@article{oai:mie-u.repo.nii.ac.jp:00003511,
 author = {伊藤, 信成 and ITOH, Nobunari},
 journal = {三重大学教育学部研究紀要, 自然科学・人文科学・社会科学・教育科学},
 month = {Mar},
 note = {application/pdf, Astronomy is categorized into earth science for high school curriculum in Japan. Although absolute number of students who take earth science class is small, the number is gradually increasing due to the new official curriculum guidelines started on 2011. Therefore, it is important not only for students but teachers who are not good at teaching astronomy to provide appropriate learning materials for promoting a better understanding. Star
Color is one of the most essential characteristics. As stellar color difference can be easily detected by naked eyes and it gives us information for stellar temperature, the estimation of stellar surface temperature is thought to be a familiar them to high school students. Then an astronomical learning program for estimating stellar surface temperature was developed using B, V, Rc, and Ic band archived image data opened by national astronomical observatory Japan. In this program, students can semi-automatically estimate stellar temperature by input the stellar brightness in each band into a spreadsheet contained a macro program. To evaluate the efficiency of the learning program, the trial practice of the program was carried out. As a result, the program got favorable response from over 90% of experimental participants. It is also found that the program is effective for students who have less learning about astronomy.},
 pages = {27--33},
 title = {アーカイブデータを用いた恒星の表面温度推定用教材の開発},
 volume = {65},
 year = {2014}
}