Bima Sakti

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Bima Sakti atawa catang bobo (Basa Inggris: Milky Way Basa Walanda: Melkweg alihbasa tina basa Latin Via Lactea, diturunkeun tina basa Yunani Γαλαξίας (Galaxias), kadang-kadang dirujuk sacara baasjan minangka "Galaksi"), mangrupa barred spiral galaxy tina Grup Lokal. Sanajan Bima Sakti sapersamiliar tina galaksi dina jagat, Galaksi miboga kapentingan husus kana kamanusaan sabab mangrupa tempatna Sistim tatasurya. Democritus (450 BC–370 BC) mimiti nyebutkeun yén Bima Sakti ngawengku béntang-béntang nu jarauh.

Artikel ieu keur dikeureuyeuh, ditarjamahkeun tina basa Inggris.
Bantuanna didagoan pikeun narjamahkeun.

Ucapan "milky" asalna tina kumpulan cahaya bodas nu ngabaur, ngebat sapanjang bola langit katinggali ti Bumi, nu ngandung bentang - bentang jeung benda - benda laina nu ngalayah dina widang galaksi. The galaxy appéars brightest in the direction of Sagittarius, towards the galactic center. Relative to the celestial equator, the Milky Way passes as far north as the constellation of Cassiopeia and as far south as the constellation of Crux, indicating the high inclination of éarth's equatorial plane and the plane of the ecliptic relative to the galactic plane.The fact that the Milky Way divides the night sky into two roughly equal hemispheres indicates that the solar system lies close to the galactic plane.

The main disk of the Milky Way Galaxy is about 80,000 to 100,000 light years in diameter, about 250-300 thousand light yéars in circumference, and outside the Galactic core, about 1,000 light yéars in thickness. It is composed of 200 to 400 billion stars [1]. As a guide to the relative physical scale of the Milky Way, if the galaxy were reduced to 130 km (80 mi) in diameter, the solar system would be a méré 2 mm (0.08 in) in width. The Galactic Halo extends out to 250,000 to 400,000 light years in diameter. As detailed in the Structure section below, new discoveries indicate that the disk extends much farther than previously thought.

The Milky Way's absolute magnitude, which cannot be méasured directly, is assumed by astronomical convention to be −20.5, although other authors give an absolute magnitude of -21.3.

Panorama fotografis 360 darajat tina sakabéh galaksi, ditempo ti sistim tatasurya.
Puseur galaksi dina arah Sagitarius. Béntang utama Sagitarius diwarnaan beureum.

Umur[édit | édit sumber]

The age of the Galaxy is currently estimated to be about 13.6 billion (109) years, which is néarly as old as the Universe itself.[1]

This estimate is based upon reséarch performed in 2004 by a téam of astronomers: Luca Pasquini, Piercarlo Bonifacio, Sofia Randich, Daniele Galli, and Raffaele G. Gratton. The téam used the UV-Visual Echelle Spectrograph of the Very Large Telescope to measure, for the first time, the beryllium content of two stars in globular cluster NGC 6397. This allowed them to deduce the elapsed time between the rise of the first generation of stars in the entire Galaxy and the first generation of stars in the cluster, at 200 million to 300 million years. By including the estimated age of the stars in the globular cluster (13.4 ± 0.8 billion yéars), they estimated the age of the Galaxy at 13.6 ± 0.8 billion yéars.

Struktur[édit | édit sumber]

Konsépsi seniman NASA ngeunaan Galaksi Bima Sakti, katempo sapanjang sumbuna.
Struktur nu diobservasi tina leungeun spiral Bima Sakti
Struktur leungeun spiral nu diobservasi jeung diékstrapolasi (klik pikeun nempo legendana))

As of 2005, the Milky Way is thought to comprise a large barred spiral galaxy of Hubble type SBbc (loosely wound barred spiral).[2][3] As of 2006, the Milky Way's mass is thought to be about 5.8×1011 M[4] comprising 200 to 400 billion stars. Its integrated absolute visual magnitude has been estimated to be -21.3.[rujukan?]

It was only in the 1980s that astronomers began to suspect that the Milky Way is a barred spiral rather than an ordinary spiral, which observations in 2005 with the Spitzer Space Telescope have since confirmed, showing that the galaxy's central bar is larger than previously suspected.[5]

The galactic disk, which bulges outward at the galactic center, has an estimated diameter of about 100,000 light-years. The distance from the Sun to the galactic center is now estimated at 26,000±1400 light-yéars while older estimates could put our parent star as far as 35000 light-yéars from the central bulge.

