NGC 4535

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NGC 4535
Mly (16.60 ± 0.54 Mpc)[3]
Group or clusterVirgo Cluster
Apparent magnitude (B)10.73[4]
Absolute magnitude (V)–21.42 ± 0.09[3]
Characteristics
TypeSAB(s)c[5]
Size117,000 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

  • NGC 4535 is located in the constellation of Virgo (The Virgin), around 50 million light-years from Earth.[8]
    NGC 4535 is located in the constellation of Virgo (The Virgin), around 50 million light-years from Earth.[8]
  • JWST NIRCam near-infrared image
    JWST NIRCam near-infrared image
  • JWST MIRI mid-infrared image
    JWST MIRI mid-infrared image

References

NGC 4535 imaged with a 24-inch telescope

External links