AstronomyHubble views a glistening red nebula Westerhout 5

Hubble views a glistening red nebula Westerhout 5

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Credit score: NASA’s Hubble House Telescope, ESA/Hubble, R. Sahai

Simply in time for the autumn foliage season, this picture from the NASA/ESA Hubble House Telescope encompasses a glistening scene in crimson. It reveals a small area of the nebula Westerhout 5, which lies about 7,000 light-years from Earth. Suffused with shiny crimson mild, this luminous picture hosts a wide range of attention-grabbing options, together with a free-floating Evaporating Gaseous Globule (frEGG).

The frEGG on this picture is the small tadpole-shaped darkish area within the higher center-left. This buoyant-looking bubble is lumbered with two names—[KAG2008] globule 13 and J025838.6+604259.

FrEGGs are a selected class of Evaporating Gaseous Globules (EGGs). Each frEGGs and EGGs are denser areas of fuel that photoevaporate much less simply than the much less dense fuel surrounding them. Photoevaporation happens when fuel is ionized and dispersed away by an intense supply of radiation—usually younger, scorching stars releasing huge quantities of ultraviolet (UV) mild. EGGs had been recognized pretty just lately, most notably on the suggestions of the enduring Pillars of Creation captured by Hubble in 1995.

FrEGGs had been labeled much more just lately and are distinguished from EGGs as a result of they’re indifferent and have a definite ‘head-tail’ form. FrEGGs and EGGs are of specific curiosity as a result of their density makes it harder for intense UV radiation, present in areas wealthy in young stars, to penetrate them. Their relative opacity implies that the fuel inside them is protected against ionization and photoevaporation. Astronomers suppose that is necessary for the formation of protostars, and that many FrEGGs and EGGs play host to the delivery of latest stars.

The frEGG on this picture is a darkish spot within the sea of crimson mild. The crimson coloration is a kind of sunshine emission generally known as H-alpha emission. H-alpha happens when a really energetic electron inside a hydrogen atom loses a set quantity of its power, releasing this distinctive crimson mild because it turns into much less energetic.

Supplied by
European House Company (ESA)

Quotation:
Hubble views a glistening crimson nebula Westerhout 5 (2023, October 2)
retrieved 2 October 2023
from https://phys.org/information/2023-10-hubble-views-glistening-red-nebula.html

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