Astronomy Concepts
This page introduces the foundational astronomical concepts used throughout the Surya Siddhanta. It begins with how the sky itself is observed and structured — the geocentric model, the ecliptic, the nakṣatras, and the grahas that travel along the ecliptic. It then introduces the orbital reference points used to correct a graha's idealized circular motion toward its true position.
Foundations of Observation
In the Surya Siddhanta, the Earth is fixed in both position and rotation, and everything revolves around it. The text views the sky from the vantage of the northern hemisphere. This places the ecliptic, nakṣatras, zodiac, and planets to the south. This means east is to the left and west is to the right. These directions are reversed in the southern hemisphere.
Vayu, inadequately translated as wind, is the word for the force that causes movement in the Vedic paradigm. The specific vayu that moves the planets is called pravaha-vayu. The word means a flowing, carrying current or wind; in the cosmic context, it causes the eastward flow of the planets along their orbits (SS 2.3).
Motion of Stars and Planets
Two simultaneous motions govern everything in the sky. The first is shared by all celestial bodies — stars, planets, Sun, and Moon — and is caused by Pravaha-vayu carrying the entire celestial sphere westward once per day. This is why everything rises in the east and sets in the west. The second motion belongs to the planets alone. While being carried westward by Pravaha, the planets also have their own slower eastward movement along the ecliptic, gradually shifting position against the background of stars over days, weeks, and months. The following model illustrates both motions simultaneously.
The Ecliptic
The ecliptic is the eastward path the Sun traces against the backdrop of the stars. The planets all travel within a band centered on the ecliptic, and this band is what the zodiac and nakṣatras are measured along.
The ecliptic is tilted around 24 degrees from the celestial equator. The two points where the celestial equator and ecliptic cross are called the equinoxes. This tilt is what causes the seasons. When the Sun is north of the celestial equator, the northern hemisphere has summer while the southern hemisphere has winter — and the reverse when the Sun crosses south.
As the Sun travels along the ecliptic, its declination — its height relative to the celestial equator — rises and falls throughout the year. When the Sun's declination reaches its highest point, this is called the summer solstice. When it reaches its lowest point, this is the winter solstice.
The ecliptic gets its name from eclipses — which occur when the Sun and Moon are aligned not just in longitude, but also near the point where the Moon's path crosses the ecliptic.
90° top-down
The Nakṣatras
The nakṣatras are 27 star groupings, each spanning 13°20′ (SS 2.64). Like the rest of the celestial sphere, they circle the sky once a day. The Surya Siddhanta states that at the end of Kṛta Yuga, all planets' mean positions were at 0° Aries (SS 1.57) — the end of Revatī, the last nakṣatra. We take this point, the start of Aśvinī, as the first nakṣatra.
Nakṣatra is fairly translated as "constellation" — both refer to groupings of stars marking positions in the sky. What differs is which constellations: the 27 nakṣatras and the 88 Western constellations carve the sky into different clusters. The nakṣatras divide only the ecliptic — the band the Sun, Moon, and planets travel through — into 27 equal segments of 13°20′ each; the Western constellations cover the whole sky in irregular, unrelated shapes.
Each nakṣatra's span comes from dividing the full circle, expressed in arcminutes, equally among the 27 nakṣatras.
