Near-Infrared Spectral Monitoring of Triton with IRTF/SpeX II: Spatial Distribution and Evolution of Ices

Published in 2010: Icarus 205, 594-604.

W.M. Grundy1,2, L.A. Young1,3, J.A. Stansberry4, M.W. Buie3, C.B. Olkin1,3, and E.F. Young1,3

(1) Visiting/remote observer at the Infrared Telescope Facility, operated by the University of Hawaii under Cooperative Agreement NCC 5-538 with the National Aeronautics and Space Administration, Science Mission Directorate, Planetary Astronomy Program.

(2) Lowell Observatory, Flagstaff AZ.

(3) Southwest Research Institute, Boulder CO.

(4) Steward Observatory, University of Arizona, Tucson AZ.

Download the PDF preprint.


Abstract

This report arises from an ongoing program to monitor Neptune's largest moon Triton spectroscopically in the 0.8 to 2.4 μm range using IRTF/SpeX. Our objective is to search for changes on Triton's surface as witnessed by changes in the infrared absorption bands of its surface ices N2, CH4, H2O, CO, and CO2. We have recorded infrared spectra of Triton on 53 nights over the ten apparitions from 2000 through 2009. The data generally confirm our previously reported diurnal spectral variations of the ice absorption bands (Grundy and Young 2004). Nitrogen ice shows a large amplitude variation, with much stronger absorption on Triton's Neptune-facing hemisphere. We present evidence for seasonal evolution of Triton's N2 ice: the 2.15 μm absorption band appears to be diminishing, especially on the Neptune-facing hemisphere. Although it is mostly dissolved in N2 ice, Triton's CH4 ice shows a very different longitudinal variation from the N2 ice, challenging assumptions of how the two ices behave. Unlike Triton's CH4 ice, the CO ice does exhibit longitudinal variation very similar to the N2 ice, implying that CO and N2 condense and sublimate together, maintaining a consistent mixing ratio. Absorptions by H2O and CO2 ices show negligible variation as Triton rotates, implying very uniform and/or high latitude spatial distributions for those two non-volatile ices.


Fig. 10. Triton's observed longitudinal spectral variations shown on a consistent logarithmic scale of relative variation along with the Voyager clear filter approach lightcurve from Smith et al. (1989, bottom).


