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What is a M type star?

An M-type star, or red dwarf, is a common, cool, low-mass star known for its reddish-orange color, faintness, and extremely long lifespan, burning hydrogen very slowly, making them the most numerous star type in the Milky Way, though usually hard to see individually. They have surface temperatures between 2,400 to 3,700 Kelvin and are identified by strong titanium oxide bands in their spectra.
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What are M-type stars?

Description: A star with spectral type "M". Astronomers identify M-type stars by the presence of molecular absorption bands, primarily from titanium oxide, in their spectra. They have typical (effective) temperatures between around 2500 kelvins (K) and 3700 K. Compared to other stars, they appear red to human eyes.
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What is a M-type asteroid?

M-type (metallic-type, aka M-class) asteroids are a spectral class of asteroids which appear to contain higher concentrations of metal phases (e.g. iron-nickel) than other asteroid classes, and are widely thought to be the source of iron meteorites.
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How long do M-type stars last?

We can divide these numbers: 0.3/0.04 = 7.5 , thus an M star lives 7.5 times as long as the Sun, or 75 billion years. We can think of M stars as like a "Smart Car", they are small, but get good gas mileage, while O stars are like Escalades--a large, gas-guzzling SUV. It is big, and burns a lot of fuel.
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Is an M star hotter than an O star?

Stars in the 'O' class are the most massive and hottest, stars in the 'M' class are the smallest and coolest. If you look closely at stars in the sky, you notice they are not all the same colour. Some appear redder, and some appear bluer. The colour of light a star gives off is controlled by its temperature.
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Timeline of an M type star

Is our Sun an M type star?

The Sun is a G-type main-sequence star that makes up about 99.86% of the mass of the Solar System. It has an absolute magnitude of +4.83, estimated to be brighter than about 85% of the stars in the Milky Way, most of which are red dwarfs.
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Can planets orbit an M-star?

The most common type of star in the universe is the M dwarf, making up ~70% of all stars. Because M dwarfs are so common, and because we know exoplanets are common, it is only natural that we have found many exoplanets orbiting M-dwarf stars.
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How old is the oldest star in space?

Oddly enough, the star which presently has the oldest age determination, the so-called Methuselah star, has an estimated age of 14.5 billion.
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What are the 7 types of stars?

The 7 main types of stars, classified by temperature and spectral class (hottest to coolest), are O, B, A, F, G, K, and M, often remembered by the mnemonic "Oh Be A Fine Girl/Guy, Kiss Me". These categories indicate temperature (O is hottest/blue, M is coolest/red) and are subdivided numerically (0-9), with other classes like white dwarfs, neutron stars, brown dwarfs, and supergiants existing outside this core sequence.
 
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What is the heaviest element a star can burn?

As described above, a massive star becomes like an onion with the heaviest element, iron, fused in the center, and concentric shells of lighter elements out to helium and hydrogen.
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What asteroid is supposed to hit Earth in 2027?

Based on new tracking measurements taken this week, the International Asteroid Warning Network (IAWN) has confirmed that asteroid 2017 PDC is on a course that will almost certainly impact Earth on July 21, 2027, less than nine years from now.
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Why shouldn't you pick up a meteorite?

You shouldn't pick up a fresh meteorite with bare hands primarily to protect the meteorite from contamination by skin oils and microbes, which can cause rust and dull its unique fusion crust, but also to preserve scientific data like its magnetic record. While generally safe for humans (not radioactive, just cold), handling with gloves or tongs preserves its pristine condition for study, and you should contact experts (museums, universities) rather than keeping it as a personal trinket.
 
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Are M-type asteroids rare?

The future of asteroid mining lies on Type-M asteroids: a rare and valuable type of asteroid that features high concentration of metallic and rare components.
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Why is Alpha Centauri special?

Alpha Centauri is special because it's the closest star system to our Sun, a triple-star system (A, B, and Proxima Centauri) with sun-like stars, making it our best nearby target for potential exoplanet discoveries, especially with Proxima Centauri hosting planets in or near its habitable zone, offering prime opportunities for studying other solar systems and future interstellar missions.
 
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What is the rarest type of star?

The rarest type of star, especially among main-sequence stars, are O-type stars, which are extremely hot, massive, luminous, and short-lived, making up only about 0.00003% of all stars, but other truly rare types include Wolf-Rayet stars, carbon stars, and exotic objects like Thorne-Zytkow objects or certain pulsar-white dwarfs, existing in very limited numbers or stages of stellar life. 
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Can M type stars have planets?

Planets within the HZ of M-dwarf stars (cooler and much less luminous than our sun) or closer to their host star are likely to be tidally locked2 and may have temperatures adequate for liquid water, at least on part of their surface, under a broad range of atmospheric conditions3.
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What is the most powerful star type?

Magnetars: All neutron stars have strong magnetic fields. But a magnetar's can be 10 trillion times stronger than a refrigerator magnet's and up to a thousand times stronger than a typical neutron star's.
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What is the lifespan of an M-star?

A typical Class M star has a mass of 0.20 (0.08 to 0.45) solar masses (M☉), a radius of 0.3 (≤0.7) solar radii, a luminosity of 0.01 (≤0.08) solar luminosities, a surface temperature of 3,000 K (2,400 K to 3,790 K), and a lifespan of 1 to 10 trillion years.
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What is an M-star in astronomy?

M stars are defined as yellow supergiants that exhibit apparent mode switching and are typically found at high galactic latitudes, potentially representing either normal massive supergiants located far from the galactic plane or older post-AGB stars.
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What star is only visible every 80 years?

This cycle, unique to T CrB, occurs roughly every 80 years. Recent observations show T CrB is mimicking the behavior seen before its last explosion in 1946, suggesting the nova could erupt as early as September 2024. Once it does, the star will shine brightly for about a week before fading.
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What is the oldest known thing in the universe?

With a redshift of z = 8.2, at the time of observation, the burst was the most distant known object of any kind with a spectroscopic redshift. GRB 090423 was also the oldest known object in the Universe, apart from the Methuselah star. The light from the burst took approximately 13 billion years to reach Earth.
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What's the biggest star in the universe?

The biggest known star in the universe by size is often cited as UY Scuti, a red hypergiant with a radius roughly 1,700 times that of our Sun, extending past Jupiter's orbit if placed in our solar system. However, astronomy is always advancing, and some newer data suggests Stephenson 2-18 (St2-18) might be even larger, potentially extending past Saturn's orbit, though its size is still debated and measured differently. For mass, R136a1 holds the record as the most massive star known.
 
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Does the Bible say God created the planets?

The Bible doesn't explicitly name or detail other planets but strongly implies God created a vast cosmos with "worlds" beyond Earth, focusing on His glory and humanity's relationship with Him, with some verses suggesting "other realms" and others focusing on Earth's unique role, leaving the existence of life on other planets an open question within its text, though some traditions interpret specific verses as pointing to multiple inhabited worlds. 
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Which planet is dark for 42 years?

The planet that experiences 42 years of darkness (and 42 years of light) is Uranus, due to its extreme axial tilt, causing one pole to face away from the Sun for decades while the other faces it continuously during its 84-year orbit.
 
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Why are there no stars in NASA photos?

Stars are absent in many NASA photos because the cameras are set to capture bright foreground subjects like Earth or the Moon, requiring fast shutter speeds and small apertures that are too quick and narrow to capture faint starlight, much like taking a picture of a bright streetlamp at night. The extreme brightness of the sunlit scene overpowers the dim stars, which need much longer exposures to show up, but longer exposures would completely overexpose the main subject, creating a "dynamic range" problem cameras can't handle in one shot. 
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