433 Eros

Template:Short description Template:About Template:Use dmy dates {{#invoke:infobox|infoboxTemplate | class = vcard | titleclass = fn org | title = 433 Eros | image = {{#invoke:InfoboxImage|InfoboxImage|image=Eros - PIA02923 (color).jpg|upright={{#if:||1.1}}|alt=}} | caption = Eros – composite image of the north polar region, with the craters Psyche above and Himeros below. The long ridge Hinks Dorsum, believed to be a thrust fault, can be seen snaking diagonally between them. The smaller crater in the foreground is Narcissus. Watters, (2011) | headerstyle = {{#if:#D6D6D6|background-color:#D6D6D6|background-color:#E0CCFF}} | labelstyle = max-width:{{#if:||11em}}; | autoheaders = y

| header1 = Discovery<ref name=JPLdata-2017-06-04/>

| header10 = {{#if:|Designations|Designations}}

| label11 = Template:Longitem | data11 = (433) Eros | label12 = Pronunciation | data12 = Template:IPAc-en<ref>Template:OED</ref> | label13 = Template:Longitem | data13 = {{#invoke:Lang|lang}}, Template:Transliteration<ref name=Schmadel-2007/> | label14 = Template:Longitem | data14 = Template:Hlist | label15 = Template:Longitem | data15 = Template:Hlist | label16 = Adjectives | data16 = Erotian Template:IPAc-en<ref>John Amabile (2016) Changing the Worlds: The For-Profit Plan to Mine Asteroids and Terraform Two Planets in One Human Lifetime</ref> | label17 = Symbol | data17 = File:Eros symbol (bold).svg (astrological)

| header20 = Orbital characteristics{{#ifeq:|yes| (barycentric)}}<ref name=JPLdata-2017-06-04/>

| data21 = | data22 = {{#if:4 September 2017 (JD 2458000.5) |Epoch 4 September 2017 (JD 2458000.5)}} | data23 = {{#if:0 | Uncertainty parameter 0}} | label24 = Observation arc | data24 = 53.89 yr (19,683 days) | label25 = Earliest precovery date | data25 = 29 October 1893 | label26 = {{#switch:{{{apsis}}} |apsis|gee|barion|center|centre|(apsis)=Apo{{{apsis}}} |Ap{{#if:|{{{apsis}}}|helion}}}} | data26 = 1.7825 AU | label27 = Peri{{#if:|{{{apsis}}}|helion}} | data27 = 1.1334 AU | label28 = Peri{{#if:|{{{apsis}}}|apsis}} | data28 = | label29 = {{#switch:{{{apsis}}} |helion|astron=Ap{{{apsis}}} |Apo{{#if:|{{{apsis}}}|apsis}}}} | data29 = | label30 = Periastron | data30 = | label31 = Apoastron | data31 = | label32 = Template:Longitem | data32 = 1.4579 AU | label33 = Template:Longitem | data33 = | label34 = Eccentricity | data34 = 0.2226 | label35 = Template:Longitem | data35 = 1.76 yr (643 days) | label36 = Template:Longitem | data36 = | label37 = Template:Longitem | data37 = | label38 = Template:Longitem | data38 = 71.280° | label39 = Template:Longitem | data39 = Template:Deg2DMS / day | label40 = Inclination | data40 = 10.828° | label41 = Template:Longitem | data41 = | label42 = Template:Longitem | data42 = 304.32° | label43 = Template:Longitem | data43 = | label44 = Template:Longitem | data44 = | label45 = Template:Longitem | data45 = 178.82° | label46 = Template:Nowrap | data46 = | label47 = Satellite of | data47 = | label48 = Group | data48 = | label49 = {{#switch: |yes|true=Satellites |Known satellites}} | data49 = | label50 = Star | data50 = | label51 = Earth MOID | data51 = 0.1505 AU (58.6 LD) | label52 = Mercury MOID | data52 = | label53 = Venus MOID | data53 = | label54 = Mars MOID | data54 = 0.2407 Template:Sc | label55 = Jupiter MOID | data55 = | label56 = Saturn MOID | data56 = | label57 = Uranus MOID | data57 = | label58 = Neptune MOID | data58 = | label59 = T_Jupiter | data59 =

