To solve this problem, we need to determine the orbital parameters using the given information and then calculate the eccentricity, eccentric anomaly, and areal velocity. Let's break it down into steps:

Given:

• Altitude: $h = 1800 \, \text{km}$
• Radial velocity: $v_r = -5 \, \text{km/s}$
• Transverse velocity: $v_t = 6 \, \text{km/s}$
• Radius of the Earth: $R = 6400 \, \text{km}$
• Gravitational parameter: $\mu = 398601 \, \text{km}^3/\text{s}^2$
• Radius from the Earth's center: $r = R + h = 6400 \, \text{km} + 1800 \, \text{km} = 8200 \, \text{km}$

Step 1: Determine the eccentricity of the orbit

The specific orbital energy $\epsilon$ is given by: $\epsilon = \frac{v^2}{2} - \frac{\mu}{r}$ where the total velocity $v$ is given by: $v = \sqrt{v_r^2 + v_t^2}$

The semi-major axis $a$ can be found using the specific orbital energy: $\epsilon = -\frac{\mu}{2a}$

Step 2: Calculate the eccentricity $e$

The eccentricity $e$ is related to the radial velocity $v_r$, transverse velocity $v_t$, semi-major axis $a$, and the gravitational parameter $\mu$ by: $e = \sqrt{1 + \frac{2\epsilon h^2}{\mu^2}}$

Step 3: Determine the eccentric anomaly $E$

The eccentric anomaly $E$ can be found using the relationship between the true anomaly $\theta$, eccentricity $e$, and $r$: $\tan\left(\frac{\theta}{2}\right) = \sqrt{\frac{1+e}{1-e}} \tan\left(\frac{E}{2}\right)$

Step 4: Calculate the areal velocity

The areal velocity $\text{Areal Velocity}$ is given by: $\text{Areal Velocity} = \frac{r \times v_t}{2}$

Let's calculate these values.Here are the calculated results:

1. Semi-major axis $a$: $11{,}005.07 \, \text{km}$
2. Eccentricity $e$: $0.6695$
3. Areal velocity: $24{,}600 \, \text{km}^2/\text{s}$

To find the eccentric anomaly $E$ at the time $t_0$, we would need the true anomaly or additional information about the satellite's position relative to the perigee. However, with the current data, the above values summarize the satellite's orbit and its dynamic properties.

Would you like more details or have any questions?

Here are some related questions you might find interesting:

1. How does the eccentricity impact the shape of the orbit?
2. What would the orbital period be given the semi-major axis $a$?
3. How is the areal velocity connected to Kepler's second law?
4. How does the radial velocity affect the satellite's motion over time?
5. What would happen to the orbit if the transverse velocity were doubled?

Tip: The eccentricity $e$ of an orbit determines how elliptical the orbit is, with $e = 0$ being a perfect circle and $e \to 1$ being a highly elongated ellipse.