Time

The measurement of time in KSP is kept according to both Earth and Kerbin-specific units. Hours, minutes, and seconds progress exactly as they would on Earth, whereas days are defined by Kerbin's rotation, resulting in a solar day of about six hours (sunset occurring at the third hour). Prior to version 0.23.5, the game relied on a timeline which measured days in Earth-time (1 day ≈ 24 hours) meaning a single day included three sunrises.

Mission time

During a mission, the time elapsed since launch is called Elapsed Time or MET for short. When clicking on the mission clock in the top left of GUI, you can switch between MET and Kerbin time elapsed since the beginning of the savegame.

Kerbin calendar

The following table outlines the orbital period and frequency of each celestial body in the Kerbol System. The following table calculates Earth Months as 365 days/12 months/year ≈ 30.4 days. A sidereal Kerbin day is 6 hours long, the Mun has an orbital period of 38.6 hours which defines a Kerbin month, and Kerbin has an orbital period of 2556.5 hours which defines a Kerbin year.

Celestial Body	Parent	Hours	Kerbin			Earth			Revolutions per Hour	Revolutions per Kerbin			Revolutions per Earth
			Days	Months	Years	Days	Months	Years		Day	Month	Year	Day	Month	Year
Moho	Kerbol	615.49	102.58	15.95	0.24	25.65	0.84	0.07	0.00	0.01	0.06	4.15	0.04	1.19	14.23
Eve	Kerbol	1571.7	261.95	40.72	0.61	65.49	2.15	0.18	0.00	0.00	0.02	1.63	0.02	0.46	5.57
Gilly	Eve	107.9	17.98	2.80	0.04	4.50	0.15	0.01	0.01	0.06	0.36	23.69	0.22	6.77	81.19
Kerbin	Kerbol	2556.50	426.08	66.23	1.00	106.52	3.50	0.29	0.00	0.00	0.02	1.00	0.01	0.29	3.43
Mun	Kerbin	38.60	6.43	1.00	0.02	1.61	0.05	0.00	0.03	0.16	1.00	66.23	0.62	18.91	226.94
Minmus	Kerbin	299.50	49.92	7.76	0.12	12.48	0.41	0.03	0.00	0.02	0.13	8.54	0.08	2.44	29.25
Duna	Kerbol	4809.80	801.63	124.61	1.88	200.41	6.59	0.55	0.00	0.00	0.01	0.53	0.00	0.15	1.82
Ike	Duna	18.20	3.03	0.47	0.01	0.76	0.02	0.00	0.05	0.33	2.12	140.47	1.32	40.11	481.32
Dres	Kerbol	13303.60	2217.27	344.65	5.20	554.32	18.22	1.52	0.00	0.00	0.00	0.19	0.00	0.05	0.66
Jool	Kerbol	29072.60	4845.43	753.18	11.37	1211.36	39.83	3.32	0.00	0.00	0.00	0.09	0.00	0.03	0.30
Laythe	Jool	14.70	2.45	0.38	0.01	0.61	0.02	0.00	0.07	0.41	2.63	173.91	1.63	49.66	595.92
Vall	Jool	29.43	4.91	0.76	0.01	1.23	0.04	0.00	0.03	0.20	1.31	86.87	0.82	24.80	297.66
Tylo	Jool	58.87	9.81	1.53	0.02	2.45	0.08	0.01	0.02	0.10	0.66	43.43	0.41	12.40	148.80
Bop	Jool	110.92	18.49	2.87	0.04	4.62	0.15	0.01	0.01	0.05	0.35	23.05	0.22	6.58	78.98
Pol	Jool	153.70	25.62	3.98	0.06	6.40	0.21	0.02	0.01	0.04	0.25	16.63	0.16	4.75	56.99
Eeloo	Kerbol	43608.90	7268.15	1129.76	17.06	1817.04	59.74	4.98	0.00	0.00	0.00	0.06	0.00	0.02	0.20

Phase angles

The phase angle determine the angular distance between two bodies around the same object. The phase angle of a body exactly on the other side of the central body is 180°. If the central body is on one side, and the two compared bodies are in line, the phase angle is 0°.

With the starting phase angles listed below it is possible to calculate the phase angle at any given moment. This information can be used to determine if both bodies are aligned for a transfer orbit. To calculate this value, the revolutions per second (RPS) for both bodies is required. This is the inverse of the orbital period:

$r={\frac {1}{p}}$

Where:

• $r$ is the revolutions per time unit
• $p$ is the orbital period in the time unit

Both time units are second for RPS

The phase angle change per second is then simply the subtraction of the origin from the target's planet RPS. This also tells when the current alignment repeat again, by inverting the phase angle change again. This time is called synodic orbital period.

$p_{\text{synodic}}=\left\vert {\frac {1}{{\frac {1}{p_{t}}}-{\frac {1}{p_{o}}}}}\right\vert$

Where:

• $p_{\text{synodic}}$ is the synodic orbital period
• $p_{t}$ is the sidereal orbital period of the targeted body
• $p_{o}$ is the sidereal orbital period of the original body

There are calculation tools available online which tell which is the best phase angle for an efficient transfer. Knowing this, the first alignment date can be calculated by first subtracting the starting phase angle from the desired phase angle. This gives the required first change with needs to be divided by the the phase angle change to determine how long it takes to get the first alignment.

Starting phase angles

The following table shows the phase angle in degrees and revolutions of each planet at the beginning of each game (UT = 0s).

Planet	Degrees	Revolutions
Moho	84.92°	0.23589
Eve	15.00°	0.04167
Duna	135.51°	0.37642
Jool	238.43°	0.66231
Dres	10.02°	0.02783
Eeloo	309.98°	0.86106

Example

The revolutions per second for Duna is:

$r={\frac {1}{17315400s}}=5.77520589\cdot 10^{-8}Hz$

The phase angle change per second relative to Kerbin is then:

$r_{\text{relative}}=r_{\text{Duna}}-r_{\text{Kerbin}}=-5.09017\cdot 10^{-8}Hz$

The optimal phase angle for a transfer from Kerbin to Duna is 0.12323 revolutions or 44.3628°. The starting phase angle is 0.37642 revolutions so the first time change required is -0.25319 revolutions.

$t_{0}={\frac {\beta }{r_{\text{relative}}}}={\frac {\beta }{r_{\text{Duna}}-r_{\text{Kerbin}}}}={\frac {-0.25319}{-5.09017\cdot 10^{-8}Hz}}=4974119s$

The transfer windows will then repeat periodically using the synodic period between both bodies:

$p_{\text{synodic}}=\left\vert {\frac {1}{{\frac {1}{p_{\text{Duna}}}}-{\frac {1}{p_{\text{Kerbin}}}}}}\right\vert =\left\vert {\frac {1}{-5.09017\cdot 10^{-8}Hz}}\right\vert =19645709s$

$t_{n}=t_{0}+n\cdot p_{\text{synodic}}$

See also

• Time warp