HD 268835 and Protoplanetary disk

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between HD 268835 and Protoplanetary disk

HD 268835 vs. Protoplanetary disk

HD 268835 (or R66) (30 SM) is one of two stars that were identified by NASA's Spitzer space telescope in the Milky Way's nearest neighbor galaxy, the Large Magellanic Cloud (the other being R 126 or HD 37974), as being circled by monstrous dust disks that are theorised to be the origin of planets. A protoplanetary disk is a rotating circumstellar disk of dense gas and dust surrounding a young newly formed star, a T Tauri star, or Herbig Ae/Be star.

Similarities between HD 268835 and Protoplanetary disk

HD 268835 and Protoplanetary disk have 2 things in common (in Unionpedia): Kuiper belt, Planet.

Kuiper belt

The Kuiper belt, occasionally called the Edgeworth–Kuiper belt, is a circumstellar disc in the outer Solar System, extending from the orbit of Neptune (at 30 AU) to approximately 50 AU from the Sun.

HD 268835 and Kuiper belt · Kuiper belt and Protoplanetary disk · See more »

Planet

A planet is an astronomical body orbiting a star or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its neighbouring region of planetesimals.

HD 268835 and Planet · Planet and Protoplanetary disk · See more »

The list above answers the following questions

What HD 268835 and Protoplanetary disk have in common
What are the similarities between HD 268835 and Protoplanetary disk

HD 268835 and Protoplanetary disk Comparison

HD 268835 has 15 relations, while Protoplanetary disk has 56. As they have in common 2, the Jaccard index is 2.82% = 2 / (15 + 56).

References

This article shows the relationship between HD 268835 and Protoplanetary disk. To access each article from which the information was extracted, please visit:

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