Discovery of the Bright Trans-Neptunian Object 2000 EB[TINF]173[/TINF]

We describe the discovery circumstances and photometric properties of 2000 EB 173 , now one of the brightest trans-Neptunian objects (TNOs) with opposition magnitude m R = 18.9 and also one of the largest Plutinos, found with the drift-scanning camera of the Quasar Equatorial Survey Team, attached to the 1 m Schmidt telescope of the National Observatory of Venezuela. We measure B - V = 0.99 ± 0.14 and V - R = 0.57 ± 0.05, a red color observed for many fainter TNOs. At our magnitude limit m R = 20.1 ± 0.20, our single detection reveals a sky density of 0.015 TNOs per square degree (the error bars are 68% confidence limits), consistent with fainter surveys showing a cumulative number proportional to 10 . Assuming an inclination distribution of TNOs with FWHM exceeding 30°, it is likely that 100 to several hundred objects brighter than m R = 20.1 remain to be discovered.