是 的一個 星系。 维基共享资源 上的相關多媒體資源： NGC 1810 NED – SEDS – SIMBAD – VizieR –

Arp 273 is a pair of interacting galaxies, 300 million light years away in the constellation Andromeda. It was first described in the Atlas of Peculiar Galaxies, compiled by Halton Arp in 1966. [5] . The larger of the spiral galaxies, known as UGC 1810, is about five times more massive than the smaller galaxy. [6] .

2021年6月28日 · Historical Identification: Per Dreyer, NGC 1810 (= GC 1023 = JH 2746, Dunlop 235, 1860 RA 05 03 09, NPD 156 34.3) is "considerably faint, small, round, a little brighter middle, globular cluster following (to the east)".

View coin specifications and analysis for 1810 50C MS in our Capped Bust Lettered Edge Half Dollars category. With price & auction data.

2020年10月19日 · The featured galaxy is labelled UGC 1810 by itself, but together with its collisional partner is known as Arp 273. The overall shape of UGC 1810 — in particular its blue outer ring — is likely a result of wild and violent gravitational interactions.

NGC 1810 NGC 1810 is a open cluster located in the constellation of Dorado. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 1810: ... Right Ascension (RA) units = HH:MM:SS.SS Declination (Dec) units = DD:MM:SS.SS

Numismatic specification data and valuation estimates provided by Active Interest Media’s NumisMaster. Click on "Shop" to search for the coin on eBay. Scroll below to see all grades. When you click on links to various merchants on this site and make a purchase, this can result in this site earning a commission.

This 1810 large cent has been certified as VF-20 by NGC, one of the top two coin grading services. This coin has a population of only 45 coins! This coin has a mintage of 1,458,500. Population of 45 coins at this grade level with 60 graded higher. NGC encapsulation guarantees the coin’s VF-20 condition.

NGC 1810 je otvoreni skup u zviježđu Zlatnoj ribi.Izvori

UGC 1810 is the larger of the two spiral galaxies. It has an abnormal spiral structure that is tidally distorted by the gravitational tidal pull of the companion galaxy UGC 1813 south of it. The large, outer arm of UGC 1810 appears partially as a ring. This feature is seen when interacting galaxies actually pass through one another.