Misplaced Pages

#296703

68-467: NGC 4565 is a giant spiral galaxy more luminous than the Andromeda Galaxy . Much speculation exists in literature as to the nature of the central bulge. In the absence of clear-cut dynamical data on the motions of stars in the bulge, the photometric data alone cannot adjudge among various options put forth. However, its exponential shape suggested that it is a barred spiral galaxy . Studies with

136-410: A distance estimate of 500,000 ly (3.2 × 10  AU). Although this estimate is about fivefold lower than the best estimates now available, it was the first known estimate of the distance to Andromeda that was correct to within an order of magnitude (i.e., to within a factor of ten of the current estimates, which place the distance around 2.5 million light-years ). Curtis became a proponent of

204-413: A drawing of Andromeda's spiral structure . In 1864, William Huggins noted that the spectrum of Andromeda differed from that of a gaseous nebula. The spectrum of Andromeda displays a continuum of frequencies , superimposed with dark absorption lines that help identify the chemical composition of an object. Andromeda's spectrum is very similar to the spectra of individual stars, and from this, it

272-520: A galaxy in the B-band (445 nm wavelength of light, in the blue part of the visible spectrum ) reaches 25 mag/arcsec . The Third Reference Catalogue of Bright Galaxies (RC3) used this standard for Andromeda in 1991, yielding an isophotal diameter of 46.56 kiloparsecs (152,000 light-years) at a distance of 2.5 million light-years. An earlier estimate from 1981 gave a diameter for Andromeda at 54 kiloparsecs (176,000 light-years). A study in 2005 by

340-529: A galaxy that lies in the "green valley" of the Galaxy color-magnitude diagram (see below ). Supernovae erupt in the Andromeda Galaxy's star-filled disk and eject these heavier elements into space. Over the Andromeda Galaxy's lifetime, nearly half of the heavy elements made by its stars have been ejected far beyond the galaxy's 200,000-light-year-diameter stellar disk. The estimated luminosity of

408-480: A great star formation phase, but is now in a relative state of quiescence, whereas the Milky Way is experiencing more active star formation. Should this continue, the luminosity of the Milky Way may eventually overtake that of the Andromeda Galaxy. According to recent studies, the Andromeda Galaxy lies in what is known in the galaxy color–magnitude diagram as the "green valley", a region populated by galaxies like

476-527: A large lenticular galaxy . With an apparent magnitude of 3.4, the Andromeda Galaxy is among the brightest of the Messier objects , and is visible to the naked eye from Earth on moonless nights, even when viewed from areas with moderate light pollution . The Andromeda Galaxy is visible to the naked eye in dark skies. Around the year 964 CE , the Persian astronomer Abd al-Rahman al-Sufi described

544-455: A metallicity correction of −0.2 mag dex in (O/H), an estimate of 2.57 ± 0.06 million light-years (1.625 × 10  ± 3.8 × 10 astronomical units ) was derived. A 2004 Cepheid variable method estimated the distance to be 2.51 ± 0.13 million light-years (770 ± 40 kpc). In 2005, an eclipsing binary star was discovered in the Andromeda Galaxy. The binary is made up of two hot blue stars of types O and B. By studying

612-488: A possibly lower mass for the Andromeda Galaxy and a higher mass for the Milky Way. The Andromeda Galaxy has a diameter of about 46.56 kpc (152,000 ly), making it the largest member of the Local Group of galaxies in terms of extension. The Milky Way and Andromeda galaxies are expected to collide with each other in around 4–5 billion years, merging to potentially form a giant elliptical galaxy or

680-513: A radius of 33,000 ly (2.1 × 10  AU), where it reaches a peak of 250 km/s (160 mi/s). The velocities slowly decline beyond that distance, dropping to around 200 km/s (120 mi/s) at 80,000 ly (5.1 × 10  AU). These velocity measurements imply a concentrated mass of about 6 × 10   M ☉ in the nucleus . The total mass of the galaxy increases linearly out to 45,000 ly (2.8 × 10  AU), then more slowly beyond that radius. The spiral arms of

748-587: A slightly warped and extended disk under deep optical surveys, likely due to ongoing interactions with neighboring satellite galaxies or other galaxies in the Coma I group. GALEX images show the slight warp at the edge of the disc more clearly than other surveys. Using the LOw-Frequency ARray (LOFAR), astronomers of the University of Hamburg discovered a diffuse radio halo around NGC 4565. During

