Inertia and List of first black Major League Baseball players: Difference between pages

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Below is a list of the [[baseball color line|first]] [[Black people|black]] players in [[Major League Baseball]] by team and chronological order, since the abolition of the [[Baseball color line]]. During the 1880s, [[Moses Fleetwood Walker]] had played for Toledo of the [[American Association (19th century)|American Association]] (his brother [[Welday Walker]] also played a few games with the club), and it was essentially against Fleetwood Walker that the line was originally drawn.
{{quote|''The vis insita, or innate force of matter is a power of resisting, by which every body, as much as in it lies, endeavors to preserve in its present state, whether it be of rest, or of moving uniformly forward in a right line.<!--There is a citation in the text immediately preceding the quote.-->}}


{| class="wikitable"
In common usage, however, people may also use the term "inertia" to refer to an object's "amount of resistance to change in velocity" (which is quantified by its [[mass]]), and sometimes its [[momentum]], depending on context (e.g. "this object has a lot of inertia"). The term "inertia" is more properly understood as a shorthand for "the principle of inertia" as described by Newton in [[Newton's First Law of Motion]] which, expressed simply, says: "An object that is not subject to any outside forces moves at a constant velocity, covering equal distances in equal times along a straight-line path." In even simpler terms, inertia means "A body in motion tends to remain in motion, a body at rest tends to remain at rest." On the surface of the Earth the nature of inertia is often masked by the effects of [[friction]] which brings moving objects to rest relatively quickly unless they are coasting on wheels, well [[lubrication|lubricated]], or perhaps [[falling]] or going downhill (and thus being [[acceleration|accelerated]] by [[gravity]]). This is what misled classical theorists such as Aristotle who believed objects moved only so long as force was being applied to them.<ref>Pages 2 to 4, Section 1.1, "Skating", Chapter 1, "Things that Move", Louis Bloomfield, Professor of Physics at the University of Virginia, ''How Everything Works: Making Physics Out of the Ordinary'', John Wiley & Sons (2007), hardcover, 720 pages, ISBN 978-0-471-74817-5</ref>
!Player
!Team
!Date <ref>{{cite web |url=http://mlb.mlb.com/news/article.jsp?ymd=20070412&content_id=1895202&vkey=news_mlb&fext=.jsp&c_id=mlb |title=Robinson's many peers follow his lead |accessdate=2007-10-11 |author=O'Connell, Jack |date=2007-04-13 |work= |publisher=MLB.com}}</ref>
|-
|[[Jackie Robinson]]
|[[Los Angeles Dodgers|Brooklyn Dodgers]], NL
|April 15, 1947
|-
|[[Larry Doby]]
|[[Cleveland Indians]], AL
|July 5, 1947
|-
|[[Hank Thompson (baseball)|Hank Thompson]]
|[[Baltimore Orioles|St. Louis Browns]], AL
|July 17, 1947
|-
|[[Monte Irvin]]
|rowspan=2|[[San Francisco Giants|New York Giants]], NL
|rowspan=2|July 8, 1949
|-
|[[Hank Thompson (baseball)|Hank Thompson]]
|-
|[[Sam Jethroe]]
|[[Atlanta Braves|Boston Braves]], NL
|April 18, 1950
|-
|[[Minnie Miñoso]]
|[[Chicago White Sox]], AL
|May 1, 1951
|-
|[[Bob Trice]]
|[[Oakland Athletics|Philadelphia Athletics]], AL
|Sept. 13, 1953
|-
|[[Ernie Banks]]
|[[Chicago Cubs]], NL
|Sept. 17, 1953
|-
|[[Curt Roberts]]
|[[Pittsburgh Pirates]], NL
|April 13, 1954
|-
|[[Tom Alston]]
|[[St. Louis Cardinals]], NL
|April 13, 1954
|-
|[[Nino Escalera]]
|rowspan=2|[[Cincinnati Reds]], NL
|rowspan=2|April 17, 1954
|-
|[[Chuck Harmon]]
|-
|[[Carlos Paula]]
|[[Minnesota Twins|Washington Senators]], AL
|Sept. 6, 1954
|-
|[[Elston Howard]]
|[[New York Yankees]], AL
|April 14, 1955
|-
|[[John Kennedy (baseball 1957)|John Kennedy]]
|[[Philadelphia Phillies]], NL
|April 22, 1957
|-
|[[Ozzie Virgil, Sr.]]
|[[Detroit Tigers]], AL
|June 6, 1958
|-
|[[Pumpsie Green]]
|[[Boston Red Sox]], AL
|July 21, 1959
|}


