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54-701: (Redirected from SS Meteor ) A number of ships have been named Meteor after a meteor or shooting star , including the following: Naval and Government vessels [ edit ] HMS  Meteor , several ships of the Royal Navy SMS ; Meteor , several ships of the German Navy USAT ; Meteor , a troop transport of the US Army, built 1899 as Chester W. Chapin USS ; Meteor , several ships of

108-892: A British coastal passenger ship, later with the Romanian Government SS ; Meteor  (1896) , a whaleback freighter on the Great Lakes, now a museum ship in Superior, Wisconsin SS ; Meteor  (1904) , an ocean liner built for the Hamburg America Line, and later with Bergen Line; sunk by aircraft 9 March 1945 One of several Type C2 ships built for the United States Maritime Commission: SS ; Meteor  (1941) (MC hull number 127, Type C2-T), built by Tampa Shipbuilding; transferred to

162-661: A Soviet seagoing passenger hydrofoil design; over 400 built from 1959 to 2006 Yachts [ edit ] Meteor (1887 yacht) (1887), Kaiser Wilhelm II's yacht, formerly Thistle Meteor (1902 yacht) (1902)  [ de ] , Kaiser Wilhelm II's yacht See also [ edit ] HMS Meteorite , an experimental submarine References [ edit ] ^ " Hermes (5617260)" . Miramar Ship Index . Retrieved 2024-03-31 . ^ " Meteor (1091097)" . Miramar Ship Index . Retrieved 2024-03-31 . ^ Michael, Chris. "Post-office Steam Packets" . Liverpool University. Archived from

216-440: A certain amount of meteoroids are shed. The meteoroids spread out along the entire orbit of the comet to form a meteoroid stream, also known as a "dust trail" (as opposed to a comet's "dust tail" caused by the very small particles that are quickly blown away by solar radiation pressure). The frequency of fireball sightings increases by about 10–30% during the weeks of vernal equinox . Even meteorite falls are more common during

270-457: A cosmic origin. After reviewing historical records, Heinrich Wilhelm Matthias Olbers predicted the storm's return in 1867, drawing other astronomers' attention to the phenomenon. Hubert A. Newton 's more thorough historical work led to a refined prediction of 1866, which proved correct. With Giovanni Schiaparelli 's success in connecting the Leonids (as they are called) with comet Tempel-Tuttle ,

324-738: A deviation for any object causing a meteor. Objects smaller than meteoroids are classified as micrometeoroids and interplanetary dust . The Minor Planet Center does not use the term "meteoroid". Almost all meteoroids contain extraterrestrial nickel and iron. They have three main classifications: iron, stone, and stony-iron. Some stone meteoroids contain grain-like inclusions known as chondrules and are called chondrites . Stony meteoroids without these features are called " achondrites ", which are typically formed from extraterrestrial igneous activity; they contain little or no extraterrestrial iron. The composition of meteoroids can be inferred as they pass through Earth's atmosphere from their trajectories and

378-535: A generic large crater-forming projectile in a manner "to imply that we do not know the precise nature of the impacting body ... whether it is a rocky or metallic asteroid, or an icy comet for example". Meteoroids also hit other bodies in the Solar System. On such stony bodies as the Moon or Mars that have little or no atmosphere, they leave enduring craters. Meteoroid collisions with solid Solar System objects, including

432-418: A meteoroid would be between 100 μm and 10 m (33 ft) across. In 2010, following the discovery of asteroids below 10 m in size, Rubin and Grossman proposed a revision of the previous definition of meteoroid to objects between 10 μm (0.00039 in) and one meter (3 ft 3 in) in diameter in order to maintain the distinction. According to Rubin and Grossman, the minimum size of an asteroid

486-582: A more rigid definition. It defines a fireball as a meteor that would have a magnitude of −3 or brighter if seen at zenith . This definition corrects for the greater distance between an observer and a meteor near the horizon. For example, a meteor of magnitude −1 at 5 degrees above the horizon would be classified as a fireball because, if the observer had been directly below the meteor, it would have appeared as magnitude −6. Fireballs reaching apparent magnitude −14 or brighter are called bolides . The IAU has no official definition of "bolide", and generally considers

540-484: A quarter that of ice, to nickel-iron rich dense rocks. The study of meteorites also gives insights into the composition of non-ephemeral meteoroids. Most meteoroids come from the asteroid belt , having been perturbed by the gravitational influences of planets, but others are particles from comets , giving rise to meteor showers . Some meteoroids are fragments from bodies such as Mars or the Moon , that have been thrown into space by an impact. Meteoroids travel around

