Nebulosa planetaria

Bracci di spirale per una planetaria

Pubblicato 13/10/2016 | Da Barbara Bubbi

This planetary nebula is called PK 329-02.2 and is located in the constellation of Norma in the southern sky. It is also sometimes referred to as Menzel 2, or Mz 2, named after the astronomer Donald Menzel who discovered the nebula in 1922. When stars that are around the mass of the Sun reach their final stages of life, they shed their outer layers into space, which appear as glowing clouds of gas called planetary nebulae. The ejection of mass in stellar burnout is irregular and not symmetrical, so that planetary nebulae can have very complex shapes. In the case of Menzel 2 the nebula forms a winding blue cloud that perfectly aligns with two stars at its centre. In 1999 astronomers discovered that the star at the upper right is in fact the central star of the nebula, and the star to the lower left is probably a true physical companion of the central star. For tens of thousands of years the stellar core will be cocooned in spectacular clouds of gas and then, over a period of a few thousand years, the gas will fade away into the depths of the Universe. The curving structure of Menzel 2 resembles a last goodbye before the star reaches its final stage of retirement as a white dwarf. A version of this image was entered into the Hubble's Hidden Treasures image processing competition by contestant Serge Meunier.

I due bracci di spirale che si dispiegano dal centro di questa spettacolare immagine potrebbero far pensare ad una galassia. Ma questo oggetto è di natura diversa: PK 329-02.2 è una nebulosa planetaria all’interno della Via Lattea. Questo che osserviamo è l’ultimo respiro di una stella morente. Continua a leggere→

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Hubble – The Ghostbuster

Pubblicato 14/08/2016 | Da Barbara Bubbi

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Il telescopio spaziale Hubble ha ripreso un colorato fantasma cosmico, i resti incandescenti di una stella morente chiamata NGC 6369. Questa brillante apparizione è nota agli astrofili come Nebulosa Piccolo Fantasma (Little Ghost Nebula), perché appare come una piccola nube spettrale ed evanescente che circonda una debole stella centrale. Continua a leggere→

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Viaggio cosmico di una nebulosa a forma di farfalla

Pubblicato 29/07/2016 | Da Barbara Bubbi

The breathtaking butterfly-like planetary nebula NGC 6881 is visible here in an image taken by the NASA/ESA Hubble Space Telescope. Located in the constellation of Cygnus, it is formed of an inner nebula, estimated to be about one fifth of a light-year across, and symmetrical “wings” that spread out about one light-year from one tip to the other. The symmetry could be due to a binary star at the nebula’s centre. NGC 6881 has a dying star at its core which is about 60% of the mass of the Sun. It is an example of a quadrupolar planetary nebula, made from two pairs of bipolar lobes pointing in different directions, and consisting of four pairs of flat rings. There are also three rings in the centre. A planetary nebula is a cloud of ionised gas, emitting light of various colours. It typically forms when a dying star — a red giant — throws off its outer layers, because of pulsations and strong stellar winds. The star’s exposed hot, luminous core starts emitting ultraviolet radiation, exciting the outer layers of the star, which then become a newly born planetary nebula. At some point, the nebula is bound to dissolve in space, leaving the central star as a white dwarf — the final evolutionary state of stars. The name “planetary” dates back to the 18th century, when such nebulae were first discovered — and when viewed through small optical telescopes, they looked a lot like giant planets. Planetary nebulae usually live for a few tens of thousands of years, a short phase in the lifetime of a star. The image was taken through three filters which isolate the specific wavelength of light emitted by nitrogen (shown in red), hydrogen (shown in green) and oxygen (shown in blue).

Il telescopio Hubble ha immortalato un’affascinante nebulosa planetaria, simile ad una delicata farfalla, denominata NGC 6881.

Situata nella costellazione del Cigno, è formata da una nube interna, che si estende per circa un quinto di anno luce, e da “ali” simmetriche che si espandono per circa un anno luce da un’estremità all’altra. La simmetria potrebbe essere dovuta ad una stella binaria nel centro della nebulosa. Continua a leggere→

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