SECTION 10

#1732783721297

816-402: Is actually a barred spiral galaxy , like the Milky Way, with Andromeda's bar major axis oriented 55 degrees anti-clockwise from the disc major axis. There are various methods used in astronomy in defining the size of a galaxy, and each method can yield different results concerning one another. The most commonly employed is the D 25 standard, the isophote where the photometric brightness of

884-676: Is called 2C 56 in the 2C radio astronomy catalog. In 2009, an occurrence of microlensing —a phenomenon caused by the deflection of light by a massive object—may have led to the first discovery of a planet in the Andromeda Galaxy. In 2020, observations of linearly polarized radio emission with the Westerbork Synthesis Radio Telescope , the Effelsberg 100-m Radio Telescope , and the Very Large Array revealed ordered magnetic fields aligned along

952-505: Is cataloged as Messier 31 , M31 , and NGC 224 . Andromeda has a D 25 isophotal diameter of about 46.56 kiloparsecs (152,000 light-years ) and is approximately 765 kpc (2.5 million light-years) from Earth. The galaxy's name stems from the area of Earth's sky in which it appears, the constellation of Andromeda , which itself is named after the princess who was the wife of Perseus in Greek mythology . The virial mass of

1020-494: Is hidden from visible light images of the galaxy because it is composed primarily of cold dust, and most of the star formation that is taking place in the Andromeda Galaxy is concentrated there. Later studies with the help of the Spitzer Space Telescope showed how the Andromeda Galaxy's spiral structure in the infrared appears to be composed of two spiral arms that emerge from a central bar and continue beyond

1088-414: Is measured to be ≈ 160  km/s (100  mi/s ). It has been proposed that the observed double nucleus could be explained if P1 is the projection of a disk of stars in an eccentric orbit around the central black hole. The eccentricity is such that stars linger at the orbital apocenter , creating a concentration of stars. It has been postulated that such an eccentric disk could have been formed from

1156-435: Is only half of the Milky Way's newer mass, calculated in 2019 at 1.5 × 10   M ☉ . In addition to stars, the Andromeda Galaxy's interstellar medium contains at least 7.2 × 10   M ☉ in the form of neutral hydrogen , at least 3.4 × 10   M ☉ as molecular hydrogen (within its innermost 10 kiloparsecs), and 5.4 × 10   M ☉ of dust . The Andromeda Galaxy

1224-458: Is surrounded by a massive halo of hot gas that is estimated to contain half the mass of the stars in the galaxy. The nearly invisible halo stretches about a million light-years from its host galaxy, halfway to our Milky Way Galaxy. Simulations of galaxies indicate the halo formed at the same time as the Andromeda Galaxy. The halo is enriched in elements heavier than hydrogen and helium, formed from supernovae , and its properties are those expected for

1292-487: Is the second-brightest galaxy within a radius of 10 megaparsecs of the Milky Way, after the Sombrero Galaxy , with an absolute magnitude of around −22.21 or close ). An estimation done with the help of Spitzer Space Telescope published in 2010 suggests an absolute magnitude (in the blue) of −20.89 (that with a color index of +0.63 translates to an absolute visual magnitude of −21.52, compared to −20.9 for

1360-522: Is the spectral age of the galaxy's cosmic ray electrons, during which they are transported into the warp. This indicates that NGC 4565 may be in the aftermath of a period with more intense star formation . Andromeda Galaxy The Andromeda Galaxy is a barred spiral galaxy and is the nearest major galaxy to the Milky Way . It was originally named the Andromeda Nebula and

1428-474: The Cartwheel encounter . Studies of the extended halo of the Andromeda Galaxy show that it is roughly comparable to that of the Milky Way, with stars in the halo being generally " metal-poor ", and increasingly so with greater distance. This evidence indicates that the two galaxies have followed similar evolutionary paths. They are likely to have accreted and assimilated about 100–200 low-mass galaxies during

SECTION 20

#1732783721297

1496-484: The European Space Agency 's Infrared Space Observatory demonstrated that the overall form of the Andromeda Galaxy may be transitioning into a ring galaxy . The gas and dust within the galaxy are generally formed into several overlapping rings, with a particularly prominent ring formed at a radius of 32,000 ly (9.8 kpc) from the core, nicknamed by some astronomers the ring of fire . This ring

1564-494: The Hubble Space Telescope was used to image the Andromeda Galaxy's inner nucleus. The nucleus consists of two concentrations separated by 1.5  pc (4.9  ly ). The brighter concentration, designated as P1, is offset from the center of the galaxy. The dimmer concentration, P2, falls at the true center of the galaxy and contains an embedded star cluster, called P3, containing many UV -bright A-stars and

