Neptune and Titan observed with Keck Telescope adaptive optics

We report on observations taken during engineering science validation time using the new adaptive optics system at the 10-m Keck II Telescope. We observed Neptune and Titan at near- infrared wavelengths. These objects are ideal for adaptive optics imaging because they are bright and small, yet have many diffraction-limited resolution elements across their disks. In addition Neptune and Titan have prominent physical features, some of which change markedly with time. We have observed infrared-bright 'storms' on Neptune, and very low- albedo surface regions on Titan, Saturn's largest moon. Spatial resolution on Neptune and Titan was 0.05 - 0.06 and 0.04 - 0.05 arc sec, respectively.

[1]  S. K. Croft,et al.  Voyager 2 at Neptune: Imaging Science Results , 1989, Science.

[2]  John B. Shoven,et al.  I , Edinburgh Medical and Surgical Journal.

[3]  H. Hammel,et al.  Atmospheric Structure of Neptune in 1994, 1995, and 1996 , 1997 .

[4]  D. S. Acton,et al.  First Light Adaptive Optics Images from the Keck II Telescope: A New Era of High Angular Resolution Imagery , 2000 .

[5]  T. Owen,et al.  Titan's surface and troposphere, investigated with ground-based, near-infrared observations. , 1991, Icarus.

[6]  G. G. Stokes "J." , 1890, The New Yale Book of Quotations.

[7]  M. Allen,et al.  Photochemistry of the atmosphere of Titan: comparison between model and observations. , 1984, The Astrophysical journal. Supplement series.

[8]  Neptune's Cloud Structure and Activity: Ground-Based Monitoring with Adaptive Optics , 1998 .

[9]  J. Lunine,et al.  Ethane Ocean on Titan , 1983, Science.

[10]  Mark T. Lemmon,et al.  Titan's Surface, Revealed by HST Imaging , 1996 .

[11]  Donald T. Gavel,et al.  Titan: High-Resolution Speckle Images from the Keck Telescope , 1999 .

[12]  S. Limaye,et al.  Clouds and Circulation on Neptune: Implications of 1991 HST Observations , 1995 .

[13]  Malcolm J. Northcott,et al.  First ground-based adaptive optics observations of Neptune and Proteus , 1997 .

[14]  H. Hammel,et al.  Clouds and hazes in the atmosphere of Neptune. , 1995 .

[15]  E. Gendron,et al.  Spatially Resolved Images of Titan by Means of Adaptive Optics , 1997 .

[16]  D. Muhleman Radar Investigations of Mars, Merrcury, and Titan , 1995 .