No, we worry about a global energy equilibrium being rapidly moved in a single direction.
Do those phases oscillate about some sort of consistent mean?
The escape velocity at earth’s distance is about 42 km/second
From Escape velocity - Wikipedia
The earth is currently at 30 km/sec
The cheapest way is to boost the earths mass up 12 km/second pro-grade (directly in the line of the orbit - actually instantaneous pro-grade… as you apply the acceleration you keep it in the actual direction of movement. ) … Its more expensive to do it by applying the force in some other direction than pro-grade…
Your other question sure reduce the mass of the sun to make the escape velocity (kinetic energy) lesser… changes the orbit of the earth too
When the Sun leaves the Main sequence it will star losing mass comparatively rapidly, due to a vastly increased solar wind. Some estimates say that this loss will be enough to move the Earth’s orbit out beyond the edge of the Sun’s red giant phase; others aren’t so sure.
http://www.astronomy.ohio-state.edu/~pogge/Lectures/vistas97.html
By that stage the Earth will have lost its magnetic field due to cooling of the core, so it may no longer have an atmosphere.
Well, that would take care of the “season’s issue”. You should collect $3.
[quote=“Jonathan_Chance, post:20, topic:757193”]
Two things:
- What is the amount of energy required to move the Earth in such a manner?
From here:
I suppose if you were working very long time scales and could engineer some sort of mass that would stay at a constant distance from the Earth you could, eventually, shift the orbit outward…but we’d probably be talking millions of years (or 10’s of millions of years), and today there is no practical way to even start working on something like that…especially if we were wanting to live through the experience.
Note that you wouldn’t have to accelerate the Earth to escape velocity in order to move it outwards by a few miilion kilometres. Although the energy required would still be vast.
According to current theories the ice ages on our planet are significantly affected by minor changes in the eccentricity of our orbit; changing the shape of our orbit artificially would certainly cause some very significant changes in our climate.
This is happening right now, but the rate of solar mass loss is so low that it’s pretty negligable. AIUI, the Earth is currently moving away from the Sun about 15 cm/year, but most of that is due to tidal drag.
…I fail to see the relevance of that image to anything in the quoted post or to the thread in general.
There used to be a website that showed the effect of a passing star on the inner planets. I can’t find it now.
How is this made manifest in the elliptical orbit?
This one ROGUE STAR ?
Not really sure. The annual increase (15 cm/year) was calculated by a couple Russians (Gregoriy A. Krasinsky and Victor A. Brumberg) using (I think) timing of comunications to interplanetary probes. This paper says that it is probably due to tidal drag. I’m going to guess that it mainly shows up in a change in the semi-major axis.
Semi-major- does that mean the orbit becomes more elliptical with time?
It would if my guess were right. But after thinking it over, I realized that it’s wrong. Since tidal drag is a slow continuous process, it should show up as an increase everywhere along the orbit.