| header60 = Proper orbital elements

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({{#expr:365.25*360/1 round 3}} d) }} | label66 = Template:Longitem | data66 = {{#if:|{{{perihelion_rate}}} arcsec Template:\yr }} | label67 = Template:Longitem | data67 = {{#if:|{{{node_rate}}} arcsec Template:\yr}}

| header70 = Template:Anchor{{#if:yes| Physical characteristics|Physical characteristics}}

| label71 = Dimensions | data71 = Template:Ubl | label72 = Template:Longitem | data72 = | label73 = Template:Longitem | data73 = | label74 = Template:Longitem | data74 = | label75 = Template:Longitem | data75 = | label76 = Flattening | data76 = | label77 = Circumference | data77 = | label78 = Template:Longitem | data78 = | label79 = Volume | data79 = | label80 = Mass | data80 = Template:Val<ref name=Yeomans-Antreas-etal-2000/> | label81 = Template:Longitem | data81 = Template:Val<ref name=JPLdata-2017-06-04/><ref name=Yeomans-Antreas-etal-2000/> | label82 = Template:Longitem | data82 = | label83 = Template:Longitem | data83 = | label84 = Template:Longitem | data84 = | label85 = Template:Longitem | data85 = 5.270 h<ref name=JPLdata-2017-06-04/> | label86 = Template:Longitem | data86 = | label87 = Template:Longitem | data87 = | label88 = Template:Longitem | data88 = | label89 = Template:Longitem | data89 = | label90 = Template:Longitem | data90 = | label91 = Template:Longitem | data91 = | label92 = Template:Longitem | data92 = | label93 = {{#if:yes |Template:Longitem |Albedo}} | data93 = Template:Val<ref name=JPLdata-2017-06-04/> | label94 = Temperature | data94 =

| data100 = {{#if:|

Surface temp.	min	mean	max
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{{{temp_name2}}}
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| header110 = Atmosphere

| below = {{#if:||Template:Reflist }}

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433 Eros is a stony asteroid of the Amor group, and the first discovered, and second-largest near-Earth object. It has an elongated shape and a volume-equivalent diameter of approximately Template:Convert. Visited by the NEAR Shoemaker space probe in 1998, it became the first asteroid ever studied from its own orbit.

The asteroid was discovered by German astronomer C. G. Witt at the Berlin Observatory on 13 August 1898 in an eccentric orbit between Mars and Earth. It was later named after Eros, a god from Greek mythology, the son of Aphrodite. He is identified with the planet Venus.<ref name=Schmadel-2007>Template:Cite book</ref>

HistoryEdit

DiscoveryEdit

Eros was discovered on 13 August 1898 by Carl Gustav Witt at Berlin Urania Observatory and Auguste Charlois at Nice Observatory<ref name=Scholl-Schmadel-2002/> and temporarily labeled D.Q.<ref>Template:Cite news Template:Open access</ref> Witt was taking a two-hour exposure of beta Aquarii to secure astrometric positions of asteroid 185 Eunike.<ref name=Yeomans-2014/>

NameEdit

Eros is named after the Greek god of love, Erōs. It was the first minor planet to be given a male name;<ref name=Schmadel-2007/> the break with earlier tradition was made because it was the first near-Earth asteroid discovered.

Later studiesEdit

During the opposition of 1900–1901, a worldwide program was launched to make parallax measurements of Eros to determine the solar parallax (or distance to the Sun), with the results published in 1910 by Arthur Hinks of Cambridge<ref name=Hinks-1909/> and Charles D. Perrine of the Lick Observatory, University of California.<ref name="Perrine1910" /> Perrine published progress reports in 1906<ref name=Perrine1906/> and 1908.<ref name=Perrine1908/> He took 965 photographs with the Crossley Reflector and selected 525 for measurement.<ref name=Campbell-1906/> A similar program was then carried out, during a closer approach, in 1930–1931 by Harold Spencer Jones.<ref name=Jones-1941/> The value of the Astronomical Unit (roughly the Earth-Sun distance) obtained by this program was considered definitive until 1968, when radar and dynamical parallax methods started producing more precise measurements.

