Форма представления | Статьи в зарубежных журналах и сборниках |
Год публикации | 2023 |
Язык | английский |
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Бикмаев Ильфан Фяритович, автор
Гумеров Рустам Исхакович, автор
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Библиографическое описание на языке оригинала |
Erece O, Khamitov I.M, Kaplan M, Physical properties of the slow-rotating near-Earth asteroid (2059) Baboquivari from one apparition//Planetary and Space Science. - 2023. - Vol.232, Is.. - Art. №105698. |
Аннотация |
we carried out photometric, spectroscopic, and for the first time, polarimetric observations of the Amor-type near-Earth asteroid (2059) Baboquivari. Our findings represent the first reliable determination of Baboquivari's physical properties. We used data from a 1m-class telescope (T100) along with ALCDEF data for photometric analyses and a 1.5-m-class telescope (RTT150) for polarimetric, spectroscopic, and additional photometric observations. We obtained the synodic rotation period of Baboquivari as 129.93 ? 2.31 h and the standard phase function parameters H and G as 16.05 ? 0.05, 0.22 ? 0.02, respectively. Our colour index (V-R) measurement of 0.45 ? 0.02 is consistent with spectroscopic observations, indicating an S (or sub-S) spectral type. Using the polarimetric and spectroscopic data, we found that the geometric albedo is 0.15 ? 0.03, and the spectral type is Sq. Based on the estimated albedo and absolute magnitude, Baboquivari has an effective diameter of 2.12 ? 0.21 km. Due to the scattered data in the light curve, its slow rotation and location among the NEAs suggest that Baboquivari may be a non-principal axis (NPA) rotator. |
Ключевые слова |
Minor planets; Near-earth asteroids: individual: (2059) Baboquivari; Methods: observational; Techniques: photometry; Polarimetry; Spectroscopy; |
Название журнала |
PLANETARY AND SPACE SCIENCE
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URL |
https://www.scopus.com/inward/record.uri?eid=2-s2.0-85159143491&doi=10.1016%2fj.pss.2023.105698&partnerID=40&md5=5282ce9d54e89cd5fea15d87041c1292 |
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https://repository.kpfu.ru/?p_id=286463 |
Полная запись метаданных |
Поле DC |
Значение |
Язык |
dc.contributor.author |
Бикмаев Ильфан Фяритович |
ru_RU |
dc.contributor.author |
Гумеров Рустам Исхакович |
ru_RU |
dc.date.accessioned |
2023-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2023-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2023 |
ru_RU |
dc.identifier.citation |
Erece O, Khamitov I.M, Kaplan M, Physical properties of the slow-rotating near-Earth asteroid (2059) Baboquivari from one apparition//Planetary and Space Science. - 2023. - Vol.232, Is.. - Art. №105698. |
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/?p_id=286463 |
ru_RU |
dc.description.abstract |
PLANETARY AND SPACE SCIENCE |
ru_RU |
dc.description.abstract |
we carried out photometric, spectroscopic, and for the first time, polarimetric observations of the Amor-type near-Earth asteroid (2059) Baboquivari. Our findings represent the first reliable determination of Baboquivari's physical properties. We used data from a 1m-class telescope (T100) along with ALCDEF data for photometric analyses and a 1.5-m-class telescope (RTT150) for polarimetric, spectroscopic, and additional photometric observations. We obtained the synodic rotation period of Baboquivari as 129.93 ? 2.31 h and the standard phase function parameters H and G as 16.05 ? 0.05, 0.22 ? 0.02, respectively. Our colour index (V-R) measurement of 0.45 ? 0.02 is consistent with spectroscopic observations, indicating an S (or sub-S) spectral type. Using the polarimetric and spectroscopic data, we found that the geometric albedo is 0.15 ? 0.03, and the spectral type is Sq. Based on the estimated albedo and absolute magnitude, Baboquivari has an effective diameter of 2.12 ? 0.21 km. Due to the scattered data in the light curve, its slow rotation and location among the NEAs suggest that Baboquivari may be a non-principal axis (NPA) rotator. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
|
ru_RU |
dc.title |
Physical properties of the slow-rotating near-Earth asteroid (2059) Baboquivari from one apparition |
ru_RU |
dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
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