1632-561: The Keck telescopes shows the existence of a tenuous sprinkle of stars, or galactic halo , extending outward from the galaxy. The stars in this halo behave differently from the ones in Andromeda's main galactic disc, where they show rather disorganized orbital motions as opposed to the stars in the main disc having more orderly orbits and uniform velocities of 200 km/s. This diffuse halo extends outwards away from Andromeda's main disc with

1700-551: The Triangulum Galaxy (M33) might have had a very close passage 2–4 billion years ago, but it seems unlikely from the last measurements from the Hubble Space Telescope. At least four distinct techniques have been used to estimate distances from Earth to the Andromeda Galaxy. In 2003, using the infrared surface brightness fluctuations (I-SBF) and adjusting for the new period-luminosity value and

1768-401: The rotational velocity of the Andromeda Galaxy as a function of radial distance from the core. The rotational velocity has a maximum value of 225 km/s (140 mi/s) at 1,300  ly (82,000,000  AU ) from the core, and it has its minimum possibly as low as 50 km/s (31 mi/s) at 7,000 ly (440,000,000 AU) from the core. Further out, rotational velocity rises out to

1836-417: The supermassive black hole , called M31* . The black hole is classified as a low-luminosity AGN (LLAGN) and it was detected only in radio wavelengths and in x-rays . It was quiescent in 2004–2005, but it was highly variable in 2006–2007. The mass of M31* was measured at 3–5 × 10 M ☉ in 1993, and at 1.1–2.3 × 10 M ☉ in 2005. The velocity dispersion of material around it

1904-565: The "10-kpc ring" of gas and star formation. The estimated distance of the Andromeda Galaxy from our own was doubled in 1953 when it was discovered that there is a second, dimmer type of Cepheid variable star . In the 1990s, measurements of both standard red giants as well as red clump stars from the Hipparcos satellite measurements were used to calibrate the Cepheid distances. A major merger occurred 2 to 3 billion years ago at

1972-421: The Andromeda Galaxy are outlined by a series of HII regions , first studied in great detail by Walter Baade and described by him as resembling "beads on a string". His studies show two spiral arms that appear to be tightly wound, although they are more widely spaced than in our galaxy. His descriptions of the spiral structure, as each arm crosses the major axis of the Andromeda Galaxy, are as follows : Since

2040-587: The Andromeda Galaxy in his Book of Fixed Stars as a "nebulous smear" or "small cloud". Star charts of that period labeled it as the Little Cloud . In 1612, the German astronomer Simon Marius gave an early description of the Andromeda Galaxy based on telescopic observations. Pierre Louis Maupertuis conjectured in 1745 that the blurry spot was an island universe. Charles Messier cataloged Andromeda as object M31 in 1764 and incorrectly credited Marius as

2108-415: The Andromeda Galaxy is of the same order of magnitude as that of the Milky Way, at 1  trillion solar masses (2.0 × 10 kilograms ). The mass of either galaxy is difficult to estimate with any accuracy, but it was long thought that the Andromeda Galaxy was more massive than the Milky Way by a margin of some 25% to 50%. However, this has been called into question by early 21st-century studies indicating

NGC 4565 - Misplaced Pages Continue

2176-407: The Andromeda Galaxy is seen close to edge-on, it is difficult to study its spiral structure. Rectified images of the galaxy seem to show a fairly normal spiral galaxy, exhibiting two continuous trailing arms that are separated from each other by a minimum of about 13,000  ly (820,000,000  AU ) and that can be followed outward from a distance of roughly 1,600 ly (100,000,000 AU) from

2244-429: The Andromeda Galaxy's spheroid was determined to have a higher stellar density than that of the Milky Way, and its galactic stellar disk was estimated at twice the diameter of that of the Milky Way. The total mass of the Andromeda Galaxy is estimated to be between 8 × 10   M ☉ and 1.1 × 10   M ☉ . The stellar mass of M31 is 10–15 × 10   M ☉ , with 30% of that mass in

2312-470: The Andromeda Galaxy's halo (including dark matter ) gave a value of approximately 1.5 × 10   M ☉ , compared to 8 × 10   M ☉ for the Milky Way. This contradicted even earlier measurements that seemed to indicate that the Andromeda Galaxy and Milky Way are almost equal in mass. In 2018, the earlier measurements for equality of mass were re-established by radio results as approximately 8 × 10   M ☉ . In 2006,

