page_title: NGC 4036
hierarchical_section_title: NGC 4036
caption_attribution_description: English: This week’s NASA/ESA Hubble Space Telescope image showcases the galaxy NGC 4036: a lenticular galaxy some 70 million light-years away in the constellation of Ursa Major (the Great Bear). This galaxy is known for its irregular lanes of dust, which form a swirling spiral pattern around the centre of the galaxy. This core is surrounded by an extended, hazy aura of gas and dust that stretches further out into space and causes the warm, fuzzy glow that can be seen here. The centre itself is also intriguing; it is something known as a LINER-type (Low-Ionisation Nuclear Emission-line Region) galactic nucleus, meaning that it displays particular emission lines within its spectrum. The particularly bright star visible slightly to the right of the galactic centre is not within the galaxy itself; it sits between us and NGC 4036, adding a burst of brightness to the scene. Due to its relative brightness, this galaxy can be seen using an amateur telescope, making it a favourite amongst backyard astronomers and astrophotography aficionados.
context_page_description: NGC 4036 is the New General Catalogue identifier for a lenticular galaxy in the northern circumpolar constellation of Ursa Major. In the Carnegie Atlas of Galaxies, it is described as being "characterized by an irregular
  pattern of dust lanes threaded through the disc in an 'embryonic' spiral pattern indicating a mixed S0/Sa form." It is located near the Big Dipper, a little to the north of the mid-way point between the stars Alpha Ursae Majoris and Delta Ursae Majoris. With a visual magnitude of 10.7, it can be dimly viewed using a 4 in aperture telescope.
  The visual dimensions of this galaxy are 2.703 × 1.027 arc minutes, with the major axis having a position angle of 85°. The galaxy is being viewed nearly edge-on, with an inclination of 18° to the line of sight from the Earth. It is moving away from us with a heliocentric radial velocity of 1,445 km/s. The estimated visual luminosity of the galaxy is 4.2×10¹⁰ L⊙, or 42 billion times the brightness of the Sun. Photographs show a tightly wound spiral pattern in the galactic disk, with three dust lanes—the southern side of the galaxy appears dimmer due to the dust configuration.
context_section_description: NGC 4036 is the New General Catalogue identifier for a lenticular galaxy  in the northern circumpolar constellation of Ursa Major. In the Carnegie Atlas of Galaxies, it is described as being "characterized by an irregular
  pattern of dust lanes threaded through the disc in an 'embryonic' spiral pattern indicating a mixed S0/Sa form." It is located near the Big Dipper, a little to the north of the mid-way point between the stars Alpha Ursae Majoris and Delta Ursae Majoris. With a visual magnitude of 10.7, it can be dimly viewed using a 4 in (10 cm) aperture telescope.
  The visual dimensions of this galaxy are 2.703 × 1.027 arc minutes, with the major axis having a position angle of 85°. The galaxy is being viewed nearly edge-on, with an inclination of 18° to the line of sight from the Earth. It is moving away from us with a heliocentric radial velocity of 1,445 km/s. The estimated visual luminosity of the galaxy is 4.2×10¹⁰ L⊙, or 42 billion times the brightness of the Sun. Photographs show a tightly wound spiral pattern in the galactic disk, with three dust lanes—the southern side of the galaxy appears dimmer due to the dust configuration. The mass of the free gas and dust in the galaxy is about 1.7×10⁹ M⊙ and 4.4×10⁵ M⊙, respectively, with around 7×10⁴ M⊙ of the gas being in an ionized state.
  This is a type of active galaxy known as a LINER, which means that it shows emission lines of ionized gas in the region of its nucleus. Chemically, the stars at the center of the nucleus have a higher metallicity than in the neighboring regions. It appears that there is a tilted disk of stars orbiting the nucleus within a radius of 820 ly (250 pc). The galactic bulge itself appears triaxial with the ionized gas concentrated near the center of this bulge region. Images of the galaxy with the Hubble Space Telescope show a wispy disk of dust on all sides of the nucleus, with what appears to be the tendrilous remains of an ionization cone leading away 4 arc seconds to the northeast. Such features are common in Seyfert galaxies.
  On July 23, 2007, Type Ia supernova SN 2007gi was discovered by Koichi Itagaki near the central bulge of this galaxy. It reached peak magnitude around August 14, then steadily declined in brightness thereafter. Materials identified in the spectrum included silicon, calcium, and sulfur moving outward at velocities of around 15,500 km/s. This is a 50% higher velocity than what is normally observed with supernovae of this type.
  NGC 4036 is a member of the LGG 266 galaxy group, along with NGC 4041, IC 758, UGC 7009, and UGC 7019. It is located just 17 arc minutes from NGC 4041, and the two form a pair with a projected separation of around 470 kly (143 kpc).
caption: Image of NGC 4036 taken by the Hubble Space Telescope
exif: {"Image ImageDescription": "This week\u2019s NASA/ESA Hubble Space Telescope image showcases the galaxy\u00a0NGC 4036: a lenticular galaxy some 70 million light-years away in the constellation of Ursa Major (the Great Bear). This galaxy is known for its irregular lanes of dust, which form a swirling spiral pattern around the centre of the galaxy. This core is surrounded by an extended, hazy aura of gas and dust that stretches further out into space and causes the warm, fuzzy glow that can be seen here. The centre itself is also intriguing; it is something known as a LINER-type (Low-Ionisation Nuclear Emission-line Region) galactic nucleus, meaning that it displays particular emission lines within its spectrum. The particularly bright star visible slightly to the right of the galactic centre is not within the galaxy itself; it sits between us and NGC 4036, adding a burst of brightness to the scene. Due to its relative brightness, this galaxy can be seen using an amateur telescope, making it a favourite amongst backyard astronomers and astrophotography aficionados.", "Image Software": "Adobe Photoshop CC (Windows)", "Image DateTime": "2018:02:14 15:30:19"}