Eros was the first asteroid detected by the Arecibo Observatory's radar system.<ref name=Butrica-1996/><ref name="AsteroidRadarAstronomy"/>

Eros was one of the first asteroids visited by a spacecraft, the first one orbited, and the first one soft-landed on. NASA spacecraft NEAR Shoemaker entered orbit around Eros in 2000, and landed in 2001.

Mars-crosserEdit

Eros is a Mars-crosser asteroid, the first known to come within the orbit of Mars. Its orbit is inclined at about 10.8° to the solar ecliptic, it is above the plane of the ecliptic when it crosses Mars' orbit, so the two orbits do not intersect. Objects in such an orbit can remain there for only a few hundred million years before the orbit is perturbed by gravitational interactions. Dynamical system modeling suggests that Eros may evolve into an Earth-crosser within as short an interval as two million years, and has a roughly 50% chance of doing so over a time scale of Template:10^~Template:10^ years.<ref name=Michel-Farin-Froesc-1996/> It is a potential Earth impactor,<ref name=Michel-Farin-Froesc-1996/> about five times larger than the impactor that created Chicxulub crater and led to the extinction of the non-avian dinosaurs.Template:Efn

NEAR Shoemaker survey and landingEdit

The NEAR Shoemaker probe visited Eros twice, first with a brief flyby in 1998, and then by orbiting it in 2000, when it extensively photographed its surface. On 12 February 2001, at the end of its mission, it landed on the asteroid's surface using its maneuvering jets.

This was the first time a Near Earth asteroid was closely visited by a spacecraft.<ref>Template:Cite magazine</ref>

Animation of NEAR Shoemaker trajectory.gif

Animation of NEAR Shoemaker trajectory from 19 February 1996 to 12 February 2001.Template:Hlist.
Animation of NEAR Shoemaker trajectory around 433 Eros.gif

Animation of NEAR Shoemaker Template:'s trajectory around 433 Eros from 1 April 2000 to 12 February 2001.
Template:Legend2 Template:·Template:Legend2

Physical characteristicsEdit

Surface gravity depends on the distance from a spot on the surface to the center of a body's mass. Eros's surface gravity varies greatly because Eros is not a sphere but an elongated peanut-shaped object. The daytime temperature on Eros can reach about Template:Convert at perihelion. Nighttime measurements fall near Template:Convert. Eros's density is 2.67 g/cm³, about the same as the density of Earth's crust.

NEAR scientists have found that most of the larger rocks strewn across Eros were ejected from a single crater in an impact approximately 1 billion years ago.<ref name=Thomas-Veverka-2001/> (The crater involved was proposed to be named "Shoemaker", but is not recognized as such by the International Astronomical Union (IAU), and has been formally designated Charlois Regio.) This event may also be responsible for the 40 percent of the Erotian surface that is devoid of craters smaller than 0.5 kilometers across. It was originally thought that the debris thrown up by the collision filled in the smaller craters. An analysis of crater densities over the surface indicates that the areas with lower crater density are within 9 kilometers of the impact point. Some of the lower density areas were found on the opposite side of the asteroid but still within 9 kilometers.<ref name=Thomas-Robinson-2005/>

It is thought that seismic shockwaves propagate through the asteroid, shaking smaller craters into rubble. Since Eros is irregularly shaped, parts of the surface antipodal to the point of impact can be within 9 kilometres of the impact point (measured in a straight line through the asteroid) even though some intervening parts of the surface are more than 9 kilometres away in straight-line distance. A suitable analogy would be the distance from the top centre of a bun to the bottom centre as compared to the distance from the top centre to a point on the bun's circumference: top-to-bottom is a longer distance than top-to-periphery when measured along the surface but shorter than it in direct straight-line terms.<ref name=Thomas-Robinson-2005/> Compression from the same impact is believed to have created the thrust fault Hinks Dorsum.<ref name=Watters-Thomas-2011/>

