Pictor-I-Zwerggalaxie
| Galaxie Pictor-I-Zwerggalaxie | |
|---|---|
| Pictor 1 | |
 | |
| AladinLite | |
| Sternbild | Maler |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 04h 43m 47,4s |
| Deklination | -50° 16′ 58,8″ |
| Erscheinungsbild | |
| Morphologischer Typ | dSph |
| Helligkeit (visuell) | (17,2 ± 0,2) mag |
| Physikalische Daten | |
| Zugehörigkeit | Lokale Gruppe |
| Entfernung | 372.000 Lj / 114.000 pc |
| Absolute Helligkeit | (−3,1 ± 0,2) mag |
| Geschichte | |
| Entdeckung | Dark Energy Survey |
| Entdeckungsdatum | 2015 |
| Katalogbezeichnungen | |
| Pic I dSph | |
Die Pictor-I-Zwerggalaxie, kurz auch Pictor I oder Pictor 1, ist eine im Jahr 2015 entdeckte Zwerggalaxie des Typs dSph im Sternbild Maler in der Lokalen Gruppe und eine der Satellitengalaxien der Milchstraße.[1][2]
Die Entfernung zur Erde beträgt ca. 372.000 Lichtjahre.
Eigenschaften
Pic I dSph besitzt einen Halblichtradius von ′, was bei einer Entfernung von etwa 114 kpc einer Größe von () pc entspricht.
Weiteres
- Liste der Galaxien der Lokalen Gruppe
Weblinks
Einzelnachweise
- ↑ Sergey E. Koposov, Vasily Belokurov, Gabriel Torrealba, N. Wyn Evans: Beasts of the Southern Wild. Discovery of a large number of Ultra Faint satellites in the vicinity of the Magellanic Clouds. In: The Astrophysical Journal. 805, 10. März 2015, S. 130. doi:10.1088/0004-637X/805/2/130.
- ↑ DES Collaboration: Eight New Milky Way Companions Discovered in First-Year Dark Energy Survey Data. In: The Astrophysical Journal. 807, 10. März 2015, S. 50. doi:10.1088/0004-637X/807/1/50.
Antlia 2 | Aquarius-II | Bootes-I | Bootes-II | Bootes-III | Canes-Venatici-I | Canes-Venatici-II | Canis-Major-Zwerg | Carina-Zwerg | Cetus-II | Crater-II | Columba-I | Coma-Berenices-Zwerg | Draco-Zwerg | Draco-II | Eridanus-II | Eridanus-III | Fornax-Zwerg | Grus-I | Grus-II | Hercules-Zwerg | Horologium-I | Horologium-II | Hydra-II | Hydrus-I | Indus-II | Leo-I | Leo-II | Leo-IV | Leo T Leo V | Große Magellansche Wolke | Kleine Magellansche Wolke | Pegasus-III | Phoenix-Zwerg | Phoenix-II | Pictor-I | Pisces-I | Pisces-II | Reticulum-II | Reticulum-III | Sagittarius-Zwerg | Sagittarius-II | Segue 1 | Segue 2 | Sculptor-Zwerg | Sextans-Zwerg | Triangulum II | Tucana-II | Tucana-III | Tucana-IV | Tucana-V | Ursa Major-I | Ursa Major-II | Ursa-Minor-Zwerg | Willman 1
Auf dieser Seite verwendete Medien
Caption from NASA: Like early explorers mapping the continents of our globe, astronomers are busy charting the spiral structure of our galaxy, the Milky Way. Using infrared images from NASA's Spitzer Space Telescope, scientists have discovered that the Milky Way's elegant spiral structure is dominated by just two arms wrapping off the ends of a central bar of stars. Previously, our galaxy was thought to possess four major arms.
This artist's concept illustrates the new view of the Milky Way, along with other findings presented at the 212th American Astronomical Society meeting in St. Louis, Mo. The galaxy's two major arms (Scutum-Centaurus and Perseus) can be seen attached to the ends of a thick central bar, while the two now-demoted minor arms (Norma and Sagittarius) are less distinct and located between the major arms. The major arms consist of the highest densities of both young and old stars; the minor arms are primarily filled with gas and pockets of star-forming activity.
The artist's concept also includes a new spiral arm, called the "Far-3 kiloparsec arm," discovered via a radio-telescope survey of gas in the Milky Way. This arm is shorter than the two major arms and lies along the bar of the galaxy.
Our sun lies near a small, partial arm called the Orion Arm, or Orion Spur, located between the Sagittarius and Perseus arms.