An Introduction to the True Astronomy: Or, Astronomical Lectures,: Read in the Astronomical School of the University of Oxford

Æquator Aftronomers alfo alſo Altitude Angle Aphelion appear Arch arife Axis becauſe Body called Center Circle Circle of Latitude Co-fine Comet conftantly Conjunction Courſe defcribe Degrees Diameter Difference diftant Disk Diſtance diurnal Motion Eaft Earth Eccentrick Eclipfe Ecliptick equal Equator Equinoctial fame feem feen fhall fhew fhining fhould fince firft firſt fixed Stars fmall fome fometimes ftance ftill fuch fuppofe greateſt Heavens Horizon Hours increaſe inferior Planets Interfection itſelf Jupiter Latitude Lect Lecture lefs likewife Longitude Mars mean Anomaly Meaſure Meridian Minutes Moon Moon's moſt move muſt Nodes Number obferved oppofite Orbit paffes paffing thro Parallax parallel Penumbra Perihelion perpendicular Place Planet Plate Pofition Point Pole Proportion Quadrant Radius reft reprefent rifes right Afcenfion right Line round the Sun Saturn ſeen Semidiameter Shadow ſhall Sine Spectator Sun's Teleſcope thefe thence theſe thofe tion Triangle true true Anomaly Velocity Venus Vertex vifible Weft whofe