Note: Teams are not listed again if they move to a new city. Also, since the beginning of expansion in 1961, all expansion teams have been integrated from their first game, so those teams are not listed.
==History and development of the concept==
===Early bsfdjgasghafoo


===Chinese theories===
==See also==
*[[History of baseball in the United States]]

*[[Negro league baseball]]
[[Mozi]] (Chinese: 墨子; pinyin: Mòzǐ; ca. 470 BCE–ca. 390 BCE), a philosopher who lived in China during the [[Hundred Schools of Thought]] period (early [[Warring States Period]]), composed or collected his thought in the book Mozi, which contains the following sentence: 'The cessation of motion is due to the opposing force ... If there is no opposing force ... the motion will never stop. This is as true as that an ox is not a horse.' which, according to Joseph Needham, is a precursor to Newton's first law of motion.
*[[List of Negro League baseball players]]

===Islamic theories===
{{main|Islamic physics}}

Several [[Islamic science|Muslim scientists]] from the [[Islamic Golden Age|medieval Islamic world]] wrote [[Arabic language|Arabic]] treatises on theories of [[Motion (physics)|motion]]. In the early 11th century, the Islamic scientist [[Ibn al-Haytham]] (Arabic: ابن الهيثم) ([[List of Latinised names|Latinized]] as ''Alhacen'') hypothesized that an object will move perpetually unless a force causes it to stop or change direction. Alhacen's model of motion thus bears resemblance to the law of inertia (now known as [[Newton's laws of motion|Newton's first law of motion]]) later stated by [[Galileo Galilei]] in the 16th century.<ref name=Salam>[[Abdus Salam]] (1984), "Islam and Science". In C. H. Lai (1987), ''Ideals and Realities: Selected Essays of Abdus Salam'', 2nd ed., World Scientific, Singapore, p. 179-213.</ref>

Alhacen's contemporary, the [[Persian people|Persian]] scientist [[Avicenna|Ibn Sina]] (Latinized as ''Avicenna'') developed an elaborate theory of motion, in which he made a distinction between the [[inclination]] and [[force]] of a [[projectile]], and concluded that motion was a result of an inclination (''mayl'') transferred to the projectile by the thrower, and that [[projectile motion]] in a vacuum would not cease.<ref name=Espinoza>Fernando Espinoza (2005). "An analysis of the historical development of ideas about motion and its implications for teaching", ''Physics Education'' '''40''' (2), p. 141.</ref> He viewed inclination as a permanent force whose effect is dissipated by external forces such as [[air resistance]].<ref>[[Aydin Sayili]] (1987), "Ibn Sīnā and Buridan virtue for non-natural motion."}}</ref> <ref name=Espinoza/> Avicenna also referred to ''mayl'' to as being proportional to [[weight]] times [[velocity]], which was similar to Newton's theory of [[momentum]].<ref>[[Aydin Sayili]] (1987), "Ibn Sīnā and Buridan on the Motion of the Projectile", ''Annals of the New York Academy of Sciences'' '''500''' (1), p. 477–482:
{{quote|"Thus he considered impetus as proportional to weight times velocity. In other words, his conception of impetus comes very close to the concept of momentum of Newtonian mechanics."}}</ref> Avicenna's concept of ''mayl'' was later used in [[Jean Buridan]]'s [[theory of impetus]].

[[Abū Rayhān al-Bīrūnī]] (973-1048) was the first physicist to realize that [[acceleration]] is connected with non-uniform motion.<ref name=Biruni>{{MacTutor|id=Al-Biruni|title=Al-Biruni}}</ref> The first scientist to reject Aristotle's idea that a constant force produces uniform motion was the Arabic Muslim physicist and philosopher [[Hibat Allah Abu'l-Barakat al-Baghdaadi]] in the early 12th century. He was the first to argue that a force applied continuously produces [[acceleration]], which is considered "the fundamental law of [[classical mechanics]]",<ref>{{cite encyclopedia
| last = Pines
| first = Shlomo
| title = Abu'l-Barakāt al-Baghdādī , Hibat Allah
| encyclopedia = [[Dictionary of Scientific Biography]]
| volume = 1
| pages = 26-28
| publisher = Charles Scribner's Sons
| location = New York
| date = 1970
| isbn = 0684101149
}}
<br>([[cf.]] Abel B. Franco (October 2003). "Avempace, Projectile Motion, and Impetus Theory", ''Journal of the History of Ideas'' '''64''' (4), p. 521-546 [528].)</ref> and vaguely foreshadows [[Newton's second law of motion]].

