One perspective (heh) involves the following relation among position vectors: $$\vec{r}_{A\rightarrow C} = \vec{r}_{A\rightarrow B} + \vec{r}_{B\rightarrow C}.$$ These position vectors can be for anything; object $A$ could be a house, object $B$ an ant, and object $C$ a leaf on the river. Here's a diagram to help:

So if you want to know the position of object $C$ relative to object $A$, you just have to know the position of some other object $B$ relative to those others.

To answer your question, you can apply this same idea to the solar system: $$\vec{r}_{\mathrm{Sun} \rightarrow X} = \vec{r}_{\mathrm{Sun} \rightarrow \mathrm{Earth}} + \vec{r}_{\mathrm{Earth} \rightarrow X}.$$ Or in pictures:

The position of planet $X$ relative to the sun can be found if we know Earth's position relative to the Sun and planet $X$'s position relative to Earth. In this way, measurements of a planet's position as measured from here on Earth can be used to get a map of the solar system..

There is the added complication of knowing distance to planets and coming up with a convenient coordinate system in order to actually come up with values for these position vectors. Others may have better information on that.

One perspective (heh) involves the following relation among position vectors: $$\vec{r}_{A\rightarrow C} = \vec{r}_{A\rightarrow B} + \vec{r}_{B\rightarrow C}.$$ These position vectors can be for anything; object $A$ could be a house, object $B$ an ant, and object $C$ a leaf on the river. Here's a diagram to help:

So if you want to know the position of object $C$ relative to object $A$ (the bold dark arrow), you just have to know the position of some other object $B$ relative to those others.

To answer your question, you can apply this same idea to the solar system: $$\vec{r}_{\mathrm{Sun} \rightarrow X} = \vec{r}_{\mathrm{Sun} \rightarrow \mathrm{Earth}} + \vec{r}_{\mathrm{Earth} \rightarrow X}.$$ Or in pictures:

The position of planet $X$ relative to the sun (bold dark arrow, which is what we want) can be found if we know Earth's position relative to the Sun and planet $X$'s position relative to Earth. In this way, measurements of a planet's position as measured from here on Earth can be used to get a map of the solar system..

There is the added complication of knowing distance to planets and coming up with a convenient coordinate system in order to actually come up with values for these position vectors. Others may have better information on that.

One perspective (heh) involves the following relation among position vectors: $$\vec{r}_{A\rightarrow C} = \vec{r}_{A\rightarrow B} + \vec{r}_{B\rightarrow C}.$$ These position vectors can be for anything; object $A$ could be a house, object $B$ an ant, and object $C$ a leaf on the river. In particular, $$\vec{r}_{\mathrm{Sun} \rightarrow X} = \vec{r}_{\mathrm{Sun} \rightarrow \mathrm{Earth}} + \vec{r}_{\mathrm{Earth} \rightarrow X}.$$ The position of planet $X$ relative to the sun can be found if we know Earth's position relative to the Sun and planet $X$'s position relative to Earth. In this way, measurements of a planet's position relative to Earth can be used.

There is the added complication of knowing distance to planets and coming up with a convenient coordinate system in order to actually come up with values for these position vectors. Others may have better information on that.

One perspective (heh) involves the following relation among position vectors: $$\vec{r}_{A\rightarrow C} = \vec{r}_{A\rightarrow B} + \vec{r}_{B\rightarrow C}.$$ These position vectors can be for anything; object $A$ could be a house, object $B$ an ant, and object $C$ a leaf on the river. Here's a diagram to help:

So if you want to know the position of object $C$ relative to object $A$, you just have to know the position of some other object $B$ relative to those others.

To answer your question, you can apply this same idea to the solar system: $$\vec{r}_{\mathrm{Sun} \rightarrow X} = \vec{r}_{\mathrm{Sun} \rightarrow \mathrm{Earth}} + \vec{r}_{\mathrm{Earth} \rightarrow X}.$$ Or in pictures:

The position of planet $X$ relative to the sun can be found if we know Earth's position relative to the Sun and planet $X$'s position relative to Earth. In this way, measurements of a planet's position as measured from here on Earth can be used to get a map of the solar system..

There is the added complication of knowing distance to planets and coming up with a convenient coordinate system in order to actually come up with values for these position vectors. Others may have better information on that.