{"title":"Observation of Three Variable Stars and an Asteroid Using Small Telescopes in the\n United Arab Emirates (UAE)","authors":"M. Odeh, M. Al-Wardat","doi":"10.5140/jass.2023.40.1.19","DOIUrl":null,"url":null,"abstract":"We present the results of using small telescopes in the United Arab Emirates\n (UAE) for observing variable stars and asteroids. Two telescopes, namely, 5”\n apochromatic refractor and 14” Schmidt-Cassegrain, at Al-Khatim Observatory (M44) were\n used for the observations. The targets were the three variable stars RR GEM, AG LMi, and\n DL CMi and the asteroid 22 Kalliope. We found a good consistency between our light\n curves and published ones for the calibration targets, i.e., the asteroid 22 Kalliope\n and the variable star RR GEM. According to previous studies, AG LMi has two suggested\n periods, 16.3 hours and 32.62 hours. Our results clearly confirm the second one, with a\n period of 32.6175 hours. The star DL CMi has several suggested periods as per previous\n studies, such as 4.0173 days, 1.9606 days, and 2.0086 days. Our observations confirm the\n first one, with a period of 4.0159 days. These results demonstrate the effectiveness of\n using small telescopes for observing variable stars and asteroids. This work provides\n some recommendations on using small telescopes for such observations.","PeriodicalId":44366,"journal":{"name":"Journal of Astronomy and Space Sciences","volume":null,"pages":null},"PeriodicalIF":0.6000,"publicationDate":"2023-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Astronomy and Space Sciences","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.5140/jass.2023.40.1.19","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
We present the results of using small telescopes in the United Arab Emirates
(UAE) for observing variable stars and asteroids. Two telescopes, namely, 5”
apochromatic refractor and 14” Schmidt-Cassegrain, at Al-Khatim Observatory (M44) were
used for the observations. The targets were the three variable stars RR GEM, AG LMi, and
DL CMi and the asteroid 22 Kalliope. We found a good consistency between our light
curves and published ones for the calibration targets, i.e., the asteroid 22 Kalliope
and the variable star RR GEM. According to previous studies, AG LMi has two suggested
periods, 16.3 hours and 32.62 hours. Our results clearly confirm the second one, with a
period of 32.6175 hours. The star DL CMi has several suggested periods as per previous
studies, such as 4.0173 days, 1.9606 days, and 2.0086 days. Our observations confirm the
first one, with a period of 4.0159 days. These results demonstrate the effectiveness of
using small telescopes for observing variable stars and asteroids. This work provides
some recommendations on using small telescopes for such observations.
期刊介绍:
JASS aims for the promotion of global awareness and understanding of space science and related applications. Unlike other journals that focus either on space science or on space technologies, it intends to bridge the two communities of space science and technologies, by providing opportunities to exchange ideas and viewpoints in a single journal. Topics suitable for publication in JASS include researches in the following fields: space astronomy, solar physics, magnetospheric and ionospheric physics, cosmic ray, space weather, and planetary sciences; space instrumentation, satellite dynamics, geodesy, spacecraft control, and spacecraft navigation. However, the topics covered by JASS are not restricted to those mentioned above as the journal also encourages submission of research results in all other branches related to space science and technologies. Even though JASS was established on the heritage and achievements of the Korean space science community, it is now open to the worldwide community, while maintaining a high standard as a leading international journal. Hence, it solicits papers from the international community with a vision of global collaboration in the fields of space science and technologies.