NGC 4535
Appearance
NGC 4535 | |
---|---|
Group or cluster | Virgo Cluster |
Apparent magnitude (B) | 10.73[4] |
Absolute magnitude (V) | –21.42 ± 0.09[3] |
Characteristics | |
Type | SAB(s)c[5] |
Size | 117,000 ly |
Apparent size (V) | 11′.8 × 11′.0[6] |
Other designations | |
CGCG 42-159, IRAS 12318+0828, MCG 1-32-104, PGC 41812, UGC 7727, VCC 1555 |
NGC 4535 is a
inclined by an angle of 43° to the line of sight from the Earth.[4] The morphological classification of NGC 4535 in the De Vaucouleurs system is SAB(s)c,[5] which indicates a bar structure across the core (SAB), no ring (s), and loosely wound spiral arms (c). The inner part of the galaxy has two spiral arms, which branch into multiple arms further away. The small[6] nucleus is of type HII, meaning the spectrum resembles that of an H II region.[5]
During 1999, the Hubble Space Telescope was used to observe Cepheid variable stars in NGC 4535. The period-luminosity relationship for these objects yielded a distance modulus of 31.02 ± 0.26 magnitude. This corresponded to a physical distance estimate of 52.2 ± 6.2 Mly (16.0 ± 1.9) Mpc, which was consistent with distance estimates for other members of the Virgo Cluster.[7]
Gallery
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NGC 4535 is located in the constellation of Virgo (The Virgin), around 50 million light-years from Earth.[8]
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JWST MIRI mid-infrared image
References
- ^ S2CID 18913331.
- S2CID 11672751.
- ^ S2CID 118666841. See Table 2.
- ^ S2CID 56003345.
- ^ S2CID 6040382.
- ^ ISBN 978-0521820486.
- S2CID 119352682.
- ^ "Colours of the Lost Galaxy". esahubble.org/. Retrieved 29 January 2021.
![](http://upload.wikimedia.org/wikipedia/commons/thumb/e/e9/N4535s.jpg/220px-N4535s.jpg)
External links
Media related to NGC 4535 at Wikimedia Commons
- NGC 4535 on