Exploring the Dimmest Stars: A Look into Faint and Brown Dwarfs Visible to the Naked Eye
The sun is the brightest and most luminous thing on the planet. It also has the honor of being the closest star to the earth. Although it is a low status on the cosmic level. The Sun is brighter than 85% of the stars in the Milky Way. The phase which Sun is passing through at this time is called Main Sequence phase. Most of the stars in the universe are passing through this phase of their life. The Sun is increasing its brightness by 1% every 10 million years. With so many stars in the universe, it's not surprising that there are stars that are smaller, brighter, and fainter than the Sun. For example, BETELGEUSE, which is in the constellation Orion, is 14,000 times brighter than the Sun. and 61Cygni AB in the Cygnus constellation. It is the faintest star in the sky visible to the naked eye.
Magnitude scale is used to measure the brightness of stars. It also has two types
- Apparent magnitude
- Absolute magnitude
1. Apparent magnitude: It depends on how bright the star appears from Earth. This scale does not reflect the true brightness of the star. Distance and interstellar dust directly affect the brightness of celestial bodies.
2. Absolute Magnitude: This scale measures the brightness of a celestial body at a fixed distance (which is 10 parsecs). 10 parsecs consists of 5.32 light years.
When amateur astronomers look at the sky, they only focus on how bright one celestial body is compared to another. That is, they only consider the external intensity, and Professional astronomers are interested in the true brightness of a star. That is, which of the two objects at the same distance appears brighter. In their view, absolute intensity is more important.
In this article we are studying stars whose absolute magnitude is less than that of the Sun and which are visible to the naked eye. The stars whose absolute magnitude is less than that of the Sun are called faint stars. These stars are brown in color and much smaller than a normal star, so they are also called brown dwarfs. When they are at their hottest, they look reddish-orange. And in a relatively cool condition, they are seen in a magenta color. Brown dwarfs are also evidence that star formation does not always result in a conventional star. Since brown dwarfs are not very large (but much larger than a planet), their cores are not hot enough to trigger nuclear fusion. Therefore, they are very difficult to detect even with the most sensitive telescopes. They are detected in infrared wavelengths. But distinguishing them from other low-mass stars is still a difficult step.
The honor of the first discovered brown dwarf goes to Glaze 229b. It was discovered in 1994 and its location in the constellation Lepus was confirmed in 1995. Luhman 16A is the closest faint star to Earth (5.6 light-years away) of the Luhman 16 system in the constellation Vela. The faintest known brown dwarf, 2mass jo9393548, is the 5th closest faint star, 17 light-years from Earth. This star in the constellation Antlia is a million times dimmer than our Sun.
The Milky Way is a billion times fainter than the Sun in the visible spectrum, along with another brown dwarf. We can see 9000 stars with an apparent magnitude of 0.6 with the naked eye. The absolute magnitude of our Sun is 83.4, which means that after 10 parsecs, we will be able to see the Sun shining with an apparent magnitude of 83.4. Interestingly, out of these 9000 stars, only 42 stars have an absolute magnitude less than the Sun. And a star that is dimmer than the Sun must be very bright or very close to be visible with or without binoculars. And there are quite a few stars within 10 prisms of Earth. Only 5% of the 9000 stars are within this distance. Because, The remaining 95% of stars are far from this limit and are still visible, so it is obvious that they are brighter than the Sun.
The 10 faintest stars in the night sky are those less bright than the Sun in absolute magnitude and brighter than 5.6 in apparent magnitude and can be seen with the naked eye:
Name: 61 Cygni AB
Constellation: Cygnus
Coordinates: (21h 06m 55s) + (+38° 44′ 41″)
(RA/Dec): App: 4.8
Magnitude: Abs: 8.3
Name: Epsilon Indi
Constellation: Indus
Coordinates: (22h 03m 22s) + (-56° 47′ 10″)
(RA/Dec): App: 4.8
Magnitude: Abs: 6.9
Name: Tau Ceti
Constellation: Seats
Coordinates: (01h 44m 04s) + (-15° 56′ 15″)
(RA/Dec): App: 3.5
Magnitude: Abs: 5.7
Significance: Tau Ceti is a star in the constellation Cetus, about 11.9 light years away from Earth. It's similar in mass and size to the Sun, but much older and less active. It's also known to have at least four exoplanets orbiting it.The brightest of the dim stars, resembling the Sun in its spectrum and is less luminous than the Sun in absolute magnitude.
Number: 5
Name: 85 Pegasi
Constellation: Pegasus
Coordinates: (00h 02m 10s) + (+27° 04′ 56″)
(RA/Dec): App: 6.4
Magnitude: Abs: 5.3
Name: Sigma Draconis
Constellation: Draco
Coordinates: (19h 32m 22s) + (+69° 39′ 40”)
(RA/Dec): App: 4.7
Magnitude: Abs: 5.9
Name: 70 Ophiuchus
Constellation: Ophiuchus
Coordinates: (18h 05m 27s) + (+02° 29′ 00”)
(RA/Dec): App: 6.1
Magnitude: Abs: 5.5
Name: Mu Cassiopeiae
Constellation: Cassiopeia
Coordinates: (01h 08m 16s) + (+54° 55′ 13”)
(RA/Dec): App: 5.2
Magnitude: Abs: 5.8
Name: 61 Ursae Majoris
Constellation: Ursa Major
Coordinates: (11h 41m 03s) + (+34° 12′ 06”)
(RA/Dec): App: 5.4
Magnitude: Abs: 5.5
Name: 54 Piscium
Constellation: Pisces
Coordinates: (00h 39m 22s) + (+21° 15′ 02”)
(RA/Dec): App: 5.9
Magnitude: Abs: 5.7
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