137032 (1998 UO1)

Data

Number 137032
Provisional Designation 1998 UO1
Type Apollo, NEO
Diameter 1.055 km
Absolute Magnitude, H 16.6
Rotation period 2.925 h
Geometric Albedo 0.183
Eccentricity 0.7632
Semi-major axis 1.595 au
Inclination 25.49 °
Discovery Date 1998-10-19
Discovery Means LINEAR at Socorro

Radar Experiments

Doppler-Only (Continuous Wave) Echo Power Spectra

2010-10-02

2010-10-02, 1998UO1.oct02.s1Hz.cw.png

2010-09-30

2010-09-30, 1998UO1.sep30.s1Hz.cw.gif

2010-10-02, 1998UO1.oct02.s1Hz.cw.png

Description

Echo power spectrum obtained on 2010-10-2 smoothed to a frequency resolution of 1 Hz. Power in the opposite circular (OC) polarization as transmitted is the solid line while the power in the same circular (SC) polarization as transmitted is the dashed line. The polariation ratio on this date was 0.07.

Observation Date: 2010-10-02 (20:45:33-20:52:47)

Resolution: 1 Hz

Polarization Ratio: 0.07

Download Options:

CSV file is the raw data corresponding to the viewed cw spectra. The CSV file consists of three columns. The first column is the doppler frequency (Hz), the second column is the echo power in the same sense (SC) and the third column is the echo power in the opposite sense (OC). Echo power is in units of standard deviation above the noise baseline.
2010-09-30, 1998UO1.sep30.s1Hz.cw.gif

Description

Echo power spectrum obtained on 2010-9-30 smoothed to a frequency resolution of 1 Hz. Power in the opposite circular (OC) polarization as transmitted is the solid line while the power in the same circular (SC) polarization as transmitted is the dashed line. The polariation ratio on this date was 0.32.

Observation Date: 2010-09-30 (19:42:46-20:46:11)

Resolution: 1 Hz

Polarization Ratio: 0.32

Download Options:

CSV file is the raw data corresponding to the viewed cw spectra. The CSV file consists of three columns. The first column is the doppler frequency (Hz), the second column is the echo power in the same sense (SC) and the third column is the echo power in the opposite sense (OC). Echo power is in units of standard deviation above the noise baseline.

Additional Information


  • NASA Jet Propulsion Laboratory Small-Body Database entry

 

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