72:@0.058599:0.966559:0.074760:0.966559:0.074760:0.950779:0.058599:0.950779:0.000000:0.000000
Segunda ley de Kepler:@0.404235:0.084854:0.580251:0.084854:0.580251:0.067171:0.404235:0.067171:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
El radio vector de un planeta y el Sol barren áreas iguales en tiempos :@0.404235:0.101562:0.895840:0.101562:0.895840:0.085064:0.404235:0.085064:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
iguales.:@0.404235:0.118912:0.454804:0.118912:0.454804:0.102415:0.404235:0.102415:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
 :@0.414020:0.339338:0.416901:0.339338:0.416901:0.327861:0.414020:0.327861:0.000000
Figura 2.12.:@0.416901:0.339338:0.471380:0.339338:0.471380:0.327861:0.416901:0.327861:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
m:@0.822771:0.276229:0.835528:0.276229:0.835528:0.261923:0.822771:0.261923:0.000000
1:@0.835527:0.278889:0.839767:0.278889:0.839767:0.270549:0.835527:0.270549:0.000000
m:@0.823756:0.200528:0.836513:0.200528:0.836513:0.186223:0.823756:0.186223:0.000000
1:@0.836512:0.203188:0.840752:0.203188:0.840752:0.194848:0.836512:0.194848:0.000000
m:@0.458377:0.216477:0.471133:0.216477:0.471133:0.202171:0.458377:0.202171:0.000000
1:@0.471132:0.219137:0.475372:0.219137:0.475372:0.210797:0.471132:0.210797:0.000000
m:@0.458377:0.256133:0.471133:0.256133:0.471133:0.241828:0.458377:0.241828:0.000000
1:@0.471132:0.258793:0.475372:0.258793:0.475372:0.250453:0.471132:0.250453:0.000000
F:@0.542360:0.261014:0.549189:0.261014:0.549189:0.246709:0.542360:0.246709:0.000000
1:@0.549190:0.263674:0.553430:0.263674:0.553430:0.255334:0.549190:0.255334:0.000000
F:@0.755795:0.258906:0.762625:0.258906:0.762625:0.244600:0.755795:0.244600:0.000000
2:@0.762625:0.261566:0.766865:0.261566:0.766865:0.253226:0.762625:0.253226:0.000000
Δ:@0.849850:0.235035:0.859897:0.235035:0.859897:0.221161:0.849850:0.221161:0.000000
T:@0.859897:0.234813:0.868467:0.234813:0.868467:0.220508:0.859897:0.220508:0.000000
t  = 0:@0.843283:0.296729:0.876555:0.296725:0.876555:0.282420:0.843283:0.282424:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
0:@0.848265:0.299385:0.852505:0.299385:0.852505:0.291045:0.848265:0.291045:0.000000
t  = 0:@0.426391:0.203118:0.459651:0.203124:0.459651:0.188819:0.426391:0.188813:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
0:@0.431360:0.205783:0.435600:0.205783:0.435600:0.197443:0.431360:0.197443:0.000000
t  = x:@0.832916:0.182818:0.865522:0.182815:0.865522:0.168510:0.832916:0.168513:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
1:@0.837889:0.185475:0.842129:0.185475:0.842129:0.177135:0.837889:0.177135:0.000000
t  = x:@0.417968:0.267575:0.450582:0.267570:0.450582:0.253264:0.417968:0.253270:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
1:@0.422945:0.270229:0.427185:0.270229:0.427185:0.261889:0.422945:0.261889:0.000000
A:@0.787745:0.234486:0.797595:0.234486:0.797595:0.220181:0.787745:0.220181:0.000000
1:@0.797603:0.237149:0.801843:0.237149:0.801843:0.228809:0.797603:0.228809:0.000000
A:@0.514963:0.233084:0.524813:0.233084:0.524813:0.218779:0.514963:0.218779:0.000000
2:@0.524813:0.235745:0.529053:0.235745:0.529053:0.227405:0.524813:0.227405:0.000000
r:@0.605329:0.217193:0.610812:0.217193:0.610812:0.202888:0.605329:0.202888:0.000000
r:@0.779289:0.210969:0.784772:0.210969:0.784772:0.196663:0.779289:0.196663:0.000000
r:@0.775749:0.262528:0.781232:0.262528:0.781232:0.248223:0.775749:0.248223:0.000000
r:@0.608867:0.259187:0.614350:0.259187:0.614350:0.244882:0.608867:0.244882:0.000000
En la Figura 2.12., tenemos a un planeta de masa (:@0.404235:0.386661:0.772698:0.386661:0.772698:0.370163:0.404235:0.370163:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
m:@0.772698:0.386777:0.787494:0.386777:0.787494:0.370308:0.772698:0.370308:0.000000
1:@0.787447:0.390006:0.792153:0.390006:0.792153:0.380405:0.787447:0.380405:0.000000
) moviéndose :@0.792155:0.386661:0.895916:0.386661:0.895916:0.370163:0.792155:0.370163:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
alrededor del Sol. Al vector posición entre el planeta y el Sol en cual-:@0.404229:0.404012:0.891754:0.404012:0.891754:0.387514:0.404229:0.387514:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
quier instante lo denominamos  . :@0.404229:0.421362:0.644215:0.421362:0.644215:0.404865:0.404229:0.404865:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
r:@0.631288:0.421478:0.637318:0.421478:0.637318:0.405009:0.631288:0.405009:0.000000
