Ojú-ìwé

Àwọn ààyè-iṣẹ́

Jupiter's outermost large moon, one of the most heavily cratered objects known.

NASA, ESA, CSA, STScI; J. DePasquale, A. Koekemoer, A. Pagan (STScI) (CC BY 4.0)

The most cratered surface in the solar system: a face that has barely changed for billions of years.

Callisto’s dark, ancient surface is saturated with impact craters, showing little geological activity for billions of years.

It orbits outside Jupiter’s most intense radiation belts, which is why it has been suggested as a possible future base for human exploration of the Jupiter system.

Àwọn ìṣàmúlò-ètò ààyè-iṣẹ́

JPL SSD: Planetary Satellite Physical Parameters

Àwọn àṣẹ
Ìṣàmúlò-ètò	4,821 km	[1]
Àwọn Ìṣàmúlò-ètò	1.076 × 10²³ kg	[1]
Ìjánu-ìṣàmúlò-ètò	1.834 g/cm³	[1]
Ìṣàfihàn ààyè-iṣẹ́	1.24 m/s²	Tí a fì ṣẹ̀dà láti inú àtòjọ-ẹ̀yàn ààyè-iṣẹ́
Ìjánu-ìṣàmúlò-ètò	2.44 km/s	Tí a fì ṣẹ̀dà láti inú àtòjọ-ẹ̀yàn ààyè-iṣẹ́
Ìjánu-ìsún	16.7 ọj	[2]
Àwọn ààyè-iṣẹ́	16.7 ọj	[2]
Ìjánu-ìró láti Jupiter	1,882,700 km	[2]
Ìwọ̀n tí o bá jẹ́ kanna ní gbogbo àkókò Jupiter

Àwọn ìrànwọ́ àti àkọlé lòòlù àwọn módè́ì tí a fi pamọ́ fún ìmọ̀. Kò yẹ ki wọn lò fún ìṣàfihàn, ìṣàmúlò-ètò àti àwọn ìṣẹ̀dá iṣẹ́. Àwọn ìwé-ẹ̀rì ní ọ̀fẹ̀ àti àwọn ààyè-iṣẹ́ kò ní ìgbà gbà. Ka àwọn ìṣàmúlò-ètò ìròyìn