2380-406: The Andromeda Galaxy, ~2.6 × 10   L ☉ , is about 25% higher than that of our own galaxy. However, the galaxy has a high inclination as seen from Earth, and its interstellar dust absorbs an unknown amount of light, so it is difficult to estimate its actual brightness and other authors have given other values for the luminosity of the Andromeda Galaxy (some authors even propose it

2448-425: The Andromeda location, involving two galaxies with a mass ratio of approximately 4. The discovery of a recent merger in the Andromeda galaxy was first based on interpreting its anomalous age-velocity dispersion relation, as well as the fact that 2 billion years ago, star formation throughout Andromeda's disk was much more active than today. Modeling of this violent collision shows that it has formed most of

2516-487: The German philosopher Immanuel Kant proposed the hypothesis that the Milky Way is only one of many galaxies in his book Universal Natural History and Theory of the Heavens . Arguing that a structure like the Milky Way would look like a circular nebula viewed from above and like an ellipsoid if viewed from an angle, he concluded that the observed elliptical nebulae like Andromeda, which could not be explained otherwise at

2584-489: The Milky Way Galaxy. There are approximately 460 globular clusters associated with the Andromeda Galaxy. The most massive of these clusters, identified as Mayall II , nicknamed Globular One, has a greater luminosity than any other known globular cluster in the Local Group of galaxies. It contains several million stars and is about twice as luminous as Omega Centauri , the brightest known globular cluster in

2652-435: The Milky Way in transition from the "blue cloud" (galaxies actively forming new stars) to the "red sequence" (galaxies that lack star formation). Star formation activity in green valley galaxies is slowing as they run out of star-forming gas in the interstellar medium. In simulated galaxies with similar properties to the Andromeda Galaxy, star formation is expected to extinguish within about five billion years, even accounting for

2720-466: The Milky Way), and a total luminosity in that wavelength of 3.64 × 10   L ☉ . The rate of star formation in the Milky Way is much higher, with the Andromeda Galaxy producing only about one solar mass per year compared to 3–5 solar masses for the Milky Way. The rate of novae in the Milky Way is also double that of the Andromeda Galaxy. This suggests that the latter once experienced

2788-435: The Milky Way. Globular One (or G1) has several stellar populations and a structure too massive for an ordinary globular. As a result, some consider G1 to be the remnant core of a dwarf galaxy that was consumed by Andromeda in the distant past. The globular with the greatest apparent brightness is G76 which is located in the southwest arm's eastern half. Another massive globular cluster, named 037-B327 and discovered in 2006 as

NGC 4565 - Misplaced Pages Continue

2856-515: The central bulge , 56% in the disk , and the remaining 14% in the stellar halo . The radio results (similar mass to the Milky Way Galaxy) should be taken as likeliest as of 2018, although clearly, this matter is still under active investigation by several research groups worldwide. As of 2019, current calculations based on escape velocity and dynamical mass measurements put the Andromeda Galaxy at 0.8 × 10   M ☉ , which

2924-407: The core. Alternative spiral structures have been proposed such as a single spiral arm or a flocculent pattern of long, filamentary, and thick spiral arms. The most likely cause of the distortions of the spiral pattern is thought to be interaction with galaxy satellites M32 and M110 . This can be seen by the displacement of the neutral hydrogen clouds from the stars. In 1998, images from

2992-618: The diameter of 67.45 kiloparsecs (220,000 light-years). The galaxy is inclined an estimated 77° relative to Earth (where an angle of 90° would be edge-on). Analysis of the cross-sectional shape of the galaxy appears to demonstrate a pronounced, S-shaped warp, rather than just a flat disk. A possible cause of such a warp could be gravitational interaction with the satellite galaxies near the Andromeda Galaxy. The Galaxy M33 could be responsible for some warp in Andromeda's arms, though more precise distances and radial velocities are required. Spectroscopic studies have provided detailed measurements of

3060-471: The discoverer despite it being visible to the naked eye. In 1785, the astronomer William Herschel noted a faint reddish hue in the core region of Andromeda. He believed Andromeda to be the nearest of all the "great nebulae ", and based on the color and magnitude of the nebula , he incorrectly guessed that it was no more than 2,000 times the distance of Sirius , or roughly 18,000  ly (5.5  kpc ). In 1850, William Parsons, 3rd Earl of Rosse , made

