<Observations>
  <FileVersion>2.10</FileVersion>
  <Event>
    <Date>2025|1|2|13.2</Date>
    <Details>
      <Star>UCAC4|491-045603|3|3148146916993989120|7.6781178552|8.171470824|0.17|0.15|0.01|0|7.70106919|8.1133379|14.38|14.05|13.56|0</Star>
        <StarIssues>1.05|0|0|0|1.20|10|0.00|0.00|0.00|0.00</StarIssues>
      <Asteroid>26833|1990 RE|-6.71397425|1.88696421|-0.0011413|0.0015531|0.0000016|-0.0000002|4.35634|0.00020|11.8|1.0|18.24</Asteroid>
      <EventFits>
        <SolveFlags>1|1|0|0|0|0|0|0|0</SolveFlags>
        <EllipticFit>0.00|0.00|1.00|1.00|0.0|0|0|0|0.00|0.00</EllipticFit>
        <EllipseUncertainty>0.16|0.58|||</EllipseUncertainty>
      </EventFits>
    </Details>
    <Observations>
      <Observer>
        <ID>1|Katsuhiko Kitazaki||0|Musashino, Tokyo|JP|+139 33 41.2|+35 42 37.0|66| |40|6|a|a</ID>
        <Conditions>1|1|6.9||[7.0,6.8:338.0]Since the target star was dark (14.0 mag), the frame exposure time was increased (338 msec) to improvethe S/N ratio.</Conditions>
        <D>13 17 47.10|D|0.05||| </D>
        <R>13 17 48.33|R|0.05||| </R>
      </Observer>
      <Prediction>2|+140  0  0. |+35 41 14. |13 17 45.24|JPL#44+Ephem:2025-Feb-12</Prediction>
    </Observations>
    <Added>2025|2|15</Added>
    <LastEdited>2023|7|17</LastEdited>
  </Event>
</Observations>
