A Search for Distant Satellites of Neptune

Michael J.I. Brown and Rachel L. Webster, PASA, 15 (3), 325
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Nereid

There has been considerable discussion in the literature about the rotation of Nereid and the amplitude of its light curve (Schaefer and Schaefer 1988a, Schaefer and Schaefer 1988b, Bus and Larson 1989, Williams, Jones and Taylor 1991, Thomas, Veverka and Helfenstein 1991, Dobrovolskis 1995, Buratti, Goguen and Mosher 1997). A summary of these papers is provided by Buratti, Goguen and Mosher 1997. While our tex2html_wrap_inline144 R band images of Nereid only measure the light curve for 1 hour on each night, a large magnitude change would be strong evidence of a large amplitude (tex2html_wrap_inline148) light curve similar to those reported by Schaefer and Schaefer (1988a, 1988b) and Williams, Jones and Taylor (1991).

The observations and data reduction are described in the previous section. Each tex2html_wrap_inline116 R band image was used (rather than the combined images) so any rapid changes of the magnitude of Nereid could be easily detected. SExtractor (Bertin and Arnouts 1996) was used to obtain the photometry of Nereid and this photometry is summarised in Table 2.

Table 2 shows that the magnitude of Nereid does not significantly change on either night of observation. A tex2html_wrap_inline154 magnitude increase is seen between the two nights but the error estimate for this magnitude change does not include systematic errors which may have varied between the two nights of observations. It should also be noted that Nereid is in a busy field during the observations and this could introduce a bias into the magnitude estimates. Our measured lightcurve for Nereid is consistent with observations by Thomas, Veverka and Helfenstein (1991) and Buratti, Goguen and Mosher (1997) who also found no large variations of Nereid's magnitude. Our R band magnitudes are also similar to those reported by Buratti, Goguen and Mosher (1997). We can not rule out a large amplitude light curve for Nereid, however, our observations are consistent with Nereid having a light curve with tex2html_wrap_inline158.

Table 2. Nereid Photometry

UT Date UT time R band magnitude
and tex2html_wrap_inline162 error
30 Sep 1997 9:40 tex2html_wrap_inline164
30 Sep 1997 9:52 tex2html_wrap_inline164
30 Sep 1997 10:04 tex2html_wrap_inline168
30 Sep 1997 10:16 tex2html_wrap_inline170
30 Sep 1997 10:28 tex2html_wrap_inline164
30 Sep 1997 10:40 tex2html_wrap_inline174
30 Sep 1997 10:52 tex2html_wrap_inline176
30 Sep 1997 Average tex2html_wrap_inline178
 1 Oct 1997 10:03 tex2html_wrap_inline180
 1 Oct 1997 10:14 tex2html_wrap_inline180
 1 Oct 1997 10:40 tex2html_wrap_inline184
 1 Oct 1997 10:52 tex2html_wrap_inline186
 1 Oct 1997 11:04 tex2html_wrap_inline188
 1 Oct 1997 Average tex2html_wrap_inline190
 


Next Section: Conclusions
Title/Abstract Page: A Search for Distant
Previous Section: Observations and Analysis
Contents Page: Volume 15, Number 3

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