Data products associated with this paper

Circumstances of Triton Observations
UT datelonlatminutes
2000/07/22 9:17344.5-50.0 9
2001/07/03 11:56310.3-49.947
2001/07/04 12:05 11.9-49.967
2001/07/05 12:39 74.6-49.948
2001/07/06 12:03134.3-49.964
2001/07/07 12:07195.7-49.956
2001/07/08 11:44255.9-49.980
2002/07/15 9:24 0.7-49.852
2002/07/16 9:24 61.9-49.854
2002/07/17 9:53124.3-49.884
2002/07/18 9:36184.8-49.864
2002/07/19 9:31245.8-49.868
2002/07/20 9:27306.9-49.868
2002/07/21 9:29 8.2-49.868
2002/07/22 9:21 69.1-49.884
2002/08/16 11:10164.1-49.996
2002/09/16 6:19249.5-49.984
2002/10/03 6:32211.0-49.948
2003/07/04 13:58101.0-49.664
2003/07/29 11:59186.5-49.728
2003/08/10 10:09196.4-49.758
2003/09/10 9:32292.6-49.840
2003/10/16 5:51327.5-49.888
2004/06/28 13:07194.9-49.3152
2004/07/28 11:44228.0-49.436
2004/08/12 12:19 67.7-49.552
2004/09/12 10:51161.7-49.648
2004/10/21 6:13 18.0-49.652
2005/07/04 13:06244.3-48.9146
2005/08/01 10:22151.5-49.144
2005/08/04 9:53333.9-49.176
2005/09/19 8:02265.2-49.368
2006/05/26 14:52 62.3-48.440
2006/06/26 13:39157.9-48.5128
2006/07/26 11:01188.0-48.672
2006/08/30 9:14166.0-48.848
2006/10/28 5:59170.3-49.068
2007/06/21 13:15252.6-47.9136
2007/06/22 13:10313.7-47.9160
2007/06/23 13:18 15.2-47.9128
2007/06/24 14:06 78.5-47.988
2007/06/25 13:13137.5-47.9132
2007/06/26 13:09198.6-47.9172
2007/06/27 13:16260.1-47.9132
2007/08/01 11:59239.8-48.116
2008/06/24 14:36182.9-47.356
2008/07/14 10:57318.3-47.472
2008/08/12 12:24297.5-47.644
2008/09/01 7:02 68.1-47.856
2008/09/28 9:55288.5-48.060
2009/06/22 14:35102.2-46.632
2009/06/24 14:25224.3-46.680
2009/07/21 12:07 71.7-46.864
2009/08/13 12:07 39.8-47.056
2009/08/31 11:07 60.0-47.242
2009/09/07 9:07122.5-47.268
2010/08/07 11:08 71.9-46.356
2010/08/30 9:55 36.9-46.580
2011/06/07 15:01348.0-45.124
2011/06/11 15:01233.0-45.128
2011/06/12 14:23292.7-45.186
2011/06/20 14:40 63.4-45.150
2011/06/28 14:31193.0-45.260
2011/08/06 12:04 54.8-45.560
2011/08/23 9:08 8.1-45.664
2011/09/18 9:42161.3-45.956
2011/11/13 6:07341.4-46.2144
2012/06/25 14:19111.6-44.380
2012/07/18 14:43 81.1-44.566
2012/09/02 7:01357.9-44.972
2012/09/05 9:44188.5-45.0284
2012/09/08 8:41 9.5-45.0200
2012/09/09 9:52 73.7-45.0224
2012/09/10 9:51134.9-45.0228
2012/09/12 10:03257.9-45.1232
2012/09/13 8:54316.1-45.1248
2013/07/23 15:11 70.1-43.6 36
2013/07/25 14:55191.9-43.6 48
2013/07/28 14:57 15.7-43.6 56
2014/08/04 13:49122.9-42.8135
2014/08/05 13:19182.9-42.8155
2014/08/06 13:10243.7-42.8175
2014/08/10 12:57128.1-42.8167
2014/08/11 12:59189.4-42.9171
2015/07/03 14:00 5.2-41.5108
2015/07/22 13:60 88.8-41.6143
2015/08/02 14:49 44.5-41.7 48
2015/10/01 05:31192.6-42.8 68
2016/07/31 13:40 21.7-40.7150
2016/08/16 12:19278.0-40.9144
2016/09/06 9:02115.3-41.2 72
2016/11/05 5:28180.1-41.8 80
2017/07/08 14:19 96.0-39.4 88
2017/07/30 10:46354.3-39.6 88
2017/08/13 11:40133.9-39.7 64
2017/09/12 10:04166.7-40.2 64
2018/09/26 9:52344.6-39.3 84
2019/08/27 11:15352.5-37.6167
2019/08/28 11:28 54.3-37.6159
2019/08/29 11:58116.8-37.7179
2019/08/31 12:26240.5-37.7147
2019/09/01 11:60300.6-37.7175
2019/09/02 11:36 0.8-37.7183
2020/06/30 14:23150.8-35.8 64
2020/07/30 13:06185.0-36.0 48
2020/08/30 11:05278.2-36.5 48
2020/10/04 10:29259.7-37.1 54
2020/10/31 9:28110.4-37.4 48
2020/11/25 6:16193.3-37.5 48
2021/07/14 14:23329.3-34.7 80
2021/07/27 14:23 45.6-34.8 68
2021/09/18 10:33 41.3-35.5 64
2021/10/22 8:03316.8-36.1 60
2022/07/25 14:10323.5-33.5 76
2022/08/06 13:30336.7-33.6 64
2022/09/04 11:10306.7-34.0 60
2022/09/27 9:06269.7-34.4 56
2022/10/23 7:09 56.8-34.8 60
2023/08/10 14:13264.5-32.3 64
2023/10/04 9:45 21.0-33.2 52
2023/10/22 8:29 39.9-33.5 64
2023/11/12 6:18240.3-33.8 64

(see preprint for details regarding data up to 2009/07/21)

(contact Will Grundy, Leslie Young, and Bryan Holler for details on the more recent data)