Here is a comment on the physics behind planetary diameters which are derived from the nebular hypothesis proposed by the rshis of long ago (and reproposed in the 18th century). The planets condensed from a solar nebula!
The planets are too far away to estimate diameters without powerful telescopes.Diameters can be estimated only by scaling rules based on physics.
“The Surya Siddhanta also estimates the diameters of the planets. The estimate for the diameter of Mercury is 3,008 miles, an error of less than 1% from the currently accepted diameter of 3,032 miles. It also estimates the diameter of Saturn as 73,882 miles, which again has an error of less than 1% from the currently accepted diameter of 74,580. Its estimate for the diameter of Mars is 3,772 miles, which has an error within 11% of the currently accepted diameter of 4,218 miles. It also estimated the diameter of Venus as 4,011 miles and Jupiter as 41,624 miles, which are roughly half the currently accepted values, 7,523 miles and 88,748 miles, respectively.” from the wiki at
https://en.wikipedia.org/wiki/Surya_Siddhanta
[The Surya Siddhanta is the name of a Sanskrit treatise in Indian astronomy from late … It calculates the earth’s diameter to be 8,000 miles (modern: 7,928 miles), diameter of moon as 2,400 miles (actual ~2,160) and the distance between moon …
How were the planetary sizes determined? What are the possible scaling rules? Let us define
D = Planetary diameter
R= Orbit radius
M = planetary mass ~ D^3
T = Orbit time = 2 Pi/ Omega
I = angular momentum = Integral of R^2 dm .Omega ~ R^2 D^3/ T
Possible relations: (This law of gravitation is most unlikely to be known so early in History)
If force is G M_sun M_planet /R^2 = Mplanet. Omega^2 R
R^3. Omega^2 = constant
R^3 ~T^2
Snow plow theory:
Larger radii sweep more particles leading to bigger planets
D^3 ~ 2Pi R no pf particles ~ 2Pi R n. volume ~ 2 pi R R. thickness
~ R^2 if thickness is fixed, n being number density
Or
D^3 ~ R^2
Thin disk:
In this case the planet grows to bigger than the thickness and
D^3 ~ R^3 or D ~ R
It appears that ancients assumed the last possibility. The planetary diameter scales with the orbital size.
It appears that ancients assumed the last possibility. The planetary diameter scales with the orbital size.
Body mile(D) “Relative Size `Relative size (modern)
Mercury 3008. 0.38
3.87E-01
Venus 4011.00
0.50 `7.20E-01
Earth 8.00E+03 1.00
1.00E+00
Mars “3.77E+03 “0.47 `1.52E+00
Jupiter 4.16E+04 5.20
5.19E+00
Saturn 7.39E+04 “9.24E+00 9.24 9.53E+00
( Ignore the`. I had to use it to line numbers up.) Relative size is from Surya Siddhanta and is compared to modern measurements of orbits compared to Earth’s orbit. Venus and Mars have the most disagreement . They are the rocky planets. The agreement is very good in general. Especially good for gas giants!
Conclusion: The vedas predicted planetary sizes using the acretion model from the initial solar nebula. So it automatically means they were the first to hit upon the idea of sun-centered planetary system!
This also means Indian Astronomy was developed by Indians with no input from the Greeks. No others have planetary diameters! The kalachakra was a giant astronomical clock and was used to calculate orbits of planets visible to the naked eye from which planet sizes were determined, a far cry from the flat earth theory of Christianity! See
https://www.quora.com/How-was-kalachakra-used-in-Indian-Asronomy
This uses four dials, one of which is the Zodiac, the same as the Greek one, most likely copied by the Greeks, an exact translation from Sanskrit! For fixed stars, the kalachakra uses bright stars with Sanskrit names. The Indians have been observing stars from long enough to know the period of nutation of Earth is 27,000 years. At least 5000 years of data is required.
Rg Veda is variously dated from 1500 BC to 8000 BC (from internal evidence on the order of time when River Saraswati was still flowing). (The internal reference also mentions a big earthquake that made River Saraswati stop flowing because of tectonic shifts.)
No luck was involved! Just thinking smart!
Let me add background information on astronomy of ancient India.
There were many before Aryabhata.