Esta ley nos indica que si el planeta (:@0.404229:0.456064:0.672201:0.456064:0.672201:0.439566:0.404229:0.439566:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
m:@0.672201:0.456180:0.686997:0.456180:0.686997:0.439711:0.672201:0.439711:0.000000
1:@0.687000:0.459409:0.691706:0.459409:0.691706:0.449808:0.687000:0.449808:0.000000
) se mueve de la posición 1 :@0.691706:0.456064:0.895911:0.456064:0.895911:0.439566:0.691706:0.439566:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
a la 2, en un tiempo Δt, y en otro momento se mueve en el mismo :@0.404229:0.473415:0.896000:0.473415:0.896000:0.456917:0.404229:0.456917:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
tiempo :@0.404229:0.491011:0.460580:0.491011:0.460580:0.474514:0.404229:0.474514:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
Δt :@0.460773:0.491127:0.481849:0.491127:0.481849:0.474658:0.460773:0.474658:0.000000:0.000000:0.000000
de la posición 3 a la posición 4, las áreas correspondientes :@0.482042:0.491011:0.895950:0.491011:0.895950:0.474514:0.482042:0.474514:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
que barren el vector  , en un tiempo :@0.404229:0.508608:0.669597:0.508619:0.669597:0.492121:0.404229:0.492110:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
:@0.552842:0.498930:0.560397:0.498930:0.560397:0.482873:0.552842:0.482873:0.000000
r:@0.552579:0.508349:0.558347:0.508349:0.558347:0.492597:0.552579:0.492597:0.000000
Δt,:@0.668808:0.508735:0.688959:0.508735:0.688959:0.492266:0.668808:0.492266:0.000000:0.000000:0.000000
 son iguales. De la Figura 2.12.:@0.688959:0.508619:0.891745:0.508619:0.891745:0.492121:0.688959:0.492121:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
decimos que:    =:@0.404238:0.526216:0.537744:0.526221:0.537744:0.509724:0.404238:0.509718:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
A:@0.506824:0.526331:0.518094:0.526331:0.518094:0.509863:0.506824:0.509863:0.000000
1:@0.518089:0.529567:0.522795:0.529567:0.522795:0.519965:0.518089:0.519965:0.000000
 A:@0.537744:0.526337:0.553157:0.526337:0.553157:0.509868:0.537744:0.509868:0.000000:0.000000
2:@0.553157:0.529567:0.557863:0.529567:0.557863:0.519965:0.553157:0.519965:0.000000
.:@0.557862:0.526221:0.560617:0.526221:0.560617:0.509724:0.557862:0.509724:0.000000
Tercera ley o ley armónica:@0.404235:0.563075:0.612374:0.563075:0.612374:0.545392:0.404235:0.545392:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
Para cualquier planeta, el cuadrado de su período orbital es direc-:@0.404235:0.579782:0.891761:0.579782:0.891761:0.563285:0.404235:0.563285:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
tamente proporcional al cubo de la longitud del semieje mayor de :@0.404235:0.597133:0.895938:0.597133:0.895938:0.580635:0.404235:0.580635:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
órbita elíptica.:@0.404235:0.614484:0.505238:0.614484:0.505238:0.597986:0.404235:0.597986:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
k = :@0.536606:0.649301:0.564021:0.649301:0.564021:0.632832:0.536606:0.632832:0.000000:0.000000:0.000000:0.000000
        es constante de Kepler,:@0.564021:0.649185:0.759405:0.649185:0.759405:0.632688:0.564021:0.632688:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
donde::@0.404235:0.673664:0.453881:0.673664:0.453881:0.657167:0.404235:0.657167:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
T:@0.404235:0.708482:0.414041:0.708482:0.414041:0.692013:0.404235:0.692013:0.000000
 es el período del planeta, :@0.414041:0.708366:0.599195:0.708366:0.599195:0.691868:0.414041:0.691868:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
r:@0.404235:0.725832:0.410265:0.725832:0.410265:0.709364:0.404235:0.709364:0.000000
 es la distancia promedio al Sol.  :@0.410265:0.725717:0.639057:0.725717:0.639057:0.709219:0.410265:0.709219:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
Cuanto más alejados están los planetas del Sol, más lento se mueven.:@0.404235:0.760418:0.891759:0.760418:0.891759:0.743920:0.404235:0.743920:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
Las leyes se aplican a todos los planetas y cuerpos celestes que orbi-:@0.404235:0.777769:0.891711:0.777769:0.891711:0.761271:0.404235:0.761271:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
tan bajo la influencia de la gravedad.:@0.404235:0.795120:0.661828:0.795120:0.661828:0.778622:0.404235:0.778622:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
La importancia de las leyes de Kepler, entre otros aspectos, se debe :@0.404235:0.829821:0.895936:0.829821:0.895936:0.813323:0.404235:0.813323:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