Full Circle × Arc-minutes per Degree = Arc-minutes in a Full Circle
360° × 60′ = 21,600′
Arc-minutes in a Full Circle ÷ Nakṣatras = Arc-minutes per Nakṣatra
21,600′ ÷ 27 = 800′
Arc-minutes per Nakṣatra ÷ Arc-minutes per Degree = Degrees per Nakṣatra
800′ ÷ 60 = 13°20′
| # | Nakṣatra | Degree Range |
|---|---|---|
| 1 | Aśvinī | 0°00′ – 13°20′ |
| 2 | Bharaṇī | 13°20′ – 26°40′ |
| 3 | Kṛttikā | 26°40′ – 40°00′ |
| 4 | Rohiṇī | 40°00′ – 53°20′ |
| 5 | Mṛgaśīrṣa | 53°20′ – 66°40′ |
| 6 | Ārdrā | 66°40′ – 80°00′ |
| 7 | Punarvasu | 80°00′ – 93°20′ |
| 8 | Puṣya | 93°20′ – 106°40′ |
| 9 | Āśleṣā | 106°40′ – 120°00′ |
| 10 | Maghā | 120°00′ – 133°20′ |
| 11 | Pūrva Phalgunī | 133°20′ – 146°40′ |
| 12 | Uttara Phalgunī | 146°40′ – 160°00′ |
| 13 | Hasta | 160°00′ – 173°20′ |
| 14 | Citrā | 173°20′ – 186°40′ |
| 15 | Svātī | 186°40′ – 200°00′ |
| 16 | Viśākhā | 200°00′ – 213°20′ |
| 17 | Anurādhā | 213°20′ – 226°40′ |
| 18 | Jyeṣṭhā | 226°40′ – 240°00′ |
| 19 | Mūla | 240°00′ – 253°20′ |
| 20 | Pūrva Āṣāḍhā | 253°20′ – 266°40′ |
| 21 | Uttara Āṣāḍhā | 266°40′ – 280°00′ |
| Abhijit* | ~276°40′ – 283°20′ | |
| 22 | Śravaṇa | 280°00′ – 293°20′ |
| 23 | Dhaniṣṭhā | 293°20′ – 306°40′ |
| 24 | Śatabhiṣā | 306°40′ – 320°00′ |
| 25 | Pūrva Bhādrapadā | 320°00′ – 333°20′ |
| 26 | Uttara Bhādrapadā | 333°20′ – 346°40′ |
| 27 | Revatī | 346°40′ – 360°00′ |
*Abhijit is a common 28th nakṣatra that sits between Uttara Āṣāḍhā and Śravaṇa.
The Grahas
The word graha comes from the Sanskrit root grah — to seize or grasp. They are the celestial bodies that move along the ecliptic: Sūrya (Sun), Candra (Moon), Maṅgala (Mars), Budha (Mercury), Bṛhaspati (Jupiter), Śukra (Venus), Śani (Saturn), and the lunar nodes Rāhu and Ketu. The Sun plays a central role even in this geocentric model, and its position is used to determine the true positions of the grahas.
In modern cosmology, the Sun is a star and the Moon is a natural satellite — neither qualifies as a planet. In the Vedic paradigm, both are grahas. Uranus and Neptune are not mentioned in this work. They are not visible to the naked eye. Bodies that cannot be seen exert no influence in the Vedic framework.
The word planet comes from the Greek planetes — wanderer. The Greeks named these bodies by their motion against the fixed stars. The Vedic tradition named them by their influence on earthly life, both temporal and metaphysical. Same objects, two entirely different frameworks for what matters about them.
Rāhu and Ketu
Rāhu and Ketu are the two points where the Moon's orbital path intersects the ecliptic, 180° apart. They are involved in both lunar and solar eclipses, though they themselves are never visible — the eclipse itself is their form on this plane of existence. Their presence in eclipses gives them real influence in people's lives, which is why they are classified as grahas.
Orbital Reference Points
The Surya Siddhanta tracks four kinds of reference points for a graha: its bhagaṇa (revolution rate), its mandocca (apogee), its śīghroca (node of conjunction), and its pāta (node of intersection). Not every graha has all four. The Sun has no śīghroca, since it is itself the reference point the śīghra correction is built around. It has no pāta either, since it defines the ecliptic itself, leaving no separate path for it to cross. The Moon also has no śīghroca, since its motion is purely geocentric rather than an artifact of Earth's own motion around the Sun. The five remaining grahas — Mercury, Venus, Mars, Jupiter, and Saturn — carry all four. Together, these reference points are what allow a graha's true position, in longitude and, where pāta applies, in latitude, to be calculated. Each is examined in its own section below.
