Lenticular galaxy changing into a less defined elliptical galaxy
Space news (The evolution of galaxies: transition periods; lenticular galaxies) – 140 million light-years away toward the constellation Virgo –
The Hubble Space Telescope image of lenticular galaxy NGC 5010 seen here shows an older spiral galaxy in transition to an elliptical type. Lenticular type galaxies are considered a transition phase between spiral and elliptical galaxies. Presently, it has characteristics astronomers find in both spiral and elliptical galaxies, but will eventually evolve into a less defined elliptical galaxy.
All of the blue, fast-living stars that existed in spiral galaxy NGC 5010 have aged into older red stars as it transitioned into a lenticular galaxy. The vast majority of stars seen in this image are red and elderly, with only a few younger, blue stars sprinkled like fairy dust across dark, dusty, remnants of spiral arms. It has also started to develop a bigger bulge in its disk as it starts to take on a more rounded shape characteristic of lenticular and sometimes elliptical galaxies.
The orientation of the galaxy’s sideways to the telescope in this image. View elliptical galaxy NGC 5010 far in the future from the same reference point and older, red stars will exist within it. It could have a circular, long, narrow or even cigar shape since all are characteristic of elliptical galaxies. No matter its shape, this elliptical galaxy will contain even less gas and dust than it did when it was younger and brighter.
Lens-shaped galaxies have characteristics astronomers see in elliptical and spiral galaxies
Space news (lenticular galaxies) – 50 million light-years from Earth, in the constellation of Canes Venatici (The Hunting Dogs) –
This Hubble Space Telescope image of lenticular galaxy NGC 4111 shows an island universe with a more chaotic past than first thought. Lenticular or lens-shaped galaxies are labelled S0 on the Hubble Tuning Fork and are classified as a transitional type between spiral and elliptical galaxies.
Lenticular galaxies host older stars as observed in elliptical galaxies and include a disc as seenin spiral galaxies. However, they have a bulge and thin disc, which hasn’t been observed in elliptical galaxies. They also don’t have arms and the gas and dust detected in spiral galaxies.
NGC 4111 appears as a thin sliver of lights in this image because Hubble’s viewing the edge of the galaxy. At first glance, this island universe looks relatively quiet, but there are regions suggesting a more chaotic past. Pillars of dark filaments silhouetted against the bright core of the galaxy and running through the centre at right angles to the thin disc. Dark filaments of dust and gas astronomers associate with a ring of materialorbiting its core.
This ring of orbiting material isn’t aligned with the main disc of NGC 4111, which has astrophysicists thinking it could be the remains of a smaller galaxy it collided with long ago. Considering the possible mass and volume of this past meal, indigestion probably isn’t unexpected.
Astronomy News – The galaxies you’ll view during your “Journey to the Beginning of Space and Time” are like grains of sand on the beach, or snowflakes, with no two galaxies looking exactly the same to viewers. Astronomers have also viewed a number of different types of galaxies and they have given each a specific name, usually based on the overall shape of the galaxy. Composed of millions or even billions of individual stars, each particular type of galaxy viewed, so far, has also been given a designation, or name, by which we all can tell the difference between the individual galaxies in the infinity of galaxies we view in the night sky above us. It was Edwin Hubble who first did the work with photographic plates taken during the early part of the twentieth century that allowed him to determine the nebulous objects astronomers had been viewing for years were actually vast islands of stars we call galaxies. Edwin Hubble also cataloged the galaxies he viewed into three major classes, or types, according to their physical shape.
A percentage of the galaxies will resemble huge pinwheels and have been given the name spiral galaxies by astronomers viewing these objects. Spiral galaxies are generally composed of a bright central nucleus with older stars, with two sweeping arms of younger stars, open clusters, and diffuse nebulae unfolding in space and time. The Milky Way in which we reside is one such spiral galaxy among the multitudes of such galaxies in the universe and Sol is located about two-thirds of the way from the center of the galaxy.
Astronomers have broken down spiral galaxies into five subclasses of spiral galaxies, according to how tightly the arms of a galaxy are wrapped around the nucleus of the spiral galaxy in question. Spiral galaxies with the tightest arms are Sa spiral galaxies, Sb spiral galaxies are next in order, with more loosely armed Sc, comparatively rare Sd, and S0 spiral galaxies almost appearing to be a transitional form between spiral galaxies and another type of galaxy.
Barred galaxies exhibit an odd, bar-like feature passing through the nucleus of the galaxy, and the spiral arms of barred galaxies start to unwind from the ends of the central bar, rather than from the nucleus of the galaxy. Barred galaxies are also classified according to the tightness of the spiral arms and have designations SBa, SBb, and SBc.
Elliptical galaxies are the most plentiful type of galaxy we have viewed during the human “Journey to the Beginning of Space and Time.” Elliptical galaxies actually have no hint of spiral arms and appear as huge, oval spheres with no discernible internal structure of any kind. Elliptical galaxies are classified according to how round they appear, with E0 elliptical galaxies appearing almost perfectly spherical, E4 elliptical galaxies looking like an oddly shaped football, and E7 elliptical galaxies looking flat as compared to the other classifications. Elliptical galaxies appear to be composed mostly of older stars and you’ll notice they lack luminosity as you view them.
Infinite is a human term
Galaxies that appear to have no distinctive shape are referred to as irregular galaxies and irregular galaxies have been viewed a lot less in the night sky than the other types. This doesn’t necessarily mean irregular galaxies appear in fewer numbers in the universe, but it does mean that the percentage of the universe we have viewed from Earth appears to contain fewer irregular galaxies than the other types.
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