Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Twin paradox
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
==Specific example== Consider a space ship traveling from Earth to the nearest star system: a distance {{nowrap|''d'' {{=}} 4 light}} years away, at a speed {{nowrap|''v'' {{=}} 0.8''c''}} (i.e., 80% of the speed of light). To make the numbers easy, the ship is assumed to attain full speed in a negligible time upon departure (even though it would actually take about 9 months accelerating at [[Standard gravity|1 ''g'']] to get up to speed). Similarly, at the end of the outgoing trip, the change in direction needed to start the return trip is assumed to occur in a negligible time. This can also be modelled by assuming that the ship is already in motion at the beginning of the experiment and that the return event is modelled by a [[Dirac delta]] [[Distribution (mathematics)|distribution]] acceleration.<ref name='Minguzzi' /> The parties will observe the situation as follows:<ref>{{cite book |title=Textbook Of Engineering Physics, Part I |first1=Mahesh C. |last1=Jain |publisher=PHI Learning Pvt |year=2009 |isbn=978-8120338623 |page=74 |url=https://books.google.com/books?id=DqZlU3RJTywC&pg=PA74}} [https://books.google.com/books?id=DqZlU3RJTywC&pg=PA74 Extract of page 74] </ref><ref>{{cite book |title=Introduction to Relativity |first1=P. L. |last1=Sardesai |publisher=New Age International |year=2004 |isbn=8122415202 |pages=27β28 |url=https://books.google.com/books?id=CX5GyYwnVLcC&pg=PA27}} [https://books.google.com/books?id=CX5GyYwnVLcC&pg=PA27 Extract of page 27] </ref> === Earth perspective === The Earth-based mission control reasons about the journey this way: the round trip will take {{nowrap|''t'' {{=}} 2''d''/''v'' {{=}} 10 years}} in Earth time (''i.e.'' everybody who stays on Earth will be 10 years older when the ship returns). The amount of time as measured on the ship's clocks and the aging of the travelers during their trip will be reduced by the factor <math>\alpha = \scriptstyle{\sqrt{1 - v^2/c^2}}</math>, the reciprocal of the [[Lorentz factor]] (time dilation). In this case {{nowrap|''Ξ±'' {{=}} 0.6}} and the travelers will have aged only {{nowrap|0.6 Γ 10 {{=}} 6 years}} when they return. === Travellers' perspective === The ship's crew members also calculate the particulars of their trip from their perspective. They know that the distant star system and the Earth are moving relative to the ship at speed ''v'' during the trip. In their rest frame the distance between the Earth and the star system is {{nowrap|''Ξ± d'' {{=}} 0.6 Γ 4 {{=}} 2.4 light}} years ([[length contraction]]), for both the outward and return journeys. Each half of the journey takes {{nowrap|''Ξ± d'' / ''v'' {{=}} 2.4 / 0.8 {{=}} 3 years}}, and the round trip takes twice as long (6 years). Their calculations show that they will arrive home having aged 6 years. The travelers' final calculation about their aging is in complete agreement with the calculations of those on Earth, though they experience the trip quite differently from those who stay at home. === Conclusion === {| class="wikitable" |+ Readings on Earth's and spaceship's clocks ! Event || Earth<br>(years) !! Spaceship<br>(years) |- | Departure || 0 || 0 |- | End of outgoing trip =<br>Beginning of ingoing trip || 5 || 3 |- | Arrival || 10 || 6 |} No matter what method they use to predict the clock readings, everybody will agree about them. If twins are born on the day the ship leaves, and one goes on the journey while the other stays on Earth, they will meet again when the traveler is 6 years old and the stay-at-home twin is 10 years old.
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)