594-560: A second. Meteors were not known to be an astronomical phenomenon until early in the nineteenth century. Before that, they were seen in the West as an atmospheric phenomenon, like lightning, and were not connected with strange stories of rocks falling from the sky. In 1807, Yale University chemistry professor Benjamin Silliman investigated a meteorite that fell in Weston, Connecticut . Silliman believed

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648-412: A size scale larger than 10 cm (3.9 in) to several meters meteor visibility is due to the atmospheric ram pressure (not friction) that heats the meteoroid so that it glows and creates a shining trail of gases and melted meteoroid particles. The gases include vaporised meteoroid material and atmospheric gases that heat up when the meteoroid passes through the atmosphere. Most meteors glow for about

702-453: A specific stream of space debris . A number of specific meteors have been observed, largely by members of the public and largely by accident, but with enough detail that orbits of the meteoroids producing the meteors have been calculated. The atmospheric velocities of meteors result from the movement of Earth around the Sun at about 30 km/s (67,000 mph), the orbital speeds of meteoroids, and

756-489: Is called meteoric dust or just meteor dust. Meteor dust particles can persist in the atmosphere for up to several months. These particles might affect climate, both by scattering electromagnetic radiation and by catalyzing chemical reactions in the upper atmosphere. Meteoroids or their fragments achieve dark flight after deceleration to terminal velocity . Dark flight starts when they decelerate to about 2–4 km/s (4,500–8,900 mph). Larger fragments fall further down

810-628: Is different from Wikidata All set index articles Meteoroid A meteor or shooting star is the visible passage of a meteoroid, comet, or asteroid entering Earth's atmosphere . At a speed typically in excess of 20 km/s (72,000 km/h; 45,000 mph), aerodynamic heating of that object produces a streak of light, both from the glowing object and the trail of glowing particles that it leaves in its wake. Meteors typically become visible when they are about 100 km (62 mi) above sea level. A series of many meteors appearing seconds or minutes apart and appearing to originate from

864-555: Is given by what can be discovered from Earth-bound telescopes, so the distinction between meteoroid and asteroid is fuzzy. Some of the smallest asteroids discovered (based on absolute magnitude H ) are 2008 TS 26 with H = 33.2 and 2011 CQ 1 with H = 32.1 both with an estimated size of one m (3 ft 3 in). In April 2017, the IAU adopted an official revision of its definition, limiting size to between 30 μm (0.0012 in) and one meter in diameter, but allowing for

918-467: The Greek βολίς ( bolis ) which can mean a missile or to flash . If the magnitude of a bolide reaches −17 or brighter it is known as a superbolide . A relatively small percentage of fireballs hit Earth's atmosphere and then pass out again: these are termed Earth-grazing fireballs . Such an event happened in broad daylight over North America in 1972 . Another rare phenomenon is a meteor procession , where

972-499: The Phoenicids can make atmospheric entry at as slow as about 11 km/s. On January 17, 2013, at 05:21 PST, a one-meter-sized comet from the Oort cloud entered Earth atmosphere over California and Nevada . The object had a retrograde orbit with perihelion at 0.98 ± 0.03  AU . It approached from the direction of the constellation Virgo (which was in the south about 50° above

1026-528: The article wizard to submit a draft for review, or request a new article . Search for " Meteor (Schiff, 1902) " in existing articles. Look for pages within Misplaced Pages that link to this title . Other reasons this message may be displayed: If a page was recently created here, it may not be visible yet because of a delay in updating the database; wait a few minutes or try the purge function . Titles on Misplaced Pages are case sensitive except for

1080-438: The gravity well of Earth. Meteors become visible between about 75 to 120 km (250,000 to 390,000 ft) above Earth. They usually disintegrate at altitudes of 50 to 95 km (160,000 to 310,000 ft). Meteors have roughly a fifty percent chance of a daylight (or near daylight) collision with Earth. Most meteors are, however, observed at night, when darkness allows fainter objects to be recognized. For bodies with

1134-403: The strewn field . The visible light produced by a meteor may take on various hues, depending on the chemical composition of the meteoroid, and the speed of its movement through the atmosphere. As layers of the meteoroid abrade and ionize, the colour of the light emitted may change according to the layering of minerals. Colours of meteors depend on the relative influence of the metallic content of

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1188-523: The British Post Office Meteor (1915), a German survey ship Meteor (1964), a German research vessel Meteor (1986), a German research vessel a new German research vessel under construction, completion planned for 2026 Merchant ships [ edit ] Meteor , a British schooner; destroyed in an accidental explosion in February 1834 SS  Meteor  (1887) ,