A phenomenon named dust ponds were discovered in the asteroid in October 2000. Dust ponds are a phenomenon where pockets of dust are seen in airless celestial bodies. These are smooth deposits of dust accumulated in depressions on the surface of the body (like craters), contrasting from the rocky terrain around them. <ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> They typically have different color and albedo compared to the surrounding areas. The asteroid contains lots of large craters more than 200 m in diameter. Their number is near to the saturation point of these craters. But craters smaller than that are relatively low. Suggesting that some process of erasure has covered them up. The floors of some craters are covered with smooth and flat areas (less than 10° slope). Such dust ponds are characterized by slightly bluer colour compared to the surrounding terrain. 334 of such ponds are identified, with a diameter of 10m. 255 of these are larger than 30m, and 231 (or 91%) are found within 30° from equator.

Data from the Near Earth Asteroid Rendezvous spacecraft collected on Eros in December 1998 suggests that it could contain 20 billion tonnes of aluminum and similar amounts of metals that are rare on Earth, such as gold and platinum.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

Visibility from EarthEdit

File:Eros path 2012.png

Path in sky during opposition 2011/2012

On 31 January 2012, Eros passed Earth at Template:Convert,<ref name=jpl-close/><ref name=NEODyS-close-2011/> about 70 times the distance to the Moon, with a visual magnitude of +8.1.<ref name=AstDys-Eros2012/> During rare oppositions, every 81 years, such as in 1975 and 2056, Eros can reach a magnitude of +7.0,<ref name=NEODys-Eros-2137/> which is brighter than Neptune and brighter than any main-belt asteroid except 1 Ceres, 4 Vesta and, rarely, 2 Pallas and 7 Iris. Under this condition, the asteroid actually appears to stop, but unlike the normal condition for a body in heliocentric conjunction with Earth, its retrograde motion is very small. For example, in January and February 2137, it moves retrograde only 34 minutes in right ascension.<ref name=JPLdata-2017-06-04/>

In popular cultureEdit

In the novel and television series The Expanse, a catastrophic science experiment is unleashed on a civilian population living within tunnels cut through Eros. This so-called "Eros Incident" ends with the asteroid mysteriously breaking its usual orbit and crashing into Venus.<ref>Template:Cite news</ref>

It makes an appearance in the novel (and its film adaptation) Ender's Game by Orson Scott Card, serving as a base for humanity and the location of Command School after having been captured from the invading aliens (the Formics) prior to the initial novel who had used the asteroid as their forward operating base in their previous invasion.<ref>Template:Cite book</ref>

In the Space Angel episode 'Visitors from Outer Space' (title text not quite matching narration), Scott McCloud and his crew are forced to destroy Eros by deflecting it into the Sun, after it becomes a hazard to spacecraft navigation.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

It is the setting for the entirety of the plot of the novel Captive Universe by Harry Harrison.

During Grant Morrison's relaunch of the Justice League, Eros was used to imprison the General after attacking the Justice League.<ref>JLA #24 (December 1998)</ref>

GalleryEdit

Eros rotation Dec. 3-4 2000.gif

Animation of the rotation of Eros
433eros.jpg

View from one end of Eros across the gouge on its side towards the opposite end
PIA02467 NEAR's First Whole-Eros Mosaic from Orbit.jpg

First mosaic image of Eros taken from an orbiting spacecraft
PIA02487 Glimpses into Eros' Shadows.jpg

Mosaic image of Eros
433 Eros first look.jpg

At Template:Convert across, the crater Psyche is Eros's second largest.
Erosregolith.jpg

Regolith of Eros, seen during NEAR's descent; area shown is about 12 meters (40 feet) across
Eros May 7 2013.PNG

Orbital diagram of Eros with locations on 7 May 2013
Eros orbit 2018.png

Orbital diagram of Eros with locations on 1 January 2018
Eros, Vesta and Ceres size comparison.jpg

Size comparison of Vesta, Ceres and Eros
PIA02475 Eros' Bland Butterscotch Colors.jpg

Six views of Eros in approximate natural color from NEAR-Shoemaker in February 2000
PIA02471 Eros in Stereo.jpg

Stereo image of Eros