Galactic features of spiral galaxy NGC 3430
NGC 3430 is a spiral galaxy without an open, distinct arm centre bar. It has since been classified as a SAc galaxy. Edwin Hubble used it to characterise a variety of galaxy types, such as spiral, elliptical, lenticular, barred, and irregular ones. Numerous additional galaxies are in close proximity to NGC 3430. In NGC 3430, one is close enough to provide enough gravitational pull to start star formation. It is found in the constellation Leo Minor, which is 100 million light-years away from Earth.
It is possible to see spots that are clearly visible as bright-blue colours outside of the galaxy’s main spiral structure. NGC 3430 is a galactic spiral that has the appearance of radiating outward from a pinwheel-shaped configuration of arms. Dark dust lanes and brilliant star-forming zones characterise these spiral regions.
Studies conducted in the late nineties reveal indications of tidal interactions with NGC 3430, a nearby galaxy, which may have an impact on the structure of the galaxy.
What is the Hubble telescope? What does it do?
In 1990, NASA and the European Space Agency (ESA) launched the Hubble Space Telescope (HST), a space-based observatory. It travels at a height of roughly 547 kilometres (340 miles) around the Earth. Hubble is able to take detailed pictures and analyse light from astronomical objects because it is outfitted with sophisticated cameras and spectrographs. Observing far-off galaxies, exploring deep space, researching exoplanets, comprehending cosmic events, and calculating the universe’s expansion are some of its major accomplishments. The public’s interest in astronomy has been piqued and scientific knowledge has been greatly enhanced by Hubble’s discoveries.
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