对火星轨道变化问题的最后解释(第1/10页)

作者君在作品相关中其实已经解释过这个问题。

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以下是文章内容：

long-term

integrations

and

stability

of

plaary

orbits

in

our

solar

system

abstract

we

present

the

results

of

very

long-term

numerical

integrations

of

plaary

orbital

tions

over

109

-yr

time-spans

inc露ding

all

nine

plas.

a

quick

inspection

of

our

numerical

data

shows

that

the

plaary

tion，

at

least

in

our

simple

dynamical

del，

seems

to

be

quite

stable

even

over

this

very

long

time-span.

a

closer

look

at

the

lowest-frequency

oscillations

using

a

low-pass

filter

shows

us

the

potentially

diffusive

character

of

terrestrial

plaary

tion，

especially

that

of

mercury.

the

behaviour

of

the

eentricity

of

mercury

in

our

integrations

is

qualitatively

similar

to

the

results

from

jacques

laskars

secular

perturbation

theory

(e.g.

emax～

0.35

over

～±

4

gyr).

however，

there

are

no

apparent

secular

increases

of

eentricity

or

inclination

in

any

orbital

elements

of

the

plas，

which

may

be

revealed

by

still

longer-term

numerical

integrations.

we

have

also

performed

a

couple

of

trial

integrations

inc露ding

tions

of

the

outer

five

plas

over

the

duration

of

±

5

x

1010

yr.

the

result

indicates

that

the

three

major

resonances

in

the

neptune–p露to

system

have

been

maintained

over

the

1011-yr

time-span.

1

introduction

1.1definition

of

the

problem

the

question

of

the

stability

of

our

solar

system

has

been

debated

over

several

混dred

years，

since

the

era

of

newton.

the

problem

has

attracted

many

faus

mathematicians

over

the

years

and

has

played

a

central

role

in

the

development

of

non-linear

dynamics

and

chaos

theory.

however，

we

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