1242-472: The Moon, Mercury , Callisto , Ganymede , and most small moons and asteroids , create impact craters, which are the dominant geographic features of many of those objects. On other planets and moons with active surface geological processes, such as Earth, Venus , Mars , Europa , Io , and Titan , visible impact craters may become eroded , buried, or transformed by tectonics over time. In early literature, before

1296-444: The Sun in a variety of orbits and at various velocities. The fastest move at about 42 km/s (94,000 mph) through space in the vicinity of Earth's orbit. This is escape velocity from the Sun, equal to the square root of two times Earth's speed, and is the upper speed limit of objects in the vicinity of Earth, unless they come from interstellar space. Earth travels at about 29.6 km/s (66,000 mph), so when meteoroids meet

1350-690: The United States Navy Meteoro (1848), a brigantine that served in the Mexican and Chilean navies Meteor (1877), a salvage vessel, built as Hermes , that served in the Russian and Soviet navies 1916–1958 Meteor (1887), a gunboat of the Austro-Hungarian Navy Meteoro -class , a class of Spanish offshore patrol vessels Meteoro (2009) , the first-of-class PS  Meteor  (1821) , an early steam packet of

1404-521: The United States Navy as Arcturus -class attack cargo ship USS Electra (AKA-4); scrapped in 1974 SS  Meteor  (1943) (MC hull number 292, Type C2-S-B1), built by Moore Dry Dock; sold for commercial use under the name American Miller in 1948; scrapped in 1970 MV  Meteor  (1955) , a cruise ship of Bergen Line, then later with Epirotiki Line as Neptune ; scrapped in 2002 Meteor-class (hydrofoil)  [ ru ] ,

1458-456: The atmosphere and hits the ground without being destroyed. Meteorites are sometimes, but not always, found in association with hypervelocity impact craters ; during energetic collisions, the entire impactor may be vaporized, leaving no meteorites. Geologists use the term, "bolide", in a different sense from astronomers to indicate a very large impactor . For example, the USGS uses the term to mean

1512-604: The atmosphere as a meteor and has impacted the ground. In 1961, the International Astronomical Union (IAU) defined a meteoroid as "a solid object moving in interplanetary space, of a size considerably smaller than an asteroid and considerably larger than an atom". In 1995, Beech and Steel, writing in the Quarterly Journal of the Royal Astronomical Society , proposed a new definition where

1566-417: The atmosphere head-on (which only occurs when meteors are in a retrograde orbit such as the Leonids , which are associated with the retrograde comet 55P/Tempel–Tuttle ) the combined speed may reach about 71 km/s (160,000 mph) (see Specific energy#Astrodynamics ). Meteoroids moving through Earth's orbital space average about 20 km/s (45,000 mph), but due to Earth's gravity meteors such as

1620-399: The atmosphere, and thus ionization trails can be found in the upper atmosphere more or less continuously. When radio waves are bounced off these trails, it is called meteor burst communications . Meteor radars can measure atmospheric density and winds by measuring the decay rate and Doppler shift of a meteor trail. Most meteoroids burn up when they enter the atmosphere. The left-over debris

1674-569: The cosmic origin of meteors was firmly established. Still, they remain an atmospheric phenomenon and retain their name "meteor" from the Greek word for "atmospheric". A fireball is a brighter-than-usual meteor that also becomes visible when about 100 km from sea level. The International Astronomical Union (IAU) defines a fireball as "a meteor brighter than any of the planets" ( apparent magnitude −4 or greater). The International Meteor Organization (an amateur organization that studies meteors) has

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1728-433: The early evening, increasing chances of eyewitness reports. This explains a part, but perhaps not all of the seasonal variation. Research is in progress for mapping the orbits of the meteors to gain a better understanding of the phenomenon. In a range of countries networks of sky observing installations have been set up to monitor meteors. A meteorite is a portion of a meteoroid or asteroid that survives its passage through

1782-486: The ecliptic is (in the northern hemisphere) high in the sky in the late afternoon and early evening. This means that fireball radiants with an asteroidal source are high in the sky (facilitating relatively high rates) at the moment the meteoroids "catch up" with Earth, coming from behind going in the same direction as Earth. This causes relatively low relative speeds and from this low entry speeds, which facilitates survival of meteorites. It also generates high fireball rates in