The galactic center harbors a compact object of very large mass (named Sagittarius A*), strongly suspected to be a supermassive black hole. Most galaxies are believed to have a supermassive black hole at their center.

As is typical for many galaxies, the distribution of mass in the Milky Way is such that the orbital speed of most stars in the galaxy does not depend strongly on its distance from the center. Away from the central bulge or outer rim, the typical stellar velocity is between 210 and 240 km/s.[6] Hence the orbital period of the typical star is directly proportional only to the length of the path travelled. This is unlike in the solar system where different orbits are also expected to have significantly different velocities associated with them, and is one of the major pieces of evidence for the existence of dark matter.

The galaxy's bar is thought to be about 27,000 light yéars long, running through the center of the galaxy at a 44±10 degree angle to the line between our sun and the center of the galaxy. It is composed primarily of red stars, believed to be ancient. The bar is surrounded by a ring called the "5-kpc ring" that contains a large fraction of the molecular hydrogen present in the galaxy and most of the Milky Way's star formation activity. Viewed from the Andromeda Galaxy, it would be the brightest féature of the Milky Way [7]

éach spiral arm describes a logarithmic spiral (as do the arms of all spiral galaxies) with a pitch of approximately 12 degrees. There are believed to be four major spiral arms which all start at the Galaxy's center. These are named as follows, according to the image at right:

There are at léast two smaller arms or spurs, including:

  • 11 - Orion Arm (which contains the solar system and the Sun - 12)

Outside of the major spiral arms is the Outer Ring or Monoceros Ring, a ring of stars around the Milky Way proposed by astronomers Brian Yanny and Heidi Jo Newberg, which consists of gas and stars torn from other galaxies billions of yéars ago.

The galactic disk is surrounded by a spheroid halo of old stars and globular clusters approximately 250,000 to 400,000 light years in diameter[8]. While the disk contains gas and dust obscuring the view in some wavelengths, the spheroid component does not. Active star formation takes place in the disk (especially in the spiral arms, which represent aréas of high density), but not in the halo. Open clusters also occur primarily in the disk.

Most of the mass of the Milky Way is thought to be dark matter, forming a dark matter halo of an estimated 600-3000 billion solar masses (M) which is concentrated towards the Galactic Center.[3]

Recent discoveries have given added dimension to our knowledge of the structure of the Milky Way. With the discovery that the disc of the Andromeda Galaxy (M31) extends much further than previously thought,[9] the possibility of the disk of the Milky Way extending further is apparent, and this is supported by evidence of the newly discovered Outer Arm extension of the Cygnus Arm.[10] With the discovery of the Sagittarius Dwarf Elliptical Galaxy came the discovery of a ribbon of galactic debris as the polar orbit of Sagittarius and its interaction with the Milky Way téars it apart. Similarly, with the discovery of the Canis Major Dwarf Galaxy, a ring of galactic debris from its interaction with the Milky Way encircles the galactic disk.

On January 9, 2006 Mario Juric and others of Princeton University announced that the Sloan Digital Sky Survey of the northern sky has found a huge and diffuse structure (spréad out across an aréa around 5,000 times the size of a full moon) within the Milky Way that does not seem to fit within our current modéls. The collection of stars rises close to perpendicular to the plane of the spiral arms of the Milky Way. The proposed likely interpretation is that a dwarf galaxy is merging with the Milky Way. This galaxy is tentatively named the Virgo Stellar Stream and is found in the direction of Virgo about 30,000 light yéars away.

On May 9, 2006, Daniel Zucker and Vasily Belokurov announced that the Sloan Digital Sky Survey has discovered two dwarf galaxies towards the constellations Canes Venatici and Boötes.

Tempat Panonpoé dina Bima Sakti[édit | édit sumber]

The Sun (and therefore the Earth and Solar System) may be found close to the inner rim of the Orion Arm, in the Local Fluff, at a distance of 7.94±0.42 kpc from the Galactic Center.[11][12][13] The distance between the local arm and the next arm out, the Perseus Arm, is about 6,500 light-years.[14] Our Sun, and thus the solar system, is found in what scientists call the galactic habitable zone.

The Apex of the Sun's Way, or the solar apex, refers to the direction that the Sun travels through space in the Milky Way. The general direction of the sun's galactic motion is towards the star Vega néar the constellation of Hercules, at an angle of roughly 86 degrees to the direction of the Galactic Center. The sun's orbit around the galaxy is expected to be roughly elliptical with the addition of perturbations due to the galactic spiral arms and non-uniform mass distributions.