a que estas definen la trayectoria y el movimiento de los planetas, :@0.404235:0.847172:0.895946:0.847172:0.895946:0.830674:0.404235:0.830674:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
asteroides y cometas alrededor del Sol, ya que la rapidez de los astros :@0.404235:0.864523:0.895836:0.864523:0.895836:0.848025:0.404235:0.848025:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
no es constante. Como su trayectoria es elíptica, cuando un astro está :@0.404235:0.881873:0.895880:0.881873:0.895880:0.865376:0.404235:0.865376:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
más cerca del Sol (perihelio), se mueve más rápido que cuando está :@0.404235:0.899224:0.895826:0.899224:0.895826:0.882727:0.404235:0.882727:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
más alejado (afelio).:@0.404235:0.916575:0.544272:0.916575:0.544272:0.900077:0.404235:0.900077:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
Archivo editorial:@0.906920:0.323581:0.906920:0.277277:0.895452:0.277277:0.895452:0.323581:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
Mira :@0.191333:0.188500:0.226461:0.188500:0.226461:0.173238:0.191333:0.173238:0.000000:0.000000:0.000000:0.000000:0.000000
el video: :@0.226320:0.188302:0.281779:0.188302:0.281779:0.173238:0.226320:0.173238:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
lynk.:@0.281639:0.188468:0.310602:0.188468:0.310602:0.173871:0.281639:0.173871:0.000000:0.000000:0.000000:0.000000:0.000000
ec/12f17:@0.153349:0.203556:0.204963:0.203556:0.204963:0.188959:0.153349:0.188959:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
Discútelo:@0.153344:0.330651:0.217090:0.330651:0.217090:0.315390:0.153344:0.315390:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
 en clase con tus :@0.217090:0.330453:0.327608:0.330453:0.327608:0.315390:0.217090:0.315390:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
compañeros.:@0.153344:0.346295:0.236965:0.346295:0.236965:0.331232:0.153344:0.331232:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
Competencia digital:@0.187773:0.161686:0.350462:0.161686:0.350462:0.144004:0.187773:0.144004:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
T:@0.568406:0.641603:0.578212:0.641603:0.578212:0.625134:0.568406:0.625134:0.000000
2:@0.578598:0.635135:0.583552:0.635135:0.583552:0.625517:0.578598:0.625517:0.000000
r:@0.570294:0.658953:0.576324:0.658953:0.576324:0.642485:0.570294:0.642485:0.000000
3:@0.576710:0.652486:0.581664:0.652486:0.581664:0.642868:0.576710:0.642868:0.000000
Shutterstock, 1724115913:@0.381872:0.860617:0.381872:0.789117:0.370403:0.789117:0.370403:0.860617:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
Competencia :@0.196294:0.565982:0.293917:0.565982:0.293917:0.550510:0.196294:0.550510:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
socioemocional:@0.196294:0.578550:0.306669:0.578550:0.306669:0.563078:0.196294:0.563078:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
La pasión de Johannes :@0.199880:0.603025:0.344748:0.603025:0.344748:0.587962:0.199880:0.587962:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
Kepler por la astronomía se ori-:@0.153337:0.618867:0.351575:0.618867:0.351575:0.603804:0.153337:0.603804:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
ginó de niño, al observar varios :@0.153337:0.634709:0.351869:0.634709:0.351869:0.619646:0.153337:0.619646:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
fenómenos cósmicos, como la :@0.153337:0.650551:0.348565:0.650551:0.348565:0.635488:0.153337:0.635488:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
llegada de un cometa en 1577 y :@0.153337:0.666393:0.357781:0.666393:0.357781:0.651330:0.153337:0.651330:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
el aparecimiento de un eclipse :@0.153337:0.682235:0.348759:0.682235:0.348759:0.667172:0.153337:0.667172:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
lunar, en 1580.:@0.153337:0.698077:0.242765:0.698077:0.242765:0.683014:0.153337:0.683014:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
¿Qué temas te han motivado a ti :@0.153344:0.877831:0.364737:0.877831:0.364737:0.862767:0.153344:0.862767:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
para seguir la carrera profesional :@0.153344:0.893673:0.359743:0.893673:0.359743:0.878609:0.153344:0.878609:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000
a la que aspiras? :@0.153344:0.909515:0.256965:0.909515:0.256965:0.894451:0.153344:0.894451:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000:0.000000