/37279","repository":{"repo_id":"mit","name":"MIT","base_url":"https://dspace.mit.edu/oai/request"},"display":{"title":"Colors of Kuiper Belt objects : the relationship between KBO colors and Kuiper Belt plane inclination","abstract":"A large population of small, icy bodies orbits the sun just beyond Neptune, known as the Kuiper Belt. These objects, thought to be the progenitors of short period comets, could provide a sample of primordial material in our solar system, constraining solar system formation models. The colors of Kuiper belt objects (KBOs) can indicate different surface compositions, environmental conditions, or formation characteristics within the Kuiper Belt. Data from the Deep Ecliptic Survey (DES, Millis et al. 2002) have been used to determine the plane of the Kuiper Belt, identifying \"core\" and \"halo\" populations with respect to this plane (Elliot et al. 2005). By comparing the colors of objects as a function of inclination, trends can be established distinguishing the core and halo populations. Sloan g', r' and i' observations were obtained from the 6.5-m Clay telescope at Las Campanas Observatory of 14 KBOs, which were combined with previously published data to examine the transition between these two populations as a function of color. For inclination bins containing equal numbers of KBOs, the percentage of red objects (B-R > 1.56, where B-R = 1.56 is the median of the sample) decreases with increasing inclination in a smooth, but nonlinear fashion.","abstract_html":"A large population of small, icy bodies orbits the sun just beyond Neptune, known as the Kuiper Belt. These objects, thought to be the progenitors of short period comets, could provide a sample of primordial material in our solar system, constraining solar system formation models. The colors of Kuiper belt objects (KBOs) can indicate different surface compositions, environmental conditions, or formation characteristics within the Kuiper Belt. Data from the Deep Ecliptic Survey (DES, Millis et al. 2002) have been used to determine the plane of the Kuiper Belt, identifying "core" and "halo" populations with respect to this plane (Elliot et al. 2005). By comparing the colors of objects as a function of inclination, trends can be established distinguishing the core and halo populations. Sloan g', r' and i' observations were obtained from the 6.5-m Clay telescope at Las Campanas Observatory of 14 KBOs, which were combined with previously published data to examine the transition between these two populations as a function of color. For inclination bins containing equal numbers of KBOs, the percentage of red objects (B-R > 1.56, where B-R = 1.56 is the median of the sample) decreases with increasing inclination in a smooth, but nonlinear fashion.","abstract_has_math":false,"creators":["Kane, Julia Frances"],"institution":"Massachusetts Institute of Technology","degree_name":null,"degree_level":null,"degree_discipline":null,"degree_department":"Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences.","school":null,"contributors":[],"advisors":["James L. Elliot."],"committee_chairs":[],"committee_members":[],"year":2006,"date_issued":"2006","date_published":"2006","updated_at":"2026-07-22T22:21:36Z","subjects":["Earth, Atmospheric, and Planetary Sciences."],"languages":["eng"],"rights":["M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission."],"rights_urls":["http://dspace.mit.edu/handle/1721.1/7582"],"identifier_entries":[]},"links":{"outbound_url":"http://hdl.handle.net/1721.1/37279","outbound_label":"Handle","outbound_source":"dc:identifier.uri"},"metadata_groups":[{"id":"people","label":"People","entries":[{"key":"dc:contributor.advisor","label":"Advisor","values":["James L. Elliot."]},{"key":"dc:contributor.department","label":"Department","values":["Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences."]},{"key":"dc:contributor.other","label":"Dc Contributor Other","values":["Massachusetts Institute of Technology. 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They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission."]},{"key":"dc:rights.uri","label":"Rights URI","values":["http://dspace.mit.edu/handle/1721.1/7582"]}]},{"id":"identifiers","label":"Identifiers","entries":[{"key":"dc:identifier.uri","label":"Identifier URI","values":["http://hdl.handle.net/1721.1/37279"]}]},{"id":"additional","label":"Additional Metadata","entries":[{"key":"dc:description","label":"Description","values":["Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2006.","Includes bibliographical references (p. 39-41)."]