Bhagaṇa
Bhagaṇa is the number of complete revolutions a graha makes along the ecliptic in one Mahāyuga. The bhagaṇa allows us to find the mean longitude, a foundational value that every other calculation is built on.
Revolution Table
| Graha | Bhagaṇa per Mahāyuga | Civil Days per Revolution (WWR) | Daily Motion | Period (Years) |
|---|---|---|---|---|
| Sūrya (Sun) | 4,320,0001 | 365.25876 | 0.98560° | 1.00000 |
| Candra (Moon) | 57,753,3362 | 27.32167 | 13.17635° | 0.07480 |
| Budha (Mercury) | 4,320,0001 | 365.25876 | 0.98560° | 1.00000 |
| Śukra (Venus) | 4,320,0001 | 365.25876 | 0.98560° | 1.00000 |
| Maṅgala (Mars) | 2,296,8322 | 686.99749 | 0.52402° | 1.88085 |
| Bṛhaspati (Jupiter) | 364,2203 | 4,332.32065 | 0.08310° | 11.86096 |
| Śani (Saturn) | 146,5684 | 10,765.77307 | 0.03344° | 29.47437 |
| Rāhu / Ketu | −232,2385 | 6,794.39983 | −0.05298° | 18.60161 |
| Zodiac | 1,582,237,8286 | 0.99727 | 360.98560° | 0.00273 |
1 SS 1.29 2 SS 1.30 3 SS 1.31 4 SS 1.32 5 SS 1.33 6 SS 1.34
The Civil Days per Revolution and Daily Motion columns above are derived as follows, using the Sun's row as an example:
Civil Days per Revolution = Civil Days per Caturyuga ÷ Bhagaṇa Revolutions
1,577,917,828 (SS 1.37) ÷ 4,320,000 = 365.25876 (Sun)
Daily Motion = 360° ÷ Civil Days per Revolution
360 ÷ 365.25876 = 0.98560° (Sun)
Mandocca - Node of Apsis
The graha's real path isn't a perfect circle. It's closer to an ellipse, so it moves faster at one point in its orbit and slower at the opposite point. Mandocca is that slowest point, and it's what the manda correction is built around to determine the graha's true position.
Apogee and perigee are the official geocentric terms for an orbit's two apsides: apogee is the farthest point from Earth, perigee the closest. Mandocca is the graha's apogee. Its perigee, diametrically opposite, is called nīca. In a heliocentric view, the same two points are called perihelion and aphelion.
Manda Rates
| Graha | Revolutions per Kalpa | Revolutions per Caturyuga | Daily Motion (rev/day) |
|---|---|---|---|
| Sūrya (Sun) | 3871 | 0.387 | 0.387 / 1,577,917,828 |
| Candra (Moon) | — | 488,2032 | 0.11139°/day |
| Budha (Mercury) | 3681 | 0.368 | 0.368 / 1,577,917,828 |
| Śukra (Venus) | 5351 | 0.535 | 0.535 / 1,577,917,828 |
| Maṅgala (Mars) | 2041 | 0.204 | 0.204 / 1,577,917,828 |
| Bṛhaspati (Jupiter) | 9001 | 0.900 | 0.900 / 1,577,917,828 |
| Śani (Saturn) | 391 | 0.039 | 0.039 / 1,577,917,828 |
1 SS 1.41–42 2 SS 1.33
Śīghroca - Node of Conjunction
If one observes the behavior of the planets in relation to the Sun, they will show odd behavior at various times. Mercury and Venus sometimes appear in the morning sky and sometimes in the evening sky, like a pendulum anchored to the Sun. Mars, Jupiter, and Saturn, on the other hand, slow down at certain intervals or even reverse course.
