2.15 2025|11|6|15.0

UCAC4|554-023488|3|3375069207679123968|6.2576266797|20.681860195|0.28|0.20|0.00|0|6.28364367|20.6741740|14.86|14.35|13.67|0 1.15|0|0|0|1.20|10|0.00|0.00|0.00|0.00| 1269|Rollandia|-2.40283437|-0.19472111|-0.0045500|0.0003142|0.0000008|0.0000000|2.89496|0.00048|103.3|5.8|14.81 1|1|0|0|0|0|0|0|0 -3.2|-49.4|103.3|103.3|0.0|1|0|0|0.0|0.0 1.3|0.4||| 2025|11|6|15.2509529|0.336|0.00 1269|-3323.9|2006.5|-1.5113|0.9067|0.0188|0.0188|0|2|0|f4|19.3|40.9|1.00|0.93|9.00|-9.00 1269|-183.1|2260.7|2025|11|6.6269222|0.0000560|9.4|1.0296|18.8|355.186|0 ||

1|Katsuhiko Kitazaki||0|Musashino, Tokyo|JP|+139 33 41.2|+35 42 37.0|66| |40|6|a|a 3|1|2.7||[2.7,2.7:144.0]The moon was near the target star, and the small size of Mag Dolp resulted in a poor signal-to-noiseratio. The reappearance was gradual. 15 15 0.48|D|0.10||| 15 15 4.6|R|0.6||| 2|Takeshi Nemoto||0|Tama, Tokyo|JP|+139 27 34.7|+35 38 58.5|50| |25|2|a|a 2|1|4.2||[4.3,4.1:490.0] 15 15 0.52|D|0.13||| 15 15 8.09|R|0.14||| 3|+140 0 0. |+35 18 18. |15 15 4.18|JPL#73+Ephem 2026|1|23 2023|7|17