... just over 100 MBAs (1.6 unknown to every 1 known) per square degree are detectable to R=22 in a 2 m survey based on the INT data, while our two best ecliptic Blanco fields away from opposition lead to 135 MBAs (2 unknown to every 1 known) to R=23 ...
... Integrations are required only (i) to determine the location in the ecliptic, relative to the Earth's orbit, of a single ... Density in the ecliptic of the cross section of the 1899 Leonid trail encountered by the Earth in 1999, for one example ...
... a 0 than listed in Table 1 in order to cross the ecliptic at the correct time ... cross section on intersection with the ecliptic, but with a concentration towards ... Figure 1 -- Cross section in (x; y) ecliptic coordinates of trail generated in 1899 ...
... enough that the velo city relative to Mars is dominated by the ecliptic component ... of the relative velocity becomes significant compared to the ecliptic component ...
... so that by p ointing at fields in the ecliptic plane, the roll of the spacecraft is ... p ointings each lasting 75 days along the ecliptic plane some of the fields will b ...
... of Aries' is the name given to the point where the Ecliptic crosses the Celestial Equator, and is the point from which all ... ТљТљ And of course the points along the ecliptic marking the Sun's greatest Northerly and Southerly declinations, and thusТ ...
... not stray too far from the Ecliptic and so cannot reach M31.б Although Palma occupies the asteroid Main Belt, it has an unusually high orbital inclination, and on this occasion itб will beб about 34 degrees north of the Ecliptic such that it crosses in ...