| 词条 | NGC 4217 |
| 释义 |
| name = | image = File:M106HunterWilson.jpg | caption = NGC 4217 (lower right) next to M106 (upper left) | epoch = | pronounce = | constellation name = Canes Venatici | ra = {{RA|12|15|50.900}} | dec = {{DEC|±47|05|30.44}} | z = | h_radial_v = | gal_v = | dist_ly = {{convert|60|Mly|Mpc|abbr=on|lk=on}} | group_cluster = | type = | mass = | mass_light_ratio = | size = | stars = | appmag_v = | appmag_b = | absmag_v = | size_v = 4.553 x 1.548 arcminutes | notes = | names = | references = }} NGC 4217 is an edge-on spiral galaxy which lies approximately 60 million light-years ( 18 million parsecs ) away in the constellation of Canes Venatici.[1] It is a possible companion galaxy to M106 (also known as NGC 4258). References1. ^{{cite web|title=NGC 4217 is an edge-on spiral galaxy which lies approximately 60 million light years away in the constellation of Canes Venatici.|url=https://www.pinterest.com/pin/501518108477227366/}} 2. ^{{cite web|title=Dust filaments of NGC 4217|url=http://www.spacetelescope.org/images/potw1503a/|website=www.spacetelescope.org|publisher=ESA/Hubble|accessdate=20 January 2015}} External links
1 : NGC objects |
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