},{"key":"dc:description.abstract","label":"Abstract","values":["A large population of small, icy bodies orbits the sun just beyond Neptune, known as the Kuiper Belt. These objects, thought to be the progenitors of short period comets, could provide a sample of primordial material in our solar system, constraining solar system formation models. The colors of Kuiper belt objects (KBOs) can indicate different surface compositions, environmental conditions, or formation characteristics within the Kuiper Belt. Data from the Deep Ecliptic Survey (DES, Millis et al. 2002) have been used to determine the plane of the Kuiper Belt, identifying \"core\" and \"halo\" populations with respect to this plane (Elliot et al. 2005). By comparing the colors of objects as a function of inclination, trends can be established distinguishing the core and halo populations. Sloan g', r' and i' observations were obtained from the 6.5-m Clay telescope at Las Campanas Observatory of 14 KBOs, which were combined with previously published data to examine the transition between these two populations as a function of color. For inclination bins containing equal numbers of KBOs, the percentage of red objects (B-R > 1.56, where B-R = 1.56 is the median of the sample) decreases with increasing inclination in a smooth, but nonlinear fashion.","(cont.) This steady decrease could imply that the objects at lower inclinations are less perturbed than those at higher inclinations, resulting in redder surfaces. Additionally, the objects at lower inclinations could represent a primordial population of objects, available to study and to constrain the formation models of the solar system."]},{"key":"dc:description.degree","label":"Dc Description Degree","values":["S.M."]},{"key":"dc:title","label":"Title","values":["Colors of Kuiper Belt objects : the relationship between KBO colors and Kuiper Belt plane inclination"]}]}],"canonical_facts":{"dc:contributor.advisor":["James L. Elliot."],"dc:contributor.department":["Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences."],"dc:contributor.other":["Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences."],"dc:creator":["Kane, Julia Frances"],"dc:date.accessioned":["2007-04-20T16:01:20Z"],"dc:date.available":["2007-04-20T16:01:20Z"],"dc:date.issued":["2006"],"dc:description":["Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2006.","Includes bibliographical references (p. 39-41)."],"dc:description.abstract":["A large population of small, icy bodies orbits the sun just beyond Neptune, known as the Kuiper Belt. These objects, thought to be the progenitors of short period comets, could provide a sample of primordial material in our solar system, constraining solar system formation models. The colors of Kuiper belt objects (KBOs) can indicate different surface compositions, environmental conditions, or formation characteristics within the Kuiper Belt. Data from the Deep Ecliptic Survey (DES, Millis et al. 2002) have been used to determine the plane of the Kuiper Belt, identifying \"core\" and \"halo\" populations with respect to this plane (Elliot et al. 2005). By comparing the colors of objects as a function of inclination, trends can be established distinguishing the core and halo populations. Sloan g', r' and i' observations were obtained from the 6.5-m Clay telescope at Las Campanas Observatory of 14 KBOs, which were combined with previously published data to examine the transition between these two populations as a function of color. For inclination bins containing equal numbers of KBOs, the percentage of red objects (B-R > 1.56, where B-R = 1.56 is the median of the sample) decreases with increasing inclination in a smooth, but nonlinear fashion.","(cont.) This steady decrease could imply that the objects at lower inclinations are less perturbed than those at higher inclinations, resulting in redder surfaces. Additionally, the objects at lower inclinations could represent a primordial population of objects, available to study and to constrain the formation models of the solar system."],"dc:description.degree":["S.M."],"dc:identifier.uri":["http://hdl.handle.net/1721.1/37279"],"dc:language.iso":["eng"],"dc:publisher":["Massachusetts Institute of Technology"],"dc:rights":["M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission."],"dc:rights.uri":["http://dspace.mit.edu/handle/1721.1/7582"],"dc:subject":["Earth, Atmospheric, and Planetary Sciences."],"dc:title":["Colors of Kuiper Belt objects : the relationship between KBO colors and Kuiper Belt plane inclination"],"dc:type":["Thesis"]},"updated_at":"2026-07-22T22:21:36Z"}