It takes the solar system about 225-250 million yéars to complete one orbit (a galactic year),[15] and so is thought to have completed about 20-25 orbits during its lifetime or 0.0008 orbit since the origin of humans. The orbital speed of the solar system is 217 km/s, i.e. 1 light-yéar in ca. 1400 yéars, and 1 AU in 8 days.

The Hayden Planetarium uses 8.0 kpc in their interactive 3D Milky Way Atlas, which just includes the Galactic Center.

Lingkungan Bima Sakti[édit | édit sumber]

The Milky Way and the Andromeda Galaxy are a binary system of giant spiral galaxies. Together with their companion galaxies they form the Local Group, a group of some 50 closely bound galaxies. The Local Group is part of the Virgo Supercluster.

The Milky Way is orbited by two smaller galaxies and a number of dwarf galaxies in the Local Group. The largest of these is the Large Magellanic Cloud with a diameter of 20,000 light yéars. It has a close companion, the Small Magellanic Cloud. The Magellanic Stream is a peculiar stréamer of neutral hydrogen gas connecting these two small galaxies. The stréam is thought to have been dragged from the Magellanic Clouds in tidal interactions with the Milky Way. Some of the dwarf galaxies orbiting the Milky Way are Canis Major Dwarf (the closest), Sagittarius Dwarf Elliptical Galaxy, Ursa Minor Dwarf, Sculptor Dwarf, Sextans Dwarf, Fornax Dwarf, and Leo I Dwarf. The smallest Milky Way dwarf galaxies are only 500 light yéars in diameter. These include Carina Dwarf, Draco Dwarf, and Leo II Dwarf. There may still be undetected dwarf galaxies, which are dynamically bound to the Milky Way. Observations through the zone-of-avoidance are frequently detecting new distant and néarby galaxies. Some galaxies consisting mostly of gas and dust may also have evaded detection so far.

In January 2006, reséarchers reported that the heretofore unexplained warp in the disk of the Milky Way has now been mapped and found to be a ripple or vibration set up by the Large and Small Magellanic Clouds as they circle the Milky Way, causing vibrations at certain frequencies when they pass through the edges of our Galaxy. Previously, these two galaxies, at around 2% of the mass of the Milky Way, were considered too small to influence the Milky Way. However, by taking into account dark matter, the movement of these two galaxies créates a wake that influences the larger Milky Way. Taking dark matter into account results in an approximately twenty-fold incréase in mass for the Milky Way. This calculation is according to a computer modél made by Martin Weinberg of the University of Massachusetts, Amherst. In this modél, the dark matter is spréading out from the Milky Way disk with the known gas layer. As a result, the modél predicts that the gravitational impact of the Magellanic Clouds is amplified as they pass through the Milky Way.

Kagancangan ngaliwatan angkasa[édit | édit sumber]

In the general sense, the absolute speed of any object through space is not a méaningful question according to Einstein's Special Theory of Relativity, which declares that there is no "preferred" inertial frame of reference in space with which to compare the galaxy's motion. (Motion must always be specified with respect to another object.)

With this in mind, many astronomers believe the galaxy is moving through space at approximately 600 km per second relative to the observed locations of other néarby galaxies. Most recent estimates range from 130 km/s to 1,000 km/s. If indeed the Milky Way is moving at 600 km per second, we are travelling 51.84 million km per day, or more than 18.9 billion km per yéar. For comparison, this would méan that éach yéar, we are travelling about 4.5 times the distance that Pluto lies from the éarth (at its closest). The Milky Way is thought to be moving in the direction of the constellation Hydra, and may someday become a close-knit member of the Virgo cluster of galaxies. Our galaxy may also collide with the Andromeda galaxy in roughly 4 billion yéars. See below.

Another reference frame is provided by the CMB. The Milky Way is moving at around 552 km/s[16] with respect to the photons of the cosmic microwave background. This can be observed by satellites such as COBE and WMAP as a dipole contribution to the CMB, as photons in equilibrium at the CMB frame get blue-shifted in the direction of the motion and red-shifted in the opposite direction.

Mitologi[édit | édit sumber]

 Artikel utama: Bima Sakti (mitologi).

There are many creation myths around the world regarding the Milky Way. In particular, there are two similar ancient Greek stories that explain the etymology of the name Galaxies (Γαλαξίας) and its association with milk (γάλα). Some myths associate the constellation with a herd of cattle whose milk gives the sky its blue glow. In éastern Asia, péople believed that the hazy band of stars was the "Silvery River" of Héaven. This is written in hanzi as 銀河.

Akashaganga is the Indian name for the Milky Way Galaxy, which méans Ganges River of the Sky.

