The probe has been located, along its projected nominal path, with quite high precision, within 0.13±0.09 arcsec, or 0.9±0.6 km. Spacecraft color appears to be red, with (V-Rc)=1.1±0.2 and a bolometric correction to the Rc band of (Bol-Rc)=-1.1±0.2. The apparent magnitude, Rc=20.8±0.2, is much fainter than originally expected. These features lead to suggest a lower limit for the Bond albedo α=0.11±0.05 and confirm that incident Sun light is strongly reddened by Gaia through its on-board MLI blankets covering the solar shield.
Relying on the Gaia figures, we found that VLT-class telescopes could yet be able to probe distant spacecraft heading Mars, up to 30 million km away, while a broader optical coverage of the forthcoming missions to Venus and Mars could be envisaged, providing to deal with space vehicles of minimum effective area A⩾106 cm2. In addition to L2 surveys, 2 m-class telescopes could also effectively flank standard radar-ranging techniques in deep-space probe tracking along Earth’s gravity-assist maneuvers for interplanetary missions.