Barkas:Potw1749a Pallas crop.png

Konten halaman tidak didukung dalam bahasa lain.
Saka Wikipédia Jawa, bauwarna mardika basa Jawa

Potw1749a_Pallas_crop.png(314 × 316 piksel, ukuran barkas: 37 KB, jinis MIME: image/png)

Barkas iki saka Wikimedia Commons lan kena kanggo proyèk liya. Panyandraning kaca panyandra barkasé kapacak ing ngisor.

Ringkesan

Panyandra
English: VLT's SPHERE spies rocky worlds

From the description at File:Potw1749a.tif:

These images were taken by ESO's SPHERE (Spectro-Polarimetric High-Contrast Exoplanet Research) instrument, installed on the Very Large Telescope at the Paranal Observatory, Chile. These strikingly-detailed views reveal four of the millions of rocky bodies in the main asteroid belt, a ring of asteroids between Mars and Jupiter that separates the rocky inner planets of the Solar System from the gaseous and icy outer planets.

Clockwise from top left, the asteroids shown here are 29 Amphitrite, 324 Bamberga, 2 Pallas, and 89 Julia. Named after the Greek goddess Pallas Athena, 2 Pallas is about 510 kilometres wide. This makes it the third largest asteroid in the main belt and one of the biggest asteroids in the entire Solar System. It contains about 7% of the mass of the entire asteroid belt — so hefty that it was once classified as a planet. A third of the size of 2 Pallas, 89 Julia is thought to be named after St Julia of Corsica. Its stony composition led to its classification as an S-type asteroid. Another S-type asteroid is 29 Amphitrite, which was only discovered in 1854. 324 Bamberga, one of the largest C-type asteroid in the asteroid belt, was discovered even later: Johann Palisa found it in 1892. Today, it is understood that C-type asteroids may actually be bodies from the outer Solar System following the migration of the giant planets. As such, they may contain ice in their interior.

Although the asteroid belt is often portrayed in science fiction as a place of violent collisions, packed full of large rocks too dangerous for even the most skilled of space pilots to navigate, it is actually very sparse. In total, the asteroid belt contains just 4% of the mass of the Moon, with about half of this mass contained in the four largest residents: Ceres, 4 Vesta, 2 Pallas, and 10 Hygiea.
Tanggal 4 December 2017, 06:00 (release)
Sumber cropped from File:Potw1749a.tif, which was obtained from http://www.eso.org/public/images/potw1749a/
Juru pangarang Credit: ESO/Vernazza et al.

Lisènsi

This media was created by the European Southern Observatory (ESO).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts and captions, are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible."
To the uploader: You must provide a link (URL) to the original file and the authorship information if available.
w:id:Creative Commons
atribusi
Berkas ini dilisensikan di bawah lisensi Creative Commons Atribusi 4.0 Internasional.
Kowé kena:
  • ngedum – nyalin, nyebar, lan ngirim karya
  • nyampur – ngolah karya
Sangisoré kahanan mangkéné:
  • atribusi – Kowé kudu mènèhi krédhit kang patut, mènèhi pranala lisènsi, lan kandha yèn ana owah-owahan. Kowé bisa tumindak sasenengmu, nanging ora teges kang duwé lisènsi njurung lakumu.

Captions

Add a one-line explanation of what this file represents

Items portrayed in this file

gegambaran

status hak cipta Indonesia

berhak cipta Indonesia

lisensi Indonesia

CC BY 4.0 Indonesia

Sajarahing berkas

Klik ing tanggal/wektuné saprelu ndeleng rupané barkasé nalika tanggal iku.

Tanggal/WektuGambar cilikAlang ujurNaragunaTanggepan
saiki22 Maret 2019 00.03Gambar cilik kanggo owahan 22 Maret 2019 00.03314 × 316 (37 KB)KwamikagamiUser created page with UploadWizard

Kaca ing ngisor iki nganggo barkas iki:

Panggunané barkas sajagat

Wiki liya ngisor iki nganggo barkas iki:

Deleng naraguna liyané sadonya saka kaca iki.

Métadhatah