M700 Survey Scanner

M700 Survey Scanner
Scanner by Experimental Engineering Group
Radial size		Small, Radial mounted
Cost	(total)	1 500.00
Mass	(total)	0.200 t
Drag		0.2
Max. Temp.		2000 K
Impact Tolerance		7 m/s
Research		Scanning Tech
Unlock cost		4 500
Since version		1.0
Part configuration		SurveyScanner.cfg
Mode		Orbital
Resource		All
Scanning time		5 s
Science bonus		10
Min. Altitude		25 000 m
Max. Altitude		1 500 000 m
Packed volume		None

The M700 Survey Scanner is an orbital low resolution resource scanner. It provides a low-detail map of an entire celestial body's resource concentration. This can then be used to target specific areas for further scanning with the higher-resolution M4435 Narrow-Band Scanner or Surface Scanning Module.

Note that in the stock game, the only resource to scan for is Ore. Some mods add other resources; the orbital scan works similarly for these.

Product description

“

This orbital survey scanner uses a combination of advanced sensor technology and witchcraft to provide information on a planet or moons natural resources. These images can be viewed either in flight, or in relative safety and comfort back at the KSC. Be sure to bring an antenna capable of transmitting the information back, and sufficient power. — Experimental Engineering Group

”

Usage

Deployed for operation

Once the scanner is in a polar orbit between specific altitudes (see below), it must be opened (Deploy Scanner), and then the scan can be performed (Perform orbital survey). Rather than taking half a sidereal day, which would be more realistic, a scan of the entire body is completed instantly. This generates a large amount of data, which the scanner does not store but rather attempts to transmit immediately, requiring an antenna, a CommNet connection to KSC, and a substantial amount of energy (see below).

A successfully transmitted orbital scan earns 10 science points, and counts as a science broadcast in terms of "world's firsts" (that is, if you perform a resource scan before transmitting any other science data from that celestial body, you will receive a "We have transmitted our first science from X" accomplishment.)

The scan is a once per body operation. After the scan, the scanner can be retracted to its folded position, and either left in place as a polar relay satellite (if it has a relay antenna), sent to scan another body (if enough fuel remains for the transfer), or destroyed.

The Mun in false color after completing an orbital survey

The resource map resulting from the scan is displayed as an overlay on the view of the planet, either while controlling any craft, or in the Tracking Station. If controlling the scanner while it is deployed, the overlay can be toggled by right-clicking the scanner and selecting Toggle Overlay; if you retract the scanner, the resource view is automatically turned off. Otherwise, to toggle the overlay, center the map view on the celestial body and then click on the Resources icon on the right hand side of the window. There are options for changing the presentation of this information: you can modify the displayed color, style, and cutoff point (the minimum resource concentration shown).

Because the scanner is lightweight, a final stage for establishing the needed orbit can be small, with e.g. a FL-T200 and Spark for propulsion. Transmitting the scan will also require a sufficiently strong antenna and battery storage for the transmission. Since the scanner is bulky and not a good aerodynamic shape, the launch vehicle should use a fairing or cargo bay to avoid high drag and possible loss of control.

Scanning orbit requirements

The scanner can only perform an orbital survey if in a stable polar orbit between 80° and 100° at medium altitude.

Celestial body	Radius	Altitude
		Min.	Max.
Kerbol	261.6 Mm	N/A	N/A
Moho	250 km	25 km	1.25 Mm
Eve	700 km	70 km	1.5 Mm
Gilly	13 km	25 km	65 km
Kerbin	600 km	60 km	1.5 Mm
Mun	200 km	25 km	1000 km
Minmus	60 km	25 km	300 km
Duna	320 km	32 km	1.5 Mm
Ike	130 km	25 km	650 km
Dres	138 km	25 km	690 km
Jool	6 Mm	600 km	1.5 Mm
Laythe	500 km	50 km	1.5 Mm
Vall	300 km	30 km	1.5 Mm
Tylo	600 km	60 km	1.5 Mm
Bop	65 km	25 km	325 km
Pol	44 km	25 km	220 km
Eeloo	210 km	25 km	1.05 Mm

The minimum and maximum scanning altitudes are based on the radius of the body it is scanning:

• The minimum altitude is one-tenth of the body radius or 25 km, whichever is higher.
• The maximum altitude is five times the body radius or 1.5 Mm, whichever is lower.

Reaching a polar orbit

There are three ways to establish a polar orbit: by launching into that orbit from the surface, by adjusting course before entering the body's sphere of influence (and subsequent orbital insertion burn), or via a plane change maneuver.

Since plane change maneuvers are costly, it is usually preferable to avoid or minimize them. When scanning Kerbin, it is best to launch your rocket into the 90° plane. For other bodies, you can use a mid-course correction to move your closest approach above one of the poles, then perform insertion burn there.

If you have already established another orbit, a plane change maneuver will be required to use the scanner. It takes less energy to perform plane change maneuvers at high altitudes, due to the decreased orbital velocity. Additionally, eccentric orbits have a much lower orbital velocity at apoapsis than circular orbits of the same altitude.

For sufficiently large inclination changes, using three maneuvers rather than a single plane change maneuver can save delta-v, at the cost of time. (For circular initial and target orbits, the crossover point is 37° of inclination change.) An initial prograde burn at periapsis raises apoapsis, a cheaper plane change burn is performed at the apoapsis of the resulting eccentric orbit, then a retrograde burn at periapsis brings the apoapsis back down to the target altitude.