In the early 16th century, [[al-Birjandi]], in his analysis on the [[Earth's rotation]], developed a hypothesis similar to Galileo's notion of "circular inertia",<ref>{{Harv|Ragep|2001b|pp=63-4}}</ref> which he described in the following [[Experiment|observational test]]:

{{quote|"The small or large rock will fall to the Earth along the path of a line that is perpendicular to the plane (''sath'') of the horizon; this is witnessed by experience (''tajriba''). And this perpendicular is away from the tangent point of the Earth’s sphere and the plane of the perceived (''hissi'') horizon. This point moves with the motion of the Earth and thus there will be no difference in place of fall of the two rocks."<ref>{{Harv|Ragep|2001a|pp=152-3}}</ref>}}

===Theory of impetus===
{{main|Theory of impetus}}
{{seealso|Conactus}}

In the 14th century, [[Jean Buridan]] rejected the notion that a motion-generating property, which he named ''impetus'', dissipated spontaneously. Buridan's position was that a moving object would be arrested by the resistance of the air and the weight of the body which would oppose its impetus.<ref>Jean Buridan: Quaestiones on Aristotle's Physics (quoted at http://brahms.phy.vanderbilt.edu/a203/impetus_theory.html)</ref> Buridan also maintained that impetus increased with speed; thus, his initial idea of impetus was similar in many ways to the modern concept of [[momentum]]. Despite the obvious similarities to more modern ideas of inertia, Buridan saw his theory as only a modification to Aristotle's basic philosophy, maintaining many other [[peripatetic]] views, including the belief that there was still a fundamental difference between an object in motion and an object at rest. Buridan also maintained that impetus could be not only linear, but also circular in nature, causing objects (such as celestial bodies) to move in a circle.
Buridan's thought was followed up by his pupil [[Albert of Saxony (philosopher)|Albert of Saxony]] (1316-1390) and the [[Oxford Calculators]], who performed various experiments that further undermined the classical, Aristotelian view. Their work in turn was elaborated by [[Nicole Oresme]] who pioneered the practice of demonstrating laws of motion in the form of graphs.


The law of inertia states that it is the tendency of an object to resist a change in motion. According to Newton's words, an object will stay at rest and an object will stay in motion unless acted on by an outside force (e.g.,[[gravity]], [[friction]], [[matter]]).The Aristotelian division of motion into mundane and celestial became increasingly problematic in the face of the conclusions of [[Nicolaus Copernicus]] in the 16th century, who argued that the earth (and everything on it) was in fact never "at rest", but was actually in constant motion around the sun.<ref>[http://webexhibits.org/calendars/year-text-Copernicus.html Nicholas Copernicus: The Revolutions of the Heavenly Spheres], 1543</ref> [[Galileo]], in his further development of the Copernican model, recognized these problems with the then-accepted nature of motion and, at least partially as a result, included a restatement of Aristotle's description of motion in a void as a basic physical principle:

<blockquote>A body moving on a level surface will continue in the same direction at a constant speed unless disturbed.</blockquote>

It is also worth nothing that Galileo later went on to conclude that based on this initial premise of inertia, it is impossible to tell the difference between a moving object and a stationary one without some outside reference to compare it against.<ref>[http://webexhibits.org/calendars/year-text-Galileo.html Galileo: Dialogue Concerning the Two Chief World Systems], 1631 ([[Dialogue Concerning the Two Chief World Systems|Wikipedia Article]])</ref> This observation ultimately came to be the basis for [[Einstein]] to develop the theory of [[Special Relativity]].

Galileo's concept of inertia would later come to be refined and codified by [[Isaac Newton]] as the first of his [[Newton's laws of motion|Laws of Motion]] (first published in Newton's work, ''[[Philosophiae Naturalis Principia Mathematica]]'', in 1687):

<blockquote>Unless acted upon by an unbalanced force, an object will maintain a constant velocity.</blockquote>

Note that "velocity" in this context is defined as a [[vector (physics)|vector]], thus Newton's "constant velocity" implies both constant speed and constant direction (and also includes the case of zero speed, or no motion). Since initial publication, Newton's Laws of Motion (and by extension this first law) have come to form the basis for the almost universally accepted branch of [[physics]] now termed [[classical mechanics]].

