2023 年 9 月 13 日 (319) 木卫二掩星,为遮住参宿四做准备

Q1 Earth and Planetary Sciences
J. L. Ortiz, M. Kretlow, C. Schnabel, N. Morales, J. Flores-Mart'in, M. S. Gonz'alez, F. Casarramona, A. Selva, C. Perell'o, A. Rom'an-Reche, S. Alonso, J. Rizos, R. Gonccalves, A. Castillo, J. Madiedo, P. M. S'anchez, J. M. F. and'ujar, J. L. Maestre, E. Smith, M. Gil, V. Pelenjow, S. M. Soriano, J. Mart'i, P. Luque-Escamilla, R. Casas, J. D. Casal, J. Rovira, F. Aceituno, V. Dekert, V. D. O. Guimer'a, J. Estepa, Y. Kilic, Rodrigo Leiva, P. Santos-Sanz, R. Duffard, E. Fern'andez-Valenzuela, M. Vara-Lubiano, A. Alvarez-Candal, F. Rommel
{"title":"2023 年 9 月 13 日 (319) 木卫二掩星,为遮住参宿四做准备","authors":"J. L. Ortiz, M. Kretlow, C. Schnabel, N. Morales, J. Flores-Mart'in, M. S. Gonz'alez, F. Casarramona, A. Selva, C. Perell'o, A. Rom'an-Reche, S. Alonso, J. Rizos, R. Gonccalves, A. Castillo, J. Madiedo, P. M. S'anchez, J. M. F. and'ujar, J. L. Maestre, E. Smith, M. Gil, V. Pelenjow, S. M. Soriano, J. Mart'i, P. Luque-Escamilla, R. Casas, J. D. Casal, J. Rovira, F. Aceituno, V. Dekert, V. D. O. Guimer'a, J. Estepa, Y. Kilic, Rodrigo Leiva, P. Santos-Sanz, R. Duffard, E. Fern'andez-Valenzuela, M. Vara-Lubiano, A. Alvarez-Candal, F. Rommel","doi":"10.1093/mnrasl/slad179","DOIUrl":null,"url":null,"abstract":"On 12 December 2023, the star α Orionis will be occulted by asteroid (319) Leona. This represents an extraordinary and unique opportunity to analyze the brightness distribution of Betelgeuse’s photosphere with extreme angular resolution by studying lightcurves from different points on Earth and at different wavelengths. Here we present observations of another occultation by asteroid Leona, on 13 September 2023, whose goal was to determine Leona’s projected shape and size in preparation for the December 12th event and its interpretation. The occultation campaign was highly successful with 25 positive detections from 17 different sites and a near miss. The effective diameter in projected area derived from the positive detections was 66 ± 2 km using an elliptical fit to the instantaneous limb. The body is highly elongated, with dimensions of 79.6 ± 2.2 km x 54.8 ± 1.3 km in its long and short axis, respectively, at occultation time. This result, in combination with dense time series photometry of Leona that we recently obtained, together with archival sparse photometry, allowed us to predict the angular size of the asteroid for the Betelgeuse event and to simulate the expected brightness change. Also, an accurate position coming from the occultation is provided, to improve the orbit of Leona.","PeriodicalId":18951,"journal":{"name":"Monthly Notices of the Royal Astronomical Society: Letters","volume":"24 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2023-09-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"The stellar occultation by (319) Leona on 13 September 2023 in preparation for the occultation of Betelgeuse\",\"authors\":\"J. L. Ortiz, M. Kretlow, C. Schnabel, N. Morales, J. Flores-Mart'in, M. S. Gonz'alez, F. Casarramona, A. Selva, C. Perell'o, A. Rom'an-Reche, S. Alonso, J. Rizos, R. Gonccalves, A. Castillo, J. Madiedo, P. M. S'anchez, J. M. F. and'ujar, J. L. Maestre, E. Smith, M. Gil, V. Pelenjow, S. M. Soriano, J. Mart'i, P. Luque-Escamilla, R. Casas, J. D. Casal, J. Rovira, F. Aceituno, V. Dekert, V. D. O. Guimer'a, J. Estepa, Y. Kilic, Rodrigo Leiva, P. Santos-Sanz, R. Duffard, E. Fern'andez-Valenzuela, M. Vara-Lubiano, A. Alvarez-Candal, F. Rommel\",\"doi\":\"10.1093/mnrasl/slad179\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"On 12 December 2023, the star α Orionis will be occulted by asteroid (319) Leona. This represents an extraordinary and unique opportunity to analyze the brightness distribution of Betelgeuse’s photosphere with extreme angular resolution by studying lightcurves from different points on Earth and at different wavelengths. Here we present observations of another occultation by asteroid Leona, on 13 September 2023, whose goal was to determine Leona’s projected shape and size in preparation for the December 12th event and its interpretation. The occultation campaign was highly successful with 25 positive detections from 17 different sites and a near miss. The effective diameter in projected area derived from the positive detections was 66 ± 2 km using an elliptical fit to the instantaneous limb. The body is highly elongated, with dimensions of 79.6 ± 2.2 km x 54.8 ± 1.3 km in its long and short axis, respectively, at occultation time. This result, in combination with dense time series photometry of Leona that we recently obtained, together with archival sparse photometry, allowed us to predict the angular size of the asteroid for the Betelgeuse event and to simulate the expected brightness change. Also, an accurate position coming from the occultation is provided, to improve the orbit of Leona.\",\"PeriodicalId\":18951,\"journal\":{\"name\":\"Monthly Notices of the Royal Astronomical Society: Letters\",\"volume\":\"24 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2023-09-21\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Monthly Notices of the Royal Astronomical Society: Letters\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1093/mnrasl/slad179\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"Earth and Planetary Sciences\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Monthly Notices of the Royal Astronomical Society: Letters","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1093/mnrasl/slad179","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"Earth and Planetary Sciences","Score":null,"Total":0}
引用次数: 0