The most costly case is starting in an equatorial orbit and adjusting inclination directly to 90° with a single burn. The following table shows the delta-v required to make such a 90° turn at the minimum and maximum operational altitudes for the M700. The last column shows the delta-v required if the turn is made at apoapsis while in an eccentric orbit bounded by the minimum and maximum operational altitudes.

Planet	Min. altitude	Delta v	Max. altitude	Delta v	Eccentric Delta v
Moho	25km	1107.4m/s	1250km	474.1m/s	263.9m/s
Eve	70km	4607.2m/s	1500km	2725.6m/s	1962.3m/s
Gilly	25km	20.9m/s	65km	14.6m/s	11.8m/s
Kerbin	60km	3721.6m/s	1500km	1834.1m/s	1268.3m/s
Mun	25km	760.9m/s	1000km	329.5m/s	185.2m/s
Minmus	25km	203.8m/s	300km	99.1m/s	61.2m/s
Duna	32km	1308.6m/s	1500km	575.5m/s	327.6m/s
Ike	25km	489.5m/s	650km	218.2m/s	125.6m/s
Dres	25km	513.4m/s	690km	227.8m/s	130.7m/s
Jool	600km	9252.4m/s	1500km	8679.5m/s	8398.1m/s
Laythe	50km	2671.1m/s	1500km	1400.7m/s	920.0m/s
Vall	30km	1121.4m/s	1500km	480.2m/s	267.3m/s
Tylo	60km	2925.9m/s	1500km	1640.3m/s	1134.4m/s
Bop	25km	235.1m/s	325km	112.9m/s	69.2m/s
Pol	25km	144.6m/s	220km	73.9m/s	47.6m/s
Eeloo	25km	795.8m/s	1050km	343.7m/s	192.7m/s

Electricity and time required

Each body generates a certain amount of data when scanned, measured in Mits. The data size correlates with the size of the body; Jool produces the most—1200 Mits—and Gilly the least—just 3 Mits. Roughly, the amount of data required for a survey is .205 mits per radial kilometer.

As with any science transmission:

• More data requires more time and electricity to transmit, and different antennas have different speeds and efficiencies.
• Though having multiple antennas affects range, only one antenna at a time is used for transmission, without stacking; the time and power required are determined by that antenna.
• By default, if the energy required exceeds the craft's battery storage (plus energy generated during the transmission), the transmission will fail. Right-clicking the antenna and switching Require Complete to Allow Partial allows the antenna to keep trying to send the remaining data chunks while more electricity is generated. This can dramatically reduce the amount of battery storage required. However, Allow Partial may make the craft impossible to control during the lengthened transmission time, and the transmission may be lost if you switch away from the craft while it's retrying.

The following tables list the size of the scan data for each body, and the time and electricity required to transmit that data with a given antenna.

Energy (⚡)

Body	Kerbol	Kerbin	Mun	Minmus	Moho	Eve	Duna	Ike	Jool	Laythe	Vall	Bop	Tylo	Gilly	Pol	Dres	Eeloo
Mits	–	123	42	15	51	141	66	27	1200	102	63	15	123	3	9	30	45
Communotron 16	–	738	252	90	306	846	396	162	7200	612	378	90	738	18	54	180	270
Communotron 16-S	–	738	252	90	306	846	396	162	7200	612	378	90	738	18	54	180	270
Communotron DTS-M1	–	738	252	90	306	846	396	162	7200	612	378	90	738	18	54	180	270
Communotron HG-55	–	820	280	100	340	940	440	180	8004	680	420	100	820	20	60	200	300
Communotron 88-88	–	1230	420	150	510	1410	660	270	12000	1020	630	150	1230	30	90	300	450
HG-5 High Gain Antenna	–	1107	378	135	459	1269	594	243	10800	918	567	135	1107	27	81	270	405
RA-2 Relay Antenna	–	2952	1008	360	1224	3384	1584	648	28800	2448	1512	360	2952	72	216	720	1080
RA-15 Relay Antenna	–	1476	504	180	612	1692	792	324	14400	1224	756	180	1476	36	108	360	540
RA-100 Relay Antenna	–	738	252	90	306	846	396	162	7200	612	378	90	738	18	54	180	270

Time (s)

Body	Kerbol	Kerbin	Mun	Minmus	Moho	Eve	Duna	Ike	Jool	Laythe	Vall	Bop	Tylo	Gilly	Pol	Dres	Eeloo
Mits	–	123	42	15	51	141	66	27	1200	102	63	15	123	3	9	30	45
Communotron 16	–	37	13	5	15	42	20	8	360	31	19	5	37	1	3	9	14
Communotron 16-S	–	37	13	5	15	42	20	8	360	31	19	5	37	1	3	9	14
Communotron DTS-M1	–	22	7	3	9	25	12	5	210	18	11	3	22	1	2	5	8
Communotron HG-55	–	6	2	1	3	7	3	1	60	5	3	1	6	0	0	2	2
Communotron 88-88	–	6	2	1	3	7	3	1	60	5	3	1	6	0	0	2	2
HG-5 High Gain Antenna	–	22	7	3	9	25	12	5	210	18	11	3	22	1	2	5	8
RA-2 Relay Antenna	–	43	15	5	18	49	23	9	420	36	22	5	43	1	3	10	16
RA-15 Relay Antenna	–	22	7	3	9	25	12	5	210	18	11	3	22	1	2	5	8
RA-100 Relay Antenna	–	11	4	1	4	12	6	2	105	9	6	1	11	0	1	3	4

Changes

1.0

• Initial release