Article snapshot taken from Wikipedia with creative commons attribution-sharealike license.
Give it a read and then ask your questions in the chat.
We can research this topic together.
Star in the constellation Fornax
You can help expand this article with text translated from the corresponding article in Spanish. (September 2023) Click for important translation instructions.
Machine translation, like DeepL or Google Translate, is a useful starting point for translations, but translators must revise errors as necessary and confirm that the translation is accurate, rather than simply copy-pasting machine-translated text into the English Misplaced Pages.
Consider adding a topic to this template: there are already 1,131 articles in the main category, and specifying|topic= will aid in categorization.
Do not translate text that appears unreliable or low-quality. If possible, verify the text with references provided in the foreign-language article.
You must provide copyright attribution in the edit summary accompanying your translation by providing an interlanguage link to the source of your translation. A model attribution edit summary is Content in this edit is translated from the existing Spanish Misplaced Pages article at ]; see its history for attribution.
You may also add the template {{Translated|es|Rho Fornacis}} to the talk page.
Rho Fornacis is a yellow-orange giant of spectral type G6III with an effective temperature of 4884 K.
It is similar, though somewhat hotter, than β Fornacis and π Fornacis, stars also in Fornax.
The diameter of Rho Fornacis is 9.9 times larger than the solar diameter but its mass is barely 1% greater than that of the Sun.
Its age is estimated at 5180 ± 3170 million years.
Rho Fornacis is a thick disk star, unlike most stars in our environment. Arcturus (α Boötis) and ε Fornacis, the latter in this same constellation, are examples of thick disk stars.
The eccentricity of its orbit around the Galactic Center (e = 0.56) is considerably greater than that of the Sun (e = 0.16), star of the thin disk.
Consequently, it shows a low metallicity—relative abundance of elements heavier than helium—, less than half that of the solar ( = -0 ,35).
Elements such as aluminum, calcium and sodium are equally deficient.
As in other similar stars, the oxygen/iron ratio is higher than in the Sun ( = 0.33).