1836-919: The 💕 Look for Meteor (Schiff, 1902) on one of Misplaced Pages's sister projects : [REDACTED] Wiktionary (dictionary) [REDACTED] Wikibooks (textbooks) [REDACTED] Wikiquote (quotations) [REDACTED] Wikisource (library) [REDACTED] Wikiversity (learning resources) [REDACTED] Commons (media) [REDACTED] Wikivoyage (travel guide) [REDACTED] Wikinews (news source) [REDACTED] Wikidata (linked database) [REDACTED] Wikispecies (species directory) Misplaced Pages does not have an article with this exact name. Please search for Meteor (Schiff, 1902) in Misplaced Pages to check for alternative titles or spellings. You need to log in or create an account and be autoconfirmed to create new articles. Alternatively, you can use

1890-514: The generation of these sounds may partially explain them. For example, scientists at NASA suggested that the turbulent ionized wake of a meteor interacts with Earth's magnetic field , generating pulses of radio waves . As the trail dissipates, megawatts of electromagnetic power could be released, with a peak in the power spectrum at audio frequencies . Physical vibrations induced by the electromagnetic impulses would then be heard if they are powerful enough to make grasses, plants, eyeglass frames,

1944-452: The hearer's own body (see microwave auditory effect ), and other conductive materials vibrate. This proposed mechanism, although proven plausible by laboratory work, remains unsupported by corresponding measurements in the field. Sound recordings made under controlled conditions in Mongolia in 1998 support the contention that the sounds are real. (Also see Bolide .) A meteor shower is

1998-400: The heat of entry and force of impact. A noted 4-metre (13 ft) asteroid , 2008 TC 3 , was observed in space on a collision course with Earth on 6 October 2008 and entered Earth's atmosphere the next day, striking a remote area of northern Sudan. It was the first time that a meteoroid had been observed in space and tracked prior to impacting Earth. NASA has produced a map showing

2052-516: The horizon at the time), and collided head-on with Earth's atmosphere at 72 ± 6 km/s (161,000 ± 13,000 mph) vaporising more than 100 km (330,000 ft) above ground over a period of several seconds. When meteoroids intersect with Earth's atmosphere at night, they are likely to become visible as meteors . If meteoroids survive the entry through the atmosphere and reach Earth's surface, they are called meteorites . Meteorites are transformed in structure and chemistry by

2106-658: The light spectra of the resulting meteor. Their effects on radio signals also give information, especially useful for daytime meteors, which are otherwise very difficult to observe. From these trajectory measurements, meteoroids have been found to have many different orbits, some clustering in streams (see meteor showers ) often associated with a parent comet , others apparently sporadic. Debris from meteoroid streams may eventually be scattered into other orbits. The light spectra, combined with trajectory and light curve measurements, have yielded various compositions and densities, ranging from fragile snowball-like objects with density about

2160-628: The meteor breaks up into several fireballs traveling nearly parallel to the surface of Earth. A steadily growing number of fireballs are recorded at the American Meteor Society every year. There are probably more than 500,000 fireballs a year, but most go unnoticed because most occur over the ocean and half occur during daytime. A European Fireball Network and a NASA All-sky Fireball Network detect and track many fireballs. The entry of meteoroids into Earth's atmosphere produces three main effects: ionization of atmospheric molecules, dust that

2214-474: The meteor had a cosmic origin, but meteors did not attract much attention from astronomers until the spectacular meteor storm of November 1833. People all across the eastern United States saw thousands of meteors, radiating from a single point in the sky. Careful observers noticed that the radiant , as the point is called, moved with the stars, staying in the constellation Leo. The astronomer Denison Olmsted extensively studied this storm, concluding that it had

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2268-413: The meteoroid sheds, and the sound of passage. During the entry of a meteoroid or asteroid into the upper atmosphere , an ionization trail is created, where the air molecules are ionized by the passage of the meteor. Such ionization trails can last up to 45 minutes at a time. Small, sand-grain sized meteoroids are entering the atmosphere constantly, essentially every few seconds in any given region of

2322-565: The meteoroid versus the superheated air plasma, which its passage engenders: The sound generated by a meteor in the upper atmosphere, such as a sonic boom , typically arrives many seconds after the visual light from a meteor disappears. Occasionally, as with the Leonid meteor shower of 2001, "crackling", "swishing", or "hissing" sounds have been reported, occurring at the same instant as a meteor flare. Similar sounds have also been reported during intense displays of Earth's auroras . Theories on

2376-413: The most notable asteroid collisions with Earth and its atmosphere from 1994 to 2013 from data gathered by U.S. government sensors (see below). A meteor , known colloquially as a shooting star or falling star , is the visible passage of a glowing meteoroid , micrometeoroid , comet or asteroid through Earth's atmosphere, after being heated to incandescence by collisions with air molecules in