3128-563: The distance estimate to Andromeda, as well as the remainder of the universe. In 1950, radio emissions from the Andromeda Galaxy were detected by Robert Hanbury Brown and Cyril Hazard at the Jodrell Bank Observatory . The first radio maps of the galaxy were made in the 1950s by John Baldwin and collaborators at the Cambridge Radio Astronomy Group . The core of the Andromeda Galaxy

3196-453: The distribution of stars in P1 does not suggest that there is a black hole at its center. Apparently, by late 1968, no X-rays had been detected from the Andromeda Galaxy. A balloon flight on 20 October 1970 set an upper limit for detectable hard X-rays from the Andromeda Galaxy. The Swift BAT all-sky survey successfully detected hard X-rays coming from a region centered 6 arcseconds away from

3264-588: The dust clouds in our own galaxy, as well as historical observations of the Andromeda Galaxy's significant Doppler shift . In 1922, Ernst Öpik presented a method to estimate the distance of Andromeda using the measured velocities of its stars. His result placed the Andromeda Nebula far outside our galaxy at a distance of about 450 kpc (1,500 kly). Edwin Hubble settled the debate in 1925 when he identified extragalactic Cepheid variable stars for

3332-407: The eclipses of the stars, astronomers were able to measure their sizes. Knowing the sizes and temperatures of the stars, they were able to measure their absolute magnitude . When the visual and absolute magnitudes are known, the distance to the star can be calculated. The stars lie at a distance of 2.52 × 10 ^  ± 0.14 × 10 ^  ly (1.594 × 10  ± 8.9 × 10  AU) and

3400-419: The expected, short-term increase in the rate of star formation due to the collision between the Andromeda Galaxy and the Milky Way. Based on its appearance in visible light, the Andromeda Galaxy is classified as an SA(s)b galaxy in the de Vaucouleurs–Sandage extended classification system of spiral galaxies. However, infrared data from the 2MASS survey and the Spitzer Space Telescope showed that Andromeda

3468-469: The first photographs of Andromeda, which was still commonly thought to be a nebula within our galaxy. Roberts mistook Andromeda and similar "spiral nebulae" as star systems being formed . In 1912, Vesto Slipher used spectroscopy to measure the radial velocity of Andromeda with respect to the Solar System —the largest velocity yet measured, at 300 km/s (190 mi/s). As early as 1755,

SECTION 50

#1732783721297

3536-499: The first time on astronomical photos of Andromeda. These were made using the 100-inch (2.5 m) Hooker telescope , and they enabled the distance of the Great Andromeda Nebula to be determined. His measurement demonstrated conclusively that this feature was not a cluster of stars and gas within our own galaxy, but an entirely separate galaxy located a significant distance from the Milky Way. In 1943, Walter Baade

3604-483: The galactic center and has about 10 M ☉ . It was discovered through data collected by the European Space Agency 's XMM-Newton probe and was subsequently observed by NASA 's Swift Gamma-Ray Burst Mission and Chandra X-Ray Observatory , the Very Large Array , and the Very Long Baseline Array . The microquasar was the first observed within the Andromeda Galaxy and the first outside of

3672-588: The galaxy center. The emission above 25 keV was later found to be originating from a single source named 3XMM J004232.1+411314 , and identified as a binary system where a compact object (a neutron star or a black hole) accretes matter from a star. Multiple X-ray sources have since been detected in the Andromeda Galaxy, using observations from the European Space Agency 's (ESA) XMM-Newton orbiting observatory. Robin Barnard et al. hypothesized that these are candidate black holes or neutron stars , which are heating

3740-492: The galaxy's (metal-rich) galactic halo , including the Giant Stream, and also the extended thick disk, the young age thin disk, and the static 10 kpc ring. During this epoch, its rate of star formation would have been very high , to the point of becoming a luminous infrared galaxy for roughly 100 million years. Modeling also recovers the bulge profile, the large bar, and the overall halo density profile. Andromeda and

3808-486: The help of the Spitzer Space Telescope not only confirmed the presence of a central bar but also showed a pseudobulge within it as well as an inner ring. NGC 4565 has at least two satellite galaxies , one of which is interacting with it. It has a population of roughly 240 globular clusters , more than the Milky Way . NGC 4565 is one of the brightest member galaxies of the Coma I Group . This edge-on galaxy exhibits

3876-405: The incoming gas to millions of kelvins and emitting X-rays. Neutron stars and black holes can be distinguished mainly by measuring their masses. An observation campaign of NuSTAR space mission identified 40 objects of this kind in the galaxy. In 2012, a microquasar , a radio burst emanating from a smaller black hole was detected in the Andromeda Galaxy. The progenitor black hole is located near