The actual term "inertia" was first introduced by [[Johannes Kepler]] in his ''Epitome Astronomiae Copernicanae'' (published in three parts from 1618-1621); however, the meaning of Kepler's term (which he derived from the Latin word for "idleness" or "laziness") was not quite the same as its modern interpretation. Kepler defined inertia only in terms of a resistance to movement, once again based on the presumption that rest was a natural state which did not need explanation. It was not until the later work of Galileo and Newton unified rest and motion in one principle that the term "inertia" could be applied to these concepts as it is today.

Nevertheless, despite defining the concept so elegantly in his laws of motion, even Newton did not actually use the term "inertia" to refer to his First Law. In fact, Newton originally viewed the

===Relativity===

[[Albert Einstein]]'s theory of [[Special Relativity]], as proposed in his 1905 paper, "On the Electrodynamics of Moving Bodies," was built on the understanding of inertia and [[inertial reference frames]] developed by Galileo and Newton. While this revolutionary theory did significantly change the meaning of many Newtonian concepts such as [[mass]], [[energy]], and [[distance]], Einstein's concept of inertia remained unchanged from Newton's original meaning (in fact the entire theory was based on Newton's definition of inertia). However, this resulted in a limitation inherent in Special Relativity that it could only apply when reference frames were ''inertial'' in nature (meaning when no acceleration was present). In an attempt to address this limitation, Einstein proceeded to develop his theory of [[General Relativity]] ("The Foundation of the General Theory of Relativity," 1916), which ultimately provided a unified theory for both ''inertial'' and ''noninertial'' (accelerated) reference frames. However, in order to accomplish this, in General Relativity Einstein found it necessary to redefine several fundamental aspects of the universe (such as gravity) in terms of a new concept of "curvature" of [[spacetime]], instead of the more traditional system of forces understood by Newton.

As a result of this redefinition, Einstein also redefined the concept of "inertia" in terms of [[geodesic deviation]] instead, with some subtle but significant additional implications. The result of this is that according to General Relativity, when dealing with very large scales, the traditional Newtonian idea of "inertia" does not actually apply, and cannot necessarily be relied upon. Luckily, for sufficiently small regions of spacetime, the Special Theory can still be used, in which inertia still means the same (and works the same) as in the classical model. Towards the end of his life it seems as if Einstein had become convinced that ''space-time'' is a new form of [[Luminiferous aether|aether]], in some way serving as a reference frame for the property of inertia<ref>Kostro, Ludwik; ''Einstein and the Ether'' Montreal, Apeiron (2000). ISBN 0-9683689-4-8</ref>.

Another profound, perhaps the most well-known, conclusion of the theory of Special Relativity was that energy and mass are not separate things, but are, in fact, interchangeable. This new relationship, however, also carried with it new implications for the concept of inertia. The logical conclusion of Special Relativity was that if mass exhibits the principle of inertia, then inertia must also apply to energy as well. This theory, and subsequent experiments confirming some of its conclusions, have also served to radically expand the definition of inertia in some contexts to apply to a much wider context including energy as well as matter.

==Interpretations==
===According to Isaac Asimov===
According to [[Isaac Asimov]] in "Understanding Physics": "This tendency for motion (or for rest) to maintain itself steadily unless made to do otherwise by some interfering force can be viewed as a kind of "laziness," a kind of unwillingness to make a change. And indeed, [[Isaac Newton|Newton's]] [[Newton's first law of motion|first law of motion ]]
as [[Isaac Asimov]] goes on to explain, "Newton's laws of motion represent assumptions and definitions and are not subject to proof. In particular, the notion of 'inertia' is as much an assumption as Aristotle's notion of 'natural place.'...To be sure, the new relativistic view of the universe advanced by Einstein makes it plain that in some respects Newton's laws of motion are only approximations...At ordinary velocities and distance, however, the approximations are extremely good."

=== Mass and 'inertia' ===

[[Physics]] and [[mathematics]] appear to be less inclined to use the original concept of inertia as

:<math>P = mv</math>

The factor ''m'' is referred to as [[inertial mass]].

But mass as related to 'inertia' of a body can be defined also by the formula:

:<math>F = ma</math>

By this formula, the greater its mass, the less a body accelerates under given force. Masses <math>m</math> defined by the formula (1) and (2) are equal because the formula (2) is a consequence of the formula (1) if mass does not depend on time and speed. Thus, "mass is the quantitative or numerical measure of body’s inertia, that is of its resistance to being accelerated".

This meaning of a ''body's inertia'' therefore is altered from the original meaning as "a tendency to maintain momentum" to a description of the measure of how difficult it is to change the momentum of a body.