2430-402: The northern hemisphere's spring season. Although this phenomenon has been known for quite some time, the reason behind the anomaly is not fully understood by scientists. Some researchers attribute this to an intrinsic variation in the meteoroid population along Earth's orbit, with a peak in big fireball-producing debris around spring and early summer. Others have pointed out that during this period

2484-676: The original on 15 March 2023 . Retrieved 31 March 2024 . [REDACTED] [REDACTED] List of ships with the same or similar names This article includes a list of ships with the same or similar names. If an internal link for a specific ship led you here, you may wish to change the link to point directly to the intended ship article, if one exists. Retrieved from " https://en.wikipedia.org/w/index.php?title=List_of_ships_named_Meteor&oldid=1249989916 " Categories : Set index articles on ships Ship names Hidden categories: CS1 German-language sources (de) Articles with short description Short description

2538-549: The original meteorite, created or modified by an impact of a meteorite is called impactite . Solar System   → Local Interstellar Cloud   → Local Bubble   → Gould Belt   → Orion Arm   → Milky Way   → Milky Way subgroup   → Local Group → Local Sheet → Virgo Supercluster → Laniakea Supercluster   → Local Hole   → Observable universe   → Universe Each arrow ( → ) may be read as "within" or "part of". Meteor (Schiff, 1902) From Misplaced Pages,

2592-790: The original on 3 February 2024 . Retrieved 31 March 2024 . ^ "FS Meteor" (in German). Universität Hamburg. Archived from the original on 25 February 2014 . Retrieved 31 March 2024 . ^ https://www.nordsee-zeitung.de/Bremerhaven/Bau-des-Forschungsschiffs-Meteor-Werften-vereinen-ihr-Know-how-227974.html ^ " Meteor (1091097)" . Miramar Ship Index . Retrieved 2024-03-31 . ^ " Meteor (1143316)" . Miramar Ship Index . Retrieved 2024-03-31 . ^ " Meteor (5233535)" . Miramar Ship Index . Retrieved 2024-03-31 . ^ "Winged ships: Soviet hydrofoils forgotten and reborn" . Russia Beyond . Moscow. 11 September 2021. Archived from

2646-415: The result of an interaction between a planet, such as Earth, and streams of debris from a comet or other source. The passage of Earth through cosmic debris from comets and other sources is a recurring event in many cases. Comets can produce debris by water vapor drag, as demonstrated by Fred Whipple in 1951, and by breakup. Each time a comet swings by the Sun in its orbit , some of its ice vaporizes and

2700-403: The same fixed point in the sky is called a meteor shower . An estimated 25 million meteoroids, micrometeoroids and other space debris enter Earth's atmosphere each day, which results in an estimated 15,000 tonnes of that material entering the atmosphere each year. A meteorite is the remains of a meteoroid that has survived the ablation of its surface material during its passage through

2754-415: The significance of impact cratering was widely recognised, the terms cryptoexplosion or cryptovolcanic structure were often used to describe what are now recognised as impact-related features on Earth. Molten terrestrial material ejected from a meteorite impact crater can cool and solidify into an object known as a tektite . These are often mistaken for meteorites. Terrestrial rock, sometimes with pieces of

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2808-399: The size of a grain of sand, i.e. they are usually millimeter-sized or smaller. Meteoroid sizes can be calculated from their mass and density which, in turn, can be estimated from the observed meteor trajectory in the upper atmosphere. Meteors may occur in showers , which arise when Earth passes through a stream of debris left by a comet, or as "random" or "sporadic" meteors, not associated with

2862-473: The term synonymous with "fireball". Astronomers often use "bolide" to identify an exceptionally bright fireball, particularly one that explodes in a meteor air burst . They are sometimes called detonating fireballs. It may also be used to mean a fireball which creates audible sounds. In the late twentieth century, bolide has also come to mean any object that hits Earth and explodes, with no regard to its composition (asteroid or comet). The word bolide comes from

2916-551: The upper atmosphere, creating a streak of light via its rapid motion and sometimes also by shedding glowing material in its wake. Although a meteor may seem to be a few thousand feet from the Earth, meteors typically occur in the mesosphere at altitudes from 76 to 100 km (250,000 to 330,000 ft). The root word meteor comes from the Greek meteōros , meaning "high in the air". Millions of meteors occur in Earth's atmosphere daily. Most meteoroids that cause meteors are about

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