摘要

2023 年 12 月 12 日,猎户座α星将被小行星 (319) 利昂娜掩星。这是一个非同寻常的独特机会,我们可以通过研究来自地球上不同点和不同波长的光曲线,以极高的角度分辨率分析参宿四光球的亮度分布。在此,我们介绍 2023 年 9 月 13 日对小行星利昂娜的另一次掩星观测,其目的是确定利昂娜的预计形状和大小,为 12 月 12 日的掩星活动及其解释做准备。这次掩星活动非常成功,在 17 个不同地点共探测到 25 次正面掩星和一次近距离掩星。通过对瞬时边缘进行椭圆拟合,从正面探测到的投影面积得出的有效直径为 66 ± 2 千米。天体高度拉长,掩星时长轴和短轴的尺寸分别为 79.6 ± 2.2 千米 x 54.8 ± 1.3 千米。这一结果与我们最近获得的利昂娜密集时间序列光度测量以及档案稀疏光度测量相结合,使我们能够预测该小行星在贝特宙斯事件中的角度大小,并模拟预期的亮度变化。此外,我们还提供了掩星产生的精确位置,以改进利昂娜的轨道。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The stellar occultation by (319) Leona on 13 September 2023 in preparation for the occultation of Betelgeuse
On 12 December 2023, the star α Orionis will be occulted by asteroid (319) Leona. This represents an extraordinary and unique opportunity to analyze the brightness distribution of Betelgeuse’s photosphere with extreme angular resolution by studying lightcurves from different points on Earth and at different wavelengths. Here we present observations of another occultation by asteroid Leona, on 13 September 2023, whose goal was to determine Leona’s projected shape and size in preparation for the December 12th event and its interpretation. The occultation campaign was highly successful with 25 positive detections from 17 different sites and a near miss. The effective diameter in projected area derived from the positive detections was 66 ± 2 km using an elliptical fit to the instantaneous limb. The body is highly elongated, with dimensions of 79.6 ± 2.2 km x 54.8 ± 1.3 km in its long and short axis, respectively, at occultation time. This result, in combination with dense time series photometry of Leona that we recently obtained, together with archival sparse photometry, allowed us to predict the angular size of the asteroid for the Betelgeuse event and to simulate the expected brightness change. Also, an accurate position coming from the occultation is provided, to improve the orbit of Leona.
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters Earth and Planetary Sciences-Space and Planetary Science
CiteScore
8.80
自引率
0.00%
发文量
136
期刊介绍: For papers that merit urgent publication, MNRAS Letters, the online section of Monthly Notices of the Royal Astronomical Society, publishes short, topical and significant research in all fields of astronomy. Letters should be self-contained and describe the results of an original study whose rapid publication might be expected to have a significant influence on the subsequent development of research in the associated subject area. The 5-page limit must be respected. Authors are required to state their reasons for seeking publication in the form of a Letter when submitting their manuscript.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信