=== Inertial mass ===
The only difference there appears to be between inertial mass and gravitational mass is the method used to determine them.

[[Gravitational mass]] is measured by comparing the force of gravity of an unknown mass to the force of [[gravity]] of a known mass. This is typically done with some sort of balance scale. The beauty of this method is that no matter where, or on what planet you are, the masses will always balance out because the gravitational acceleration on each object will be the same. This does break down near supermassive objects such as black holes and neutron stars due to the high gradient of the gravitational field around such objects.

Inertial mass is found by applying a known force to an unknown mass, measuring the acceleration, and applying Newton's Second Law, '''m = F/a'''. This gives an accurate value for mass, limited only by the accuracy of the measurements. When astronauts need to be weighed in outer space, they actually find their inertial mass in a special chair.

The interesting thing is that, physically, no difference has been found between gravitational and inertial mass. Many experiments have been performed to check the values and the experiments always agree to within the margin of error for the experiment. [[Einstein]] used the fact that gravitational and inertial mass were equal to begin his [[Theory of General Relativity]] in which he postulated that gravitational mass was the same as inertial mass, and that the acceleration of gravity is a result of a 'valley' or slope in the [[space-time continuum]] that masses 'fell down' much as pennies spiral around a hole in the common donation toy at a chain store.

Since Einstein used inertial mass to describe [[Special Relativity]], inertial mass is closely related to [[relativistic mass]] and is therefore different from [[rest mass]].

=== Inertial frames ===
In a location such as a steadily moving railway carriage, a dropped ball (as seen by an observer in the carriage) would behave as it would if it were dropped in a stationary carriage. The ball would simply descend vertically. It is possible to ignore the motion of the carriage by defining it as an [[inertial frame]]. In a moving but non-accelerating frame, the ball behaves normally because the train and its contents continue to move at a constant velocity. Before being dropped, the ball was traveling with the train at the same speed, and the ball's inertia ensured that it continued to move in the same speed and direction as the train, even while dropping. Note that, here, it is inertia which ensured that, not its mass.

In an [[inertial frame]] all the observers in uniform (non-accelerating) motion will observe the same laws of physics. However observers in another inertial frame can make a simple, and intuitively obvious, transformation (the [[Galilean transformation]]), to convert their observations. Thus, an observer from outside the moving train could deduce that the dropped ball within the carriage fell vertically downwards.

However, in frames which are experiencing acceleration (''non-inertial frames''), objects appear to be affected by ''[[fictitious force]]s''. For example, if the railway carriage was accelerating, the ball would not fall vertically within the carriage but would appear to an observer to be deflected because the carriage and the ball would not be traveling at the same speed while the ball was falling. Other examples of fictitious forces occur in rotating frames such as the earth. For example, a missile at the North Pole could be aimed directly at a location and fired southwards. An observer would see it apparently deflected away from its target by a force (the [[Coriolis effect|Coriolis force]]) but in reality the southerly target has moved because earth has rotated while the missile is in flight. Because the earth is rotating, a useful inertial frame of reference is defined by the stars, which only move imperceptibly during most observations.

In summary, the principle of inertia is intimately linked with the principles of [[conservation of energy]] and [[Momentum#Conservation of momentum|conservation of momentum]].

==Rotational inertia==
Another form of inertia is ''rotational inertia'' (→ [[moment of inertia]]), which refers to the fact that a rotating rigid body maintains its state of uniform [[rotation]]al motion. Its [[angular momentum]] is unchanged, unless an external [[torque]] is applied; this is also called conservation of angular momentum. Rotational inertia often has hidden practical consequences.



==Notes==
{{reflist|2}}


==References==
==References==
{{reflist}}
*{{Harvard reference
|last=Ragep
|first=F. Jamil
|year=2001a
|title=Tusi and Copernicus: The Earth's Motion in Context
|journal=Science in Context
|volume=14
|issue=1-2
|pages=145–163
|publisher=[[Cambridge University Press]]
}}
*{{Harvard reference
|last=Ragep
|first=F. Jamil
|year=2001b
|title=Freeing Astronomy from Philosophy: An Aspect of Islamic Influence on Science
|journal=Osiris, 2nd Series
|volume=16
|issue=Science in Theistic Contexts: Cognitive Dimensions
|pages=49-64 & 66-71
}}

==External links==
*[http://www.bigs.de/en/shop/htm/flug01.html Inertia (animation)]
*[http://www.seop.leeds.ac.uk/entries/buridan/ ''Jean Buridan'' Stanford Encyclopaedia of Philosophy]
*[http://www.geom.uiuc.edu/education/calc-init/static-beam/mnt-derive.html Inertia Formula]

