... s1) {Get the ra & dec if necessary} if (s1!sun) if (s1!moon) if (s1!mercury) if (s1!venus) if(s1!mars) if(s1!jupiter) if (s1!saturn) if (s1!uranus) if(s1!neptune) {Phew! none of those, so get ra/dec} ask_for_coordinates(r) end_if end_if end_if end_if end ...
... Uranus, Neptune,) new_line write_string(Elliptical, Parabolic, or name of body with current RA and Dec) new_line new_line ask_for_string(First argument [choose one of the above],s1) {Get coordinates if not a main body: added after printing book!} if (s1 ...
... Jupiter and Saturn are significantly more enriched in heavy material (30%-60% more) than previously thought 6 Uranus & Neptune ... compared to Voyager data 0.3 0,5 0,4 1 Neptune 0.1 0,3 0,2 0.05 0.01 0,1 Uranus 0.15 0.12 0 0,8 0,9 Z 2 Nettelmann et al ...
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... Model is also relevant for terrestrial planets with deep oceans and Neptune/Uranus-mass planets, and to convective envelopes of stars] Ogilvie 2009 Favier, Barker, Baruteau & Ogilvie, 2014, MNRAS Topic 2 Tides in rotating planets with a core · Simplified ...
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... mars) set_character(c1,Y) end_if if (s1=jupiter) set_character(c1,Y) end_if if (s1=saturn) set_character(c1,Y) end_if if (s1=uranus) set_character(c1,Y) end_if if (s1=neptune) set_character(c1,Y) end_if if (s1=elliptical) set_character(c1,Y) end_if if (s1 ...
... mars) set_character(c1%p) end_if if (s1=jupiter) set_character(c1%p) end_if if (s1=saturn) set_character(c1%p) end_if if (s1=uranus) set_character(c1%p) end_if if (s1=neptune) set_character(c1%p) end_if if (s1=elliptical) set_character(c1%o) end_if if (s1 ...