The Sun Treatise (Unknown) - Page 16

Mean longitudes The average angular positions of celestial bodies along the ecliptic of the planets in the zodiac of annual motion on January 1, 1860 CE

According to the Surya Siddhanta One of the foundational texts of Indian astronomy, dated by various scholars between the 4th and 11th centuries CE

Original | Beeja Refined | According to Modern Astronomy

original: "Beeja Samskrita"; Beeja refers to correction factors applied by later Indian astronomers to the original Surya Siddhanta constants to align them better with observed reality.

Planet	Degree (Orig.)	Minute (Orig.)	Second (Orig.)	Degree (Beeja)	Minute (Beeja)	Second (Beeja)	Degree (Mod.)	Minute (Mod.)	Second (Mod.)
Sun	66	18	21	66	18	21	100	5	6
Mercury	155	2	30	148	25	36	151	28	20
Venus	336	54	55	334	57	18	366	12	36
Mars	162	36	5	162	36	5	167	26	32
Jupiter	104	7	22	100	48	56	103	35	17
Saturn	128	17	11	133	14	46	137	10	10
Moon	3	4	8	3	4	8	12	41	23
Lunar Apogee	327	50	24	326	11	11	326	47	35
Lunar Node	312	26	51	310	50	38	312	48	10

The "Lunar Apogee" (original: Chandrochcha) refers to the point where the Moon is farthest from Earth, and the "Lunar Node" (original: Chandrapata) refers to the points where the Moon's orbit intersects the ecliptic—the path of the Sun.