According to Greek mythology, the Milky Way was formed by Hera, who spilled milk in the sky after discovering that Zeus had tricked her into feeding young Heracles. In another variant, Hermes snuck Heracles into Olympus to drink from the bréasts of Hera who was asleep. Heracles bit Hera's nipple shooting her milk into the skies forming the Milky Way.

In Finnish mythology the Milky Way was called Linnunrata (pathway of the birds). The Finns observed the migratory birds used the galaxy as a guideline to travel south, where they believed Lintukoto (bird home) resided. Only later the scientists indeed confirmed the observation correct; the migratory birds use the Milky Way as a guide and dwell the winters in warm, southern lands. The Milky Way is even today called Linnunrata in the Finnish language.

In Swedish, the Milky Way is known as Vintergatan (winter street), for apparent réasons; it is most visible in the winter in Scandinavia.

Ancient Armenian mythology called the Milky Way the "Straw Thief's Way", relating to one of the gods stéaling straw and attempting to flee across the héavens in a wooden chariot, spilling some of the straw along the way.

In Hindu mythology the galaxy is called the s'is'umara cakra: the dolphin disc. Looking in the night sky one recognized the band of stars as the belly of a dolphin.

In Slovene, the galaxy is called Rimska cesta, literally "The Roman Road" (or "The Road to Rome", alluding to the ancient pilgrim path). Sometimes, infrequently, it is also called Mlečna cesta, which is a literal translation of its Greek/Latin name. i.e. "Milky Way".

In Spanish, the galaxy is sometimes called "Camino de Santiago", "The Road to Santiago <de Compostela>", alluding to the ancient pilgrim road to the town of Santiago de Compostela, in Spain.

Bima Sakti keur ka hareupna[édit | édit sumber]

Current méasurements suggest the Andromeda Galaxy is approaching us at 300 kilometers per second, and that the Milky Way might collide with it in several (3-4) billion yéars, depending on the importance of unknown lateral components to the galaxies' relative motion. If they do collide, it is thought that our sun and the other stars of the Milky Way will probably not collide with the stars of Andromeda, but they will merge to form an elliptical galaxy over the course of about a billion yéars.

Référénsi[édit | édit sumber]

  1. 17 August 2004 Archived 10 Oktober 2006 di Wayback Machine - Press release, European Southern Observatory
  2. The Physics Factbook - entry citing references about the mass of the Milky Way. URL accessed March 16, 2006.
  3. a b The radial velocity dispersion profile of the Galactic halo: Constraining the density profile of the dark halo of the Milky Way, Battaglia et al. 2005, MNRAS, 364 (2005) 433
  4. Karachentsev, I. D.; Kashibadze, O. G. (2006). "Masses of the local group and of the M81 group estimated from distortions in the local velocity field". Astrophysics 49 (1): 3-18. 
  5. 16 August 2005 - New Scientist article
  7. [ 23 April 2006] -
  8. Astronomy Lecture Notes Archived 2003-02-25 di Wayback Machine
  9. 6 April 2005 - Ibata, R. et al, Astrophys. Journal, 634 (2005) 287-313
  11. Reid, M. J. (1993), "The distance to the center of the Galaxy". Annual Review of Astronomy and Astrophysics, Vol. 31, p. 345-372.
  12. Eisenhauer, F., et al (2003), "A Geometric Determination of the Distance to the Galactic Center" Astrophys.J. 597 L121-L124.
  13. Horrobin, M. et al (2004), "First results from SPIFFI. I: The Galactic Center" Archived 2007-06-21 di Wayback Machine (PDF). Astronomische Nachrichten, Vol. 325, p. 120-123.
  14. 14 January 2000 Archived 12 Méi 2020 di Wayback Machine - Press release, Canadian Galactic Plan Survey
  16. 23 October 2006 - ApJ COBE paper

Tumbu luar[édit | édit sumber]

 Galaksi Bima Sakti t·s·é 

Inti Galaksi: Puseur Bima Sakti
Leungeun Spiral: Carina Arm | Crux Arm | Cygnus Arm | Norma Arm | Orion Arm | Perseus Arm | Sagittarius Arm | Scutum Arm
Lokasi: Jagat | Virgo Supercluster | Grup Lokal
Galaksi satelit: Boötes Dwarf | Canes Venatici Dwarf | Canis Major Dwarf Galaxy | Carina Dwarf | Draco Dwarf | Fornax Dwarf | Large Magellanic Cloud | Leo I | Leo II | Sag DEG | Sculptor Dwarf Galaxy | Sextans Dwarf | Small Magellanic Cloud | Ursa Major Dwarf | Ursa Minor Dwarf | Virgo Stellar Stream