3944-417: The large ring mentioned above. Those arms, however, are not continuous and have a segmented structure. Close examination of the inner region of the Andromeda Galaxy with the same telescope also showed a smaller dust ring that is believed to have been caused by the interaction with M32 more than 200 million years ago. Simulations show that the smaller galaxy passed through the disk of the Andromeda Galaxy along

4012-410: The latter's polar axis. This collision stripped more than half the mass from the smaller M32 and created the ring structures in Andromeda. It is the co-existence of the long-known large ring-like feature in the gas of Messier 31, together with this newly discovered inner ring-like structure, offset from the barycenter , that suggested a nearly head-on collision with the satellite M32, a milder version of

4080-440: The observations, a warp was detected in the radio continuum of NGC 4565 that is reminiscent of a neutral hydrogen line (HI) warp and identifying a slight flaring of the galaxy's radio halo. It is assumed that this flaring is caused by the warp as the vertical intensity profiles are asymmetric, which is in agreement with the warp. According to the study, a minimum age for the warp was estimated at approximately 130 million years. This

4148-413: The past 12 billion years. The stars in the extended halos of the Andromeda Galaxy and the Milky Way may extend nearly one-third the distance separating the two galaxies. The Andromeda Galaxy is known to harbor a dense and compact star cluster at its very center, similar to our own galaxy . A large telescope creates a visual impression of a star embedded in the more diffuse surrounding bulge. In 1991,

SECTION 60

#1732783721297

4216-426: The result of a previous black hole merger, where the release of gravitational waves could have "kicked" the stars into their current eccentric distribution. P2 also contains a compact disk of hot, spectral-class A stars. The A stars are not evident in redder filters, but in blue and ultraviolet light they dominate the nucleus, causing P2 to appear more prominent than P1. While at the initial time of its discovery it

4284-500: The so-called "island universes" hypothesis: that spiral nebulae were actually independent galaxies. In 1920, the Great Debate between Harlow Shapley and Curtis took place concerning the nature of the Milky Way, spiral nebulae, and the dimensions of the universe . To support his claim that the Great Andromeda Nebula is, in fact, an external galaxy, Curtis also noted the appearance of dark lanes within Andromeda that resembled

4352-408: The time, were indeed galaxies similar to the Milky Way, not nebulae, as Andromeda was commonly believed to be. In 1917, Heber Curtis observed a nova within Andromeda. After searching the photographic record, 11 more novae were discovered. Curtis noticed that these novae were, on average, 10 magnitudes fainter than those that occurred elsewhere in the sky. As a result, he was able to come up with

4420-542: The whole Andromeda Galaxy at about 2.5 × 10 ^  ly (1.6 × 10  AU). This new value is in excellent agreement with the previous, independent Cepheid-based distance value. The TRGB method was also used in 2005 giving a distance of 2.56 × 10 ^  ± 0.08 × 10 ^  ly (1.619 × 10  ± 5.1 × 10  AU). Averaged together, these distance estimates give a value of 2.54 × 10 ^  ± 0.11 × 10 ^  ly (1.606 × 10  ± 7.0 × 10  AU). Until 2018, mass estimates for

4488-470: Was deduced that Andromeda has a stellar nature. In 1885, a supernova (known as S Andromedae ) was seen in Andromeda, the first and so far only one observed in that galaxy. At the time, it was called "Nova 1885" —the difference between " novae " in the modern sense and supernovae was not yet known. Andromeda was considered to be a nearby object, and it was not realized that the "nova" was much brighter than ordinary novae. In 1888, Isaac Roberts took one of

4556-399: Was hypothesized that the brighter portion of the double nucleus is the remnant of a small galaxy "cannibalized" by the Andromeda Galaxy, this is no longer considered a viable explanation, largely because such a nucleus would have an exceedingly short lifetime due to tidal disruption by the central black hole. While this could be partially resolved if P1 had its own black hole to stabilize it,

4624-546: Was the first person to resolve stars in the central region of the Andromeda Galaxy. Baade identified two distinct populations of stars based on their metallicity , naming the young, high-velocity stars in the disk Type I and the older, red stars in the bulge Type II. This nomenclature was subsequently adopted for stars within the Milky Way and elsewhere. (The existence of two distinct populations had been noted earlier by Jan Oort .) Baade also discovered that there were two types of Cepheid variable stars, which resulted in doubling

#296703