NGC 3285B Galaxy: Largest Constellation View
- okay, here's a breakdown of the facts from the provided text, summarizing the key points about NGC 3285B and the supernova SN 2023xqm:
- * Location: NGC 3285B is a galaxy located on the edge of the Hydra I galaxy cluster, a massive collection of hundreds to thousands of galaxies bound...
- * Discovery: In 2023, the Hubble Space telescope detected a type Ia supernova within NGC 3285B, named SN 2023xqm.
okay, here’s a breakdown of the facts from the provided text, summarizing the key points about NGC 3285B and the supernova SN 2023xqm:
NGC 3285B: A Galaxy in the Hydra I Cluster
* Location: NGC 3285B is a galaxy located on the edge of the Hydra I galaxy cluster, a massive collection of hundreds to thousands of galaxies bound by gravity. This cluster is one of the largest in the local universe.
* Cluster Structure: The Hydra I cluster is dominated by two large elliptical galaxies at its center, which are 50% larger then the Milky Way (about 150,000 light-years in diameter).
* Not Centrally Located: NGC 3285B is relatively far from these central galaxies within the cluster.
Supernova SN 2023xqm
* Discovery: In 2023, the Hubble Space telescope detected a type Ia supernova within NGC 3285B, named SN 2023xqm.
* Type Ia Supernova: This type of supernova occurs when a white dwarf star accumulates material from a companion star, leading to a violent explosion.
* Brightness: SN 2023xqm released an enormous amount of energy, becoming 5 billion times brighter than the sun.
* Appearance: In the Hubble image,the supernova appears as a blue dot on the left edge of the galaxy.
Hubble’s Research
* Study of 100 Supernovae: The observations of NGC 3285B are part of a larger Hubble study of 100 Type Ia supernovae.
* Goal: The research aims to understand the distance and structure of the dust and gas created by these supernovae.
* Wavelengths: The study uses observations across ultraviolet, visible, and near-infrared wavelengths.
* Reddening Effect: Supernovae appear redder than they actually are due to the effects of dust and gas.This study will help refine distance measurements in the universe by accounting for this effect.
Source: The information comes from the NARIT National Astronomical Research Institute (via a facebook post).