The mean motion of these grahas does not account for their shifts in behavior. For that reason, a śīghra correction is needed when calculating the graha's true position. Śīghrocca is the longitudinal position of the Sun reflected on a graha's orbit, and it's the reference point this correction is measured against.
Śīghra Rates
| Graha | Śīghroca per Mahāyuga | Civil Days per Revolution (WWR) | Daily Motion | Period (Years) |
|---|---|---|---|---|
| Budha (Mercury) | 17,937,0601 | 87.96970 | 4.09232° | 0.24084 |
| Śukra (Venus) | 7,022,3762 | 224.69854 | 1.60215° | 0.61518 |
| Maṅgala (Mars) | 4,320,0003 | 365.25876 | 0.98560° | 1.00000 |
| Bṛhaspati (Jupiter) | 4,320,0003 | 365.25876 | 0.98560° | 1.00000 |
| Śani (Saturn) | 4,320,0003 | 365.25876 | 0.98560° | 1.00000 |
1 SS 1.31 2 SS 1.32 3 SS 1.29
Epicycle
The Surya Siddhanta models all planetary motion using uniform circular motion: perfect circles moving at constant speed. Since the graha's real motion isn't perfectly circular or constant, the Surya Siddhanta builds the appearance of irregularity by combining circles. The center of a smaller circle, called the epicycle, travels along the graha's mean orbit, and the graha rides the rim of that epicycle. As the graha's position shifts around the epicycle's rim, it gets pulled ahead of or behind its mean position.
Manda Epicycle
The manda epicycle accounts for the graha's true elliptical orbit. The graha's offset from the epicycle's center always points toward mandocca. So the graha is farthest from Earth and slowest exactly when the epicycle's center passes mandocca's direction. It's closest and fastest exactly when the center passes the opposite point.
Śīghra Epicycle
The śīghra epicycle accounts for the effect of Earth's own motion around the Sun. Its offset from the epicycle's center always points toward śīghroca, the Sun's own longitude, reflected onto the graha's orbit.
Mean: 0° Mandocca: 50° Śīghroca: 200°
Pāta - Node of Intersection
Pāta is the point where a graha's orbit crosses the ecliptic. It is used in the calculation of the latitude (vikṣepa).
Rāhu, Ketu, and the Moon
Rāhu and Ketu are special grahas in that they are also the pāta of the moon. Every orbit crosses the ecliptic at two points, but only one is tracked for other planets, since it's the only one relevant. The moon, in contrast, has both tracked — as Rāhu and Ketu. When the moon crosses a node at the same time the sun and moon are aligned, an eclipse occurs — solar or lunar depending on the alignment.
- Conjunction — Conjunction is when the Sun and Moon share the same longitude, which is what marks a new moon. At this point, the Moon sits directly between Earth and Sun. When the Moon also happens to be conjunct with Rāhu or Ketu at the same time, its shadow falls on Earth, and that's what gives us a solar eclipse.
- Opposition — Opposition is when the Sun and Moon are 180° apart, which is what marks a full moon. At this point, Earth sits directly between the Sun and Moon. When the Moon also happens to be conjunct with Rāhu or Ketu at the same time, Earth's shadow falls on it, and that's what gives us a lunar eclipse.
Pāta Rates
| Graha | Revolutions per Kalpa | Revolutions per Caturyuga | Daily Motion (rev/day) |
|---|---|---|---|
| Candra (Moon) | — | 232,2382 | 0.05298°/day |
| Budha (Mercury) | 4881 | 0.488 | 0.488 / 1,577,917,828 |
| Śukra (Venus) | 9031 | 0.903 | 0.903 / 1,577,917,828 |
| Maṅgala (Mars) | 2141 | 0.214 | 0.214 / 1,577,917,828 |
| Bṛhaspati (Jupiter) | 1741 | 0.174 | 0.174 / 1,577,917,828 |
| Śani (Saturn) | 6621 | 0.662 | 0.662 / 1,577,917,828 |
1 SS 1.43–44 2 SS 1.33