==Books and papers==

*Butterfield, H (1957) ''The Origins of Modern Science'' ISBN 0-7135-0160-X
*Clement, J (1982) "Students' preconceptions in introductory mechanics", ''American Journal of Physics'' vol 50, pp66-71
*Crombie, A C (1959) ''Medieval and Early Modern Science'', vol 2
*McCloskey, M (1983) "Intuitive physics", ''Scientific American'', April, pp114-123
*McCloskey, M & Carmazza, A (1980) "Curvilinear motion in the absence of external forces: naïve beliefs about the motion of objects", ''Science'' vol 210, pp1139-1141
*Masreliez, C.J., [http://www.iop.org/EJ/abstract/1402-4896/75/1/019/ ''Motion, Inertia and Special Relativity – a Novel Perspective,''] [[Physica Scripta]], (dec 2006)

{{Physics-footer}}

[[Category:Classical mechanics]]
[[Category:Introductory physics]]


{{Negro League teams}}
<!-- interwiki -->


[[Category:Negro league baseball players| ]]
[[ar:عطالة]]
[[Category:Lists of Major League Baseball players|First black Major League Baseball players by team and date]]
[[ast:Inercia]]
[[Category:Baseball lore|First black Major League Baseball players by team and date]]
[[be:Інерцыя]]
[[bs:Inercija]]
[[bg:Инертност]]
[[ca:Moment d'inèrcia]]
[[cs:Setrvačnost]]
[[da:Inerti]]
[[de:Trägheit]]
[[et:Inerts]]
[[el:Αδράνεια]]
[[es:Inercia]]
[[eo:Leĝoj de Newton pri movado#La unua leĝo de Newton pri movado: Leĝo de Inercio]]
[[fr:Inertie]]
[[ko:관성]]
[[hr:Tromost]]
[[io:Inerteso]]
[[is:Tregða]]
[[it:Inerzia]]
[[he:עקרון ההתמדה]]
[[la:Inertia]]
[[lv:Inerce]]
[[ms:Inersia]]
[[nl:Traagheid]]
[[ja:慣性]]
[[no:Treghet]]
[[nov:Inertia]]
[[pl:Bezwładność]]
[[pt:Inércia]]
[[ro:Inerţie (fizică)]]
[[ru:Закон инерции]]
[[simple:Inertia]]
[[sk:Zotrvačnosť]]
[[sl:Vztrajnost]]
[[sr:Инерција]]
[[sv:Tröghet]]
[[vi:Quán tính]]
[[tr:Eylemsizlik]]
[[uk:Інерція]]
[[zh:惯性原理]]

Revision as of 19:10, 10 October 2008

Below is a list of the first black players in Major League Baseball by team and chronological order, since the abolition of the Baseball color line. During the 1880s, Moses Fleetwood Walker had played for Toledo of the American Association (his brother Welday Walker also played a few games with the club), and it was essentially against Fleetwood Walker that the line was originally drawn.

Player Team Date [1]
Jackie Robinson Brooklyn Dodgers, NL April 15, 1947
Larry Doby Cleveland Indians, AL July 5, 1947
Hank Thompson St. Louis Browns, AL July 17, 1947
Monte Irvin New York Giants, NL July 8, 1949
Hank Thompson
Sam Jethroe Boston Braves, NL April 18, 1950
Minnie Miñoso Chicago White Sox, AL May 1, 1951
Bob Trice Philadelphia Athletics, AL Sept. 13, 1953
Ernie Banks Chicago Cubs, NL Sept. 17, 1953
Curt Roberts Pittsburgh Pirates, NL April 13, 1954
Tom Alston St. Louis Cardinals, NL April 13, 1954
Nino Escalera Cincinnati Reds, NL April 17, 1954
Chuck Harmon
Carlos Paula Washington Senators, AL Sept. 6, 1954
Elston Howard New York Yankees, AL April 14, 1955
John Kennedy Philadelphia Phillies, NL April 22, 1957
Ozzie Virgil, Sr. Detroit Tigers, AL June 6, 1958
Pumpsie Green Boston Red Sox, AL July 21, 1959

Note: Teams are not listed again if they move to a new city. Also, since the beginning of expansion in 1961, all expansion teams have been integrated from their first game, so those teams are not listed.

See also

References

  1. ^ O'Connell, Jack (2007-04-13). "Robinson's many peers follow his lead". MLB.com. Retrieved 2007-10-11.
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