Box 3. Indian Astronomers before Aryabhata
“As mentioned in the Chandogya Upanishad (VII.1.2, 4), nakshatra-vidya (science of asterisms) was among the core disciplines of study in the Vedic era. Astronomers were called nakshtra-darsa (star-observers) or gal}aka. The sage Atri (who was among the originators of the oldest Vedic hymns) and his descendants were distinguished for expertise in accnrate edipse prediction and planetary astronomy. The Rg-Veda describes a solar eclipse observed by Atri (dated 3928 BCE in [5], p.1l6; [6], pp.173-l74). The Taittiriya Brahmana (Ill.lO.9) eulogises Ahina, Devabhaga and for attaining bliss due to their absorption in the science of the Sun, i.e., astronomy ([7], pp.20-2l); sage Matsya is also mentioned (1.5.2, 1) in the context of astronomy.
Garga is the most ancient astronomer referred to in post-Vedic treatises. The Mahahharata (XII.59.ll) refers to him as the court-astronomer of the great King Prthvi. TIte cpic (IX.37.14-17) mentions that a holy tirtha on the Sarasvati was named after the
as Garga-srota ("stream of Garga"). This was the sacred place where Vrddha Garga performed ascetic penance for self-purification and attained mastery over astonomy. Rishis of high merit and rigorous discipline l1sed to assemble here to acqllire thc profollnd knowledge of astronomy from the venerated Rshi.
Ancient Indian traditions mention a list of 18 astronomy texts called siddhiintm.; ("established theories") named after SfIrya, Pitamaha, Vyasa, Vasistha, Atri, Parasara, Kasyapa, Narada, Garga, Marici, Manu, Ailgira, Lomasa, Plllisa, Cyavana, Yavana,Brughu and Saunaka.
Varahamihira (505-587 CE), himself a prominent astronomer, also mentions Asita-Devala, Maya, Badarayalla and Nagllajit. Many of the treatises by the above astronomers got lost even by the time of Varahamihira; None are available in their original forms.
While considerable astronomical knowledge is embedded in early Vedic literatures, the oldest available treatise devoted exclusively to astronomy is the Vedanta Jyothisha (G. 1300 BCE vide [6]) composed by sage Lagadha. The Vedanga era represents a transitional pcriod in Indian civilisation when the Vedic culture was on the wane and there was a consequent attempt to organise and formulate the extant knowledge and systematise them into various branches called shastras .
Aryahhatlya (499 CE) is the earliest extant astronomy treatise after the Vedanga Jyotisha. It was composed during the "Classical Age" of post-Vedic India. Towards the beginning (Ganita 1) and the end (Gola 48-50) of his text, Aryabhata had made a general acknowledgement of his predecessors." from
https://www.ias.ac.in/describe/article/reso/011/05/0058-0072
by Amar Kumar Dutta.
More info on why I am doing this:
Surya Siddhanta is dated by wiki which says : Surya Siddhanta is a Hindu text on astronomy from late 4th-century or early 5th-century CE[1] Above is verse 1.1, which pays homage to Brahma.[2 Some scholars refer to Panca siddhantika as the old Surya Siddhanta and date it to 505 CE.[17] https://en.wikipedia.org/wiki/Surya_Siddhanta
It is pretty old and gives a list of planetary diameters.
Now we have to explain how the data was known for orbit radii and how planetary diameters were calculated. They didn’t have telescopes and such in those days.
Data must have been available for whatever method was used before Surya Siddhanta.
Now I show the data was available . ( Kak says “ My discovery that the Rgveda is an altar of mantras came rather suddenly. Although I had been studying the altars described in the Shatapatha Brahmana for several months, I had never thought of any connection of these with the Rgveda. It was while reading some unrelated matter the idea flashed that the Rgveda itself is a symbolic altar. “)
It is worth reading Subash Kak’s “The Astronomical Code of the Ṛgveda (Third Edition) “ for a fascinating insight into Hindu Civilization and Astronomical knowledge.
http://citeseerx.ist.psu.edu/viewdoc/download?doi=10.1.1.695.536&rep=rep1&type=pdf
My contribution is to show that only scaling offers a way to calculate planetary sizes and the simplest is the snow plow model of accretion where larger orbits gather more particles.